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  • Öhlen, Erik
    et al.
    Karolinska Inst, Dept Clin Neurosci, Stockholm, Sweden.;Uppsala Univ, Ctr Clin Res Sormland, Eskilstuna, Sweden..
    El-Hajj, Victor Gabriel
    Karolinska Inst, Dept Clin Neurosci, Stockholm, Sweden..
    Staartjes, Victor E.
    Karolinska Inst, Dept Clin Neurosci, Stockholm, Sweden.;Löwenströmska Hosp, Capio Spine Ctr Stockholm, Upplands Väsby, Sweden.;Univ Hosp Zurich, Dept Neurosurg, Zurich, Switzerland..
    Jabbour, Pascal
    Thomas Jefferson Univ Hosp, Dept Neurol Surg, Philadelphia, PA USA..
    Edström, Erik
    Karolinska Inst, Dept Clin Neurosci, Stockholm, Sweden.;Löwenströmska Hosp, Capio Spine Ctr Stockholm, Upplands Väsby, Sweden.;Örebro Univ, Dept Med Sci, Örebro, Sweden..
    Elmi-Terander, Adrian
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Surgical Sciences, Orthopaedics and Handsurgery. Karolinska Inst, Dept Clin Neurosci, Stockholm, Sweden.;Löwenströmska Hosp, Capio Spine Ctr Stockholm, Upplands Väsby, Sweden.;Örebro Univ, Dept Med Sci, Örebro, Sweden..
    Difference in clinical presentation and surgical outcomes in pediatric and adult patients with Chiari malformation type 1: a single center retrospective study2025In: Acta Neurochirurgica, ISSN 0001-6268, E-ISSN 0942-0940, Vol. 167, no 1, article id 120Article in journal (Refereed)
    Abstract [en]

    Introduction

    Chiari malformation type 1 (CM1) is a common congenital disorder affecting both children and adults. Although pediatric and adult CM1 patients share many characteristics, the differences between the groups are not fully described.

    Method

    A comparative analysis was made of two previously defined cohorts of adult and pediatric non-syndromic CM1, surgically treated at the study center. Clinical outcomes were assessed using the Chicago Chiari outcome scale (CCOS) and radiological outcomes were measured as change in cerebellar tonsil and syringomyelia status.

    Results

    A total of 209 patients (73 pediatric, 136 adults) were included, with median ages of 11 and 33 years, respectively. The proportion of female patients (62% vs 78%) was higher in the adult population (p = 0.012). Headache (p = 0.007), neck pain (p = 0.000), vertigo (p = 0.007), and sensory symptoms (p = 0.000) were more common in adults, while scoliosis (p = 0.000) and sleep apnea (p = 0.015) were more common in the pediatric population. Preoperative imaging findings did not differ significantly. After posterior fossa decompression, both groups scored a median CCOS of 15 at early follow-up (3 vs 4 months), though the pediatric population had a more favorable distribution of CCOS scores (p = 0.003). Postoperatively, syringomyelia status did not differ significantly between groups, but cerebellar tonsil status improved more frequently in adults (64% vs 88%, p = 0.000).

    Conclusion

    This study demonstrates that while headache is the most common presenting symptom in both pediatric and adult CM1 patients, pediatric patients are more likely to present with scoliosis and sleep apnea. In contrast adult patients more frequently experience headache, neck pain, vertigo, and sensory symptoms. There were no differences in other preoperative imaging variables and outcomes were favorable for most patients in both groups.

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  • Samuelsson, Erik
    Uppsala University, Disciplinary Domain of Science and Technology, Biology, Biology Education Centre.
    Emigration patterns, habitat preferences and morphological differences in Northern pike (Esox lucius) larvae2025Independent thesis Advanced level (degree of Master (Two Years)), 30 credits / 45 HE creditsStudent thesis
    Abstract [en]

    The Baltic Sea has undergone a regime-shift. Anthropogenic and abiotic factors have caused a shift to a system which is dominated by meso-predators instead of top-predator. This regime-shift has been seen in both the pelagic and the coastal ecosystem. In some coastal areas, there has been a decrease in predatory fishes, like pike (Esox lucius) and perch (Perca fluviatilis). Recruitment failure is one explanation, and habitat destruction is part of the problem. Sympatric populations of pike in the Baltic Sea have two different spawning strategies. One part of the population spawn in shallow, vegetated areas in the Baltic Sea. The other part is anadromous and migrate to freshwater wetlands to spawn. These areas warm up fast and have higher abundance of food. Many of these wetlands have been drained to increase area for agricultural land. Some of these wetlands have been restored to promote pike recruitment in the Baltic Sea. These restored wetlands are called “Pike factories”. In this project, two restored wetlands called Snäckstavik and Kyrksjön are studied with focus on pike larvae. Larvae production, habitat preferences, diet and morphology were investigated. A transect inventory using the “white-plate”-method was used to investigate the habitat preferences of pike larvae over time in different vegetation densities. To study the emigration larvae were caught for morphology and diet analyses. The water temperature and weather were noted each day to see what influenced emigration. The results from the study were that larvae preferred dense, rather than sparse and decayed vegetation. In dense vegetation, there is higher abundance of food and gives protection from predators. Emigration started when water temperature increased, and the pike were smaller than 2 cm. In Snäckstavik the emigration peaked with higher water temperature and higher light intensity, while in Kyrksjön the emigration peaked with decreasing water-level. The morphology of the pike depended on time of emigration and diet-choice. The findings of this study show that when restoring a wetland, dense vegetation is an important factor for recruitment success.

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  • Murray, Shawn B.
    et al.
    Univ New Hampshire, Dept Nursing, 4 Lib Way, Durham, NH 03824 USA..
    Kanter, Carley
    Univ New Hampshire, Dept Nursing, 4 Lib Way, Durham, NH 03824 USA..
    O'Brien, Alyssa
    Univ New Hampshire, Dept Nursing, 4 Lib Way, Durham, NH 03824 USA..
    Clark, Kristen D.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Clinical Psychiatry. Univ New Hampshire, Dept Nursing, 4 Lib Way, Durham, NH 03824 USA..
    Faculty Inclusion of Lesbian, Gay, Bisexual, Transgender, and Queer Populations in Health Curriculum2025In: Teaching and Learning in Nursing, ISSN 1557-3087, Vol. 20, no 2, p. e395-e401Article in journal (Refereed)
    Abstract [en]

    Background:

    LGBTQ+ people have widely described harmful experiences in healthcare settings. To address this deficit in care, previous studies have focused on improving the education of nursing and allied health students to care for LGBTQ+ people, yet few evaluate faculty preparedness.

    Aim:

    This study aimed to assess faculty's LGBTQ+-related health knowledge, self-efficacy, and inclusion related to curriculum.

    Methods:

    A Qualtrics survey was developed to assess faculty's knowledge, self-efficacy, and inclusion of LGBTQ+ curriculum at a university in the United States between March 4 and April 13, 2022. Paired t-tests and correlation matrices were used to evaluate constructs. Results: Among 38 participants, LGB health content knowledge was greater than T+ knowledge. LGBTQ+ self-efficacy and inclusion were moderate, with no difference between subscales. LGBTQ+ health self-efficacy and inclusion were positively correlated.

    Conclusions:

    These findings highlight gaps in faculty knowledge and inclusion of health content, particularly related to T+ health. This study's findings form a foundation for continued efforts to improve nursing and other allied health faculty's preparedness to educate students to provide inclusive and affirming care to LGBTQ+ patients.

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  • Gredebäck, Gustaf
    et al.
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Psychology.
    Astor, Kim
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Psychology.
    Ainamani, Herbert
    Kabale Univ, Sch Med, Dept Mental Hlth, Kabale, Uganda..
    van den Berg, Linda
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Psychology.
    Forssman, Linda
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Psychology.
    Hall, Jonathan
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Peace and Conflict Research.
    Juvrud, Joshua
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Psychology.
    Kenward, Ben
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Psychology. Oxford Brookes Univ, Sch Psychol Social Work & Publ Hlth, Oxford, England..
    Mhizha, Samson
    Univ Zimbabwe, Dept Appl Psychol, Harare, Zimbabwe. Khesar Gyalpo Univ Med Sci Bhutan, Publ Heath & Allied Hlth Sci Dept, Thimphu, Bhutan..
    Wangchuk,
    Public Heath and Allied Health Sciences Department, Khesar Gyalpo University of Medical Sciences of Bhutan.
    Nyström, Pär
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Psychology.
    Infant Gaze Following Is Stable Across Markedly Different Cultures and Resilient to Family Adversities Associated With War and Climate Change2025In: Psychological Science, ISSN 0956-7976, E-ISSN 1467-9280, Vol. 36, no 4, p. 296-307Article in journal (Refereed)
    Abstract [en]

    Gaze following in infancy allows triadic social interactions and a comprehension of other individuals and their surroundings. Despite its importance for early development, its ontology is debated, with theories suggesting that gaze following is either a universal core capacity or an experience-dependent learned behavior. A critical test of these theories among 809 nine-month-olds from Africa (Uganda and Zimbabwe), Europe (Sweden), and Asia (Bhutan) demonstrated that infants follow gaze to a similar degree regardless of environmental factors such as culture, maternal well-being (postpartum depression, well-being), or traumatic family events (related to war and/or climate change). These findings suggest that gaze following may be a universal, experience-expectant process that is resilient to adversity and similar across a wide range of human experiences-a core foundation for social development.

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  • Rocha, Gustavo
    et al.
    CHU Sao Joao, Dept Neonatol, Porto, Portugal..
    Soares, Paulo
    CHU Sao Joao, Dept Neonatol, Porto, Portugal..
    Flor-De-Lima, Filipa
    CHU Sao Joao, Dept Neonatol, Porto, Portugal.;Univ Porto, Fac Med, Dept Obstet Gynecol & Pediat, Porto, Portugal..
    Amaral, Rita
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Women's and Children's Health, Paediatric Inflammation, Metabolism and Child Health Research. Univ Porto, Fac Med, Dept Community Med Informat & Hlth Decis Sci MEDCI, Porto, Portugal; Univ Porto, Fac Med, CINTESIS RISE Hlth Res Network, Porto, Portugal.
    Automated Adjustment of the Fraction of Inspired Oxygen (FiO2) and the Time Spent in Normoxemia in Preterm Infants: [O Ajuste Automático da Fração Inspirada de Oxigénio (FiO2) e o Tempo em Normoxémia em Recém-Nascidos Prematuros]2025In: Acta Médica Portuguesa, ISSN 0870-399X, E-ISSN 1646-0758, Vol. 38, no 4, p. 208-216Article in journal (Refereed)
    Abstract [en]

    Introduction: The challenge of maintaining normoxemia in preterm infants undergoing respiratory support and oxygen therapy has led to the development of closed-loop automatic control systems for FiO2. The aim of this study was to assess the effectiveness of these systems in maintaining SpO2 within a target range (90% - 94%) in preterm neonates receiving supplemental oxygen.

    Methods: We conducted a single-centre prospective study over a three-year period (2020 - 2023) including preterm infants with a gestational age < 33 weeks who received supplemental oxygen within the first 24 hours of life and either invasive or non-invasive respiratory support. The closed-loop automatic control of FiO2 used was the Predictive Intelligent Control of Oxygenation feature on Fabian® ventilators. Two groups were randomized and compared, one receiving automatic plus manual control of FiO2, and the other receiving routine manual control. Uni- and multivariable regression analyses (linear or Poisson) were used to evaluate the association between the use of closed-loop automatic control of FiO2 and the parameters of manual adjustments, hypoxemia, hyperoxemia, and normoxemia.

    Results: The study included 89 patients, of which 45 received automatic plus manual control of FiO2 and 44 received routine manual control. The first group required fewer manual adjustments of FiO2, experienced fewer episodes of hypoxemia and hyperoxemia (p < 0.002), and spent more time with SpO2 within the target range (p < 0.001), compared to the second group. After adjustment for confounding, the total time spent in normoxemia was higher when in automatic plus manual control of FiO2 (β = 81.5; 95%CI: 47.9 - 115.2, p < 0.001).

    Conclusion: The use of closed-loop automatic control of FiO2 seems feasible and was associated with fewer episodes of hypoxia and hyperoxia, thereby maintaining SpO2 within normal limits for longer periods. Additionally, it has been shown to be associated with a reduction in manual interventions.

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  • Raucci, Luisa
    et al.
    Univ Siena, Dept Biotechnol Chem & Pharm, Via A Moro 2, I-53100 Siena, Italy..
    Perrone, Cosimo Damiano
    Univ Siena, Dept Biotechnol Chem & Pharm, Via A Moro 2, I-53100 Siena, Italy..
    Barbera, Stefano
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Immunology, Genetics and Pathology, Vascular Biology. Uppsala University, Science for Life Laboratory, SciLifeLab. Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Immunology, Genetics and Pathology, Cancer Immunotherapy. Univ Siena, Dept Biotechnol Chem & Pharm, Via A Moro 2, I-53100 Siena, Italy.
    de Boer, Laurens Julius
    Univ Siena, Dept Biotechnol Chem & Pharm, Via A Moro 2, I-53100 Siena, Italy.;Univ Gustave Eiffel, COSYS, IMSE, 5 Blvd Descartes Champs sur 77, Marne la Vallee, France..
    Tosi, Gian Marco
    Univ Siena, Ophthalmol Unit, Dept Med Surg & Neurosci, I-53100 Siena, Italy..
    Brunetti, Jlenia
    Univ Siena, Dept Med Biotechnol, I-53100 Siena, Italy..
    Bracci, Luisa
    Univ Siena, Dept Med Biotechnol, I-53100 Siena, Italy..
    Pozzi, Cecilia
    Univ Siena, Dept Biotechnol Chem & Pharm, Via A Moro 2, I-53100 Siena, Italy.;Consorzio Interuniv Risonanze Magnet Met Prot CIRM, I-50019 Sesto Fiorentino, FI, Italy..
    Galvagni, Federico
    Univ Siena, Dept Biotechnol Chem & Pharm, Via A Moro 2, I-53100 Siena, Italy..
    Orlandini, Maurizio
    Univ Siena, Dept Biotechnol Chem & Pharm, Via A Moro 2, I-53100 Siena, Italy..
    Structural and antigen-binding surface definition of an anti-CD93 monoclonal antibody for the treatment of degenerative vascular eye diseases2025In: International Journal of Biological Macromolecules, ISSN 0141-8130, E-ISSN 1879-0003, Vol. 309, article id 143118Article in journal (Refereed)
    Abstract [en]

    CD93 is a receptor predominantly expressed on the surface of endothelial cells, where it plays a pivotal role in angiogenesis through its interaction with the extracellular matrix. In our previous studies, we identified the monoclonal antibody 4E1 as a potent inhibitor of angiogenesis by targeting the CD93-Multimerin-2 axis. Here, we report the development of 4E1 as a recombinant whole immunoglobulin and a single-chain variable fragment, designated sc-4E. Both formats retained the binding properties of the parental monoclonal antibody and exhibited comparable inhibitory effects on endothelial cell migration and differentiation. To elucidate the molecular basis of the 4E1-CD93 interaction, we initially employed machine learning-based modeling and docking analyses of the variable heavy and light domains of 4E1. Subsequent crystallographic analysis of sc-4E provided high-resolution structural insights, confirming and validating the predicted model. Further docking experiments and molecular dynamics simulations using the crystallographic structures of CD93 and sc-4E revealed that the interaction is primarily mediated by the CDR-H3 and CDR-L2 loops. Notably, these regions engage with the sushi-like domain of CD93, which is critical for its interaction with Multimerin-2. This comprehensive structural and functional characterization of 4E1 and sc-4E underscores their potential as anti-angiogenic agents. By effectively inhibiting endothelial cell migration and differentiation, 4E1 derivatives represent promising therapeutic candidates for the treatment of ocular vascular diseases driven by pathological angiogenesis.

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  • Lundgren Mortensen, Anja Charlotte
    et al.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Immunology, Genetics and Pathology, Cancer precision medicine. Karolinska Inst, Dept Mol Med & Surg, Stockholm, Sweden..
    Hofström, Camilla
    Persson, Helena
    Royal Inst Technol KTH, Sci Life Labs SciLifeLab, Drug Discovery & Dev, Stockholm, Sweden..
    Dahllund, Leif
    Royal Inst Technol KTH, Sci Life Labs SciLifeLab, Drug Discovery & Dev, Stockholm, Sweden..
    Frejd, Fredrik
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Immunology, Genetics and Pathology, Cancer precision medicine.
    Nestor, Marika
    Uppsala University, Science for Life Laboratory, SciLifeLab. Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Immunology, Genetics and Pathology, Cancer precision medicine.
    Affinity maturation and optimization of CD44v6-targeting antibodies for molecular radiotherapy2025In: Nuclear Medicine and Biology, ISSN 0969-8051, E-ISSN 1872-9614, Vol. 144-145, article id 109012Article in journal (Refereed)
    Abstract [en]

    Aim:

    This study aimed to improve the efficacy of the CD44v6-targeting antibody UU-40 for molecular radiotherapy through affinity maturation and IgG subclass optimization.

    M&M:

    A panel of affinity-matured antibody candidates was generated and characterized as both human IgG4 and IgG1 with LALA mutations. Surface plasmon resonance and LigandTracer analyses identified several candidates with superior affinity and off-rates compared to the parental UU-40. Biodistribution studies in xenograft models using Lutetium-177 (177Lu)-labeled antibodies showed improved tumor retention for selected candidates, particularly UU-A-155. Species cross-reactivity assays confirmed binding to cynomolgus and rabbit v6-peptides, supporting future toxicity studies.

    Results:

    The IgG1 LALA format demonstrated reduced binding to Fc gamma receptors, potentially improving the safety profile. UU-A-155 emerged as the lead candidate for clinical translation, showing superior performance in both affinity and tumor retention. Our findings highlight the importance of comprehensive in vitro and in vivo assessments in antibody development, and provides valuable insights into optimizing antibody-based molecular radiotherapy.

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  • Public defence: 2025-05-30 09:00 Rosénsalen, Uppsala
    Sejersen, Kristina
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Clinical Chemistry. Department of Medical Sciences, Section of Clinical Chemistry, Uppsala University , Uppsala, Sweden;Unilabs AB , Stockholm, Sweden.
    Analysis of calprotectin as an early marker for bacterial infection and inflammation2025Doctoral thesis, comprehensive summary (Other academic)
    Abstract [en]

    Calprotectin, a calcium-binding protein complex of S100A8 and S100A9, is abundant in neutrophils and released upon their activation. It has emerged as a potential biomarker for several inflammatory conditions, including respiratory infections, sepsis, and rheumatoid arthritis. With increasing concerns about antibiotic resistance, there is a need to accurately differentiate between bacterial and viral infections for better treatment decisions.

    This thesis investigates the diagnostic performance of calprotectin in respiratory tract infections, its activation kinetics following inflammatory stimuli, its role as a biomarker in rheumatoid arthritis, and to compare total calprotectin levels with its subunits in intensive care unit (ICU) patients with sepsis. The studies included patients with respiratory infections, post-operative inflammation, rheumatoid arthritis, and sepsis, measuring calprotectin levels in serum, plasma, and synovial fluid.

    Results showed significantly higher calprotectin levels in bacterial infections compared to viral infections and healthy controls. It outperformed procalcitonin (PCT) and Heparin-binding protein (HBP) in distinguishing bacterial from viral respiratory infections, including mycoplasma. Calprotectin levels increased rapidly (within 2 hours) following inflammation, earlier than CRP and IL-6. In rheumatoid arthritis, serum calprotectin correlated strongly with inflammatory markers, particularly in anti-citrullinated protein antibodies (ACPA)-positive patients. In ICU patients, total calprotectin performed better than its subunits (S100A8 and S100A9) in differentiating sepsis from non-sepsis cases.

    Calprotectin shows promise as a biomarker for early detection of bacterial infections and inflammation. Its rapid rise and superior ability to differentiate bacterial and viral infections highlight its potential to improve the management of respiratory infections and guide antibiotic use. However, further research is needed to standardise assays and fully understand its specificity in various clinical contexts.

    List of papers
    1. Calprotectin, a new biomarker for diagnosis of acute respiratory infections
    Open this publication in new window or tab >>Calprotectin, a new biomarker for diagnosis of acute respiratory infections
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    2020 (English)In: Scientific Reports, E-ISSN 2045-2322, Vol. 10, no 1, article id 4208Article in journal (Refereed) Published
    Abstract [en]

    Respiratory tract infections require early diagnosis and adequate treatment. With the antibiotic overuse and increment in antibiotic resistance there is an increased need to accurately distinguish between bacterial and viral infections. We investigated the diagnostic performance of calprotectin in respiratory tract infections and compared it with the performance of heparin binding protein (HBP) and procalcitonin (PCT). Biomarkers were analyzed in patients with viral respiratory infections and patients with bacterial pneumonia, mycoplasma pneumonia and streptococcal tonsillitis (n=135). Results were compared with values obtained from 144 healthy controls. All biomarkers were elevated in bacterial and viral infections compared to healthy controls. Calprotectin was significantly increased in patients with bacterial infections; bacterial pneumonia, mycoplasma pneumonia and streptococcal tonsillitis compared with viral infections. PCT was significantly elevated in patients with bacterial pneumonia compared to viral infections but not in streptococcal tonsillitis or mycoplasma caused infections. HBP was not able to distinguish between bacterial and viral causes of infections. The overall clinical performance of calprotectin in the distinction between bacterial and viral respiratory infections, including mycoplasma was greater than performance of PCT and HBP. Rapid determination of calprotectin may improve the management of respiratory tract infections and allow more precise diagnosis and selective use of antibiotics.

    Place, publisher, year, edition, pages
    NATURE PUBLISHING GROUP, 2020
    National Category
    Infectious Medicine
    Identifiers
    urn:nbn:se:uu:diva-420925 (URN)10.1038/s41598-020-61094-z (DOI)000560099000007 ()32144345 (PubMedID)
    Available from: 2020-10-05 Created: 2020-10-05 Last updated: 2025-03-26Bibliographically approved
    2. Early kinetics of calprotectin in plasma following inguinal hernia surgery
    Open this publication in new window or tab >>Early kinetics of calprotectin in plasma following inguinal hernia surgery
    2022 (English)In: Innate Immunity, ISSN 1753-4259, E-ISSN 1753-4267, Vol. 28, no 1, p. 49-54Article in journal (Refereed) Published
    Abstract [en]

    Calprotectin is one of the most abundant proteins of neutrophil granulocytes. It is released upon neutrophil activation and is considered a sensitive and clinically useful marker for neutrophil-mediated inflammation, including bacterial infections. However, early kinetics of calprotectin activation following inflammatory activation has hitherto been unknown. The aim of the present study was to determine the early phase of the kinetics of calprotectin, in comparison with the inflammatory markers CRP, IL-6, TNF-α, and procalcitonin, in plasma following a standardized temporary mild inflammatory response, using uncomplicated inguinal hernia surgery as a model. The study cohort consisted of 17 adult patients (15 male and 2 female) undergoing elective surgery for hernia. Values of calprotectin increased significantly at 2 h following surgery, and continued to increase to reach the highest level at 24-36 h after surgery, values still not exceeding upper normal reference level. This contrasts to IL-6 and CRP, for which an elevation was found first later, 4 h and 24-36 h post-surgery, respectively, for IL-6, and CRP. No significant increase was seen for TNF-α, or procalcitonin. The data demonstrate a very rapid and significant but modest increase in calprotectin following induction of mild inflammation, supporting that calprotectin can be useful for early detection of inflammatory response.

    Place, publisher, year, edition, pages
    Sage Publications, 2022
    Keywords
    Calprotectin, inflammation, inguinal hernia surgery, kinetics
    National Category
    Cardiology and Cardiovascular Disease
    Identifiers
    urn:nbn:se:uu:diva-467782 (URN)10.1177/17534259211069635 (DOI)000752294600001 ()35102763 (PubMedID)
    Available from: 2022-02-16 Created: 2022-02-16 Last updated: 2025-03-26Bibliographically approved
    3. Serum calprotectin correlates stronger with inflammation and disease activity in ACPA positive than ACPA negative rheumatoid arthritis
    Open this publication in new window or tab >>Serum calprotectin correlates stronger with inflammation and disease activity in ACPA positive than ACPA negative rheumatoid arthritis
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    2023 (English)In: Rheumatology, ISSN 1462-0324, E-ISSN 1462-0332, article id kead641Article in journal (Refereed) Epub ahead of print
    Abstract [en]

    Objectives

    The aim of the present study was to evaluate the performance of serum and SF levels of the granulocyte protein calprotectin as an inflammatory biomarker in RA patients with knee synovitis.

    Methods

    Seventy-six RA patients with ongoing knee synovitis were included. Data on DAS with 28 joints and their subcomponents and radiological destruction of the affected knee were collected. White blood cell count, CRP, ACPA against cyclic citrullinated peptide version 2 (anti-CCP2), IgM RF and calprotectin were analysed in parallel in circulation and in SF. Counts of polynuclear and mononuclear cells were measured in SF.

    Results

    Serum (S)-calprotectin correlated more strongly than SF-calprotectin with inflammatory markers and disease activity. Instead, SF-calprotectin showed a strong correlation to SF counts of white blood cells, and especially to polymorphonuclear cell counts (Spearman’s ρ = 0.72, P < 0.001). S-calprotectin showed markedly stronger correlation with inflammatory markers and disease activity in ACPA positive as compared with ACPA negative RA patients; a similar difference was observed for patients with and without IgM RF.

    Conclusion

    The particularly strong association between circulating calprotectin and inflammation in ACPA positive RA is a new argument for a specific role for polymorphonuclear granulocytes/neutrophils in this RA subset. Measurement of calprotectin in SF does not convey any additional benefit compared with measurement in the circulation in RA patients with knee synovitis.

    Place, publisher, year, edition, pages
    Oxford University Press, 2023
    Keywords
    rheumatoid arthritis, calprotectin, inflammation, anti-citrullinated peptide antibodies, antibodies against cyclic citrullinated peptide version 2, rheumatoid factor
    National Category
    Clinical Medicine
    Identifiers
    urn:nbn:se:uu:diva-525251 (URN)10.1093/rheumatology/kead641 (DOI)001123175100001 ()38048609 (PubMedID)
    Funder
    Swedish Rheumatism Association, R-982369Uppsala University, 965453Region Gavleborg, 965453Stiftelsen Konung Gustaf V:s 80-årsfond, FAI-2021-0823
    Available from: 2024-03-20 Created: 2024-03-20 Last updated: 2025-03-26Bibliographically approved
    4. Comparison of total calprotectin levels with S100A8 and S100A9 subunit levels in critically ill patients
    Open this publication in new window or tab >>Comparison of total calprotectin levels with S100A8 and S100A9 subunit levels in critically ill patients
    (English)Manuscript (preprint) (Other academic)
    Abstract [en]

    Calprotectin is a 24 kD heterodimer of calcium-binding proteins S100A8 and S100A9. At present, there is a lack of knowledge about the specificity of various methods for calprotectin detection, whether they measure only dimers between S100A8 and S100A9, S100A8-S100A8 dimers, S100A9/S100A9 dimers, or free subunits. This study aimed to compare total calprotectin levels with those of its subunits, S100A8 and S100A9, in ICU patients. This prospective observational study includes 271 sepsis and non-sepsis patients. Inclusion criteria were admission to intensive care and the presence or need for an arterial catheter. Plasma total calprotectin was measured at ICU admission and the following two days by particle-enhanced turbidimetric (PETIA) calprotectin reagents from Gentian AS and a Mindray BS380 chemistry analyzer. S100A8 and S100A9 were analyzed by commercial sandwich ELISA DY4570-05, and DY5578, R&D Systems, respectively. Sepsis was defined according to Sepsis-3 as suspected infection and a Sequential organ failure assessment (SOFA) >2 on admission. Receiver operating characteristic (ROC) analysis showed that total calprotectin had a larger area under the curve (AUC) for distinguishing sepsis from non-sepsis patients (0.67) compared to S100A8 (0.59) and S100A9 (0.52). For predicting 30-day mortality, S100A9 had a higher AUC value (0.64) than S100A8 (0.59). However, correlations between total calprotectin and its subunits were weak, indicating no significant relationship for predicting 30-day mortality, and highlighting potential issues with assay harmonization across manufacturers.

    Keywords
    Calprotectin, S100A8/S100A9, S100A8, S100A9, sepsis
    National Category
    Clinical Laboratory Medicine
    Identifiers
    urn:nbn:se:uu:diva-553394 (URN)
    Projects
    Nej
    Available from: 2025-03-26 Created: 2025-03-26 Last updated: 2025-03-28Bibliographically approved
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  • Abdollahi, Anna M.
    et al.
    Univ Helsinki, Dept Food & Nutr, POB 66, Helsinki 00014, Finland..
    Li, Xinyue
    City Univ Hong Kong, Sch Data Sci, Hong Kong, Peoples R China..
    Merikanto, Ilona
    Univ Helsinki, Fac Med, Helsinki, Finland.;Finnish Inst Hlth & Welf, Dept Publ Hlth & Welf, Helsinki, Finland.;Orton Orthopaed Hosp, Helsinki, Finland..
    Vepsäläinen, Henna
    Univ Helsinki, Dept Food & Nutr, POB 66, Helsinki 00014, Finland..
    Lehto, Reetta
    Univ Helsinki, Dept Food & Nutr, POB 66, Helsinki 00014, Finland.;Folkhalsan, Folkhalsan Res Ctr, Helsinki, Finland..
    Rahkola, Jenna
    Folkhalsan, Folkhalsan Res Ctr, Helsinki, Finland..
    Nissinen, Kaija
    Univ Helsinki, Dept Food & Nutr, POB 66, Helsinki 00014, Finland.;Seinajoki Univ Appl Sci, Sch Food & Agr, Seinajoki, Finland..
    Kanerva, Noora
    Univ Helsinki, Dept Food & Nutr, POB 66, Helsinki 00014, Finland..
    Roos, Eva
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Food Studies, Nutrition and Dietetics. Folkhalsan, Folkhalsan Res Ctr, Helsinki, Finland; Univ Helsinki, Dept Publ Hlth, Helsinki, Finland.
    Erkkola, Maijaliisa
    Univ Helsinki, Dept Food & Nutr, POB 66, Helsinki 00014, Finland..
    A tendency toward evening chronotype associates with less healthy diet among preschoolers: cross-sectional findings from the DAGIS study2024In: SLEEP Advances, E-ISSN 2632-5012, Vol. 5, no 1, article id zpae026Article in journal (Refereed)
    Abstract [en]

    Study Objectives

    Evidence suggests that adolescents and adults with a later chronotype have poorer sleep habits and are more susceptible to unhealthy behaviors, but little is known about these associations in younger children. The objective of the study was to (1) identify and compare individual chronotype tendencies among preschool-aged children and (2) investigate associations of sleep dimensions and chronotype with diet.

    Methods

    Participants were 636 3–6 years old (mean ± SD age: 4.74 ± 0.89 years, 49% girls) preschoolers from the cross-sectional Increased Health and Well-Being in Preschoolers (DAGIS) study in Finland. Sleep duration, sleep variability (in duration and midpoint), social jetlag, and midsleep on weekends adjusted for sleep debt (MSWEadj) were measured with 7-day actigraphy. Morning, intermediate, and evening chronotype tendencies were defined based on the lowest and highest 10th percentile cutoffs of MSWEadj. Food, energy, and macronutrient intake were assessed from 3-day records. Associations between sleep dimensions and diet were assessed with regression models.

    Results

    MSWEadj was 1:13 ± 14 minutes for morning (n = 64), 2:25 ± 28 minutes for intermediate (n = 560), and 3:38 ± 15 minutes for evening (n = 64) chronotype tendency. Children with an evening chronotype tendency had greater social jetlag and sleep variability. Having an evening chronotype tendency was associated with higher added sugar, higher sugary food consumption, and lower vegetable consumption compared to intermediate tendency types. A later chronotype (MSWEadj) was associated with higher sugary food consumption, as well as lower vegetable and fiber intake. Sleep duration, social jetlag, and sleep variability were not associated with diet.

    Conclusions

    Several less healthy sleep and diet behaviors were observed among children with later chronotypes. Future public health interventions aimed towards children would benefit from taking into account chronotype.

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  • Franzese, Fabio
    et al.
    SHARE BERLIN Inst, Berlin, Germany..
    Hettiarachchi, Pasan
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Occupational and Environmental Medicine.
    Holtermann, Andreas
    Natl Res Ctr Working Environm, Copenhagen, Denmark..
    Ahmadi, Matthew
    Univ Sydney, Fac Med & Hlth, Sydney, NSW, Australia.;Univ Sydney, Charles Perkins Ctr, Mackenzie Wearables Res Hub, Sydney, NSW, Australia..
    Johansson, Peter
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Occupational and Environmental Medicine. Uppsala Univ Hosp, Occupat & Environm Med, Uppsala, Sweden..
    Comparing Physical Activity Metrics From Different Placements of Thigh-Worn Accelerometers2025In: Journal for the Measurement of Physical Behaviour, ISSN 2575-6605, Vol. 8, no 1, article id 0043Article in journal (Refereed)
    Abstract [en]

    Background:

    Compared with other placements, thigh-worn accelerometers offer the advantage to accurately capture postures. However, the lack of standardized sensor placement on the thigh raises concerns about the comparability and harmonization of data across studies. This study aimed to investigate the impact of sensor placement on thigh-worn accelerometer measurements.

    Methods:

    Thirty-six participants wore two sensors simultaneously at center- and upper-thigh position on the same thigh during daily activities for several days. Metrics of vector magnitude (Euclidian Norm Minus One), postures, and activities generated by GGIR and ActiPASS were analyzed with Bland-Altman plots and linear regressions.

    Results:

    The findings revealed a significant dependence of vector magnitude on sensor placement: 1 cm higher distance between the center- and upper-thigh position was correlated with almost 1 mg higher difference in Euclidian Norm Minus One between the two positions (b = 0.94; 95% confidence interval [0.26, 1.62]). For time spent sedentary (b = 0.03; 95% confidence interval [-2.48, 2.55]) and intense physical activities (b = 0.22; 95% confidence interval [-0.10, 0.54]), the sensor position had no significant effect on the results. High concordance was also observed for other activities, such as walking, running, and sleeping.

    Conclusions:

    The analyses suggest that, despite variations in sensor placement, thigh-worn accelerometry data can be compared and harmonized for most postures and activities when analyzed by ActiPASS. The robust metrics by ActiPASS to accelerometer placements is likely because it utilizes multiple features in the acceleration signal (e.g., inclination, rotation) to classify activities and postures, rather than relying on a single feature (vector magnitude).

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  • Götze Eriksson, Rebecca
    et al.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Women's and Children's Health, Obstetrics and Reproductive Health Research.
    Skalkidou, Alkistis
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Women's and Children's Health, Obstetrics and Reproductive Health Research.
    Cruz, Natalia
    Capio Specialistctr, Stockholm, Sweden..
    Hirschberg, Angelica Linden
    Karolinska Inst, Dept Womens & Childrens Hlth, Stockholm, Sweden.;Karolinska Univ Hosp, Dept Gynecol & Reprod Med, Stockholm, Sweden..
    Iliadis, Stavros
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Women's and Children's Health, Obstetrics and Reproductive Health Research.
    Swedish physicians' knowledge of and prescribing practices for menopausal hormone therapy: A nationwide cross-sectional survey2025In: Maturitas, ISSN 0378-5122, E-ISSN 1873-4111, Vol. 197, article id 108263Article in journal (Refereed)
    Abstract [en]

    Objectives

    To investigate current prescribing practices, knowledge levels and related disparities regarding menopausal hormone therapy (MHT) among physicians in Sweden.

    Study design

    A 45-item web-based MHT-focused survey conducted February–September 2023. Participants were specialists/residents in obstetrics and gynecology (gynaecologists) and general practitioners (GPs) in Sweden.

    Main outcome measures

    Experience with MHT prescription, prescription patterns and challenges and perceived knowledge of and adherence to national guidelines among gynaecologists and GPs, analyzed quantitatively, along with potential differences between the two groups.ResultsIn total, 542 physicians answered the survey (67.9 % gynaecologists and 32.1 % GPs). Over 90 % reported meeting women with menopausal symptoms in their clinical practice and among those 94.6 % prescribed systemic MHT. GPs prescribed MHT to a significantly lesser extent than gynaecologists. GPs reported a significantly higher level of difficulty in all but one of the examined aspects of MHT prescription. GPs demonstrated significantly lower awareness of current national guidelines than gynaecologists. Regarding self-perceived assessment of MHT-related education, 47.8 % of GPs, compared with 30.6 % of gynaecologists, reported inadequate theoretical education (p < 0.001). Physicians working in metropolitan areas were more experienced in prescribing micronized progesterone and dydrogesterone.

    Conclusions

    Differences were observed between responding gynaecologists and GPs in MHT-related practices and knowledge. While GPs reported lower awareness of guidelines and encountered more challenges in prescribing MHT, nearly one-third of gynaecologists also indicated inadequate education in MHT. This study underscores the need for improved guideline awareness and accessible education to support evidence-based menopause care for the expanding midlife female population.

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  • Wockelberg, Helena
    et al.
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Government.
    Ahlbäck Öberg, Shirin
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Government.
    Governing a Dual Executive: Agents and Stewards in the Swedish Management Regime2025In: Scandinavian Journal of Public Administration, ISSN 2001-7405, E-ISSN 2001-7413Article in journal (Refereed)
    Abstract [en]

    This article analyses the tension between democratic and constitutional demands for controlover delegated mandates and contemporary trust-oriented management policies of theSwedish national executive. Competing management ideals are here analyzed in terms ofcontrol-oriented Principal-Agent (PA) models and trust-oriented Principal-Steward (PS)models. The case is studied from within three perspectives that constitute core dimensionsof the Swedish management regime: the constitutional preconditions for government-agency relations, the application of formal management instruments, and the role thatinformal instruments play in the management regime. We find that the Swedishmanagement regime is PA-oriented at its core – constitutionally and in terms of the choiceof management model for agencies – but featuring PS-oriented financial and policyautonomy for central government agencies. Informal steering is prohibited but the dominantinterpretation of the constitution is that it allows PS-oriented informal contacts that areequal, cooperative exchanges of information, including efforts to clarify formal steering.We question the validity of this conclusion as clarification of steering is too closely relatedto steering to be reliably something else. Thus, the role of informal contacts is formally andrhetorically reserved for PS-oriented use, that is, interaction on equal and cooperative terms,but in practice also entails PA-oriented top down control.

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  • Public defence: 2025-06-13 11:30 University Aula, Reykjavík (Iceland)
    Greiner, Sonja H. M.
    Uppsala University, Disciplinary Domain of Science and Technology, Earth Sciences, Department of Earth Sciences, Mineralogy Petrology and Tectonics. Nordic Volcanological Center, Institute of Earth Sciences, University of Iceland, Reykjavík, Iceland.
    The Influence of Pre-Existing Fractures and Tectonic Stress on Magmatic Dikes2025Doctoral thesis, comprehensive summary (Other academic)
    Abstract [en]

    Magmatic dikes form an integral part of volcanic systems and transport magma from depth towards the surface. Dike propagation through the Earth’s crust is affected by the mechanical properties of the crust, which is important to better understand potential effects on volcanic activity. This thesis investigates the influence of crustal heterogeneity on magmatic dikes, focusing specifically on the interaction between magma and pre-existing weaknesses and on the influence of tectonic stress. Basaltic dikes exposed in moderately fractured hyaloclastite in the extinct Dyrfjöll volcanic system, NE Iceland, showed that dikes can follow existing fractures, change strike when intersecting them without propagating into a fracture or be arrested in front of a fracture. Laboratory models of intrusions into pre-faulted crust demonstrate that the host rock cohesion and the strength contrast between intact and faulted host rock strongly control if and how faults affect intrusions. Faults additionally affect the amplitude and pattern of intrusion-associated surface deformation. Finite Element models simulated dike opening in a tectonic stress field. Comparison of these to surface deformation associated with the 2021 February-March Fagradalsfjall dike, SW Iceland, show that tectonic stress can be a sufficient driving mechanism for dike opening. The relative amount of predicted opening and shearing of the dike plane is consistent with expectations based on geological models and the area’s obliquely-spreading tectonic setting. This thesis demonstrates the complexity of dikes interacting with heterogeneous crust and the potential of considering multidisciplinary research as a key to advance understanding of such interactions. 

    List of papers
    1. Interaction between propagating basaltic dikes and pre-existing fractures: A case study in hyaloclastite from Dyrfjoll, Iceland
    Open this publication in new window or tab >>Interaction between propagating basaltic dikes and pre-existing fractures: A case study in hyaloclastite from Dyrfjoll, Iceland
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    2023 (English)In: Journal of Volcanology and Geothermal Research, ISSN 0377-0273, E-ISSN 1872-6097, Vol. 442, article id 107891Article in journal (Refereed) Published
    Abstract [en]

    Magma in the Earth's crust is commonly transported through dikes. Fractures and faults, which are common in the shallow crust, form structural weaknesses that can act as energy-efficient propagation pathways. Although examples of this are known from active and extinct volcanoes in varying host rocks, the conditions and mechanisms of how and when dikes are influenced by these structures are not yet fully understood. This study investigates how basaltic dikes propagating through hyaloclastite in the shallow crust interact with pre-existing fractures. Using virtual 3D-models from drone-based photogrammetry, we mapped basaltic dikes exposed in a caldera-filling hyaloclastite in the extinct Dyrfjoll volcano, NE-Iceland, to measure the orientations of fractures and dikes, and quantify their interactions. We observe 39 changes in strike among 45 dikes and found a strong control of the governing stress field on orientations and interactions. Three types of dike-fracture interaction were identified: (1) Dikes propagating along pre-existing fractures. This is most frequently observed for dikes following the tectonic stress field. (2) Dikes with an abrupt change in strike occurring near or at a crosscutting fracture, but without magma flow into the fracture. (3) Dikes arrested at a crosscutting fracture. Such dikes may develop offshoots near the dike tip, which may approach the fracture at different angles and be able to cut across. Understanding how dikes interact with pre-existing fractures in moderately fractured host rock such as hyalo-clastite is relevant for hazard assessment and monitoring of volcanically active areas.

    Place, publisher, year, edition, pages
    Elsevier, 2023
    Keywords
    Dike propagation, Dike-fracture interaction, Volcano-tectonic interaction, Hyaloclastite, Photogrammetry, Iceland
    National Category
    Geology Geophysics
    Identifiers
    urn:nbn:se:uu:diva-514910 (URN)10.1016/j.jvolgeores.2023.107891 (DOI)001076373000001 ()
    Available from: 2023-10-31 Created: 2023-10-31 Last updated: 2025-04-08Bibliographically approved
    2. The influence of variable host rock cohesion and magma viscosity on intrusion-fault interaction: Insights from laboratory models
    Open this publication in new window or tab >>The influence of variable host rock cohesion and magma viscosity on intrusion-fault interaction: Insights from laboratory models
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    2025 (English)In: Journal of Geophysical Research - Solid Earth, ISSN 2169-9313, E-ISSN 2169-9356, Vol. 130, no 4, article id e2024JB029870Article in journal (Refereed) Published
    Abstract [en]

    Magma transport through the Earth's shallow crust can be affected by pre-existing weaknesses like faults. Consequently, fault-channeled magma may reach the surface in unexpected locations. Hence, better understanding of magma-fault interaction is needed to improve hazard assesment. We investigate the effect of host rock cohesion and magma viscosity on intrusion-fault interaction using laboratory experiments. Vegetable oil and glucose syrup, serving as low- and high-viscosity analogue magmas, were injected into intact and faulted granular materials with variable cohesion (mixtures of silica flour and micro-glass beads), serving as a brittle plastic model crust. High-cohesion models produced sheet intrusions, that propagated along fault segments upon intersection. Low-cohesion models produced low-aspect ratio intrusions low width/thickness ratio. Without tectonic stresses, the cohesion strongly controls intrusion-fault interaction, while tested model magma viscosities exerted a weaker control. Our findings show that intrusion-fault interaction is a highly complex process and important to consider at active volcanoes.

    Place, publisher, year, edition, pages
    American Geophysical Union (AGU), 2025
    Keywords
    Analogue models, magma-fault interaction, cohesion, viscosity, intrusion, dike
    National Category
    Geophysics
    Identifiers
    urn:nbn:se:uu:diva-554095 (URN)10.1029/2024JB029870 (DOI)001474054400001 ()2-s2.0-105003818132 (Scopus ID)
    Funder
    Uppsala University
    Available from: 2025-04-07 Created: 2025-04-07 Last updated: 2025-05-09Bibliographically approved
    3. Tectonic stress as the driving mechanism for dike opening in an oblique rift setting: A deformation model of the 2021 Fagradalsfjall dike, Iceland
    Open this publication in new window or tab >>Tectonic stress as the driving mechanism for dike opening in an oblique rift setting: A deformation model of the 2021 Fagradalsfjall dike, Iceland
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    2025 (English)In: Geophysical Research Letters, ISSN 0094-8276, E-ISSN 1944-8007, Vol. 52, no 8, article id e2024GL113970Article in journal (Refereed) Published
    Abstract [en]

    Repeated dike-intrusions often occur in zones where extensional stress has accumulated. Still, geodetic modeling of observed dike-induced ground deformation often ignores the contribution of tectonic stress. On the obliquely spreading Reykjanes Peninsula, Iceland, tectonic strain build-up had been geodetically documented for three decades when a magmatic dike formed at Fagradalsfjall in 2021. We explore the contribution of tectonic stress on dike emplacement in a viscoelastic three-dimensional Finite-Element deformation model. Tectonic stress accumulation is initially simulated through plate motion, and later partially released by opening of a segmented rectangular dike. We find that surface deformation can be largely reproduced by releasing 60% of the accumulated tectonic stress. Partial stress release and low magma overpressure are consistent with successive dike intrusions and low-intensity eruptions in the area. Our model provides an approach to consistently model stress-release constrained by surface deformation.

    Place, publisher, year, edition, pages
    American Geophysical Union (AGU), 2025
    Keywords
    Volcano-tectonic interaction, ground deformation, stress, Reykjanes Peninsula, Finite Element Method, Dikes
    National Category
    Geophysics
    Identifiers
    urn:nbn:se:uu:diva-554098 (URN)10.1029/2024GL113970 (DOI)001475860000001 ()
    Available from: 2025-04-07 Created: 2025-04-07 Last updated: 2025-05-08Bibliographically approved
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  • Hofmann, Robin
    et al.
    Karolinska Inst, Sodersjukhuset, Dept Clin Sci & Educ, Div Cardiol, Sjukhusbacken 10, S-11883 Stockholm, Sweden..
    James, Stefan
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Cardiology. Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Disciplinary Domain of Medicine and Pharmacy, research centers etc., Uppsala Clinical Research Center (UCR).
    Sundqvist, Martin O.
    Karolinska Inst, Sodersjukhuset, Dept Clin Sci & Educ, Div Cardiol, Sjukhusbacken 10, S-11883 Stockholm, Sweden..
    Wärme, Jonatan
    Karolinska Inst, Sodersjukhuset, Dept Clin Sci & Educ, Div Cardiol, Sjukhusbacken 10, S-11883 Stockholm, Sweden..
    Fröbert, Ole
    Örebro Univ, Fac Hlth, Dept Cardiol, Örebro, Sweden.;Aarhus Univ, Fac Hlth, Dept Clin Med, Aarhus, Denmark..
    Angerås, Oskar
    Sahlgrens Univ Hosp, Inst Med, Dept Mol & Clin Med, Gothenburg, Sweden.;Sahlgrens Univ Hosp, Dept Cardiol, Gothenburg, Sweden..
    Hellström, Per M.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Gastroenterology/Hepatology.
    Hambraeus, Kristina
    Falun Cent Hosp, Dept Cardiol, Falun, Sweden..
    Alfredsson, Joakim
    Linköping Univ, Dept Hlth Med & Caring Sci, Linköping, Sweden.;Linköping Univ, Dept Cardiol, Linköping, Sweden..
    Erlinge, David
    Lund Univ, Dept Clin Sci, Cardiol, Lund, Sweden..
    Lauermann, Jörg
    Linköping Univ, Dept Hlth Med & Caring Sci, Linköping, Sweden.;Ryhov Hosp Jönköping, Dept Cardiol, Jönköping, Sweden..
    Lindhagen, Lars
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Disciplinary Domain of Medicine and Pharmacy, research centers etc., Uppsala Clinical Research Center (UCR).
    Östlund, Olof Petter
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Disciplinary Domain of Medicine and Pharmacy, research centers etc., Uppsala Clinical Research Center (UCR).
    Jernberg, Tomas
    Karolinska Inst, Danderyd Hosp, Dept Clin Sci, Stockholm, Sweden..
    Bäck, Magnus
    Karolinska Inst, Dept Med Solna, Stockholm, Sweden.;Karolinska Univ Hosp, Heart & Vasc Ctr, Dept Cardiol, Stockholm, Sweden..
    HELicobacter Pylori screening to prevent gastrointestinal bleeding in patients with acute Myocardial Infarction (HELP-MI SWEDEHEART): Design and rationale of a cluster randomized, crossover, registry-based clinical trial2025In: American Heart Journal, ISSN 0002-8703, E-ISSN 1097-6744, Vol. 286, p. 66-74Article in journal (Refereed)
    Abstract [en]

    Background

    The role of Helicobacter pylori ( H. pylori ) screening and eradication on reducing upper gastrointestinal bleeding (UGIB) complications after acute myocardial infarction (MI) is uncertain. The HELicobacter pylori screening to prevent gastrointestinal bleeding in patients with acute MI (HELP-MI SWEDEHEART) trial aims to determine whether systematic H. pylori screening compared to usual care reduces UGIB, mortality, and cardiovascular outcomes after MI.

    Methods

    A cluster randomized, crossover, registry-based clinical trial using SWEDEHEART as trial platform for study population definition and source for data collection in combination with nationwide Swedish health data registries. Thirty-five Swedish hospitals, organized into 18 clusters based on percutaneous coronary intervention networks, were randomized to either routine H. pylori screening for adults with acute type-1 MI or usual care. After 1 year, a 2-month blanking period was followed by a crossover to the alternate allocation for 1 year. The trial enrolment was concluded after one additional year of registry-based follow-up. The primary endpoint is UGIB. Secondary endpoints include all-cause death, cardiovascular death, readmission for MI, stroke, or heart failure. Endpoints will be reported combined (Net Adverse Clinical Events; Major Adverse Cardiac or Cerebrovascular Events) and separately. The primary analysis will include all available follow-up time corresponding to a maximum follow-up time of 3 years and 2 months.

    Conclusion

    HELP-MI SWEDEHEART aims to determine the utility of routine H. pylori screening to reduce UGIB and improve cardiovascular outcomes after MI. By integrating national registry follow-up data with a pragmatic trial design, it has the potential to provide evidence for the effect of the implementation of routine H. pylori screening as part of acute MI care.

    Trial Registration

    ClinicalTrials.gov, NCT05024864.

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  • Ström, Per
    Uppsala University, University Administration, Division for Communication and External Relations.
    Promotionsfesten i Uppsala den 23 maj 20252025Book (Other (popular science, discussion, etc.))
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  • Hultstrand, Cecilia
    et al.
    Brynskog, Ellen
    Karlsson Rosenblad, Andreas
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Statistics. Regional Cancer Centre Stockholm-Gotland, Stockholm, Sweden.
    Sunesson, Anna-Lena
    Björk-Eriksson, Thomas
    Sharp, Lena
    Low levels of awareness and motivation towards cancer prevention amongst the general public in Sweden: a cross-sectional study focusing on the European Code Against Cancer2025In: BMC Public Health, E-ISSN 1471-2458, Vol. 25, no 1, article id 1692Article in journal (Refereed)
    Abstract [en]

    Background

    The European Code Against Cancer (ECAC) aims to increase the awareness of modifiable cancer risk factors among the general public. A goal set by the European Commission was that 80% of European citizens should be aware of this code by 2025. This study aims to examine the awareness and attitudes towards the ECAC among the general public in Sweden.

    Methods

    A randomly selected sample of 1520 Swedes (18–84 years old) were recruited from a survey panel and invited to respond to an online study-specific questionnaire. The questionnaire included general questions regarding cancer prevention, as well as awareness and attitudes specific to the ECAC. Data were analysed univariately and with adjusted logistic regression, using post-stratification weights based on gender, age, education, and expressed political party orientation.

    Results

    In total, 3.7% of the respondents had heard about the ECAC before taking this survey. Respondents with a college/university education were more likely to have heard about the ECAC (odds ratio [OR] 2.23; 95% confidence interval [CI] 1.23–4.06). Males (OR 0.56; 95% CI 0.32–0.99), and those living alone (OR 0.47; 95% CI 0.23–0.95) were less likely to have heard about the ECAC. In total, 60.6% of the respondents agreed with the ECAC recommendations, while 27.4% reported that their motivation to improve their lifestyle increased after reading the ECAC.

    Conclusions

    Awareness of the ECAC among the general public in Sweden is very low. Still, a majority seem to agree with its recommendations. The results also indicate that the ECAC motivates some, but far from all, to improve their lifestyle habits to reduce their cancer risk. Consequently, further research is warranted on how the ECAC best could and should be used in order to improve cancer prevention awareness and motivation.

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  • Taliadoros, Demetris
    et al.
    Max Planck Inst Evolutionary Biol, Environm Genom, D-24306 Plon, Germany; Christian Albrechts Univ Kiel, Bot Inst, Environm Genom Grp, D-24118 Kiel, Germany.
    Potgieter, Lizel
    Max Planck Inst Evolutionary Biol, Environm Genom, D-24306 Plon, Germany.;Christian Albrechts Univ Kiel, Bot Inst, Environm Genom Grp, D-24118 Kiel, Germany.
    Dhiman, Amar
    Christian Albrechts Univ Kiel, Plant Breeding Inst, D-24118 Kiel, Germany.
    Wyatt, Nathan A.
    USDA ARS, Sugarbeet Res Unit, Edward T Schafer Agr Res Ctr, Fargo, ND USA..
    McMullan, Mark
    Earlham Inst, Norwich Res Pk, Norwich NR4 7UZ, England..
    Jung, Christian
    Christian Albrechts Univ Kiel, Plant Breeding Inst, D-24118 Kiel, Germany..
    Bolton, Melvin D.
    USDA ARS, Sugarbeet Res Unit, Edward T Schafer Agr Res Ctr, Fargo, ND USA..
    Stukenbrock, Eva H.
    Max Planck Inst Evolutionary Biol, Environm Genom, D-24306 Plon, Germany.;Christian Albrechts Univ Kiel, Bot Inst, Environm Genom Grp, D-24118 Kiel, Germany..
    Genome-wide Evidence of Host Specialization in Wild and Farmland Populations of the Fungal Leaf Spot Pathogen, Cercospora beticola2025In: Genome Biology and Evolution, E-ISSN 1759-6653, Vol. 17, no 4, article id evaf053Article in journal (Refereed)
    Abstract [en]

    One of the most recent crop species to be domesticated is sugar beet (Beta vulgaris L. ssp. vulgaris Doell.), which was bred for high sucrose content within the last few centuries in Europe. Crop domestication can also lead to the evolution of novel pathogens, which may spread across large geographical distances with their crop host. In this study, we addressed the recent evolution of the fungal pathogen causing the disease Cercospora leaf spot, Cercospora beticola. This pathogen has become increasingly important in sugar beet and table beet production worldwide. We used genome sequences of 326 C. beticola isolates collected from 4 continents from 4 closely related Beta subspecies (3 domesticated and 1 wild). We applied population genomic analyses to identify signatures of population differentiation and host specialization in C. beticola populations derived from the cultivated and wild hosts. We found evidence that C. beticola populations in agro-ecosystems likely originate from sea beet-infecting isolates. Intriguingly, host jumps from wild to cultivated beet occurred in at least 2 independent events as evidenced by our population data of C. beticola from wild beet collected in the Mediterranean and the UK. We explore the occurrence of genetic variants associated with fungicide resistance and virulence and show that standing genetic variation in C. beticola populations from both wild and domesticated plants may serve as a reservoir of functionally important alleles. Overall, our results highlight the ability of C. beticola to invade the agro-ecosystem and establish new populations, demonstrating the rapid adaptation potential of the species.

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  • Colliander Simonsson, Astrid
    Uppsala University, Disciplinary Domain of Science and Technology, Biology, Biology Education Centre.
    Identification and Diversity of Deep-sea Sponges (Porifera) from The Denmark Strait: A Taxonomic Study2025Independent thesis Basic level (degree of Bachelor), 10 credits / 15 HE creditsStudent thesis
    Abstract [en]

    Porifera is a highly diverse phylum that can be found all over our planet, being particularly important in the deep-sea. Deep-sea sponges serve a great purpose for the welfare of many other organisms, providing ecosystem services such as habitat, nutrient recycling, and food sources. They are also exposed to several anthropogenic disturbances such as trawling and climate change which increases the conservation interests regarding this group. Despite this, there is a huge knowledge gap regarding the diversity of deep-sea sponges, their abundance, as well as their distribution. One location where this is the case is in the Denmark Strait and around Iceland. The deep-sea in these regions has a unique oceanographic setting with cold Arctic waters and warm Atlantic saline waters, which allows for a great diversity of benthic communities. By examining the spicule content as well as sequencing the COI marker of specimens from the Icelandic AS11-2016 cruise, the diversity of boreo-arctic deep-sea sponges could be investigated. With the help of spicules, the classes Hexactinellida and Demospongiae were identified, as well as nine different demosponge orders. Demospongiae was the largest part of this collection, and the most abundant order was Tetractinellida. Amongst these nine orders, 52 different species were identified. With COI barcoding, a subset of specimens could be determined either to species level or identified further than with morphology. This study sheds light on the diversity of Porifera that exists in the deep-sea of the Denmark Strait and around Iceland. The diversity and rarity of some species that were found highlight the conservation value for this area, making this study particularly important regarding the distribution and diversity of deep-sea sponges.

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    Identification and Diversity of Deep-sea Sponges (Porifera) from The Denmark Strait
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    Biodiversiteten hos djuphavssvampdjur i Danmarksundet
  • Li, Zhiqiang
    et al.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Biochemistry and Microbiology, Biochemistry and Cancer. Guizhou Med Univ, Dept Immunol, Guiyang 631115, Peoples R China.
    Zhao, Wei
    Chengdu Normal Univ, Coll Chem & Life Sci, Chengdu 611130, Sichuan, Peoples R China.;Far Eastern Fed Univ, Dept Mol & Cell Biol, Russky Isl Vladivostok 690922, Russia..
    Deng, Xin
    Chengdu Normal Univ, Coll Chem & Life Sci, Chengdu 611130, Sichuan, Peoples R China..
    Yazlik, Murat Onur
    Ankara Univ, Fac Vet Med, Dept Obstet & Gynecol, TR-06070 Ankara, Turkiye..
    Özkan, Hüseyin
    Hatay Mustafa Kemal Univ, Fac Vet Med, Dept Genet, TR-31060 Hatay, Turkiye..
    Liu, Shiyi
    Chengdu Normal Univ, Coll Chem & Life Sci, Chengdu 611130, Sichuan, Peoples R China..
    Mei, Ling
    Chengdu Normal Univ, Coll Chem & Life Sci, Chengdu 611130, Sichuan, Peoples R China..
    Li, Shangfeng
    Zhi Pet Anim Hosp, Chengdu 611830, Sichuan, Peoples R China..
    Zhan, Jiasui
    Swedish Univ Agr Sci, Dept Forest Mycol & Plant Pathol, SE-75007 Uppsala, Sweden..
    Hu, Binhong
    Chengdu Normal Univ, Coll Chem & Life Sci, Chengdu 611130, Sichuan, Peoples R China.;Swedish Univ Agr Sci, Dept Forest Mycol & Plant Pathol, SE-75007 Uppsala, Sweden.;Zhi Pet Anim Hosp, Chengdu 611830, Sichuan, Peoples R China..
    FOXP3+T cells and immune dysregulation in canine pyometra2025In: Theriogenology, ISSN 0093-691X, E-ISSN 1879-3231, Vol. 242, article id 117445Article in journal (Refereed)
    Abstract [en]

    Canine pyometra is a suppurative uterine infection associated with immune dysregulation. This study investigated the role of regulatory T cells (Tregs) and associated factors in the pus accumulation within the canine uterus. Sixteen client-owned intact bitches, eight diagnosed with pyometra and the other eight healthy animals undergoing elective ovariohysterectomy, were enrolled. Blood samples were collected into ethylenediaminetetraacetic acid (EDTA)-coated tubes for flow cytometry. Tissue samples were obtained after ovariohysterectomy and used to examine localization of interleukin (IL)-2 and IL-2Rα as key regulators of Treg functions. Gene expression was analyzed by reverse transcription quantitative polymerase chain reaction (RT-qPCR). Results of flow cytometry analysis revealed a significant increase in the population of Tregs in the uterine tissue and their corresponding decrease in the peripheral blood. This shift is likely reflective of the recruitment of Tregs from the peripheral blood to the decidua in pyometra. There was a marked upregulation in the expression of IL-2 in the uterine tissue. There was dysregulation in the expression of anti-inflammatory cytokines produced by Tregs (such as IL-10) and pro-inflammatory factors secreted by effector T cells (such as RORγt and IL-17A), which gave a deeper insight into the mechanism underlying the immune dysfunction in canine pyometra. Taken together, these observations elucidate the dynamic changes in Tregs and related factors during canine uterine pyometra, thus providing a new perspective on the equilibrium of the uterine immune microenvironment.

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  • Thaichana, Pak
    et al.
    Chiang Mai Univ, Off Res Adm, Chiang Mai 50200, Thailand.;Chiang Mai Univ, Res Inst Hlth Sci, Environm Occupat Hlth Sci & Noncommunicable Dis Re, Chiang Mai 50200, Thailand..
    Sripan, Patumrat
    Chiang Mai Univ, Res Inst Hlth Sci, Res Ctr Infect Dis & Subst Use, Chiang Mai 50200, Thailand..
    Rerkasem, Amaraporn
    Chiang Mai Univ, Res Inst Hlth Sci, Environm Occupat Hlth Sci & Noncommunicable Dis Re, Chiang Mai 50200, Thailand.;Chiang Mai Univ, Res Inst Hlth Sci, Res Ctr Infect Dis & Subst Use, Chiang Mai 50200, Thailand..
    Tongsong, Theera
    Chiang Mai Univ, Fac Med, Dept Obstet & Gynecol, Chiang Mai 50200, Thailand..
    Sangsawang, Suraphan
    Reg Hlth Promot Center1 Hosp, Chiang Mai 50100, Thailand..
    Kawichai, Sawaeng
    Chiang Mai Univ, Res Inst Hlth Sci, Environm Occupat Hlth Sci & Noncommunicable Dis Re, Chiang Mai 50200, Thailand..
    Srisukkham, Worawut
    Chiang Mai Univ, Fac Sci, Dept Comp Sci, Chiang Mai 50200, Thailand..
    Wanapirak, Chanane
    Chiang Mai Univ, Fac Med, Dept Obstet & Gynecol, Chiang Mai 50200, Thailand..
    Sirilert, Sirinart
    Chiang Mai Univ, Fac Med, Dept Obstet & Gynecol, Chiang Mai 50200, Thailand..
    Mattawanon, Natnita
    Chiang Mai Univ, Fac Med, Dept Obstet & Gynecol, Chiang Mai 50200, Thailand..
    Phanpong, Chotiros
    Reg Hlth Promot Center1 Hosp, Chiang Mai 50100, Thailand..
    Ongprasert, Krongporn
    Chiang Mai Univ, Fac Med, Dept Community Med, Chiang Mai 50200, Thailand..
    Derraik, José G. B.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Women's and Children's Health, Perinatal, Neonatal and Pediatric Cardiology Research. Chiang Mai Univ, Res Inst Hlth Sci, Environm Occupat Hlth Sci & Noncommunicable Dis Re, Chiang Mai 50200, Thailand; Univ Auckland, Fac Med & Hlth Sci, Dept Paediat Child & Youth Hlth, Auckland 1010, New Zealand.
    Rerkasem, Kittipan
    Chiang Mai Univ, Res Inst Hlth Sci, Environm Occupat Hlth Sci & Noncommunicable Dis Re, Chiang Mai 50200, Thailand.;Chiang Mai Univ, Fac Med, Clin Surg Res Ctr, Dept Surg, Chiang Mai 50200, Thailand..
    Association of Maternal PM2.5 Exposure with Preterm Birth and Low Birth Weight: A Large-Scale Cohort Study in Northern Thailand (2016-2022)2025In: Toxics, E-ISSN 2305-6304, Vol. 13, no 4, article id 304Article in journal (Refereed)
    Abstract [en]

    Air pollution exposure has been increasingly linked to adverse pregnancy outcomes. This study aimed to investigate the effects of PM2.5 exposure throughout pregnancy on preterm birth, low birth weight (LBW), and small for gestational age (SGA). We analyzed a cohort of 16,965 pregnant women living in northern Thailand between 2016 and 2022. PM2.5 concentration data were collected from two air quality monitoring stations operated by the Pollution Control Department (PCD) of Thailand. Logistic regression models were used to assess the association between daily PM2.5 exposure and pregnancy outcomes. PM2.5 exposure at levels exceeding 37.5 μg/m3 throughout pregnancy significantly increased the risk of preterm birth (aOR = 2.19, p < 0.001) and LBW (aOR = 1.99, p < 0.001) compared to the reference group (15.1–37.5 μg/m3). However, exposure at levels ≤15.0 μg/m3 also increased the risk for both outcomes compared to the same reference group. Subgroup analysis of high-risk pregnant women, including women aged > 35 years, with pre-pregnancy BMI (<18.5), pregnancy-induced hypertension, and nulliparous women, showed that the range of the critical PM2.5 exposure threshold was 32.3–38.4 μg/m3 for preterm birth and 31.2–38.2 μg/m3 for LBW. This study highlights the significant association between PM2.5 exposure and adverse pregnancy outcomes and suggests the need for targeted interventions to mitigate its effects on maternal and child health.

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  • Morejón-Arrojo, Ramón D.
    et al.
    Inst Marine Sci, Loma St,14 Between 35 & 37,Plaza Revoluc, Havana 10400, Cuba..
    Lüskow, Florian
    Uppsala University, Disciplinary Domain of Science and Technology, Earth Sciences, Department of Earth Sciences, Natural Resources and Sustainable Development.
    Fernández-Alías, Alfredo
    Univ Murcia, Dept Ecol & Hydrol, Murcia 30100, Spain.;Univ Murcia, Reg Campus Int Excellence Mare Nostrum, Murcia 30100, Spain.;Univ Lille, Univ Littoral Cote Dopale, Stn Marine Wimereux, Lab Oceanol & Geosci,CNRS,IRD,UMR 8187, F-59000 Lille, France..
    Ramírez, Humberto
    Orinozo Ave,Qta Mary, Caracas 1050, Venezuela..
    Cróquer, Aldo
    Nature Conservancy, Cent Caribbean Program, Punta Cana 23000, Dominican Rep..
    First Record of a Cannonball Jellyfish Bloom (Stomolophus sp.) in Venezuelan Waters2025In: Journal of Marine Science and Engineering, E-ISSN 2077-1312, Vol. 13, no 4, article id 689Article in journal (Refereed)
    Abstract [en]

    Jellyfish blooms are dynamic events driven by environmental and anthropogenic factors. This study reports the first documented bloom of the cannonball jellyfish (Stomolophus sp.) in Venezuelan waters, observed between March and April 2024 along approximately 120 km of coastline. Reports from anglers and divers confirmed high jellyfish abundances (~3 ind. m−3) across multiple sites. Environmental analyses suggest that fluctuations in sea surface temperature, increased chlorophyll a concentrations, and high precipitation in the preceding months may have triggered strobilation and subsequent bloom formation. However, the polyps have not yet been observed in the field, and advective movement from other locations cannot be ruled out. Given the commercial importance of Stomolophus spp. in neighboring regions, this record underscores the need for continued monitoring to assess potential range expansions and their ecological and socio-economic impacts. Additionally, the emergence of this bloom raises questions about the species’ distribution patterns, potential establishment in Venezuelan waters, and possible implications for local fisheries. Our findings contribute to the broader understanding of gelatinous zooplankton dynamics in the Caribbean Sea and provide baseline information for future ecological assessments and fisheries management strategies. Further studies, including genetic analyses, are needed to confirm species identity and investigate the drivers behind this unprecedented bloom.

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  • Holmes, James D.
    et al.
    Uppsala University, Disciplinary Domain of Science and Technology, Earth Sciences, Department of Earth Sciences, Palaeobiology. Univ New England, Palaeoscience Res Ctr, Sch Environm & Rural Sci, Armidale, NSW 2351, Australia.
    Smith, Patrick M.
    Australian Museum Res Inst, Palaeontol Dept, Sydney, NSW 2010, Australia.;Macquarie Univ, Sch Nat Sci, Sydney, NSW 2109, Australia..
    Paterson, John R.
    Univ New England, Palaeoscience Res Ctr, Sch Environm & Rural Sci, Armidale, NSW 2351, Australia..
    Brock, Glenn A.
    Macquarie Univ, Sch Nat Sci, Sydney, NSW 2109, Australia..
    Betts, Marissa J.
    Univ New England, Palaeoscience Res Ctr, Sch Environm & Rural Sci, Armidale, NSW 2351, Australia..
    The Cambrian Series 2-Miaolingian boundary interval in Australia: biostratigraphic subdivision and implications for global multi-proxy correlation2025In: Earth-Science Reviews, ISSN 0012-8252, E-ISSN 1872-6828, Vol. 265, article id 105106Article in journal (Refereed)
    Abstract [en]

    The Cambrian Series 2–Miaolingian boundary interval in Australia—equivalent to the local Ordian and Templetonian stages—has long been a source of controversy, with a practical and consistent subdivision of this interval proving elusive. Recent ratification of the Miaolingian Series and Wuliuan Stage Global Boundary Stratotype Section and Point (GSSP) in South China, based primarily on the first appearance of the trilobite Oryctocephalus indicus and the coincident Redlichiine–Olenelline Extinction Carbon isotope Excursion (ROECE), highlights the importance of resolving this interval in Australia. In this contribution, we present an updated synthesis of Cambrian Series 2, upper Stage 4–Miaolingian, Wuliuan (Ordian–Templetonian) intervals across Australia, focusing on the reported ranges of small shelly fossils (SSF) and δ13C/δ18O isotope chemostratigraphy, in addition to trilobite and agnostid arthropod occurrences. Results show an underappreciated sequential series of taxon lowest occurrences across this interval. Based on these, we define two new organophosphatic brachiopod biozones: an upper Stage 4 (Ordian) Schizopholis napuru Zone, and an uppermost Stage 4–Wuliuan (upper Ordian–Templetonian) Micromitra nerranubawu Zone. Taxon ranges across these zones are consistent with the Cambrian Series 2–Miaolingian boundary at the Miaolingian/Wuliuan GSSP, allowing direct correlation with South China. Preliminary work in the Australian Stansbury and Georgina basins has revealed the promise of high-resolution SSF biostratigraphy coupled with δ13C/δ18O chemostratigraphy in addressing the ongoing issues associated with this interval. It is clear that such multi-proxy studies can assist in locating boundaries and correlating intervals across different Cambrian terranes with a high degree of precision, even when lacking index fossils such as O. indicus. Future work should focus on a systematic program of such studies within this interval, which will greatly assist in resolving correlations both within Australia and globally.

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  • Tolentino, Victor
    et al.
    Uppsala University, Disciplinary Domain of Science and Technology, Earth Sciences, Department of Earth Sciences.
    Lucero, Andres Ortega
    Univ Queensland, Sustainable Minerals Inst, WH Bryan Min & Geol Res Ctr, St Lucia, Qld 4072, Australia.;Univ Exeter, Camborne Sch Mines, Dept Earth & Environm Sci, Penryn TR10 9EZ, England..
    Koerting, Friederike
    HySpex Norsk Elekt Optikk, N-0667 Oslo, Norway..
    Savinova, Ekaterina
    Univ Queensland, Sustainable Minerals Inst, WH Bryan Min & Geol Res Ctr, St Lucia, Qld 4072, Australia..
    Hildebrand, Justus Constantin
    HySpex Norsk Elekt Optikk, N-0667 Oslo, Norway..
    Micklethwaite, Steven
    Univ Queensland, Sustainable Minerals Inst, WH Bryan Min & Geol Res Ctr, St Lucia, Qld 4072, Australia..
    Drone-Based VNIR-SWIR Hyperspectral Imaging for Environmental Monitoring of a Uranium Legacy Mine Site2025In: Drones, ISSN 2504-446X, Vol. 9, no 4, article id 313Article in journal (Refereed)
    Abstract [en]

    Growing awareness of the environmental cost of mining operations has led to increased research on monitoring and restoring legacy mine sites. Hyperspectral imaging (HSI) has emerged as a valuable tool in the mining life cycle, including post-mining environment. By detecting variations in crystal structure and physicochemical attributes on the surface of materials, HSI provides insights into site environmental and ecological conditions. Here, we explore the capabilities of drone-based HSI for mapping surface patterns related to contamination dispersal in a legacy uranium-rare earth element mine site. Hyperspectral data across the visible to near-infrared (VNIR) and short-wave infrared (SWIR) wavelength ranges (400-2500 nm) were collected over selected areas of the former Mary Kathleen mine site in Queensland, Australia. Analyses were performed using data-driven (Spectral Angle Mapper-SAM) and knowledge-based (Band Ratios-BRs) spectral processing techniques. SAM identifies contamination patterns and differentiates mineral compositions within visually similar areas. However, its accuracy is limited when mapping specific minerals, as most endmembers represent mineral groups or mixtures. BR highlights reactive surfaces and clay mixtures, reinforcing key patterns identified by SAM. The results indicate that drone-based HSI can capture and distinguish complex surface trends, demonstrating the technology's potential to enhance the assessment and monitoring of environmental conditions at a mine site.

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  • Ozer, Simon
    et al.
    Aarhus Univ, Dept Psychol & Behav Sci, Aarhus, Denmark..
    Obaidi, Milan
    Univ Copenhagen, Dept Psychol, Copenhagen, Denmark..
    Bergh, Robin
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Psychology.
    The impact of globalized conflicts: Examining attitudes toward Jews among Britons in the political context of the war in Gaza2025In: International Journal of Intercultural Relations, ISSN 0147-1767, E-ISSN 1873-7552, Vol. 107, article id 102184Article in journal (Refereed)
    Abstract [en]

    Reports have indicated an increase in anti-Jewish hostility and antisemitic incidents following the Hamas terrorist attack in Israel on October 7, 2023, and the subsequent war in Gaza. In two studies (NStudy1 = 354 and NStudy2 = 490), we experimentally investigated the impact of priming with material referring to the war in Gaza on hostility toward Jews, and on antisemitism as well as other various ethnic groups (to determine whether this exposure specifically affected attitudes toward Jews or had a broader impact on ethnic attitudes in general). We also examined the indirect relationship between political orientation and anti-Jewish hostility and antisemitism, through sociopolitical factors such as global identification, out-group identity fusion, social dominance orientation, and misanthropy. Our results showed an experimental effect of increased negative attitudes toward Jews, as well as toward Britons and Scandinavians, but did not reveal an increase in antisemitism. This effect was not replicated in Study 2, possibly due to reduced media attention. The indirect effects suggested that political orientation (left vs. right-wing) was positively associated with anti-Jewish hostility and antisemitism through social dominance orientation. In contrast, conservative political orientation was negatively associated with antisemitism through out-group identity fusion with the Palestinian people. Our findings imply two distinct political pathways to antisemitism: one linked with classical political right-wing orientation and the other to a complex identity-based conflation of attitudes toward Israel with prejudice toward the Jewish ethnic group.

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  • Larsson, Anna Lindhoff
    et al.
    Linköping Univ, Dept Surg Linköping, Linköping, Sweden.;Linköping Univ, Dept Biomed & Clin Sci, Linköping, Sweden..
    Holka, Peter
    Lund Univ, Dept Surg, Clin Sci Lund, Lund, Sweden.;Skane Univ Hosp, Lund, Sweden..
    Isaksson, Bengt
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Surgical Sciences, Upper Abdominal Surgery. Department of Surgery. Akademiska Hospital, Uppsala, Sweden.
    Hemmingsson, Oskar
    Umeå Univ, Dept Surg & Perioperat Sci, Surg, Umeå, Sweden..
    Sandström, Per
    Linköping Univ, Dept Surg Linköping, Linköping, Sweden.;Linköping Univ, Dept Biomed & Clin Sci, Linköping, Sweden..
    Bjornsson, Bergthor
    Linköping Univ, Dept Surg Linköping, Linköping, Sweden.;Linköping Univ, Dept Biomed & Clin Sci, Linköping, Sweden..
    Translation and validation of the Swedish version of the EORTC LMC-21, the disease-specific questionnaire for assessing health-related quality of life in patients with colorectal liver metastases2025In: BMC Gastroenterology, E-ISSN 1471-230X, Vol. 25, no 1, article id 281Article in journal (Refereed)
    Abstract [en]

    Purpose

    The aim of this study was to translate the health-related quality-of-life questionnaire EORTC QLQ-LMC21 into Swedish and to test its clinical and psychometric reliability and validity in patients with liver metastases from colorectal cancer (CRC) undergoing surgical treatment.

    Methods

    The Swedish versions of the EORTC QLQ-C30 and EORTC QLQ-LMC21 were administered to 250 patients with liver metastases from CRC in four Swedish hospitals before and 3 months after surgical treatment. Psychometric validation of the questionnaire´s structure, reliability, and convergent and divergent validity was performed.

    Results

    Data from 242 (97%) patients were suitable for analysis. The QLQ-LMC21 was found to be sensitive to changes over time. Cronbach´s alpha coefficient indicated good internal consistency, ranging from 0.84 to 0.89. Test–retest reliability was evaluated in 120 patients (49%), and the intraclass correlation coefficient (ICC) indicated good reproducibility, ranging from 0.67 to 0.93. Convergent and discriminant validity were demonstrated adequately in the multitrait scaling analysis. There were weak correlations between the QLQ-C30 and QLQ-LMC21, which confirms that the health problems addressed by the QLQ-LMC21 are different from those addressed by the QLQ-C30.

    Conclusions

    The Swedish version of the EORTC QLQ-LMC21 proved to be a valid and reliable questionnaire to use in conjunction with the EORTC QLQ-C30.

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  • Public defence: 2025-06-02 10:15 Lecture Hall 2, Uppsala
    Namgay, Phub
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Informatics and Media.
    Complex Dynamics of Data Ecosystems: An Inquiry into the Recurrent Patterns of Action to Manage and Analyse Data2025Doctoral thesis, comprehensive summary (Other academic)
    Abstract [en]

    The rapid datafication of society has impacted every aspect of our daily lives. However, the literature and discussions thus far on data are largely techno-centric. The agency and effect of individuals in data ecosystems are either reduced to a mere facilitative role or backgrounded in the data discourses. In this dissertation, data-related activities such as those found in data management and analytics processes were problematised as digital phenomena that await critical examination through the lens of Routine Dynamics theory.

    Four studies are presented in this dissertation that investigate how people and technologies enact intricate routines for interoperating data in digital infrastructures;  how organisations manage the interplay of humans and technologies for structuring systems and data to implement the single source of truth concept; and how knowledge management models can unpack the intersection of in-house data analytics systems and cloud services in small- and medium-sized organisations to transform raw data into actionable knowledge. The insights from applying Routine Dynamics theory in those first three studies culminated in developing a conceptual model of routines.

    The theory-informed problematisation of various data-driven activities in an empirical setting less represented in the scientific literature, such as in the nascent data ecosystem of Bhutan, advances the relevant body of knowledge with fresh perspectives on data management and analytics processes. Similarly, the rich account of data that factors in the role of humans will allow individuals and organisations to reframe narratives on data and enrich their data management and analytics practices in complex data ecosystems.

    List of papers
    1. Though we be but small: How Data Interoperability and Dynamic Routines Enabled a Data-Centric Response to COVID-19 in Bhutan
    Open this publication in new window or tab >>Though we be but small: How Data Interoperability and Dynamic Routines Enabled a Data-Centric Response to COVID-19 in Bhutan
    (English)Manuscript (preprint) (Other academic)
    Keywords
    Data Interoperability, Organisational Routines, Health Information Systems, COVID-19, ICT4D, Bhutan
    National Category
    Information Systems
    Research subject
    Information Systems; Information Systems
    Identifiers
    urn:nbn:se:uu:diva-554115 (URN)
    Available from: 2025-04-08 Created: 2025-04-08 Last updated: 2025-04-17
    2. Intricacies of Processes to Implement the Single Source of Truth Concept in a Data Ecosystem
    Open this publication in new window or tab >>Intricacies of Processes to Implement the Single Source of Truth Concept in a Data Ecosystem
    (English)Manuscript (preprint) (Other academic)
    Keywords
    Single Source of Truth, Data Ecosystem, Routine Dynamics, Bhutan
    National Category
    Information Systems
    Research subject
    Information Systems; Information Systems
    Identifiers
    urn:nbn:se:uu:diva-554116 (URN)
    Available from: 2025-04-08 Created: 2025-04-08 Last updated: 2025-04-17
    3. Knowledge Management in the Data Analytics System of Organisations in Bhutan
    Open this publication in new window or tab >>Knowledge Management in the Data Analytics System of Organisations in Bhutan
    2025 (English)In: Proceedings of the 58th Hawaii International Conference on System Sciences (HICSS) / [ed] Tung X. Bui, Hawaii, USA: University of Hawaii at Manoa , 2025, p. 5172-5181Conference paper, Published paper (Refereed)
    Abstract [en]

    A study through the lens of Routine Dynamics theory was conducted among small- and medium-sized firms in Bhutan to examine knowledge management in their data analytics system. In such an economic setting, firms perform data analytics using in-house systems together with cloud computing to transform data into knowledge, mainly for predictive insights and competitive advantage. They use just-in-time (JIT) data analytics for knowledge on demand as a pragmatic approach, thus minimising uneconomical analytics. Firms also employ an in-house platform as a service system to monetise analytical outputs and knowledge. Since the primary focus of data analytics among firms is to support administrative functions, enhance business processes, and improve profit margins, systematic construction and use of tacit and explicit knowledge have received little attention. Hence, it is high time organisations augment their data analytics systems with practical knowledge management models for creating, managing, and using knowledge in a competitive digital environment.

    Place, publisher, year, edition, pages
    Hawaii, USA: University of Hawaii at Manoa, 2025
    Keywords
    Knowledge Management, Data Analytics, Cloud Computing, Routine Dynamics Theory, Bhutan
    National Category
    Information Systems
    Research subject
    Information Systems
    Identifiers
    urn:nbn:se:uu:diva-540458 (URN)978-0-9981331-8-8 (ISBN)
    Conference
    58th Hawaii International Conference on System Sciences, January 7-10, 2025
    Available from: 2025-01-01 Created: 2025-01-01 Last updated: 2025-04-08Bibliographically approved
    4. Towards Modelling and Simulation of Organisational Routines
    Open this publication in new window or tab >>Towards Modelling and Simulation of Organisational Routines
    2024 (English)In: Computational Science – ICCS 2024: 24th International Conference, Malaga, Spain, July 2–4, 2024, Proceedings, Part VII / [ed] Leonardo Franco; Clélia de Mulatier; Maciej Paszynski; Valeria V. Krzhizhanovskaya; Jack J. Dongarra; Peter M. A. Sloot, Cham: Springer, 2024, Vol. 14838, p. 367-379Conference paper, Published paper (Refereed)
    Abstract [en]

    Organisational routines are repetitive, recognisable patterns of interdependent action by human and digital actors to accomplish tasks. Routine Dynamics is a theoretical base that informs discussion and analysis of such routines. We note that there is a knowledge gap in the literature on organisational routines to consolidate the constructs and ontologies of routines into an abstract data model. In this paper, we design and implement a data model of routines using the Unified Modelling Language. We present a demonstration to illustrate our data model’s use, and how one can then use instantiations of the model to analyse and simulate organisational routines based on real-world data. This example examines recurrent patterns of action inferred from data in the GitHub issue tracking system about the open-source software project, scikit-learn. Our study extends the theoretical/empirical understanding and knowledge base of Routine Dynamics by laying the groundwork towards examining organisational routines from a model-driven perspective that gives rise to simulating the dynamics of routines. 

    Place, publisher, year, edition, pages
    Cham: Springer, 2024
    Series
    Lecture Notes in Computer Science, ISSN 0302-9743, E-ISSN 1611-3349 ; 14838
    National Category
    Computer and Information Sciences
    Research subject
    Information Systems; Computer Science
    Identifiers
    urn:nbn:se:uu:diva-527686 (URN)10.1007/978-3-031-63783-4_27 (DOI)001279329400027 ()9783031637858 (ISBN)9783031637834 (ISBN)
    Conference
    24th International Conference on Computational Science, Málaga, Spain, July 2-4, 2024
    Available from: 2024-05-08 Created: 2024-05-08 Last updated: 2025-04-08Bibliographically approved
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  • Belanger, Janelle M.
    et al.
    Univ Calif Davis, Dept Anim Sci, Davis, CA 95616 USA..
    Gershony, Liza C.
    Univ Calif Davis, Dept Anim Sci, Davis, CA 95616 USA..
    Bell, Jerold S.
    Tufts Cummings Sch Vet Med, Dept Clin Sci, North Grafton, MA 01536 USA..
    Hytönen, Marjo K.
    Univ Helsinki, Fac Med, Dept Med & Clin Genet, Helsinki 00014, Finland.;Univ Helsinki, Fac Vet Med, Dept Vet Biosci, Helsinki 00014, Finland.;Folkhalsan Res Ctr, Helsinki 00290, Finland..
    Lohi, Hannes
    Univ Helsinki, Fac Med, Dept Med & Clin Genet, Helsinki 00014, Finland.;Univ Helsinki, Fac Vet Med, Dept Vet Biosci, Helsinki 00014, Finland.;Folkhalsan Res Ctr, Helsinki 00290, Finland..
    Lindblad-Toh, Kerstin
    Uppsala University, Science for Life Laboratory, SciLifeLab. Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Biochemistry and Microbiology, Genetics and Genomics. Broad Inst MIT & Harvard, Cambridge, MA 02142 USA..
    Tengvall, Katarina
    Uppsala University, Science for Life Laboratory, SciLifeLab. Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Biochemistry and Microbiology, Genetics and Genomics.
    Sell, Elsa
    Bearded Collie Fdn Hlth BeaCon, Milner, GA 30257 USA..
    Famula, Thomas R.
    Univ Calif Davis, Dept Anim Sci, Davis, CA 95616 USA..
    Oberbauer, Anita M.
    Univ Calif Davis, Dept Anim Sci, Davis, CA 95616 USA..
    Measures of Homozygosity and Relationship to Genetic Diversity in the Bearded Collie Breed2025In: Genes, E-ISSN 2073-4425, Vol. 16, no 4, article id 378Article in journal (Refereed)
    Abstract [en]

    Background:

    Genetic diversity in closed populations, such as pedigree dogs, is of concern for maintaining the health and vitality of the population in the face of evolving challenges. Measures of genetic diversity rely upon estimates of homozygosity without consideration of whether the homozygosity is desirable or undesirable or if heterozygosity has a functional impact. Pedigree coefficients of inbreeding have been the classical approach yet they are inadequate unless based upon the entire population.

    Methods:

    Homozygosity measures based upon pedigree analyses (n = 11,898), SNP array data (n = 244), and whole genome sequencing (n = 23) were compared in the Bearded Collie, as well as a comparison of SNP array data to a pedigree cohort (n = 5042) and a mixed-breed cohort (n = 1171).

    Results:

    Molecular measures based upon DNA are more informative on an individual's homozygosity levels than pedigree analyses, although SNP coefficients of inbreeding overestimate the level of inbreeding based on the nature of SNP array methodology. Whole genome sequence (WGS) analyses revealed that the heterozygosity observed is generally in variants having neutral or low impact, which would indicate that the variability may not contribute substantially to functional diversity in the population. The majority of high-impact variants were observed in the shortest runs of homozygosity (ROH) reflecting ancestral breeding and domestication practices. As expected, mixed-breed dogs displayed higher measures of genomic diversity than either Bearded Collies or other pedigree dogs as a whole using the current paradigm algorithm models to calculate homozygosity.

    Conclusions:

    Using typical DNA-based measures reflect only a single individual and not the population thereby failing to account for regions of homozygosity that reflect ancestral breeding, domestication history, breed-defining regions, or regions positively selected for health traits. Incorporating measures of genetic diversity into dog breeding schemes is meritorious. However, until measures of diversity can distinguish between breed-defining homozygosity and homozygosity associated with positive health alleles, the measures to use as selection tools need refinement before their widespread implementation.

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  • Arage, Getachew
    et al.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology.
    Dekkers, Koen F.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology.
    Raso, Luka Marko
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology.
    Hammar, Ulf
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology.
    Ericson, Ulrika
    Lund Univ, Dept Clin Sci Malmö, Malmö, Sweden..
    Larsson, Susanna C.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Surgical Sciences, Medical epidemiology. Karolinska Inst, Inst Environm Med, Unit Cardiovasc & Nutr Epidemiol, Stockholm, Sweden..
    Engel, Hanna
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology.
    Baldanzi, Gabriel
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology.
    Pertiwi, Kamalita
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology.
    Sayols-Baixeras, Sergi
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology. Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Surgical Sciences, Medical epidemiology. Inst Salud Carlos III, CIBER Cardiovasc Dis CIBERCV, Madrid, Spain..
    Landberg, Rikard
    Chalmers Univ Technol, Dept Life Sci, Gothenburg, Sweden..
    Sundström, Johan
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Clinical Epidemiology. Univ New South Wales, George Inst Global Hlth, Sydney, Australia..
    Smith, J. Gustav
    Gothenburg Univ, Inst Med, Dept Mol & Clin Med, Wallenberg Lab, Gothenburg, Sweden.;Sahlgrens Univ Hosp, Dept Cardiol, Gothenburg, Sweden.;Lund Univ, Dept Cardiol Clin Sci, Lund, Sweden.;Skane Univ Hosp, Lund, Sweden.;Lund Univ, Wallenberg Ctr Mol Med, Lund, Sweden.;Lund Univ, Lund Univ Diabet Ctr, Lund, Sweden..
    Engström, Gunnar
    Ärnlöv, Johan
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Disciplinary Domain of Medicine and Pharmacy, research centers etc., Center for Clinical Research Dalarna. Karolinska Inst, Dept Neurobiol Care Sci & Soc, Div Family Med & Primary Care, Huddinge, Sweden.;Dalarna Univ, Sch Hlth & Social Studies, Falun, Sweden..
    Orho-Melander, Marju
    Lund Univ, Dept Clin Sci Malmö, Malmö, Sweden..
    Lind, Lars
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Clinical Epidemiology.
    Fall, Tove
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology.
    Ahmad, Shafqat
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Molecular epidemiology. Harvard Med Sch, Brigham & Womens Hosp, Prevent Med Div, Boston, MA USA..
    Plasma metabolite profiles of meat intake and their association with cardiovascular disease risk: A population-based study in Swedish cohorts2025In: Metabolism: Clinical and Experimental, ISSN 0026-0495, E-ISSN 1532-8600, Vol. 168, article id 156188Article in journal (Refereed)
    Abstract [en]

    Background

    Higher meat intake has been associated with adverse health outcomes, including cardiovascular disease (CVD). This study investigated plasma metabolites associated with meat intake and their relation with cardiometabolic biomarkers, subclinical CVD markers, and incident CVD.

    Methods

    Associations between self-reported meat intake and 1272 plasma metabolites were investigated in the SCAPIS cohort (n = 8,819; ages 50–64). Meat-associated metabolites were further examined for relation with subclinical CVD markers in the POEM cohort (n = 502; age 50) and incident CVD in the EpiHealth cohort (n = 2,278; ages 45–75; 107 incident cases over 9.6 years follow-up). Meat intake was categorized into white, unprocessed red, and processed red meat. Linear regression analyzed associations between meat intake, metabolites and cardiometabolic biomarkers, and subclinical CVD markers, while Cox models evaluated association between meat-associated metabolites and incident CVD.

    Results

    After correction for multiple testing, 458, 368, and 403 metabolites were associated with white, unprocessed red, and processed red meat, respectively. Processed red meat-associated metabolites were associated with higher levels of fasting insulin, hemoglobin A1c, and lipoprotein(a), and were inversely associated with maximal oxygen consumption. Two metabolites, 1-palmitoyl-2-linoleoyl-GPE (16:0/18:2) (hazard ratios (HR: 1.32; 95 % CI: 1.08, 1.62)) and glutamine degradant (HR: 1.35; 95 % CI: 1.07, 1.72), that were inversely associated with intake of all meat types, were also associated with a higher risk of incident CVD.

    Conclusions

    This study provides comprehensive analysis of self-reported meat intake and plasma metabolites. The findings may enhance our understanding of the relationship between meat intake and CVD, and provide insights into underlying mechanisms.

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  • Public defence: 2025-06-12 10:00 Hambergsalen, Uppsala
    Lin, Ting
    Uppsala University, Disciplinary Domain of Science and Technology, Earth Sciences, Department of Earth Sciences, LUVAL.
    Understanding the interactions between polar lows and the ocean2025Doctoral thesis, comprehensive summary (Other academic)
    Abstract [en]

    Polar lows (PLs) are intense, high-latitude mesoscale weather systems that develop over oceanic areas near the polar regions during the cold season. Due to their association with severe weather conditions, they can significantly impact human life and socioeconomic activities. However, their small size, short lifespan, and limited observational data make forecasting PLs particularly challenging. Moreover, the complex physical mechanisms underlying their formation and intensification remain insufficiently understood, highlighting the need for further investigation.

    The ocean plays a critical role in PL development, making an accurate representation of air-sea heat fluxes essential for enhancing forecasts and improving numerical simulations. Intense PLs are often accompanied by localized gale-force winds (>30 m/s), which can extract substantial heat (>1000 W/m2) from the ocean, sufficient to leave pronounced effects on the underlying ocean. Given the strong interactions between PLs and the ocean, this thesis aims to address key knowledge gaps in this field.

    Sea spray, generated by wave breaking under high wind conditions, significantly influences turbulent heat fluxes at the air-sea interface. The first part of this thesis investigates the impact of spray-mediated heat fluxes on PLs through an atmosphere-wave coupled model. Results indicate that spray-enhanced sensible heat fluxes play a crucial role in PL development, whereas spray-enhanced latent heat fluxes have a relatively minor effect. Beyond sea spray, the ocean surface contains mesoscale structures such as eddies and fronts, which create mesoscale sea surface temperature anomalies. These anomalies can also influence air-sea turbulent heat and momentum fluxes, thereby favoring the intensification of PLs, as explored in the second part of this thesis. The third part of this thesis examines the impact of PLs on the global ocean. The findings indicate that the oceanic response to PLs exhibits strong regional variability. The Atlantic Ocean emerges as the most sensitive region.

    In the context of global warming, PL activity is expected to shift poleward as the sea ice edge retreats to higher latitudes, resulting in a reduced frequency of occurrence. However, the response of individual PL development to a warming climate remains uncertain. The final part of this thesis addresses this uncertainty by applying a pseudo-global warming approach to investigate how individual PLs respond to climate change. The results reveal a general weakening of PL intensity under warmer conditions, reflected in lower maximum surface wind speeds and higher minimum sea level pressure. Nevertheless, PL-associated precipitation is projected to intensify, primarily due to increased latent heat release in a warmer atmosphere.

    List of papers
    1. Impact of sea spray-mediated heat fluxes on polar low development
    Open this publication in new window or tab >>Impact of sea spray-mediated heat fluxes on polar low development
    2024 (English)In: Quarterly Journal of the Royal Meteorological Society, ISSN 0035-9009, E-ISSN 1477-870X, Vol. 150, no 762, p. 2976-2990Article in journal (Refereed) Published
    Abstract [en]

    Abstract Sea spray, originating from wave breaking under high wind conditions, can significantly affect turbulent heat fluxes at the air–sea interface. Even though polar lows (PLs) can become extreme weather features with gale-force wind, the impact of sea spray on their development has rarely been investigated and is not considered in operational forecast models. In this study, the impact of sea spray on the development of two PLs over the Barents Sea is studied based on sensitivity experiments with an atmosphere–wave coupled model, where the spray-mediated heat fluxes are parameterized. The results show that the impact of sea-spray-mediated heat fluxes on PL development is sensitive to the surface wind speed. In the case of the stronger PL, the higher surface wind speed results in significantly higher spray-mediated heat fluxes. Consequently, these spray-mediated heat fluxes intensify the convection and diabatic heating of the PL, resulting in its intensification. In comparison, the case with a weaker PL experiences less sea spray production and lower spray-mediated heat fluxes due to its weaker surface wind speeds. Overall, we find that spray-mediated sensible heat fluxes play an important role in the development of PLs, while the latent heat fluxes induced by sea spray have a relatively minor impact.

    Place, publisher, year, edition, pages
    John Wiley & Sons, 2024
    Keywords
    air–sea interaction, heat fluxes, polar low, sea spray
    National Category
    Meteorology and Atmospheric Sciences
    Identifiers
    urn:nbn:se:uu:diva-527829 (URN)10.1002/qj.4746 (DOI)001216374200001 ()2-s2.0-85192553215 (Scopus ID)
    Available from: 2024-05-10 Created: 2024-05-10 Last updated: 2025-04-14Bibliographically approved
    2. Influence of mesoscale sea surface temperature anomaly on polar lows
    Open this publication in new window or tab >>Influence of mesoscale sea surface temperature anomaly on polar lows
    2025 (English)In: Environmental Research Letters, E-ISSN 1748-9326, Vol. 20, no 1, article id 014051Article in journal (Refereed) Published
    Abstract [en]

    Sea surface temperature anomaly (SSTA) associated with mesoscale oceanic processes, which are prevalent throughout the ocean, can significantly influence the atmospheric boundary layer and consequently atmospheric systems. While its influences on tropical and extratropical cyclones have been well-documented, the influence of mesoscale SSTA on polar lows (PLs) remains unexplored. To bridge this knowledge gap, we conducted a series of sensitivity numerical experiments with different SST configurations. The simulation results indicate that, over the lifespan of a PL, SSTA does not significantly influence PL intensity but does enhance latent heat release. On a longer time scale, based on simulations of five winter seasons over the Nordic Sea, we found that the accumulated impact of mesoscale SSTA creates favorable environments for PL intensification, characterized by higher moisture levels and lower static stability. These results highlight the importance of considering high-resolution SST boundary conditions, i.e. resolving mesoscale SST, in climate simulations of PLs.

    Place, publisher, year, edition, pages
    Institute of Physics Publishing (IOPP), 2025
    Keywords
    polar lows, mesoscale eddies, air-sea interaction
    National Category
    Meteorology and Atmospheric Sciences
    Identifiers
    urn:nbn:se:uu:diva-547411 (URN)10.1088/1748-9326/ad9ec6 (DOI)001385258300001 ()
    Funder
    Swedish Research Council, 2022-06725Swedish Research Council, 2020-03190National Academic Infrastructure for Supercomputing in Sweden (NAISS)
    Available from: 2025-01-16 Created: 2025-01-16 Last updated: 2025-04-14Bibliographically approved
    3. Development of Polar Lows in Future Climate Scenarios over the Barents Sea
    Open this publication in new window or tab >>Development of Polar Lows in Future Climate Scenarios over the Barents Sea
    2024 (English)In: Journal of Climate, Vol. 37, no 16, p. 4239-4255Article in journal (Refereed) Published
    Abstract [en]

    Polar lows (PLs) are intense mesoscale cyclones that form over polar oceans during colder months. Characterized by high wind speeds and heavy precipitation, they profoundly impact coastal communities, shipping, and offshore activities. Amid the substantial environmental changes in polar regions due to global warming, PLs are expected to undergo noteworthy transformations. In this study, we investigate the response of PL development in the Barents Sea to climate warming based on two representative PLs. Sensitivity experiments were conducted including the PLs in the present climate and the PLs in a pseudo–global warming scenario projected by the late twenty-first century for Shared Socioeconomic Pathway (SSP) 2-4.5 and SSP 3-7.0 scenarios from phase 6 of the Coupled Model Intercomparison Project (CMIP6). In both warming climate scenarios, there is an anticipated decrease in PL intensity, in terms of the maximum surface wind speed and minimum sea level pressure. Despite the foreseen increase in latent heat release in the future climate, contributing to the enhancement of PL intensity, other primary factors such as decreased baroclinic instability, heightened atmospheric static stability, and reduced overall surface heat fluxes play pivotal roles in the overall decrease in PL intensity in the Barents Sea under warming conditions. The augmentation of surface latent heat flux, however, results in increased precipitation associated with PLs by enhancing the latent heat release. Furthermore, the regional steering flow shifts in the warming climate can influence the trajectory of PLs during their development.

    Place, publisher, year, edition, pages
    American Meteorological Society, 2024
    National Category
    Climate Science
    Identifiers
    urn:nbn:se:uu:diva-536282 (URN)10.1175/JCLI-D-24-0027.1 (DOI)001285440300001 ()
    Available from: 2024-08-15 Created: 2024-08-15 Last updated: 2025-04-14Bibliographically approved
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  • Larsson Taghizadeh, Jonas
    et al.
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Government.
    Österman, Marcus
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Government.
    Choosing the right path: The effects of pursuing general versus vocational secondary education on dropout risk and youth inactivity2025In: Economics of Education Review, ISSN 0272-7757, E-ISSN 1873-7382, Vol. 106, article id 102655Article in journal (Refereed)
    Abstract [en]

    This article presents evidence on how students’ risk of dropping out or becoming inactive (NEET) are affected by pursuing a general (academic) versus vocational upper secondary education. We use a regression discontinuity design exploiting the grade-based admission process in Sweden. The results suggest that, among those students who apply to both types of education, starting a general program is associated with a higher likelihood of not graduating on time and spending more time without employment and outside studies during early adulthood. Furthermore, students on general programs perform worse in tests for courses mandatory for graduation, compared to students on vocational programs. We also find an increased dropout risk among students starting general programs when running family fixed effects models on the population of upper secondary students.

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  • Aaij, R.
    et al.
    Nikhef Natl Inst Subat Phys, Amsterdam, Netherlands;Univ Groningen, Van Swinderen Inst, Groningen, Netherlands;Univ Maastricht, Maastricht, Netherlands.
    Adlarson, Patrik
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics. School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom.
    Eklund, Lars
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics. School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom.
    Kupsc, Andrzej
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics. School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom.
    Ruiz Vidal, Joan
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics. Dept Phys, Div Particle Phys, Lund, Sweden; School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom.
    Zunica, G.
    Ecole Polytech Fed Lausanne, Inst Phys, Lausanne, Switzerland.
    Measurement of CP asymmetry in Bs0 → Ds K± decays2025In: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, Vol. 2025, no 3, article id 139Article in journal (Refereed)
    Abstract [en]

    A measurement of the CP -violating parameters in B0s → D∓s K± decays is reported, based on the analysis of proton-proton collision data collected by the LHCb experiment corresponding to an integrated luminosity of 6 fb−1 at a centre-of-mass energy of13 TeV . The measured parameters are obtained with a decay-time dependent analysis yielding Cf = 0.791 ± 0.061 ± 0.022, A∆Γf = −0.051 ± 0.134 ± 0.058, A∆Γ¯f = −0.303 ± 0.125 ± 0.055,Sf = −0.571 ± 0.084 ± 0.023 and Sf = −0.503 ± 0.084 ± 0.025, where the first uncertainty is statistical and the second systematic. This corresponds to CP violation in the interference between mixing and decay of about 8.6 σ. Together with the value of the Bs0 mixing phase−2βs, these parameters are used to obtain a measurement of the CKM angle γ equal to (74 ± 12) modulo 180, where the uncertainty contains both statistical and systematic contributions. This result is combined with the previous LHCb measurement in this channelusing 3 fb−1 resulting in a determination of γ = (81+12−11).

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  • Zubayer, Anton
    et al.
    Linköping Univ, Dept Phys Chem & Biol IFM, Thin Film Phys Div, SE-58183 Linköping, Sweden..
    Eriksson, Fredrik
    Linköping Univ, Dept Phys Chem & Biol IFM, Thin Film Phys Div, SE-58183 Linköping, Sweden..
    Falk, Martin
    Linköping Univ, Dept Phys Chem & Biol IFM, Thin Film Phys Div, SE-58183 Linköping, Sweden..
    Lorentzon, Marcus
    Linköping Univ, Dept Phys Chem & Biol IFM, Thin Film Phys Div, SE-58183 Linköping, Sweden..
    Palisaitis, Justinas
    Linköping Univ, Dept Phys Chem & Biol IFM, Thin Film Phys Div, SE-58183 Linköping, Sweden..
    Klauser, Christine
    PSI Ctr Neutron & Muon Sci, CH-5232 Villigen, Switzerland..
    Nagy, Gyula
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Materials Physics.
    Wolf, Philipp M.
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Materials Physics.
    Pitthan, Eduardo
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Materials Physics.
    Holeňák, Radek
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Materials Physics.
    Primetzhofer, Daniel
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Materials Physics.
    Stenning, Gavin B. G.
    Rutherford Appleton Lab, ISIS Neutron & Muon Source, Didcot OX11 0QX, Oxon, England..
    Glavic, Artur
    PSI Ctr Neutron & Muon Sci, CH-5232 Villigen, Switzerland..
    Stahn, Jochen
    PSI Ctr Neutron & Muon Sci, CH-5232 Villigen, Switzerland..
    Dorri, Samira
    Linköping Univ, Dept Phys Chem & Biol IFM, Thin Film Phys Div, SE-58183 Linköping, Sweden..
    Eklund, Per
    Uppsala University, Disciplinary Domain of Science and Technology, Chemistry, Department of Chemistry - Ångström, Inorganic Chemistry. Linköping Univ, Dept Phys Chem & Biol IFM, Thin Film Phys Div, SE-58183 Linköping, Sweden.
    Birch, Jens
    Linköping Univ, Dept Phys Chem & Biol IFM, Thin Film Phys Div, SE-58183 Linköping, Sweden..
    Ghafoor, Naureen
    Linköping Univ, Dept Phys Chem & Biol IFM, Thin Film Phys Div, SE-58183 Linköping, Sweden..
    The Role of 11B4C Interlayers in Enhancing Fe/Si Multilayer Performance for Polarized Neutron Mirrors2025In: The Journal of Physical Chemistry C, ISSN 1932-7447, E-ISSN 1932-7455, Vol. 129, no 16, p. 7921-7930Article in journal (Refereed)
    Abstract [en]

    This study investigates the effects of incorporating 11B4C interlayers into Fe/Si multilayers, with a focus on interface quality, reflectivity, polarization, and magnetic properties for polarizing neutron optics. It is found that the introduction of 1–2 Å 11B4C interlayers significantly improves the interface sharpness, reducing interface width and preventing excessive Si diffusion into the Fe layers. X-ray reflectivity and polarized neutron reflectivity measurements show enhanced reflectivity and polarization, with a notable increase in polarization for 30 Å period multilayers. The inclusion of interlayers also helps prevent the formation of iron-silicides, improving both the magnetic properties and neutron optical performance. However, the impact of interlayers is less pronounced in thicker-period multilayers (100 Å), primarily due to the ratio between layer and interface widths. These results suggest that 11B4C interlayers offer a promising route for optimizing Fe/Si multilayer performance in polarizing neutron mirrors.

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  • Rich, Andrea M.
    et al.
    Swiss Fed Inst Technol, Dept Mat, Lab Met Phys & Technol, CH-8093 Zurich, Switzerland..
    Berger, Leopold
    Swiss Fed Inst Technol, Dept Mat, Lab Met Phys & Technol, CH-8093 Zurich, Switzerland..
    Deller, Robin
    Swiss Fed Inst Technol, Dept Mat, Lab Met Phys & Technol, CH-8093 Zurich, Switzerland..
    de Berardinis, Niccoló
    Uppsala University, Disciplinary Domain of Science and Technology, Technology, Department of Materials Science and Engineering. Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Cell Biology.
    Hulsart Billström, Gry
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Cell Biology. Uppsala University, Disciplinary Domain of Science and Technology, Technology, Department of Materials Science and Engineering.
    Helgason, Benedikt
    Swiss Fed Inst Technol, Inst Biomech, CH-8093 Zurich, Switzerland..
    Ferguson, Stephen J.
    Swiss Fed Inst Technol, Inst Biomech, CH-8093 Zurich, Switzerland..
    Persson, Cecilia
    Uppsala University, Disciplinary Domain of Science and Technology, Technology, Department of Materials Science and Engineering.
    Löffler, Jörg F.
    Swiss Fed Inst Technol, Dept Mat, Lab Met Phys & Technol, CH-8093 Zurich, Switzerland..
    Bioresorbable, amorphous magnesium-fiber reinforced bone cement with enhanced mechanical and biological properties2025In: Biomaterials Advances, ISSN 2772-9516, E-ISSN 2772-9508, Vol. 173, article id 214285Article in journal (Refereed)
    Abstract [en]

    In this study, we developed and characterized a fully biodegradable composite bone cement reinforced with short, randomly oriented amorphous magnesium fibers. Fibers of composition Mg60Zn35Ca5 (in at.%) with 50 μm diameter and 2 mm length were produced by wire spinning and then mixed with a magnesium calcium phosphate cement using fiber volume fractions between 10 and 20 %. The interface strength between the fibers and cement was improved by treating the fibers with diammonium hydrogen phosphate. Compared to the reference cement without fibers, flexural strength was increased by 18 % for the composites with 13 and 18 vol% fibers, and the work of fracture was increased by over 1000× in all cases (p < 0.05, n = 6). Immersion in simulated body fluid for two and four weeks showed that the cement's struvite phase degrades first, and overall, the composite degrades slower. The degradation rate can be tailored to the application by changing the fiber percentage or the cement/fiber composition. Murine pre-osteoblastic cells (MC3T3) cultured in extracts of reference and composite cements had significantly higher cell viability, and composites with 13 vol% fibers also had a significantly higher number of cells compared to the control, indicating that the fibers can enhance and promote pre-osteoblastic cell growth. The results demonstrate that amorphous magnesium fibers enhance both the mechanical and biological properties of ceramic bone cement, expanding their prospects for clinical application.

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  • Larsson, Niklas
    et al.
    Umeå Univ, Dept Diagnost & Intervent Anesthesiol & Intens Car, Umeå, Sweden..
    Claesson, Jonas
    Umeå Univ, Dept Diagnost & Intervent Anesthesiol & Intens Car, Umeå, Sweden..
    Lehtipalo, Stefan
    Umeå Univ, Dept Diagnost & Intervent Anesthesiol & Intens Car, Umeå, Sweden..
    Behndig, Annelie
    Umeå Univ, Dept Publ Hlth & Clin Med, Umeå, Sweden..
    Mobarrez, Fariborz
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Clinical Chemistry.
    Haney, Michael
    Umeå Univ, Dept Diagnost & Intervent Anesthesiol & Intens Car, Umeå, Sweden..
    Extracellular vesicle release in an experimental ventilator-induced lung injury porcine model2025In: PLOS ONE, E-ISSN 1932-6203, Vol. 20, no 4, p. e0320144-, article id e0320144Article in journal (Refereed)
    Abstract [en]

    Harmful effects of mechanical ventilation with large tidal volumes, volutrauma, may contribute much to diffuse acute lung injury. Extracellular vesicles have been noted in the context of vital organ injury. We hypothesized that extracellular vesicles from acutely injured lung can be found in both lung and blood. In a two-hit experimental porcine model, we tested if extracellular vesicles could be detected in bronchoalveolar lavage fluid and in plasma over a six-hour period of large tidal volume ventilation after surfactant depletion. After 2 hours of volutrauma, bronchoalveolar lavage fluid showed increased levels of extracellular vesicles containing nucleic acids (stained by SYTO 13) and those positive for both SYTO 13 and HMGB1. No such increase was detected in plasma at any timepoint during the six-hour experiments. This shows that nucleic acid-containing extracellular vesicles appear to be involved in progression of lung injury, possibly indicating cellular damage, but their potential to serve as diagnostic biomarkers of acute lung injury progression, based on plasma sampling, and in the very early phase, is not confirmed by these findings.

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  • Abbas, Rabia
    Uppsala University, Disciplinary Domain of Science and Technology, Biology, Biology Education Centre.
    Investigation of seasonal and interannual dynamics of surface water CO2 in Lake Erken: Ecosystem Breathing: Tracing Carbon dynamics in Lake Erken2025Independent thesis Advanced level (degree of Master (Two Years)), 20 credits / 30 HE creditsStudent thesis
    Abstract [en]

    Lakes are important in global carbon cycling and play a crucial role in the exchange of CO2 between the atmosphere and a Lake. Where lakes act mainly as a source of CO2 and sometimes as a sink, this study highlights the key dynamics of CO2 by exploring the seasonal and interannual variation of CO2 with a special focus on the surface layer of water in Lake Erken. I have worked on the data collected by high-frequency automated sensors placed at different depths for 2020 and 2021. This study focuses on the surface water layer because it has had direct contact with the atmosphere for two years, excluding the winter period from both years. I considered the daily average of all study parameters for performing statistical analysis. This study showed how the partial pressure of CO2 (pCO2)is influenced by other key variables by exploring the impact of both biological (photosynthesis and respiration) and physical processes (i.e., water temperature and windspeed). Statistical analysis showed that both years have clear seasonal patterns where pCO2 is lower in the spring, possibly due to photosynthesis, and higher in the summer and autumn due to respiration and decomposition processes. Nevertheless, there were no significant variations between the years. Univariate analysis showed a strong linear relationship between O2 and pCO2, while O2 explained 95% of the variation in pCO2.Nevertheless, other parameters such as wind speed, chlorophyll, water temperature, and Schmidt stability were found to have a lesser influence. However, multiple regressions found oxygen, chlorophyll, and wind speed to be the most significant parameters. These parameters played a significant role in photosynthetic activity, which ultimately impacted pCO2 variations. R2 stated that 98% of the variation was only due to O2 and wind speed. These results highlight the importance of biological cycling and physical conditions on pCO2.Therefore, O2 was found to be a powerful predictor of CO2 dynamics because it combines biological and physical processes. After O2, the results also illustrate that windspeed has a significant contribution to pCO2 cycling. These findings contribute to our understanding of pCO2 dynamics in lakes and advance the prediction of CO2 emissions from lakes to the atmosphere.

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  • Li, Xinxiu
    et al.
    Karolinska Inst, Dept Clin Sci Intervent & Technol, Med Digital Twin Res Grp, Stockholm, Sweden..
    Loscalzo, Joseph
    Harvard Med Sch, Brigham & Womens Hosp, Boston, MA USA..
    Mahmud, A. K. M. Firoj
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Biochemistry and Microbiology, Genetics and Genomics.
    Aly, Dina Mansour
    Karolinska Inst, Dept Clin Sci Intervent & Technol, Med Digital Twin Res Grp, Stockholm, Sweden..
    Rzhetsky, Andrey
    Univ Chicago, Inst Genom & Syst Biol, Dept Med, Chicago, IL USA.;Univ Chicago, Inst Genom & Syst Biol, Dept Human Genet, Chicago, IL USA..
    Zitnik, Marinka
    Harvard Med Sch, Dept Biomed Informat, Cambridge, MA USA.;Broad Inst MIT & Harvard, Cambridge, MA USA.;Harvard Univ, Kempner Inst Study Nat & Artificial Intelligence, Harvard Data Sci Initiat, Cambridge, MA USA..
    Benson, Mikael
    Karolinska Inst, Dept Clin Sci Intervent & Technol, Med Digital Twin Res Grp, Stockholm, Sweden..
    Digital twins as global learning health and disease models for preventive and personalized medicine2025In: Genome Medicine, E-ISSN 1756-994X, Vol. 17, no 1, article id 11Article, review/survey (Refereed)
    Abstract [en]

    Ineffective medication is a major healthcare problem causing significant patient suffering and economic costs. This issue stems from the complex nature of diseases, which involve altered interactions among thousands of genes across multiple cell types and organs. Disease progression can vary between patients and over time, influenced by genetic and environmental factors. To address this challenge, digital twins have emerged as a promising approach, which have led to international initiatives aiming at clinical implementations. Digital twins are virtual representations of health and disease processes that can integrate real-time data and simulations to predict, prevent, and personalize treatments. Early clinical applications of DTs have shown potential in areas like artificial organs, cancer, cardiology, and hospital workflow optimization. However, widespread implementation faces several challenges: (1) characterizing dynamic molecular changes across multiple biological scales; (2) developing computational methods to integrate data into DTs; (3) prioritizing disease mechanisms and therapeutic targets; (4) creating interoperable DT systems that can learn from each other; (5) designing user-friendly interfaces for patients and clinicians; (6) scaling DT technology globally for equitable healthcare access; (7) addressing ethical, regulatory, and financial considerations. Overcoming these hurdles could pave the way for more predictive, preventive, and personalized medicine, potentially transforming healthcare delivery and improving patient outcomes.

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    FULLTEXT01
  • Skogbrott Birkeland, Marianne
    et al.
    Norwegian Ctr Violence & Traumat Stress Studies, Pb 181 Nydalen, N-0406 Oslo, Norway..
    Blestad, Camilla
    Norwegian Ctr Violence & Traumat Stress Studies, Pb 181 Nydalen, N-0406 Oslo, Norway..
    Solheim Skar, Ane-Marthe
    Norwegian Ctr Violence & Traumat Stress Studies, Pb 181 Nydalen, N-0406 Oslo, Norway..
    Arnberg, Filip K.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Disciplinary Domain of Medicine and Pharmacy, research centers etc., National Centre for Disaster Psychiatry. Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences.
    Jensen, Tine K.
    Norwegian Ctr Violence & Traumat Stress Studies, Pb 181 Nydalen, N-0406 Oslo, Norway.;Univ Oslo, Dept Psychol, Oslo, Norway..
    Development and pilot-testing of an app to complement trauma-focused cognitive behavioral therapy for adolescents: [Desarrollo y prueba piloto de una App (aplicación) para complementar la terapia cognitivo-conductual focalizada en trauma para adolescentes]2025In: European Journal of Psychotraumatology, ISSN 2000-8198, E-ISSN 2000-8066, Vol. 16, no 1, article id 2481703Article in journal (Refereed)
    Abstract [en]

    Background: Apps have the potential to support psychological treatments by providing psychoeducation, increasing homework compliance, and generalizing therapeutic skills outside of sessions. However, there are few apps developed to support specific evidence-based treatment for PTSD for adolescents.

    Objective: This paper shares experiences developing an app to complement Trauma-Focused Cognitive Behavioral Therapy (TF-CBT). It also describes adolescents’ and therapists’ perceived usefulness and the potential effect of the app ‘My everyday life’ on posttraumatic stress symptoms (PTSS).

    Methods: We did a needs assessment with adolescents, therapists, and TF-CBT trainers, followed by programming and beta-testing. We carried out a mixed methods study of 59 adolescent patients (aged 13–18 years) and their therapists. Using a triangulation design, we combined quantitative data on app use and changes in PTSS with qualitative data from interviews with 10 adolescents and 10 therapists who described their experiences with the app.

    Results: The app includes psychoeducation, mental health self-monitoring, coping tools, and goal-setting functionality. The most used features were psychoeducation and breathing exercises. Few therapists actively used the monitoring progress feature. Both adolescents and therapists found the app beneficial for everyday use, though some therapists were unsure about how to integrate it with TF-CBT. Adolescents reported significant PTSS improvement during TF-CBT with the app as a complement. Adolescents with post-treatment data (n = 13) did not report significantly different PTSD improvement compared to adolescents without access to app, but the study lacked power to draw strong conclusions.

    Conclusions: The app ‘My everyday life’ can be useful for adolescents receiving TF-CBT. The therapists may benefit from clearer guidelines on how to integrate apps with evidence-based treatments. Digital tools are a promising avenue for supporting the implementation of evidence-based treatment.

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  • Lagunas-Rangel, Francisco Alejandro
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Surgical Sciences, Functional Pharmacology and Neuroscience. Latvian Inst Organ Synth, Lab Pharmaceut Pharmacol, Riga, Latvia..
    Cholesterol effects on the tumor immune microenvironment: from fundamental concepts to mechanisms and implications2025In: Frontiers in Oncology, E-ISSN 2234-943X, Vol. 15, article id 1579054Article, review/survey (Refereed)
    Abstract [en]

    In many cancers, the tumor microenvironment is enriched with cholesterol due to increased biosynthesis and uptake by cancer cells, resulting in the accumulation of cholesterol, cholesterol esters, oxysterols and other metabolites with various functions. These molecules serve as structural components, energy sources and intracellular signaling mediators, while their toxic by-products are secreted to suppress anti-tumor immune activity and prevent lipid peroxidation that could induce cancer cell apoptosis. Immune cells in the tumor microenvironment also contribute to cholesterol dynamics. Tumor-associated macrophages (TAMs) release cholesterol to support tumor cell metabolism, while myeloid-derived suppressor cells (MDSCs) also release cholesterol and consume essential metabolites such as L-arginine, which impairs T-cell proliferation and activation. Elevated cholesterol in dendritic cells impairs migration and tumor antigen presentation and, in lymphocytes, favors the development of a regulatory T cells (Treg) phenotype and inhibits the release of antitumor cytokines, further weakening the immune response. These findings suggest that targeting cholesterol metabolism is a promising strategy for cancer treatment, improving the efficacy of immune checkpoint blockade (ICB) therapies. In this manuscript, the molecular mechanisms underlying the effects of cholesterol on the tumor immune landscape are reviewed and the potential of cholesterol-lowering drugs to enhance antitumor immune responses is explored.

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  • Hildenwall, Helena
    et al.
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Women's and Children's Health, Centre for Health and Sustainability. Karolinska Inst, Dept Clin Sci Intervent & Technol, Div Pediat, Stockholm, Sweden.;Karolinska Univ Hosp, Astrid Lindgren Childrens Hosp, Stockholm, Sweden.;Karolinska Inst, Dept Global Publ Hlth, Stockholm, Sweden..
    Georgieva, Valya
    Karolinska Inst, Dept Clin Sci Intervent & Technol, Div Pediat, Stockholm, Sweden.;Karolinska Univ Hosp, Astrid Lindgren Childrens Hosp, Stockholm, Sweden..
    Luthander, Joachim
    Karolinska Univ Hosp, Astrid Lindgren Childrens Hosp, Stockholm, Sweden.;Karolinska Inst, Dept Womens & Childrens Hlth, Stockholm, Sweden..
    Ladfors, Susanne Westphal
    Univ Gothenburg, Inst Clin Sci, Sahlgrenska Acad, Dept Pediat, Gothenburg, Sweden.;Queen Silv Childrens Hosp, Gothenburg, Sweden..
    Sartz, Lisa
    Lund Univ, Skane Univ Hosp, Dept Clin Sci, Sect Pediat Nephrol, Lund, Sweden..
    Chromek, Milan
    Karolinska Inst, Dept Clin Sci Intervent & Technol, Div Pediat, Stockholm, Sweden.;Karolinska Univ Hosp, Astrid Lindgren Childrens Hosp, Stockholm, Sweden..
    Pneumococcal Hemolytic Uremic Syndrome in Children in Sweden2025In: JAMA Network Open, E-ISSN 2574-3805, Vol. 8, no 4, article id e255721Article in journal (Other academic)
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  • Wala, Jeremiah
    et al.
    Dana Farber Canc Inst, Dept Canc Biol & Med Oncol, Boston, MA 02215 USA.;Broad Inst MIT & Harvard, Cambridge, MA 02142 USA..
    Dalin, Simona
    Dana Farber Canc Inst, Dept Canc Biol & Med Oncol, Boston, MA 02215 USA.;Broad Inst MIT & Harvard, Cambridge, MA 02142 USA..
    Webster, Sophie
    Dana Farber Canc Inst, Dept Canc Biol & Med Oncol, Boston, MA 02215 USA.;Broad Inst MIT & Harvard, Cambridge, MA 02142 USA..
    Shapira, Ofer
    Dana Farber Canc Inst, Dept Canc Biol & Med Oncol, Boston, MA 02215 USA.;Broad Inst MIT & Harvard, Cambridge, MA 02142 USA..
    Busanovich, John
    Dana Farber Canc Inst, Dept Canc Biol & Med Oncol, Boston, MA 02215 USA..
    Sarmashghi, Shahab
    Broad Inst MIT & Harvard, Cambridge, MA 02142 USA..
    Beroukhim, Rameen
    Dana Farber Canc Inst, Dept Canc Biol & Med Oncol, Boston, MA 02215 USA.;Broad Inst MIT & Harvard, Cambridge, MA 02142 USA..
    Bandopadhayay, Pratiti
    Broad Inst MIT & Harvard, Cambridge, MA 02142 USA.;Dana Farber Canc Inst, Dept Pediat Oncol, Boston, MA 02215 USA..
    Rendo, Verónica
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Immunology, Genetics and Pathology, Neurooncology and neurodegeneration. Dana Farber Canc Inst, Dept Canc Biol & Med Oncol, Boston, MA 02215 USA; Broad Inst MIT & Harvard, Cambridge, MA 02142 USA.
    Recurrent breakpoints in the BRD4 locus reduce toxicity associated with gene amplification2025In: Cell Genomics, E-ISSN 2666-979X, Vol. 5, no 4, article id 100815Article in journal (Refereed)
    Abstract [en]

    Recent work by the ICGC-PCAWG consortium identified recurrent focal deletions in the BRD4 gene, decreasing expression despite increased copy number. We show that these focal deletions occur in the context of cyclin E1 amplification in breast, ovarian, and endometrial cancers, and serve to disrupt BRD4 regulatory regions and gene expression across isoforms. We analyze open reading frame screen data and find that overexpression of BRD4 long (BRD4-L) and short isoform BRD4-S(a) impairs cell growth across cell lines. We confirm these results in OVSAHO ovarian cancer cells, where the overexpression of BRD4 isoforms significantly reduces tumor growth. Next, we mimic BRD4 focal deletions using CRISPR-Cas9 technology and show that these focal deletions rescue ovarian cancer cells from toxicity associated with BRD4 overexpression, suggesting that BRD4 levels must be fine-tuned for cancer cell proliferation. Our study provides experimental evidence for the first recurrent deletion reducing toxicity in cancer, expanding the landscape of cancer progression mechanisms.

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  • Public defence: 2025-06-02 09:00 Hambergsalen, Uppsala
    Holmberg, Emma
    Uppsala University, Disciplinary Domain of Science and Technology, Earth Sciences, Department of Earth Sciences, LUVAL.
    The predictability of European temperature extremes and their health impacts under global change2025Doctoral thesis, comprehensive summary (Other academic)
    Abstract [en]

    Extreme temperature events can cause severe disruptions to society, from negative health consequences to infrastructure damage. Heat action plans, including early warning systems, are a key element in the mitigation of such impacts. Here we investigate the predictability of temperature extremes and their associated health impacts in Europe, in the context of our changing climate. We first investigate the predictability of temperature extremes from a theoretical standpoint, leveraging techniques from dynamical systems theory to quantitatively assess atmospheric persistence. Our results show a regionally and tropospheric-level dependent relationship between warm temperature extremes and atmospheric persistence. We then assess the practical predictability of hot and cold temperature extremes utilising sub-seasonal reforecast data, and the aforementioned measure of persistence. We demonstrate atmospheric persistence informing on practical predictability, measured here by forecast skill, in some cases, again with marked seasonal variation. Furthermore, local processes appear to play an important role in the endgenderment of, and forecast skill for, temperature extremes. Next, we apply methods from epidemiology to temperature forecasts, to produce heat-related mortality forecasts for 2022 and 2023. We find that heat-related mortality can, on average, be forecasted skilfully up to approximately one week. However, we emphasise the increased forecast skill in Iberia associated with the record-breaking temperatures experienced in 2022. Finally, we assess the role of changes in atmospheric circulation patterns for heat-related mortality. We note that changes in the dynamics of the atmosphere can play a reinforcing role to that of the thermodynamic warming trend, such as during the European summer of 2003. These findings could help inform the development of fit-for-purpose heat warning systems. Collectively, this thesis highlights the value in combining theoretical, and impact-focused approaches, for predicting extreme temperatures and their associated health impacts. This is imperative for society’s broader effort to adapt to a warmer climate.

    List of papers
    1. The link between European warm-temperature extremes and atmospheric persistence
    Open this publication in new window or tab >>The link between European warm-temperature extremes and atmospheric persistence
    2023 (English)In: Earth System Dynamics, ISSN 2190-4979, E-ISSN 2190-4987, Vol. 14, no 4, p. 737-765Article in journal (Refereed) Published
    Abstract [en]

    We investigate the link between warm-temperature extremes in Europe and the persistence of large-scale atmospheric-circulation patterns for both winter and summer, along with some possible physical mechanisms connecting the two. We assess atmospheric persistence, leveraging concepts from dynamical systems theory, and reconcile this approach with the more conventional meteorological views of persistence. We find that wintertime warm spells are partly associated with persistent zonal advection at the surface level but display no statistically significant persistence anomaly in the mid-troposphere. For summertime heatwaves, we find a weak yet significant link to anomalously persistent circulation patterns in the mid-troposphere, while there are few significant persistence anomalies of the surface circulation pattern. We further find no evidence of a strong warm-temperature advection signal. This suggests that other radiative and dynamical processes, for example sensible heating and adiabatic warming, as well as local effects, could play a more important role than large-scale warm-temperature advection for these events. We thus argue that persistent atmospheric configurations are not a necessary requirement for warm-temperature extremes and that the results depend to a considerable extent on region and tropospheric level.

    Place, publisher, year, edition, pages
    Copernicus Publications, 2023
    National Category
    Meteorology and Atmospheric Sciences
    Identifiers
    urn:nbn:se:uu:diva-509389 (URN)10.5194/esd-14-737-2023 (DOI)001042848900001 ()
    Funder
    EU, Horizon 2020, 956396
    Available from: 2023-08-18 Created: 2023-08-18 Last updated: 2025-04-04Bibliographically approved
    2. Forecasting atmospheric persistence and implications for the predictability of temperature and temperature extremes
    Open this publication in new window or tab >>Forecasting atmospheric persistence and implications for the predictability of temperature and temperature extremes
    2024 (English)In: Quarterly Journal of the Royal Meteorological Society, ISSN 0035-9009, E-ISSN 1477-870X, Vol. 150, no 765, p. 5518-5534Article in journal (Refereed) Published
    Abstract [en]

    Extreme temperatures can cause severe disruptions to society, from negative health consequences to infrastructure damage. Accurate and timely weather forecasts contribute to minimise these detrimental effects, by supporting early warning systems. In this context, information on the expected performance of the forecasts is valuable. Here, we investigate whether there is a relationship between the persistence of atmospheric circulation patterns in the Euro-Atlantic sector and forecast skill for temperatures and temperature extremes in Europe. We first apply an objective method to compute the persistence of large-scale atmospheric patterns to European Centre for Medium-range Weather Forecasts (ECMWF) sub-seasonal retrospective forecasts. We find that the forecasts successfully predict atmospheric persistence up to timescales of approximately two weeks. We next investigate the relationship between the persistence of an atmospheric state and the practical predictability of temperature in terms of the error in surface temperature forecasts. The relationship between the two varies depending on season and location. Nonetheless, in a number of cases atmospheric persistence provides potentially valuable information on the practical predictability of temperature. We specifically highlight the cases of wintertime temperature forecasts up to 3 weeks lead time and wintertime cold spells up to roughly two weeks lead time.

    Place, publisher, year, edition, pages
    Royal Meteorological Society, 2024
    National Category
    Meteorology and Atmospheric Sciences
    Research subject
    Meteorology
    Identifiers
    urn:nbn:se:uu:diva-541230 (URN)10.1002/qj.4885 (DOI)001357308500001 ()
    Funder
    EU, Horizon 2020Uppsala UniversityEuropean Commission, 956396EU, European Research Council, 948309
    Available from: 2024-10-28 Created: 2024-10-28 Last updated: 2025-04-04Bibliographically approved
    3. Skillful heat-related mortality forecasting during recent deadly European summers
    Open this publication in new window or tab >>Skillful heat-related mortality forecasting during recent deadly European summers
    (English)Manuscript (preprint) (Other academic)
    Abstract [en]

    Europe is a heatwave hotspot: numerous temperature records have been broken in recent summers, and roughly 60,000 and 50,000 heat-related deaths occurred in the summers of 2022 and 2023, respectively. With recent summers, like that of 2022, projected to become the new norm, there is a pressing need to further develop heat-health warning systems to help society adapt to a warming climate. Here, we forecast heat-related mortality by applying a statistical epidemiological framework to temperature forecasts extending up to two weeks in advance. Focusing on two recent and exceptional summers in Europe, namely 2022 and 2023, we evaluate the skill of the daily heat-related mortality forecasts, and assess its association with temperature. For most of Europe, milder temperatures, close to the minimum mortality temperature, are associated with more skilful heat-related mortality forecasts. However, some of the hottest regions in Europe instead showed enhanced forecast skill associated with higher temperatures. This suggests that heat-related mortality forecasts can provide valuable information in European regions associated with high levels of heat-related mortality. Consequently, we advocate for local health authorities to include information from forecasts of heat-related mortality in their heat warning systems.

    Keywords
    Heat-related mortality, early-warning systems, impact forecasting, temperature extremes, Europe
    National Category
    Meteorology and Atmospheric Sciences Climate Science Public Health, Global Health and Social Medicine
    Identifiers
    urn:nbn:se:uu:diva-553899 (URN)
    Available from: 2025-04-04 Created: 2025-04-04 Last updated: 2025-04-04
    4. Changes in atmospheric circulation patterns are associated with increased European heat-related mortality
    Open this publication in new window or tab >>Changes in atmospheric circulation patterns are associated with increased European heat-related mortality
    Show others...
    (English)Manuscript (preprint) (Other academic)
    Abstract [en]

    Heat poses a critical risk to human health around the world. Recent work has investigated how anthropogenic climate change can modulate atmospheric circulation patterns, finding that circulation patterns increasing in frequency are associated with high temperatures in Europe. Here, we investigate the role of these changes in the dynamics of the atmosphere for European heat-related mortality. We find that dynamical changes have reinforced the thermodynamic warming trend, and are associated with increased heat-related mortality in northern and central continental Europe. Furthermore, dynamical changes appear to have played an important role for the extreme temperatures of the European summer of 2003, and the associated heat-related mortality. We thus highlight the importance of considering the role of changes in atmospheric circulation patterns when investigating the role of climate change for heat events and their impacts. Furthermore, we argue that heat action plans should consider the possibility of record-shattering heat events, where dynamical changes contributing to anomalously high temperatures could coincide with the peak of the seasonal temperature cycle, as seen in 2003.

    Keywords
    Heat-related mortality, dynamical changes, heatwaves, Europe
    National Category
    Climate Science Public Health, Global Health and Social Medicine
    Identifiers
    urn:nbn:se:uu:diva-553904 (URN)
    Available from: 2025-04-04 Created: 2025-04-04 Last updated: 2025-04-04
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  • Häggholm, Ida
    et al.
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Educational Sciences, Department of Education.
    Larsson, Klara
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Educational Sciences, Department of Education.
    Små läsare och stora frågor: En intervju- och litteraturanalys av barnlitteratur i förskolan utifrån ett genusperspektiv2025Independent thesis Basic level (professional degree), 10 credits / 15 HE creditsStudent thesis
    Abstract [sv]

    I det här självständiga arbetet har vi bidragit med kunskap om hur pedagoger förhåller sig till val av barnlitteratur och metoder för att integrera ett genusperspektiv i högläsning och litteratursamtal. Det genomfördes sju stycken semistrukturerade intervjuer under två veckor med både förskollärare och barnskötare i tre olika svenska kommuner. Med teorin om didaktiska val som utgångspunkt analyserades intervjusvaren tematiskt. Detta resulterade i fem teman. De olika teman fokuserade på olika överväganden pedagoger gör vid valet av litteratur med fokus på genus, som att böckerna skulle anpassas efter barnens ålder och passa det aktuella projektet avdelningen arbetar med. Andra pedagoger hade ett specifikt mål med litteraturen och valde bok efter vad de ville uppnå med läsningen av normkritisk litteratur. Sedan undersöktes även hur pedagoger jobbar med denna litteratur ute i verksamheten. Här gavs många varierande svar mellan hur pedagogerna specifikt jobbar med barnen när hen läser boken där hen fokuserar på samtal och diskussioner om bokens innehåll, men även hur de jobbar allmänt med normkritisk litteratur på hela förskolan. Under intervjuerna gavs även förslag på böcker som pedagogerna skulle kunna jobba utifrån med fokus på genus. Dessa böcker har analyserats, tematiseras och kopplats till de svar som pedagogerna själva gav kring hur de jobbar med boken. Denna analys baserades på socialkonstruktivismens syn på genus och gav fyra teman som visar att pedagoger uppmärksammar olika egenskaper hos böcker som gör att de väljer att de läser dem för barnen. Vissa teman visades starkare som att pedagogerna ville ha mångfald och representation, medan vissa ville att barnen skulle känna igen sig i karaktärerna i böckerna. Resultatet kopplas sedan till tidigare forskning och relevant didaktisk teori. Slutligen diskuteras även studiens brister och förslag på vidare forskning. 

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  • Carlsson Uggla, Linnea
    et al.
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Educational Sciences, Department of Education.
    Gradin, Alexandra
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Educational Sciences, Department of Education.
    Kreativa uttryck i förskolan - mer än bara lek?: En kvalitativ studie om pedagogers erfarenheter av estetiska uttrycksformer2025Independent thesis Basic level (professional degree), 10 credits / 15 HE creditsStudent thesis
    Abstract [sv]

    Syftet med studien är att undersöka verbaliserade erfarenheter av estetiska uttrycksformer i förskolan, samt hur de uppfattar att dessa arbetssätt påverkar barns lärande och utveckling. Studien består av två delstudier: den första omfattar intervjuer med fem förskollärare och den andra med fem specialpedagoger. Genom att samla in båda yrkesgruppernas uppfattningar skapas en bredare förståelse för hur estetiska uttrycksformer upplevs och kommuniceras i förskolans kontext. Studien har en kvalitativ ansats och utgår teoretiskt från didaktik i förskolan med en läroplansteoretisk grund med stöd av de didaktiska frågorna vad, hur och varför. Analysen genomfördes med hjälp av tematisk analys. Resultatet från delstudie 1 visar att förskollärare uppfattar estetiska uttrycksformer som centrala för att stödja barns kommunikation, känslomässiga uttryck och delaktighet. De används för att skapa kreativa och inkluderande lärmiljöer. Hinder som brist på tid, resurser och kompetens lyfts fram som utmaningar. Resultatet från delstudie 2 lyfter specialpedagogerna fram sina erfarenheter om de estetiska uttrycksformerna och hur detta påverkar barns lärande och utveckling. De framhåller både möjligheter till fortsatt utveckling och utmaningar, såsom begränsade ekonomiska resurser. Studien betonar även vikten av barns rättigheter samt anpassning för att möta individuella behov.

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  • Rasmussen, Bengt
    et al.
    Örebro Univ, Fac Med & Hlth, Dept Med, Div Hematol, Örebro, Sweden..
    Nilsson, Lars
    Skane Univ Hosp, Dept Hematol Oncol & Radiat Phys, Lund, Sweden..
    Tobiasson, Magnus
    Karolinska Univ Hosp, Dept Hematol, Stockholm, Sweden.;Karolinska Inst, Ctr Hematol & Regenerat Med HERM, Dept Med, Stockholm, Sweden..
    Jaedersten, Martin
    Karolinska Univ Hosp, Dept Hematol, Stockholm, Sweden.;Karolinska Inst, Ctr Hematol & Regenerat Med HERM, Dept Med, Stockholm, Sweden..
    Garelius, Hege
    Sahlgrens Univ Hosp, Dept Specialist Med, Sect Hematol & Coagulat, Gothenburg, Sweden..
    Dybedal, Ingunn
    Oslo Univ Hosp, Dept Hematol, Oslo, Norway..
    Gronbaek, Kirsten
    Copenhagen Univ Hosp, Dept Hematol, Rigshosp, Copenhagen, Denmark..
    Ejerblad, Elisabeth
    Uppsala University, Disciplinary Domain of Medicine and Pharmacy, Faculty of Medicine, Department of Medical Sciences, Haematology.
    Lorenz, Fryderyk
    Umeå Univ, Dept Med Biosci, Umeå, Sweden..
    Flogegard, Max
    Falun Gen Hosp, Dept Internal Med, Falun, Sweden..
    Marcher, Claus Werenberg
    Odense Univ Hosp, Dept Hematol, Odense, Denmark..
    Cavalier, Lucia
    Karolinska Univ Hosp, Dept Clin Genet, Solna, Sweden..
    Ebeling, Freja
    Helsinki Univ Hosp, Comprehens Canc Ctr, Div Hematol, Helsinki, Finland..
    Olsnes, Astrid Marta
    Univ Bergen, Fac Med, Bergen, Norway.;Haukeland Hosp, Dept Med, Sect Hematol, Bergen, Norway.;KG Jebsen Ctr Myeloid Blood Canc, Bergen, Norway..
    Norgaard, Jan Maxwell
    Aarhus Univ Hosp, Dept Hematol, Aarhus, Denmark..
    Saft, Leonie
    Karolinska Univ, Hosp & Inst, Dept Clin Pathol & Canc Diagnost, Stockholm, Sweden..
    Mollgard, Lars
    Sahlgrens Univ Hosp, Dept Specialist Med, Sect Hematol & Coagulat, Gothenburg, Sweden..
    Hellstrom-Lindberg, Eva
    Karolinska Univ Hosp, Dept Hematol, Stockholm, Sweden.;Karolinska Inst, Ctr Hematol & Regenerat Med HERM, Dept Med, Stockholm, Sweden..
    Schlegelberger, Brigitte
    Hannover Med Sch, Dept Human Genet, Hannover, Germany..
    Goerhring, Gudrun
    Hannover Med Sch, Dept Human Genet, Hannover, Germany..
    Influence of Cytogenetics on the Outcome of Patients With High-Risk Myelodysplastic Syndrome Including Deletion 5q Treated With Azacitidine With or Without Lenalidomide2025In: Genes, Chromosomes and Cancer, ISSN 1045-2257, E-ISSN 1098-2264, Vol. 64, no 2, article id e70029Article in journal (Refereed)
    Abstract [en]

    In myelodysplastic syndromes (MDS), cytogenetic characteristics of the malignant bone marrow cells influence the clinical course. The aim of this study was to evaluate whether cytogenetics is useful to predict outcome and response in patients with del(5q) under azacitidine (AZA) +/- lenalidomide (LEN) therapy. We therefore performed comprehensive cytogenetic analyses in MDS patients with del(5q) treated within the randomized phase II trial NMDSG10B. Seventy-two patients were enrolled in the study and 46 patients (64%) had sufficient cytogenetics at inclusion and response evaluation. Karyotyping was significantly more sensitive during follow-up to detect del(5q) compared to FISH, 34 patients (97%) versus 27 patients (77%) (p = 0.027). The overall response rate (ORR) did not differ between the 11 patients with < 3 aberrations (median 1 aberration) and the 59 patients with >= 3 aberrations (median 7 aberrations, range 3-16), while >= 3 aberrations were associated with shorter overall survival (OS), 9.9 months versus 25.2 months (p = 0.004). OS was significantly shorter in patients with unbalanced translocation of 5q than patients with del (5)(q14q34), 8.4 months versus 21.1 months (p = 0.004). Both complex karyotype and multi-hit TP53 alterations were more frequent in patients with unbalanced translocations of 5q versus del (5)(q14q34), 98% and 88% versus 67% and 47% (each p = < 0.001). Most patients with cytogenetic progression had multi-hit TP53 alterations at inclusion. Cytogenetic progression occurred at a similar frequency in the AZA arm and in the AZA + LEN arm. In summary, this study in homogenously treated MDS patients with different abnormalities of 5q demonstrates the influence of cytogenetics on treatment results. Trial Registration: EudraCT number: 2011-001639-21; identifier: NCT01556477.

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  • Ablikim, M.
    et al.
    Inst High Energy Phys, Beijing 100049, Peoples R China.
    Adlarson, Patrik
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Johansson, Tord
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Kupsc, Andrzej
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics. Natl Ctr Nucl Res, PL-02093 Warsaw, Poland.
    Schönning, Karin
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Thorén, Viktor
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Wolke, Magnus
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Zu, J.
    State Key Lab Particle Detect & Elect, Beijing 100049, Peoples R China;State Key Lab Particle Detect & Elect, Hefei 230026, Peoples R China;Univ Sci & Technol China, Hefei 230026, Peoples R China.
    Search for ηc(2⁢𝑆)Þ → p ¯p and branching fraction measurements of 𝜒𝑐⁢𝐽→p ‾p via 𝜓⁡(2⁢𝑆) radiative decays2025In: Physical Review D: covering particles, fields, gravitation, and cosmology, ISSN 2470-0010, E-ISSN 2470-0029, Vol. 111, no 1, article id 012003Article in journal (Refereed)
    Abstract [en]

    Using (27.12 +/- 0.14) x 10(8) psi(2S) events collected by the BESIII detector operating at BEPCII, we search for the decay eta(c) (2S) -> p (p) over bar via the process psi(2S) -> gamma eta(c)(2S) and only find a signal with a significance of 1.7 sigma. The upper limit of the product branching fraction at the 90% confidence level is determined to be B(psi(2S) -> gamma eta(c)(2S)) B(eta(c) (2S) -> p (p) over bar)< 2.4 x 10(-7). The branching fractions of chi(cJ) -> p<(p)over bar> (J = 0, 1, 2) are also measured to be B(chi(c0) -> p (p) over bar) = (2.51 +/- 0.02 +/- 0.08) x 10(-4), B(chi(c1) -> p (p) over bar) = (8.16 +/- 0.09 +/- 0.25) x 10(-4), and B(chi(c2) -> p (p) over bar) = (8.33 +/- 0.09 +/- 0.22) x 10(-4), where the first uncertainty is statistical and the second systematic.

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    FULLTEXT01
  • Ablikim, M.
    et al.
    Inst High Energy Phys, Beijing 100049, Peoples R China.
    Adlarson, Patrik
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Johansson, Tord
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Kupsc, Andrzej
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics. Natl Ctr Nucl Res, PL-02093 Warsaw, Poland.
    Schönning, Karin
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Thorén, Viktor
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Wolke, Magnus
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics.
    Zu, J.
    State Key Lab Particle Detect & Elect, Beijing 100049, Peoples R China;Univ Sci & Technol China, Hefei 230026, Peoples R China.
    Search for lepton number violating decays of Ds+ → h-h0e+e+2025In: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, no 1, article id 109Article in journal (Refereed)
    Abstract [en]

    Based on 7.33 fb(-1) of e(+)e(-) collision data collected by the BESIII detector operating at the BEPCII collider at center-of-mass energies from 4.128 to 4.226 GeV, a search for the Majorana neutrino nu(m) is conducted in the lepton-number-violating decays of D-s(+) -> h(-)h(0)e(+)e(+). Here, h(-) represents a K- or pi(-), and h(0) represents a pi(0), K-S(0) or phi. No significant signal is observed, and the upper limits of their branching fractions at the 90% confidence level are determined to be B(D-s(+) -> phi pi(-)e(+)e(+)) < 6.9 x 10(-5), B(D-s(+) -> phi K(-)e(+)e(+)) < 9.9 x 10(-5), B(D-s(+)-> K-S(0)pi(-)e(+)e(+)) < 1.3 x 10(-5), B(D-s(+) -> K(S)(0)K(-)e(+)e(+)) < 2.9 x 10(-5), B(D-s(+) -> pi(-)pi(0)e(+)e(+)) < 2.9 x 10(-5) and B(D-s(+) -> K-pi(0)e(+)e(+)) < 3.4 x 10(-5). The Majorana neutrino is searched for with different mass assumptions within the range [0.20, 0.80] GeV/c(2) in the decay of D-s(+) -> phi e(+)nu(m) with nu(m) -> pi(-)e(+), and the upper limits of the branching fractions at the 90% confidence level are at the level of 10(-5)-10(-2), depending on the mass of the Majorana neutrino.

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    FULLTEXT01
  • Tessore, N.
    et al.
    UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England..
    Joachimi, B.
    UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England..
    Loureiro, A.
    Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden.;Imperial Coll London, Blackett Lab, Astrophys Grp, London SW7 2AZ, England..
    Hall, A.
    Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Canas-Herrera, G.
    Estec, European Space Agcy, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.;Leiden Univ, Inst Lorentz, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands..
    Tutusaus, I.
    Univ Toulouse, CNRS, IRAP, UPS,CNES, 14 Ave Edouard Belin, F-31400 Toulouse, France..
    Jeffrey, N.
    UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England..
    Naidoo, K.
    UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England..
    McEwen, J. D.
    Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England..
    Amara, A.
    Univ Surrey, Sch Math & Phys, Guildford GU2 7XH, Surrey, England..
    Andreon, S.
    INAF Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy..
    Auricchio, N.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Baccigalupi, C.
    IFPU, Via Beirut 2, I-34151 Trieste, Italy.;INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;INFN, Sez Trieste, Via Valerio 2, I-34127 Trieste, TS, Italy.;Scuola Int Super Studi Avanzati, SISSA, Via Bonomea 265, I-34136 Trieste, TS, Italy..
    Baldi, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Univ Bologna, Dipartimento Fis & Astron, Via Gobetti 93-2, I-40129 Bologna, Italy.;INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Bardelli, S.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Bernardeau, F.
    Univ Paris Saclay, CNRS, CEA, Inst Phys Theor, F-91191 Gif Sur Yvette, France.;CNRS, UMR 7095, Inst Astrophys Paris, 98 Bis Blvd Arago, F-75014 Paris, France.;Sorbonne Univ, 98 Bis Blvd Arago, F-75014 Paris, France..
    Bonino, D.
    INAF, Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, TO, Italy..
    Branchini, E.
    INAF Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy.;Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy.;INFN, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy..
    Brescia, M.
    Univ Federico II, Dept Phys E Pancini, Via Cinthia 6, I-80126 Naples, Italy.;INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.;INFN, Sect Naples, Via Cinthia 6, I-80126 Naples, Italy..
    Brinchmann, J.
    Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, PT-4150762 Porto, Portugal.;Univ Porto, Fac Ciencias, Rua Campo Alegre, P-4150007 Porto, Portugal..
    Caillat, A.
    Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France..
    Camera, S.
    INAF, Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, TO, Italy.;Univ Torino, Dipartimento Fis, Via P Giuria 1, I-10125 Turin, Italy.;INFN, Sez Torino, Via P Giuria 1, I-10125 Turin, Italy..
    Capobianco, V.
    INAF, Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, TO, Italy..
    Carbone, C.
    INAF IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy..
    Cardone, V. F.
    INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.;INFN, Sez Roma, Dipartimento Fis, Piazzale Aldo Moro 2,Edificio G Marconi, I-00185 Rome, Italy..
    Carretero, J.
    Ctr Invest Energet Medioambientales & Tecnol CIEM, Ave Complutense 40, Madrid 28040, Spain.;Port Informacio Cient, Campus UAB,C Albareda S-N, Bellaterra 08193, Barcelona, Spain..
    Casas, S.
    Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol TTK, D-52056 Aachen, Germany.;Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England..
    Castellano, M.
    INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy..
    Castignani, G.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Cavuoti, S.
    INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.;INFN, Sect Naples, Via Cinthia 6, I-80126 Naples, Italy..
    Cimatti, A.
    Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Colodro-Conde, C.
    Inst Astrofis Canarias, Calle Via Lactea S-N, San Cristobal La Laguna 38204, Tenerife, Spain..
    Congedo, G.
    Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Conselice, C. J.
    Univ Manchester, Dept Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Oxford M13 9PL, England..
    Conversi, L.
    European Space Agcy, ESRIN, Largo Galileo Galilei 1, I-00044 Rome, Italy.;ESA, ESAC, Camino Bajo Castillo S-N, Madrid 28692, Spain..
    Copin, Y.
    Univ Claude Bernard Lyon 1, CNRS, UMR 5822, IN2P3,IP2I Lyon, F-69100 Villeurbanne, France..
    Courbin, F.
    EPFL, Inst Phys, Astrophys Lab, Observ Sauverny, CH-1290 Versoix, Switzerland.;Univ Barcelona IEEC UB, Inst Ciencies Cosmos ICCUB, Marti i Franques 1, Barcelona 08028, Spain.;ICREA, Passeig Lluis Co 23, Barcelona 08010, Spain..
    Courtois, H. M.
    UCB Lyon 1, CNRS, IN2P3, IUF,IP2I Lyon, 4 Rue Enrico Fermi, F-69622 Villeurbanne, France..
    Cropper, M.
    Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England..
    Da Silva, A.
    Univ Lisbon, Dept Fis, Fac Ciencias, Edificio C8, PT-1749016 Lisbon, Portugal.;Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, P-1749016 Lisbon, Portugal..
    Degaudenzi, H.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    De Lucia, G.
    INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Dinis, J.
    Univ Lisbon, Dept Fis, Fac Ciencias, Edificio C8, PT-1749016 Lisbon, Portugal.;Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, P-1749016 Lisbon, Portugal..
    Dubath, F.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Duncan, C. A. J.
    Univ Manchester, Dept Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Oxford M13 9PL, England..
    Dupac, X.
    ESA, ESAC, Camino Bajo Castillo S-N, Madrid 28692, Spain..
    Dusini, S.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy..
    Farina, M.
    INAF Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00100 Rome, Italy..
    Farrens, S.
    Univ Paris Saclay, Univ Paris Cite, CNRS, CEA,AIM, F-91191 Gif Sur Yvette, France..
    Faustini, F.
    INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.;Italian Space Agcy, Space Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy..
    Ferriol, S.
    Univ Claude Bernard Lyon 1, CNRS, UMR 5822, IN2P3,IP2I Lyon, F-69100 Villeurbanne, France..
    Frailis, M.
    INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Franceschi, E.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Fumana, M.
    INAF IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy..
    Galeotta, S.
    INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Gillard, W.
    Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France..
    Gillis, B.
    Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Giocoli, C.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy..
    Gomez-Alvarez, P.
    ESA, ESAC, Camino Bajo Castillo S-N, Madrid 28692, Spain.;FRACTAL SLNE, Calle Tulipan 2,Portal 13 1A, Las Rozas De Madrid 28231, Spain..
    Grazian, A.
    INAF, Osservatorio Astron Padova, Via Osservatorio 5, I-35122 Padua, Italy..
    Grupp, F.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Guzzo, L.
    INAF Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy.;Univ Milan, Dipartimento Fis Aldo Pontremoli, Via Celoria 16, I-20133 Milan, Italy..
    Haugan, S. V. H.
    Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway..
    Hoekstra, H.
    Leiden Univ, Leiden Observ, Einsteinweg 55, NL-2333 CC Leiden, Netherlands..
    Holmes, W.
    CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA..
    Hormuth, F.
    Felix Hormuth Engn, Goethestr 17, D-69181 Leimen, Germany..
    Hornstrup, A.
    Tech Univ Denmark, Elektrovej 327, DK-2800 Lyngby, Denmark.;Cosm Dawn Ctr DAWN, Copenhagen, Denmark..
    Hudelot, P.
    CNRS, UMR 7095, Inst Astrophys Paris, 98 Bis Blvd Arago, F-75014 Paris, France.;Sorbonne Univ, 98 Bis Blvd Arago, F-75014 Paris, France..
    Jahnke, K.
    Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany..
    Jhabvala, M.
    NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA..
    Keihanen, E.
    Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland.;Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland..
    Kermiche, S.
    Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France..
    Kiessling, A.
    CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA..
    Kubik, B.
    Univ Claude Bernard Lyon 1, CNRS, UMR 5822, IN2P3,IP2I Lyon, F-69100 Villeurbanne, France..
    Kummel, M.
    Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Kunz, M.
    Univ Geneva, Dept Phys Theor, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland.;Univ Geneva, Ctr Astroparticle Phys, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland..
    Kurki-Suonio, H.
    Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland.;Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki, Finland..
    Ligori, S.
    INAF, Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, TO, Italy..
    Lilje, P. B.
    Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway..
    Lindholm, V.
    Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland.;Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki, Finland..
    Lloro, I.
    ASTRON, NOVA Opt Infrared Instrumentat Grp, Oude Hoogeveensedijk 4, NL-7991 PD Dwingeloo, Netherlands..
    Mainetti, G.
    CNRS, IN2P3, Ctr Calcul, 21 Ave Pierre Coubertin, F-69627 Villeurbanne, France..
    Maiorano, E.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Mansutti, O.
    INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Marggraf, O.
    Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany..
    Martinelli, M.
    INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.;INFN, Sez Roma, Dipartimento Fis, Piazzale Aldo Moro 2,Edificio G Marconi, I-00185 Rome, Italy..
    Martinet, N.
    Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France..
    Marulli, F.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy..
    Massey, R.
    Univ Durham, Inst Computat Cosmol, Dept Phys, South Rd, Durham DH1 3LE, England..
    Medinaceli, E.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Mei, S.
    Univ Paris Cite, CNRS, Astroparticule & Cosmol, F-75013 Paris, France..
    Melchior, M.
    Univ Appl Sci & Arts Northwestern Switzerland, Sch Engn, CH-5210 Windisch, Switzerland..
    Mellier, Y.
    CNRS, UMR 7095, Inst Astrophys Paris, 98 Bis Blvd Arago, F-75014 Paris, France.;Sorbonne Univ, 98 Bis Blvd Arago, F-75014 Paris, France.;Inst Astrophys Paris, 98Bis Blvd Arago, F-75014 Paris, France..
    Meneghetti, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Merlin, E.
    INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy..
    Meylan, G.
    EPFL, Inst Phys, Astrophys Lab, Observ Sauverny, CH-1290 Versoix, Switzerland..
    Mohr, J. J.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Moresco, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy..
    Morin, B.
    Univ Paris Saclay, Univ Paris Cite, CNRS, CEA,AIM, F-91191 Gif Sur Yvette, France..
    Moscardini, L.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy..
    Munari, E.
    IFPU, Via Beirut 2, I-34151 Trieste, Italy.;INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Nakajima, R.
    Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany..
    Niemi, S-M
    Padilla, C.
    Barcelona Inst Sci & Technol, IFAE, Campus UAB, Bellaterra 08193, Barcelona, Spain..
    Paltani, S.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Pasian, F.
    INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Pedersen, K.
    Univ Copenhagen, Niels Bohr Inst, DARK, Jagtvej 155, DK-2200 Copenhagen, Denmark..
    Percival, W. J.
    Univ Waterloo, Waterloo Ctr Astrophys, Waterloo, ON N2L 3G1, Canada.;Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada.;Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada..
    Pettorino, V.
    Estec, European Space Agcy, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands..
    Pires, S.
    Univ Paris Saclay, Univ Paris Cite, CNRS, CEA,AIM, F-91191 Gif Sur Yvette, France..
    Polenta, G.
    Italian Space Agcy, Space Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy..
    Poncet, M.
    Ctr Spatial Toulouse, Ctr Natl Etud Spatiales, 18 Ave Edouard Belin, F-31401 Toulouse 9, France..
    Popa, L. A.
    Inst Space Sci, Str Atomistilor 409, Ilfov 077125, Romania..
    Raison, F.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Renzi, A.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy..
    Rhodes, J.
    CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA..
    Riccio, G.
    INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy..
    Romelli, E.
    INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Roncarelli, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Rossetti, E.
    Univ Bologna, Dipartimento Fis & Astron, Via Gobetti 93-2, I-40129 Bologna, Italy..
    Saglia, R.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Sakr, Z.
    Univ Toulouse, CNRS, IRAP, UPS,CNES, 14 Ave Edouard Belin, F-31400 Toulouse, France.;Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.;Univ St Joseph, Fac Sci, Beirut, Lebanon..
    Sanchez, A. G.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Sapone, D.
    Univ Chile, FCFM, Dept Fis, Blanco Encalada 2008, Santiago, Chile..
    Sartoris, B.
    INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Schirmer, M.
    Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany..
    Schneider, P.
    Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany..
    Schrabback, T.
    Univ Innsbruck, Inst Astro & Teilchenphys, Technikerstr 25-8, A-6020 Innsbruck, Austria..
    Secroun, A.
    Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France..
    Seidel, G.
    Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany..
    Seiffert, M.
    CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA..
    Serrano, S.
    IEEC, Edifici RDIT,Campus UPC, Barcelona 08860, Spain.;Satlantis, Univ Sci Pk,Sede Bld 48940, Leioa 48940, Spain.;CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain..
    Sirignano, C.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy..
    Sirri, G.
    INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Stanco, L.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy..
    Steinwagner, J.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Tallada-Crespi, P.
    Ctr Invest Energet Medioambientales & Tecnol CIEM, Ave Complutense 40, Madrid 28040, Spain.;Port Informacio Cient, Campus UAB,C Albareda S-N, Bellaterra 08193, Barcelona, Spain..
    Taylor, A. N.
    Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Tereno, I.
    Univ Lisbon, Dept Fis, Fac Ciencias, Edificio C8, PT-1749016 Lisbon, Portugal.;Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, P-1349018 Lisbon, Portugal..
    Toledo-Moreo, R.
    Univ Politecn Cartagena, Dept Elect & Tecnol Comp, Plaza Hosp 1, Cartagena 30202, Spain..
    Torradeflot, F.
    Ctr Invest Energet Medioambientales & Tecnol CIEM, Ave Complutense 40, Madrid 28040, Spain.;Port Informacio Cient, Campus UAB,C Albareda S-N, Bellaterra 08193, Barcelona, Spain..
    Valenziano, L.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;INFN Bologna, Via Irnerio 46, I-40126 Bologna, Italy..
    Vassallo, T.
    INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Wang, Y.
    CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA..
    Weller, J.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Zamorani, G.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Zucca, E.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Biviano, A.
    IFPU, Via Beirut 2, I-34151 Trieste, Italy.;INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Bolzonella, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Boucaud, A.
    Univ Paris Cite, CNRS, Astroparticule & Cosmol, F-75013 Paris, France..
    Bozzo, E.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Burigana, C.
    INFN Bologna, Via Irnerio 46, I-40126 Bologna, Italy.;INAF, Ist Radioastron, Via Piero Gobetti 101, I-40129 Bologna, Italy..
    Calabrese, M.
    INAF IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy.;Astron Observ Autonomous Reg Aosta Valley OAVdA, Loc Lignan 39, I-11020 Nus, Aosta Valley, Italy..
    Di Ferdinando, D.
    INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Vigo, J. A. Escartin
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Finelli, F.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;INFN Bologna, Via Irnerio 46, I-40126 Bologna, Italy..
    Gracia-Carpio, J.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Matthew, S.
    Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Mauri, N.
    INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Pezzotta, A.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Pontinen, M.
    Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland..
    Scottez, V.
    Inst Astrophys Paris, 98Bis Blvd Arago, F-75014 Paris, France.;Junia, EPA Dept, 41 Bd Vauban, F-59800 Lille, France..
    Mancini, A. Spurio
    Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England.;Royal Holloway Univ London, Dept Phys, London TW20 0EX, England..
    Tenti, M.
    INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Viel, M.
    IFPU, Via Beirut 2, I-34151 Trieste, Italy.;INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;INFN, Sez Trieste, Via Valerio 2, I-34127 Trieste, TS, Italy.;Scuola Int Super Studi Avanzati, SISSA, Via Bonomea 265, I-34136 Trieste, TS, Italy.;ICSC, Ctr Nazl Ric High Performance Comp Big Data & Qua, Via Magnanelli 2, Bologna, Italy..
    Wiesmann, M.
    Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway..
    Akrami, Y.
    UAM, CSIC, Inst Fis Teor, Campus Cantoblanco, Madrid 28049, Spain.;Case Western Reserve Univ, CERCA, ISO, Dept Phys, 10900 Euclid Ave, Cleveland, OH 44106 USA..
    Anselmi, S.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.;Univ PSL, Univ Paris Cite, CNRS, Lab Univers & Theorie,Observ Paris, F-92190 Meudon, France..
    Archidiacono, M.
    Univ Milan, Dipartimento Fis Aldo Pontremoli, Via Celoria 16, I-20133 Milan, Italy.;INFN, Sez Milano, Via Celoria 16, I-20133 Milan, Italy..
    Atrio-Barandela, F.
    Univ Salamanca, Dept Fis Fundamental, Plaza Merced S-N, Salamanca 37008, Spain..
    Balaguera-Antolinez, A.
    Inst Astrofis Canarias, Calle Via Lactea S-N, San Cristobal La Laguna 38204, Tenerife, Spain.;Univ La Laguna, Dept Astrofis, San Cristobal la Laguna 38206, Tenerife, Spain..
    Ballardini, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Univ Ferrara, Dipartimento Fis & Sci Terra, Via Giuseppe Saragat 1, I-44122 Ferrara, Italy.;Ist Nazl Fis Nucl, Sez Ferrara, Via Giuseppe Saragat 1, I-44122 Ferrara, Italy..
    Benielli, D.
    Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France..
    Blanchard, A.
    Univ Toulouse, CNRS, IRAP, UPS,CNES, 14 Ave Edouard Belin, F-31400 Toulouse, France..
    Blot, L.
    Univ PSL, Univ Paris Cite, CNRS, Lab Univers & Theorie,Observ Paris, F-92190 Meudon, France.;Univ Tokyo, UTIAS, Kavli IPMU WPI, Ctr Data Driven Discovery, Kashiwa, Chiba 2778583, Japan..
    Bohringer, H.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Schellingstr 4, D-80799 Munich, Germany.;Max Planck Inst Phys & Astrophys, Boltzmannstr 8, D-85748 Garching, Germany..
    Borgani, S.
    IFPU, Via Beirut 2, I-34151 Trieste, Italy.;INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;INFN, Sez Trieste, Via Valerio 2, I-34127 Trieste, TS, Italy.;Univ Trieste, Dipartimento Fis, Sez Astron, Via Tiepolo 11, I-34131 Trieste, Italy..
    Bruton, S.
    Univ Minnesota, Minnesota Inst Astrophys, 116 Church St SE, Minneapolis, MN 55455 USA..
    Cabanac, R.
    Univ Toulouse, CNRS, IRAP, UPS,CNES, 14 Ave Edouard Belin, F-31400 Toulouse, France..
    Calabro, A.
    INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy..
    Quevedo, B. Camacho
    IEEC, Edifici RDIT,Campus UPC, Barcelona 08860, Spain.;CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain..
    Cappi, A.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Univ Cote Azur, CNRS, Lab Lagrange, Observ Cote Azur, Bd Observ,CS 34229, F-06304 Nice 4, France..
    Caro, F.
    INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy..
    Carvalho, C. S.
    Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, P-1349018 Lisbon, Portugal..
    Castro, T.
    IFPU, Via Beirut 2, I-34151 Trieste, Italy.;INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;INFN, Sez Trieste, Via Valerio 2, I-34127 Trieste, TS, Italy.;ICSC, Ctr Nazl Ric High Performance Comp Big Data & Qua, Via Magnanelli 2, Bologna, Italy..
    Chambers, K. C.
    Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA..
    Cooray, A. R.
    Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA..
    de la Torre, S.
    Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France..
    Desprez, G.
    St Marys Univ, Dept Phys & Astron, 923 Robie St, Halifax, NS B3H 3C3, Canada.;St Marys Univ, Inst Computat Astrophys, 923 Robie St, Halifax, NS B3H 3C3, Canada..
    Diaz-Sanchez, A.
    Univ Politecn Cartagena, Dept Fis Aplicada, Campus Muralla Mar, Murcia 30202, Spain..
    Di Domizio, S.
    Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy.;INFN, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy..
    Dole, H.
    Univ Paris Saclay, CNRS, Inst Astrophys Spatiale, F-91405 Orsay, France..
    Escoffier, S.
    Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France..
    Ferrari, A. G.
    INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Ferreira, P. G.
    Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England..
    Ferrero, I.
    Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway..
    Finoguenov, A.
    Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland..
    Fontana, A.
    INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy..
    Fornari, F.
    INFN Bologna, Via Irnerio 46, I-40126 Bologna, Italy..
    Gabarra, L.
    Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England..
    Ganga, K.
    Univ Paris Cite, CNRS, Astroparticule & Cosmol, F-75013 Paris, France..
    Garcia-Bellido, J.
    UAM, CSIC, Inst Fis Teor, Campus Cantoblanco, Madrid 28049, Spain..
    Gasparetto, T.
    INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Gaztanaga, E.
    Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England.;IEEC, Edifici RDIT,Campus UPC, Barcelona 08860, Spain.;CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain..
    Giacomini, F.
    INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Gianotti, F.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Gozaliasl, G.
    Aalto Univ, Dept Comp Sci, POB 15400, FI-00076 Espoo, Finland..
    Gutierrez, C. M.
    Inst Astrofis Canarias, C Via Lactea S-N, E-38200 San Cristobal la Laguna, Spain.;Univ La Laguna, Dept Astrofis, Avda Francisco Sanchez, E-38200 San Cristobal la Laguna, Spain..
    Hartley, W. G.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Hildebrandt, H.
    Ruhr Univ Bochum, Astron Inst AIRUB, Fac Phys & Astron, German Ctr Cosmol Lensing GCCL, D-44780 Bochum, Germany..
    Hjorth, J.
    Univ Copenhagen, Niels Bohr Inst, DARK, Jagtvej 155, DK-2200 Copenhagen, Denmark..
    Munoz, A. Jimenez
    Univ Grenoble Alpes, CNRS, Grenoble INP, LPSC,IN2P3, 53 Ave Martyrs, F-38000 Grenoble, France..
    Joudaki, S.
    Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England..
    Kajava, J. J. E.
    Univ Turku, Dept Phys & Astron, Vesilinnantie 5, Turku 20014, Finland.;Serco European Space Agcy ESA, Camino Bajo Castillo S-N, Madrid 28692, Spain..
    Kansal, V.
    ARC Ctr Excellence Dark Matter Particle Phys, Melbourne, Vic, Australia.;Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia..
    Karagiannis, D.
    Queen Mary Univ London, Sch Phys & Astron, Mile End Rd, London E1 4NS, England.;Univ Western Cape, Dept Phys & Astron, ZA-7535 Cape Town, South Africa..
    Kirkpatrick, C. C.
    Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland.;Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland..
    Kruk, S.
    ESA, ESAC, Camino Bajo Castillo S-N, Madrid 28692, Spain..
    Lacasa, F.
    Univ Paris Saclay, CNRS, Inst Astrophys Spatiale, F-91405 Orsay, France.;ULB, Serv Phys Theor, CP225,Blvd Triophe, B-1050 Brussels, Belgium..
    Lattanzi, M.
    Ist Nazl Fis Nucl, Sez Ferrara, Via Giuseppe Saragat 1, I-44122 Ferrara, Italy..
    Le Brun, A. M. C.
    Univ PSL, Univ Paris Cite, CNRS, Lab Univers & Theorie,Observ Paris, F-92190 Meudon, France..
    Le Graet, J.
    Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France..
    Legrand, L.
    Univ Estadual Paulista, ICTP South Amer Inst Fundamental Res, Inst Fis Teor, Sao Paulo, Brazil..
    Lesgourgues, J.
    Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol TTK, D-52056 Aachen, Germany..
    Liaudat, T. I.
    Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France..
    Macias-Perez, J.
    Univ Grenoble Alpes, CNRS, Grenoble INP, LPSC,IN2P3, 53 Ave Martyrs, F-38000 Grenoble, France..
    Magliocchetti, M.
    INAF Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00100 Rome, Italy..
    Mannucci, F.
    INAF, Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy..
    Maoli, R.
    INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.;Sapienza Univ Roma, Dipartimento Fis, Piazzale Aldo Moro 2, I-00185 Rome, Italy..
    Martin-Fleitas, J.
    Aurora Technol European Space Agcy ESA, Camino Bajo Castillo S-N, Madrid 28692, Spain..
    Martins, C. J. A. P.
    Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, PT-4150762 Porto, Portugal.;Univ Porto, Ctr Astrofis, Rua Estrelas, P-4150762 Porto, Portugal..
    Maurin, L.
    Univ Paris Saclay, CNRS, Inst Astrophys Spatiale, F-91405 Orsay, France..
    Metcalf, R. B.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy..
    Miluzio, M.
    ESA, ESAC, Camino Bajo Castillo S-N, Madrid 28692, Spain.;HE Space European Space Agcy ESA, Camino Bajo Castillo S-N, Madrid 28692, Spain..
    Monaco, P.
    IFPU, Via Beirut 2, I-34151 Trieste, Italy.;INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;INFN, Sez Trieste, Via Valerio 2, I-34127 Trieste, TS, Italy.;Univ Trieste, Dipartimento Fis, Sez Astron, Via Tiepolo 11, I-34131 Trieste, Italy..
    Montoro, A.
    IEEC, Edifici RDIT,Campus UPC, Barcelona 08860, Spain.;CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain..
    Moretti, C.
    IFPU, Via Beirut 2, I-34151 Trieste, Italy.;INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;INFN, Sez Trieste, Via Valerio 2, I-34127 Trieste, TS, Italy.;Scuola Int Super Studi Avanzati, SISSA, Via Bonomea 265, I-34136 Trieste, TS, Italy.;ICSC, Ctr Nazl Ric High Performance Comp Big Data & Qua, Via Magnanelli 2, Bologna, Italy..
    Morgante, G.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Murray, C.
    Univ Paris Cite, CNRS, Astroparticule & Cosmol, F-75013 Paris, France..
    Nadathur, S.
    Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England..
    Walton, N. A.
    Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England..
    Patrizii, L.
    INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Popa, V.
    Inst Space Sci, Str Atomistilor 409, Ilfov 077125, Romania..
    Potter, D.
    Univ Zurich, Dept Astrophys, Winterthurerstr 190, CH-8057 Zurich, Switzerland..
    Reimberg, P.
    Inst Astrophys Paris, 98Bis Blvd Arago, F-75014 Paris, France..
    Risso, I.
    INAF, Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy.;INFN, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy..
    Rocci, P-F
    Rollins, R. P.
    Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Sahlén, Martin
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Theoretical Astrophysics.
    Sarpa, E.
    INFN, Sez Trieste, Via Valerio 2, I-34127 Trieste, TS, Italy.;Scuola Int Super Studi Avanzati, SISSA, Via Bonomea 265, I-34136 Trieste, TS, Italy.;ICSC, Ctr Nazl Ric High Performance Comp Big Data & Qua, Via Magnanelli 2, Bologna, Italy..
    Schneider, A.
    Univ Zurich, Dept Astrophys, Winterthurerstr 190, CH-8057 Zurich, Switzerland..
    Sereno, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Simon, P.
    Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany..
    Tanidis, K.
    Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England..
    Tao, C.
    Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France..
    Testera, G.
    INFN, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy..
    Teyssier, R.
    Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA..
    Toft, S.
    Cosm Dawn Ctr DAWN, Copenhagen, Denmark.;Univ Copenhagen, Niels Bohr Inst, Jagtvej 128, DK-2200 Copenhagen, Denmark..
    Tosi, S.
    Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy.;INFN, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy..
    Troja, A.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy..
    Tucci, M.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Valieri, C.
    INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Valiviita, J.
    Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland.;Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki, Finland..
    Vergani, D.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Verza, G.
    NYU, Ctr Cosmol & Particle Phys, Dept Phys, New York, NY 10003 USA.;Flatiron Inst, Ctr Computat Astrophys, 162 5th Ave, New York, NY 10010 USA..
    Vielzeuf, P.
    Aix Marseille Univ, CNRS, IN2P3, CPPM, Marseille, France..
    Brown, M. L.
    Univ Manchester, Dept Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Oxford M13 9PL, England..
    Sellentin, E.
    Leiden Univ, Leiden Observ, Einsteinweg 55, NL-2333 CC Leiden, Netherlands.;Leiden Univ, Math Inst, Niels Bohrweg 1, NL-2333 CA Leiden, Netherlands..
    Euclid preparation LIX. Angular power spectra from discrete observations2025In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 694, article id A141Article in journal (Refereed)
    Abstract [en]

    In this paper we present the framework for measuring angular power spectra in the Euclid mission. The observables in galaxy surveys, such as galaxy clustering and cosmic shear, are not continuous fields, but discrete sets of data, obtained only at the positions of galaxies. We show how to compute the angular power spectra of such discrete data sets, without treating observations as maps of an underlying continuous field that is overlaid with a noise component. This formalism allows us to compute the exact theoretical expectations for our measured spectra, under a number of assumptions that we track explicitly. In particular, we obtain exact expressions for the additive biases ('shot noise') in angular galaxy clustering and cosmic shear. For efficient practical computations, we introduce a spin-weighted spherical convolution with a well-defined convolution theorem, which allows us to apply exact theoretical predictions to finite-resolution maps, including HEALPix. When validating our methodology, we find that our measurements are biased by less than 1% of their statistical uncertainty in simulations of Euclid's first data release.

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  • Lesgourgues, J.
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    Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol TTK, D-52056 Aachen, Germany..
    Schwagereit, J.
    Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol TTK, D-52056 Aachen, Germany..
    Bucko, J.
    Univ Zurich, Dept Astrophys, Winterthurerstr 190, CH-8057 Zurich, Switzerland..
    Parimbelli, G.
    CSIC, ICE, Inst Space Sci, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain.;Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy.;Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy.;Scuola Int Super Studi Avanzati, SISSA, Via Bonomea 265, I-34136 Trieste, Ts, Italy..
    Giri, S. K.
    Univ Zurich, Dept Astrophys, Winterthurerstr 190, CH-8057 Zurich, Switzerland.;KTH Royal Inst Technol, NORDITA, Hannes Alfvens Vag 12, SE-10691 Stockholm, Sweden.;Stockholm 1859 Univ, Hannes Alfvens Vag 12, SE-10691 Stockholm, Sweden..
    Hervas-Peters, F.
    Univ Zurich, Dept Astrophys, Winterthurerstr 190, CH-8057 Zurich, Switzerland.;Univ Paris Cite, Univ Paris Saclay, CEA, CNRS,AIM, F-91191 Gif Sur Yvette, France..
    Schneider, A.
    Univ Zurich, Dept Astrophys, Winterthurerstr 190, CH-8057 Zurich, Switzerland..
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    Univ Milan, Dipartimento Fis Aldo Pontremoli, Via Celoria 16, I-20133 Milan, Italy.;Ist Nazl Fis Nucl, Sez Milano, Via Celoria 16, I-20133 Milan, Italy..
    Pace, F.
    Univ Torino, Dipartimento Fis, Via P Giuria 1, I-10125 Turin, Italy.;Ist Nazl Fis Nucl, Sez Torino, Via P Giuria 1, I-10125 Turin, Italy.;INAF, Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, To, Italy..
    Sakr, Z.
    Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.;Univ Toulouse, CNRS, Inst Rech Astrophys & Planetol, UPS,CNES, 14 Ave Edouard Belin, F-31400 Toulouse, France.;Univ St Joseph, Beirut, Lebanon.;Fac Sci, Beirut, Lebanon..
    Amara, A.
    Univ Surrey, Sch Math & Phys, Guildford GU2 7XH, Surrey, England..
    Amendola, L.
    Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany..
    Andreon, S.
    INAF, Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy..
    Auricchio, N.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Aussel, H.
    Univ Paris Cite, Univ Paris Saclay, CEA, CNRS,AIM, F-91191 Gif Sur Yvette, France..
    Baldi, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Univ Bologna, Dipartimento Fis & Astron, Via Piero Gobetti 93-2, I-40129 Bologna, Italy.;Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Bardelli, S.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Bender, R.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Bodendorf, C.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Bonino, D.
    INAF, Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, To, Italy..
    Branchini, E.
    Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy.;Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy.;INAF, Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy..
    Brescia, M.
    Univ Federico II, Dept Phys E Pancini, Via Cinthia 6, I-80126 Naples, Italy.;INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.;Ist Nazl Fis Nucl, Sect Naples, Via Cinthia 6, I-80126 Naples, Italy..
    Brinchmann, J.
    Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, PT-4150762 Porto, Portugal..
    Camera, S.
    Univ Torino, Dipartimento Fis, Via P Giuria 1, I-10125 Turin, Italy.;Ist Nazl Fis Nucl, Sez Torino, Via P Giuria 1, I-10125 Turin, Italy.;INAF, Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, To, Italy..
    Capobianco, V.
    INAF, Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, To, Italy..
    Carbone, C.
    INAF, IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy..
    Cardone, V. F.
    INAF, Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.;Ist Nazl Fis Nucl, Sez Roma, Dipartimento Fis, Piazzale Aldo Moro 2,Edificio G Marconi, I-00185 Rome, Italy..
    Carretero, J.
    Ctr Invest Energet Medioambientales & Tecnol CIEM, Ave Complutense 40, Madrid 28040, Spain.;Port Informacio Cient, Campus UAB,C Albareda S-N, Bellaterra 08193, Barcelona, Spain..
    Casas, S.
    Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol TTK, D-52056 Aachen, Germany..
    Castellano, M.
    INAF, Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy..
    Cavuoti, S.
    INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy.;Ist Nazl Fis Nucl, Sect Naples, Via Cinthia 6, I-80126 Naples, Italy..
    Cimatti, A.
    Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Congedo, G.
    Univ Edinburgh, Royal Observ, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Conselice, C. J.
    Univ Manchester, Dept Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England..
    Conversi, L.
    European Space Agcy, ESRIN, Largo Galileo Galilei 1, I-00044 Rome, Italy.;ESA, ESAC, Camino Bajo Castillo S-N, Madrid 28692, Spain..
    Copin, Y.
    Univ Claude Bernard Lyon 1, CNRS, IN2P3, IP2I Lyon,UMR 5822, F-69100 Villeurbanne, France..
    Courbin, F.
    Ecole Polytech Fed Lausanne, Observ Sauverny, Astrophys Lab, Inst Phys, CH-1290 Versoix, Switzerland..
    Courtois, H. M.
    UCB Lyon 1, CNRS, IN2P3, IUF,IP2I Lyon, 4 Rue Enrico Fermi, F-69622 Villeurbanne, France..
    Da Silva, A.
    Univ Lisbon, Fac Ciencias, Dept Fis, Edificio C8, PT-1749016 Lisbon, Portugal.;Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, P-1749016 Lisbon, Portugal..
    Degaudenzi, H.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Di Giorgio, A. M.
    INAF, Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00100 Rome, Italy..
    Douspis, M.
    Univ Paris Saclay, Inst Astrophys Spatiale, CNRS, F-91405 Orsay, France..
    Dubath, F.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Dupac, X.
    ESA, ESAC, Camino Bajo Castillo S-N, Madrid 28692, Spain..
    Dusini, S.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy..
    Farina, M.
    INAF, Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00100 Rome, Italy..
    Farrens, S.
    Univ Paris Cite, Univ Paris Saclay, CEA, CNRS,AIM, F-91191 Gif Sur Yvette, France..
    Ferriol, S.
    Univ Claude Bernard Lyon 1, CNRS, IN2P3, IP2I Lyon,UMR 5822, F-69100 Villeurbanne, France..
    Fosalba, P.
    Inst Estudis Espacials Catalunya, Edifici RDIT,Campus UPC, Barcelona 08860, Spain.;CSIC, IEEC, Inst Ciencies Espai, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain..
    Frailis, M.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Franceschi, E.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Fumana, M.
    INAF, IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy..
    Galeotta, S.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Gillis, B.
    Univ Edinburgh, Royal Observ, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Giocoli, C.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy..
    Grazian, A.
    INAF, Osservatorio Astron Padova, Via Osservatorio 5, I-35122 Padua, Italy..
    Grupp, F.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Guzzo, L.
    Univ Milan, Dipartimento Fis Aldo Pontremoli, Via Celoria 16, I-20133 Milan, Italy.;Ist Nazl Fis Nucl, Sez Milano, Via Celoria 16, I-20133 Milan, Italy.;INAF, Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy..
    Haugan, S. V. H.
    Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway..
    Hoekstra, H.
    Leiden Univ, Leiden Observ, Einsteinweg 55, NL-2333 CC Leiden, Netherlands..
    Holmes, W.
    CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA..
    Hook, I.
    Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England..
    Hormuth, F.
    Felix Hormuth Engn, Goethestr 17, D-69181 Leimen, Germany..
    Hornstrup, A.
    Tech Univ Denmark, Elektrovej 327, DK-2800 Lyngby, Denmark.;Cosm Dawn Ctr DAWN, Copenhagen, Denmark..
    Jahnke, K.
    Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany..
    Joachimi, B.
    UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England..
    Keihanen, E.
    Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland.;Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland..
    Kermiche, S.
    Aix Marseille Univ, CNRS, CPPM, IN2P3, Marseille, France..
    Kiessling, A.
    CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA..
    Kubik, B.
    Univ Claude Bernard Lyon 1, CNRS, IN2P3, IP2I Lyon,UMR 5822, F-69100 Villeurbanne, France..
    Kunz, M.
    Univ Geneva, Dept Phys Theor, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland.;Univ Geneva, Ctr Astroparticle Phys, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland..
    Kurki-Suonio, H.
    Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland.;Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland..
    Laureijs, R.
    European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands..
    Ligori, S.
    INAF, Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, To, Italy..
    Lilje, P. B.
    Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway..
    Lindholm, V.
    Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland.;Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland..
    Lloro, I.
    ASTRON, NOVA Opt Infrared Instrumentat Grp, Oude Hoogeveensedijk 4, NL-7991 PD Dwingeloo, Netherlands..
    Maino, D.
    Univ Milan, Dipartimento Fis Aldo Pontremoli, Via Celoria 16, I-20133 Milan, Italy.;Ist Nazl Fis Nucl, Sez Milano, Via Celoria 16, I-20133 Milan, Italy.;INAF, IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy..
    Maiorano, E.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Mansutti, O.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Marggraf, O.
    Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany..
    Markovic, K.
    CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA..
    Martinet, N.
    Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France..
    Marulli, F.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy..
    Massey, R.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Univ Durham, Dept Phys, Ctr Extragalact Astron, South Rd, Durham DH1 3LE, England..
    Medinaceli, E.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Mei, S.
    Univ Paris Cite, CNRS, Astroparticule & Cosmol, F-75013 Paris, France..
    Mellier, Y.
    Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France.;CNRS, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.;Sorbonne Univ, 98 Bis Blvd Arago, F-75014 Paris, France..
    Meneghetti, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Merlin, E.
    INAF, Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy..
    Meylan, G.
    Ecole Polytech Fed Lausanne, Observ Sauverny, Astrophys Lab, Inst Phys, CH-1290 Versoix, Switzerland..
    Moresco, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy..
    Moscardini, L.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy..
    Munari, E.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy..
    Nakajima, R.
    Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany..
    Niemi, S-M
    European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands..
    Nightingale, J. W.
    Newcastle Univ, Sch Math Stat & Phys, Herschel Bldg, Newcastle Upon Tyne NE1 7RU, Tyne & Wear, England.;Univ Durham, Dept Phys, Inst Computat Cosmol, South Rd, Durham DH1 3LE, England..
    Padilla, C.
    Barcelona Inst Sci & Technol, Inst Fis Altes Energies, Campus UAB, Bellaterra 08193, Barcelona, Spain..
    Paltani, S.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Pasian, F.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Pedersen, K.
    Univ Aarhus, Dept Phys & Astron, Ny Munkegade 120, DK-8000 Aarhus C, Denmark..
    Percival, W. J.
    Univ Waterloo, Waterloo Ctr Astrophys, Waterloo, ON N2L 3G1, Canada.;Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada.;Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada..
    Pettorino, V.
    European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands..
    Polenta, G.
    Italian Space Agcy, Space Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy..
    Poncet, M.
    Ctr Spatial Toulouse, Ctr Natl Etud Spatiales, 18 Ave Edouard Belin, F-31401 Toulouse 9, France..
    Popa, L. A.
    Inst Space Sci, Str Atomistilor 409, Magurele 077125, Ilfov, Romania..
    Raison, F.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Rebolo, R.
    Inst Astrofis Canarias, Calle Via Lactea S-N, Tenerife 38204, Spain.;Univ La Laguna, Dept Astrofis, Tenerife 38206, Spain..
    Renzi, A.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy..
    Rhodes, J.
    CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA..
    Riccio, G.
    INAF, Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy..
    Romelli, E.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Roncarelli, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Saglia, R.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Sapone, D.
    Univ Chile, FCFM, Dept Fis, Blanco Encalada 2008, Santiago, Chile..
    Sartoris, B.
    Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany.;INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Scaramella, R.
    INAF, Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.;Ist Nazl Fis Nucl, Sez Roma, Dipartimento Fis, Piazzale Aldo Moro 2,Edificio G Marconi, I-00185 Rome, Italy..
    Schneider, P.
    Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany..
    Schrabback, T.
    Univ Innsbruck, Inst Astro & Teilchenphys, Technikerstr 25-8, A-6020 Innsbruck, Austria..
    Secroun, A.
    Aix Marseille Univ, CNRS, CPPM, IN2P3, Marseille, France..
    Seidel, G.
    Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany..
    Serrano, S.
    CSIC, ICE, Inst Space Sci, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain.;Inst Estudis Espacials Catalunya, Edifici RDIT,Campus UPC, Barcelona 08860, Spain.;Satlantis, Univ Sci Pk,Sede Bld, Leioa 48940, Spain..
    Sirignano, C.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy..
    Sirri, G.
    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Stanco, L.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy..
    Tallada-Crespi, P.
    Ctr Invest Energet Medioambientales & Tecnol CIEM, Ave Complutense 40, Madrid 28040, Spain.;Port Informacio Cient, Campus UAB,C Albareda S-N, Bellaterra 08193, Barcelona, Spain..
    Tereno, I.
    Univ Lisbon, Fac Ciencias, Dept Fis, Edificio C8, PT-1749016 Lisbon, Portugal.;Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, P-1349018 Lisbon, Portugal..
    Toledo-Moreo, R.
    Univ Politecn Cartagena, Dept Elect & Tecnol Comp, Plaza Hosp 1, Cartagena 30202, Spain..
    Torradeflot, F.
    Ctr Invest Energet Medioambientales & Tecnol CIEM, Ave Complutense 40, Madrid 28040, Spain.;Port Informacio Cient, Campus UAB,C Albareda S-N, Bellaterra 08193, Barcelona, Spain..
    Tutusaus, I.
    Univ Toulouse, CNRS, Inst Rech Astrophys & Planetol, UPS,CNES, 14 Ave Edouard Belin, F-31400 Toulouse, France..
    Valenziano, L.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;INFN Bologna, Via Irnerio 46, I-40126 Bologna, Italy..
    Vassallo, T.
    Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany.;INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Veropalumbo, A.
    Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy.;INAF, Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy..
    Wang, Y.
    CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA..
    Weller, J.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Fak Phys, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany..
    Zamorani, G.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Zucca, E.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Biviano, A.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy..
    Boucaud, A.
    Univ Paris Cite, CNRS, Astroparticule & Cosmol, F-75013 Paris, France..
    Bozzo, E.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Burigana, C.
    INFN Bologna, Via Irnerio 46, I-40126 Bologna, Italy.;INAF, Ist Radioastron, Via Piero Gobetti 101, I-40129 Bologna, Italy..
    Calabrese, M.
    INAF, IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy.;Astron Observ Autonomous Reg Aosta Valley OAVdA, Loc Lignan 39, I-11020 Nus, Aosta Valley, Italy..
    Colodro-Conde, C.
    Inst Astrofis Canarias, Calle Via Lactea S-N, Tenerife 38204, Spain..
    De Lucia, G.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Di Ferdinando, D.
    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Vigo, J. A. Escartin
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Fabbian, G.
    Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales.;Flatiron Inst, Ctr Computat Astrophys, 162 5th Ave, New York, NY 10010 USA..
    Farinelli, R.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Gracia-Carpio, J.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Ilic, S.
    Univ Toulouse, CNRS, Inst Rech Astrophys & Planetol, UPS,CNES, 14 Ave Edouard Belin, F-31400 Toulouse, France.;Univ Paris Saclay, CNRS, IJCLab, IN2P3, F-91405 Orsay, France..
    Mainetti, G.
    CNRS, IN2P3, Ctr Calcul, 21 Ave Pierre Coubertin, F-69627 Villeurbanne, France..
    Martinelli, M.
    INAF, Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.;Ist Nazl Fis Nucl, Sez Roma, Dipartimento Fis, Piazzale Aldo Moro 2,Edificio G Marconi, I-00185 Rome, Italy..
    Mauri, N.
    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Neissner, C.
    Port Informacio Cient, Campus UAB,C Albareda S-N, Bellaterra 08193, Barcelona, Spain.;Barcelona Inst Sci & Technol, Inst Fis Altes Energies, Campus UAB, Bellaterra 08193, Barcelona, Spain..
    Nucita, A. A.
    Univ Salento, Dept Math & Phys E Giorgi, Via Arnesano,CP I93, I-73100 Lecce, Italy.;INAF, Dipartimento Matemat & Fis, Sez Lecce, Via Arnesano, I-73100 Lecce, Italy.;Ist Nazl Fis Nucl, Sez Lecce, Via Arnesano,CP 193, I-73100 Lecce, Italy..
    Scottez, V.
    Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France.;Junia, EPA Dept, 41 Bd Vauban, F-59800 Lille, France..
    Tenti, M.
    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Viel, M.
    Scuola Int Super Studi Avanzati, SISSA, Via Bonomea 265, I-34136 Trieste, Ts, Italy.;INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy.;Ist Nazl Fis Nucl, Sez Trieste, Via Valerio 2, I-34127 Trieste, Ts, Italy.;Ctr Nazl Ric High Performance Comp Big Data & Qua, ICSC, Via Magnanelli 2, Bologna, Italy..
    Wiesmann, M.
    Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway..
    Akrami, Y.
    UAM, Inst Fis Teor, CSIC, Campus Cantoblanco, Madrid 28049, Spain.;Case Western Reserve Univ, Dept Phys, ISO, CERCA, 10900 Euclid Ave, Cleveland, OH 44106 USA..
    Anselmi, S.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.;Univ Paris Cite, CNRS, Univ PSL, Lab Univers & Theorie,Observ Paris, F-92190 Meudon, France..
    Baccigalupi, C.
    Scuola Int Super Studi Avanzati, SISSA, Via Bonomea 265, I-34136 Trieste, Ts, Italy.;INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy.;Ist Nazl Fis Nucl, Sez Trieste, Via Valerio 2, I-34127 Trieste, Ts, Italy..
    Ballardini, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Univ Ferrara, Dipartimento Fis & Sci Terra, Via Giuseppe Saragat 1, I-44122 Ferrara, Italy.;Ist Nazl Fis Nucl, Sez Ferrara, Via Giuseppe Saragat 1, I-44122 Ferrara, Italy..
    Bertacca, D.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;INAF, Osservatorio Astron Padova, Via Osservatorio 5, I-35122 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy..
    Blot, L.
    Univ Paris Cite, CNRS, Univ PSL, Lab Univers & Theorie,Observ Paris, F-92190 Meudon, France.;Univ Tokyo, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan..
    Boehringer, H.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Ludwig Maximilians Univ Munchen, Schellingstr 4, D-80799 Munich, Germany..
    Borgani, S.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy.;Ist Nazl Fis Nucl, Sez Trieste, Via Valerio 2, I-34127 Trieste, Ts, Italy.;Univ Trieste, Dipartimento Fis, Sez Astron, Via Tiepolo 11, I-34131 Trieste, Italy..
    Bruton, S.
    Univ Minnesota, Minnesota Inst Astrophys, 116 Church St SE, Minneapolis, MN 55455 USA..
    Cabanac, R.
    Univ Toulouse, CNRS, Inst Rech Astrophys & Planetol, UPS,CNES, 14 Ave Edouard Belin, F-31400 Toulouse, France..
    Calabro, A.
    INAF, Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy..
    Cappi, A.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Univ Cote Azur, Observ Cote Azur, CNRS, Lab Lagrange, Bd Observ,CS 34229, F-06304 Nice 4, France..
    Carvalho, C. S.
    Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, P-1349018 Lisbon, Portugal..
    Castignani, G.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Castro, T.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy.;Ist Nazl Fis Nucl, Sez Trieste, Via Valerio 2, I-34127 Trieste, Ts, Italy.;Ctr Nazl Ric High Performance Comp Big Data & Qua, ICSC, Via Magnanelli 2, Bologna, Italy..
    Chambers, K. C.
    Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA..
    Contarini, S.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy..
    Cooray, A. R.
    Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA..
    Davini, S.
    Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy..
    De Caro, B.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy..
    de la Torre, S.
    Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France..
    Desprez, G.
    St Marys Univ, Dept Phys & Astron, 923 Robie St, Halifax, NS B3H 3C3, Canada.;St Marys Univ, Inst Computat Astrophys, 923 Robie St, Halifax, NS B3H 3C3, Canada..
    Diaz-Sanchez, A.
    Univ Politecn Cartagena, Dept Fis Aplicada, Campus Muralla Mar, Murcia 30202, Spain..
    Di Domizio, S.
    Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy.;Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy..
    Dole, H.
    Univ Paris Saclay, Inst Astrophys Spatiale, CNRS, F-91405 Orsay, France..
    Escoffier, S.
    Aix Marseille Univ, CNRS, CPPM, IN2P3, Marseille, France..
    Ferrari, A. G.
    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Ferreira, P. G.
    Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England..
    Ferrero, I.
    Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway..
    Finelli, F.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;INFN Bologna, Via Irnerio 46, I-40126 Bologna, Italy..
    Fornari, F.
    INFN Bologna, Via Irnerio 46, I-40126 Bologna, Italy..
    Gabarra, L.
    Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England..
    Ganga, K.
    Univ Paris Cite, CNRS, Astroparticule & Cosmol, F-75013 Paris, France..
    Garcia-Bellido, J.
    UAM, Inst Fis Teor, CSIC, Campus Cantoblanco, Madrid 28049, Spain..
    Gaztanaga, E.
    CSIC, ICE, Inst Space Sci, Campus UAB,Carrer Can Magrans S-N, Barcelona 08193, Spain.;Inst Estudis Espacials Catalunya, Edifici RDIT,Campus UPC, Barcelona 08860, Spain.;Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England..
    Giacomini, F.
    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Gozaliasl, G.
    Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland.;Aalto Univ, Dept Comp Sci, POB 15400, FI-00076 Espoo, Finland..
    Hildebrandt, H.
    Ruhr Univ Bochum, Fac Phys & Astron, Astron Inst AIRUB, German Ctr Cosmol Lensing, D-44780 Bochum, Germany..
    Hjorth, J.
    Univ Copenhagen, Niels Bohr Inst, DARK, Jagtvej 155, DK-2200 Copenhagen, Denmark..
    Munnoz, A. Jimenez
    Univ Grenoble Alpes, CNRS, IN2P3, Grenoble INP,LPSC, 53 Ave Martyrs, F-38000 Grenoble, France..
    Joudaki, S.
    Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England..
    Kajava, J. J. E.
    Univ Turku, Dept Phys & Astron, Vesilinnantie 5, Turku 20014, Finland.;Serco European Space Agcy ESA, Camino Bajo Castillo S-N, Madrid 28692, Spain..
    Kansal, V.
    ARC Ctr Excellence Dark Matter Particle Phys, Melbourne, Vic, Australia.;Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia..
    Karagiannis, D.
    Queen Mary Univ London, Sch Phys & Astron, Mile End Rd, London E1 4NS, England.;Univ Western Cape, Dept Phys & Astron, ZA-7535 Cape Town, South Africa..
    Kirkpatrick, C. C.
    Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland.;Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland..
    Legrand, L.
    Univ Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, Sao Paulo, Brazil..
    Libet, G.
    Ctr Spatial Toulouse, Ctr Natl Etud Spatiales, 18 Ave Edouard Belin, F-31401 Toulouse 9, France..
    Loureiro, A.
    Stockholm Univ, Oskar Klein Ctr Cosmoparticle Phys, Dept Phys, SE-10691 Stockholm, Sweden.;Imperial Coll London, Astrophys Grp, Blackett Lab, London SW7 2AZ, England..
    Macias-Perez, J.
    Univ Grenoble Alpes, CNRS, IN2P3, Grenoble INP,LPSC, 53 Ave Martyrs, F-38000 Grenoble, France..
    Maggio, G.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy..
    Magliocchetti, M.
    INAF, Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00100 Rome, Italy..
    Mannucci, F.
    INAF, Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy..
    Maoli, R.
    INAF, Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.;Sapienza Univ Roma, Dipartimento Fis, Piazzale Aldo Moro 2, I-00185 Rome, Italy..
    Martins, C. J. A. P.
    Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, PT-4150762 Porto, Portugal.;Univ Porto, Ctr Astrofis, Rua Estrelas, P-4150762 Porto, Portugal..
    Matthew, S.
    Univ Edinburgh, Royal Observ, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Maurin, L.
    Univ Paris Saclay, Inst Astrophys Spatiale, CNRS, F-91405 Orsay, France..
    Metcalf, R. B.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy..
    Migliaccio, M.
    Univ Roma Tor Vergata, Dipartimento Fis, Via Ric Sci 1, Rome, Italy.;Ist Nazl Fis Nucl, Sez Roma, Via Ric Sci 1, Rome, Italy..
    Monaco, P.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy.;Ist Nazl Fis Nucl, Sez Trieste, Via Valerio 2, I-34127 Trieste, Ts, Italy.;Univ Trieste, Dipartimento Fis, Sez Astron, Via Tiepolo 11, I-34131 Trieste, Italy..
    Moretti, C.
    Scuola Int Super Studi Avanzati, SISSA, Via Bonomea 265, I-34136 Trieste, Ts, Italy.;INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy.;Ist Nazl Fis Nucl, Sez Trieste, Via Valerio 2, I-34127 Trieste, Ts, Italy.;Ctr Nazl Ric High Performance Comp Big Data & Qua, ICSC, Via Magnanelli 2, Bologna, Italy..
    Morgante, G.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Nadathur, S.
    Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England..
    Walton, N. A.
    Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England..
    Patrizii, L.
    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Pezzotta, A.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Pontinen, M.
    Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland..
    Popa, V.
    Inst Space Sci, Str Atomistilor 409, Magurele 077125, Ilfov, Romania..
    Porciani, C.
    Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany..
    Potter, D.
    Univ Zurich, Dept Astrophys, Winterthurerstr 190, CH-8057 Zurich, Switzerland..
    Reimberg, P.
    Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France..
    Risso, I.
    Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy.;Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy..
    Rocci, P-F
    Univ Paris Saclay, Inst Astrophys Spatiale, CNRS, F-91405 Orsay, France..
    Sahlén, Martin
    Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Theoretical Astrophysics.
    Sanchez, A. G.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Schewtschenko, J. A.
    Univ Edinburgh, Royal Observ, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland..
    Sefusatti, E.
    INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.;Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy.;Ist Nazl Fis Nucl, Sez Trieste, Via Valerio 2, I-34127 Trieste, Ts, Italy..
    Sereno, M.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy.;Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Simon, P.
    Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany..
    Mancini, A. Spurio
    Royal Holloway Univ London, Dept Phys, Egham TW20 0EX, Surrey, England.;Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England..
    Steinwagner, J.
    Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany..
    Tao, C.
    Aix Marseille Univ, CNRS, CPPM, IN2P3, Marseille, France..
    Tessore, N.
    UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England..
    Testera, G.
    Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy..
    Teyssier, R.
    Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA..
    Toft, S.
    Cosm Dawn Ctr DAWN, Copenhagen, Denmark.;Univ Copenhagen, Niels Bohr Inst, Jagtvej 128, DK-2200 Copenhagen, Denmark..
    Tosi, S.
    Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy.;Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy.;INAF, Osservatorio Astron Brera, Via Brera 28, I-20122 Milan, Italy..
    Troja, A.
    INFN Padova, Via Marzolo 8, I-35131 Padua, Italy.;Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy..
    Tucci, M.
    Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland..
    Valieri, C.
    Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy..
    Valiviita, J.
    Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland.;Univ Helsinki, Dept Phys, POB 64, Helsinki 00014, Finland..
    Vergani, D.
    INAF, Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy..
    Verza, G.
    Flatiron Inst, Ctr Computat Astrophys, 162 5th Ave, New York, NY 10010 USA.;NYU, Ctr Cosmol & Particle Phys, Dept Phys, New York, NY 10003 USA..
    Euclid preparation: LVI. Sensitivity to non-standard particle dark matter models2025In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 693, article id A249Article in journal (Refereed)
    Abstract [en]

    The Euclid mission of the European Space Agency will provide weak gravitational lensing and galaxy clustering surveys that can be used to constrain the standard cosmological model and its extensions, with an opportunity to test the properties of dark matter beyond the minimal cold dark matter paradigm. We present forecasts from the combination of the Euclid weak lensing and photometric galaxy clustering data on the parameters describing four interesting and representative non-minimal dark matter models: a mixture of cold and warm dark matter relics; unstable dark matter decaying either into massless or massive relics; and dark matter undergoing feeble interactions with relativistic relics. We modelled these scenarios at the level of the non-linear matter power spectrum using emulators trained on dedicated N-body simulations. We used a mock Euclid likelihood and Monte Carlo Markov chains to fit mock data and infer error bars on dark matter parameters marginalised over other parameters. We find that the Euclid photometric probe (alone or in combination with cosmic microwave background data from the Planck satellite) will be sensitive to the effect of each of the four dark matter models considered here. The improvement will be particularly spectacular for decaying and interacting dark matter models. With Euclid, the bounds on some dark matter parameters can improve by up to two orders of magnitude compared to current limits. We discuss the dependence of predicted uncertainties on different assumptions: the inclusion of photometric galaxy clustering data, the minimum angular scale taken into account, and modelling of baryonic feedback effects. We conclude that the Euclid mission will be able to measure quantities related to the dark sector of particle physics with unprecedented sensitivity. This will provide important information for model building in high-energy physics. Any hint of a deviation from the minimal cold dark matter paradigm would have profound implications for cosmology and particle physics.

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  • Public defence: 2025-06-10 13:15 Lecture Hall 1 – Ekonomikum, Uppsala
    Hussain, Amin
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Social Sciences, Department of Economics.
    Optimizing Healthcare Payments: Regulation, Payment Schemes and Value-Adjustment2025Doctoral thesis, monograph (Other academic)
    Abstract [en]

    Essay I:First-Degree Price Discrimination achieves efficiency in monopoly settings by having the producer appropriate the total surplus, while uniform pricing leads to higher consumer surplus but is inefficient. The market for multi-indication drugs – those that have multiple uses – has two features that distinguish it from a static monopoly model. Firstly, the monopoly is time-bound and is followed by a competitive market. Secondly, manufacturers have private information about which groups of patients their drug could be useful for and must incur a cost to reveal each one. I extend Bergemann et. al (2015) to this setting to develop a mechanism which maximises consumer surplus and achieves weakly higher efficiency than First-Degree Price Discrimination (which can be inefficient as the monopolist does not internalise the long-term benefit). By conditioning market segmentation on the manufacturer's revealed information, a regulator can incentivise it to conduct costly trials for the most socially beneficial uses of their drugs and maximise achievable total and consumer surplus. Ex-post, First-Degree Price Discrimination may appear as a specific case as a result of the segmentation - as such, I reveal conditions under which First-Degree Price Discrimination may be efficient. I also provide solutions for achieving market segmentation that minimizes variance in prices or individual consumer surplus while still achieving the primary aims of maximising achievable surplus. In doing so I make the case for regulators to use market segmentation as a tool to provide incentives for manufacturers. 

    Essay II: Advanced Therapy Medicinal Products (ATMPs) are novel, expensive, one-time treatments that have the potential to cure certain medical conditions, but their long-term effectiveness carries inherent risk. Risk-sharing agreements (RSAs) have been proposed as a means to mitigate the negative impacts of this uncertainty. However, traditional models of RSAs often fail to account for the irreversibility of ATMPs and their long-term implications for payers’ budgets and future decision-making, as well as the fact that payers and manufacturer interact repeatedly. 

    In this paper, I develop a model in which a payer and a manufacturer engage in an infinitely repeated stochastic game. Patients arrive following an overlapping-generations framework, and the price of treatment is negotiated based on the state of the budget and population health. Effective ATMPs free up resources in the budget for future incoming patients and increase demand. The outcomes of this game are analysed under two distinct payment structures: one where payments are made upfront for each patient and another where payments are contingent on the continued effectiveness of the ATMP. Results show that when the health benefits of the ATMP are comparable to those of an outside option, the RSA improves efficiency. However, when the health benefits of the ATMP are significantly higher, the efficiency of upfront payment can improve.

    Essay III: (with Erik Grönqvist, Per Johansson and August Wadell Leimdörfer)How should limited resources for health care be prioritized? Health economic evaluation can inform decision makers if new medical treatments are good value for money. The standard cost-effectiveness framework maximizes QALY gains without considering the distribution of these gains across individuals or groups. However, the way health is produced matters for most people. With general preferences for equity in society, also disease severity would matter for welfare when prioritizing. With public preferences over both disease severity and cost-effectiveness, and policymakers need to balance equity with efficiency. We provide evidence for how the public trades disease severity for cost-effectiveness from a novel striped-down discrete choice experiment, and we also provide a method for adjusting the ICER threshold to account for disease severity.

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  • Andersson, Evelina
    et al.
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Educational Sciences, Department of Education.
    Ceder, Ida
    Uppsala University, Disciplinary Domain of Humanities and Social Sciences, Faculty of Educational Sciences, Department of Education.
    Konkret material i matematikundervisningen: En intervjustudie om lärares upplevelser kring tillgången av konkret material2025Independent thesis Basic level (professional degree), 10 credits / 15 HE creditsStudent thesis
    Abstract [sv]

    Studiens syfte är att undersöka lärares upplevelser kring tillgången till konkret material på sex olika skolor i Uppsala län, samt i vilken utsträckning och på vilket sätt deras elever får tillgång till konkret material i årskurs 1. Vidare syftar studien till att analysera hur lärare interagerar med och använder det konkreta materialet som ett medierande redskap i undervisningspraktiken. Med särskilt fokus på dess betydelse för elevers lärande och förståelse av matematiska områden. För att besvara dessa frågor genomförs semistrukturerade intervjuer med sex behöriga lärare. I intervjuerna undersöker vi hur de arbetar med konkret material i klassrummet, hur tillgången ser ut på skolnivå samt vilka elever som får tillgången till att använda konkret material. Det insamlade materialet analyseras genom tematisk analys med utgångspunkt i sociokulturella perspektivet. Resultatet vi fick fram i studien var att alla elever hade tillgång till att använda allt konkret material i början av årskurs 1. Dock framkom det att det var framförallt elever med matematiksvårigheter som regelbundet fick tillgång till materialet under hela läsåret. Tillgången till materialet på skolorna var generellt bra och majoriteten av de undersökta skolorna hade en bra uppsättning av konkret material. I diskussionen belyser vi bland annat hur konkret material fungerar som ett medierande redskap i undervisningen, samt den positiva påverkan konkret material har på lärandet för att det aktiverar flera sinnen.

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