[{"article_processing_charge":"No","publisher":"Figshare","oa":1,"ddc":["550"],"abstract":[{"lang":"eng","text":"This zip file contains data, and analysis for the paper \"Elucidating the role of water in collagen self-assembly by isotopically modulating collagen hydration\"."}],"date_updated":"2025-09-04T13:03:56Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","main_file_link":[{"url":"https://doi.org/10.21942/UVA.24829896","open_access":"1"}],"oa_version":"Published Version","date_created":"2024-03-19T10:47:16Z","related_material":{"record":[{"status":"public","relation":"used_in_publication","id":"15116"}]},"month":"02","type":"research_data_reference","title":"Dataset Collagen Self Assembly in H2O and D2O","status":"public","extern":"1","year":"2024","_id":"15126","date_published":"2024-02-14T00:00:00Z","citation":{"ieee":"G. Giubertoni and S. Woutersen, “Dataset Collagen Self Assembly in H2O and D2O.” Figshare, 2024.","apa":"Giubertoni, G., &#38; Woutersen, S. (2024). Dataset Collagen Self Assembly in H2O and D2O. Figshare. <a href=\"https://doi.org/10.21942/UVA.24829896\">https://doi.org/10.21942/UVA.24829896</a>","ama":"Giubertoni G, Woutersen S. Dataset Collagen Self Assembly in H2O and D2O. 2024. doi:<a href=\"https://doi.org/10.21942/UVA.24829896\">10.21942/UVA.24829896</a>","ista":"Giubertoni G, Woutersen S. 2024. Dataset Collagen Self Assembly in H2O and D2O, Figshare, <a href=\"https://doi.org/10.21942/UVA.24829896\">10.21942/UVA.24829896</a>.","mla":"Giubertoni, G., and S. Woutersen. <i>Dataset Collagen Self Assembly in H2O and D2O</i>. Figshare, 2024, doi:<a href=\"https://doi.org/10.21942/UVA.24829896\">10.21942/UVA.24829896</a>.","short":"G. Giubertoni, S. Woutersen, (2024).","chicago":"Giubertoni, G., and S. Woutersen. “Dataset Collagen Self Assembly in H2O and D2O.” Figshare, 2024. <a href=\"https://doi.org/10.21942/UVA.24829896\">https://doi.org/10.21942/UVA.24829896</a>."},"doi":"10.21942/UVA.24829896","tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"day":"14","author":[{"first_name":"G.","full_name":"Giubertoni, G.","last_name":"Giubertoni"},{"first_name":"S.","full_name":"Woutersen, S.","last_name":"Woutersen"}],"has_accepted_license":"1"},{"department":[{"_id":"FlSc"},{"_id":"MiSi"},{"_id":"Bio"},{"_id":"EM-Fac"}],"isi":1,"ddc":["570"],"scopus_import":"1","article_processing_charge":"Yes (via OA deal)","month":"03","type":"journal_article","oa_version":"Published Version","tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"day":"20","doi":"10.1083/jcb.202309125","publication_identifier":{"issn":["0021-9525"],"eissn":["1540-8140"]},"volume":223,"project":[{"_id":"9B954C5C-BA93-11EA-9121-9846C619BF3A","grant_number":"P33367","name":"Structure and isoform diversity of the Arp2/3 complex"},{"_id":"7bd318a1-9f16-11ee-852c-cc9217763180","grant_number":"E435","name":"In Situ Actin Structures via Hybrid Cryo-electron Microscopy"},{"_id":"25FE9508-B435-11E9-9278-68D0E5697425","grant_number":"724373","name":"Cellular Navigation Along Spatial Gradients","call_identifier":"H2020"},{"_id":"059B463C-7A3F-11EA-A408-12923DDC885E","name":"NÃ-Fonds Preis fÃ¼r die Jungforscherin des Jahres am IST Austria"},{"_id":"2615199A-B435-11E9-9278-68D0E5697425","name":"Spatiotemporal regulation of chemokine-induced signalling in leukocyte chemotaxis","grant_number":"21317"},{"_id":"62909c6f-2b32-11ec-9570-e1476aab5308","grant_number":"CZI01","name":"CryoMinflux-guided in-situ visual proteomics and structure determination"}],"_id":"15146","article_type":"original","article_number":"e202309125","abstract":[{"text":"The extracellular matrix (ECM) serves as a scaffold for cells and plays an essential role in regulating numerous cellular processes, including cell migration and proliferation. Due to limitations in specimen preparation for conventional room-temperature electron microscopy, we lack structural knowledge on how ECM components are secreted, remodeled, and interact with surrounding cells. We have developed a 3D-ECM platform compatible with sample thinning by cryo-focused ion beam milling, the lift-out extraction procedure, and cryo-electron tomography. Our workflow implements cell-derived matrices (CDMs) grown on EM grids, resulting in a versatile tool closely mimicking ECM environments. This allows us to visualize ECM for the first time in its hydrated, native context. Our data reveal an intricate network of extracellular fibers, their positioning relative to matrix-secreting cells, and previously unresolved structural entities. Our workflow and results add to the structural atlas of the ECM, providing novel insights into its secretion and assembly.","lang":"eng"}],"file":[{"date_updated":"2024-03-25T12:52:04Z","access_level":"open_access","file_id":"15188","date_created":"2024-03-25T12:52:04Z","success":1,"file_size":11907016,"file_name":"2024_JCB_Zens.pdf","creator":"dernst","checksum":"90d1984a93660735e506c2a304bc3f73","content_type":"application/pdf","relation":"main_file"}],"oa":1,"publisher":"Rockefeller University Press","ec_funded":1,"publication":"Journal of Cell Biology","title":"Lift-out cryo-FIBSEM and cryo-ET reveal the ultrastructural landscape of extracellular matrix","acknowledgement":"Open Access funding provided by IST Austria. We thank Armel Nicolas and his team at the ISTA proteomics facility, Alois Schloegl, Stefano Elefante, and colleagues at the ISTA Scientific Computing facility, Tommaso Constanzo and Ludek Lovicar at the Electron Microsocpy Facility (EMF), and Thomas Menner at the Miba Machine shop for their support. We also thank Wanda Kukulski (University of Bern) as well as Darío Porley, Andreas Thader, and other members of the Schur group for helpful discussions. Matt Swulius and Jessica Heebner provided great support in using Dragonfly. We thank Dorotea Fracciolla (Art & Science) for support in figure illustration.\r\n\r\nThis research was supported by the Scientific Service Units of ISTA through resources provided by Scientific Computing, the Lab Support Facility, and the Electron Microscopy Facility. We acknowledge funding support from the following sources: Austrian Science Fund (FWF) grant P33367 (to F.K.M. Schur), the Federation of European Biochemical Societies (to F.K.M. Schur), Niederösterreich (NÖ) Fonds (to B. Zens), FWF grant E435 (to J.M. Hansen), European Research Council under the European Union’s Horizon 2020 research (grant agreement No. 724373) (to M. Sixt), and Jenny and Antti Wihuri Foundation (to J. Alanko). This publication has been made possible in part by CZI grant DAF2021-234754 and grant DOI https://doi.org/10.37921/812628ebpcwg from the Chan Zuckerberg Initiative DAF, an advised fund of Silicon Valley Community Foundation (to F.K.M. Schur).","date_created":"2024-03-21T06:45:51Z","date_updated":"2025-09-04T13:17:16Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","pmid":1,"language":[{"iso":"eng"}],"external_id":{"isi":["001264190100001"],"pmid":["38506714"]},"acknowledged_ssus":[{"_id":"LifeSc"},{"_id":"ScienComp"},{"_id":"EM-Fac"},{"_id":"M-Shop"}],"quality_controlled":"1","file_date_updated":"2024-03-25T12:52:04Z","corr_author":"1","citation":{"mla":"Zens, Bettina, et al. “Lift-out Cryo-FIBSEM and Cryo-ET Reveal the Ultrastructural Landscape of Extracellular Matrix.” <i>Journal of Cell Biology</i>, vol. 223, no. 6, e202309125, Rockefeller University Press, 2024, doi:<a href=\"https://doi.org/10.1083/jcb.202309125\">10.1083/jcb.202309125</a>.","ista":"Zens B, Fäßler F, Hansen J, Hauschild R, Datler J, Hodirnau V-V, Zheden V, Alanko JH, Sixt MK, Schur FK. 2024. Lift-out cryo-FIBSEM and cryo-ET reveal the ultrastructural landscape of extracellular matrix. Journal of Cell Biology. 223(6), e202309125.","apa":"Zens, B., Fäßler, F., Hansen, J., Hauschild, R., Datler, J., Hodirnau, V.-V., … Schur, F. K. (2024). Lift-out cryo-FIBSEM and cryo-ET reveal the ultrastructural landscape of extracellular matrix. <i>Journal of Cell Biology</i>. Rockefeller University Press. <a href=\"https://doi.org/10.1083/jcb.202309125\">https://doi.org/10.1083/jcb.202309125</a>","ieee":"B. Zens <i>et al.</i>, “Lift-out cryo-FIBSEM and cryo-ET reveal the ultrastructural landscape of extracellular matrix,” <i>Journal of Cell Biology</i>, vol. 223, no. 6. Rockefeller University Press, 2024.","ama":"Zens B, Fäßler F, Hansen J, et al. Lift-out cryo-FIBSEM and cryo-ET reveal the ultrastructural landscape of extracellular matrix. <i>Journal of Cell Biology</i>. 2024;223(6). doi:<a href=\"https://doi.org/10.1083/jcb.202309125\">10.1083/jcb.202309125</a>","chicago":"Zens, Bettina, Florian Fäßler, Jesse Hansen, Robert Hauschild, Julia Datler, Victor-Valentin Hodirnau, Vanessa Zheden, Jonna H Alanko, Michael K Sixt, and Florian KM Schur. “Lift-out Cryo-FIBSEM and Cryo-ET Reveal the Ultrastructural Landscape of Extracellular Matrix.” <i>Journal of Cell Biology</i>. Rockefeller University Press, 2024. <a href=\"https://doi.org/10.1083/jcb.202309125\">https://doi.org/10.1083/jcb.202309125</a>.","short":"B. Zens, F. Fäßler, J. Hansen, R. Hauschild, J. Datler, V.-V. Hodirnau, V. Zheden, J.H. Alanko, M.K. Sixt, F.K. Schur, Journal of Cell Biology 223 (2024)."},"status":"public","publication_status":"published","year":"2024","date_published":"2024-03-20T00:00:00Z","has_accepted_license":"1","author":[{"last_name":"Zens","first_name":"Bettina","full_name":"Zens, Bettina","orcid":"0000-0002-9561-1239","id":"45FD126C-F248-11E8-B48F-1D18A9856A87"},{"last_name":"Fäßler","first_name":"Florian","full_name":"Fäßler, Florian","id":"404F5528-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-7149-769X"},{"first_name":"Jesse","orcid":"0000-0001-7967-2085","id":"1063c618-6f9b-11ec-9123-f912fccded63","full_name":"Hansen, Jesse","last_name":"Hansen"},{"first_name":"Robert","orcid":"0000-0001-9843-3522","full_name":"Hauschild, Robert","id":"4E01D6B4-F248-11E8-B48F-1D18A9856A87","last_name":"Hauschild"},{"full_name":"Datler, Julia","orcid":"0000-0002-3616-8580","id":"3B12E2E6-F248-11E8-B48F-1D18A9856A87","first_name":"Julia","last_name":"Datler"},{"last_name":"Hodirnau","first_name":"Victor-Valentin","id":"3661B498-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0003-3904-947X","full_name":"Hodirnau, Victor-Valentin"},{"orcid":"0000-0002-9438-4783","id":"39C5A68A-F248-11E8-B48F-1D18A9856A87","full_name":"Zheden, Vanessa","first_name":"Vanessa","last_name":"Zheden"},{"first_name":"Jonna H","full_name":"Alanko, Jonna H","orcid":"0000-0002-7698-3061","id":"2CC12E8C-F248-11E8-B48F-1D18A9856A87","last_name":"Alanko"},{"last_name":"Sixt","first_name":"Michael K","id":"41E9FBEA-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-6620-9179","full_name":"Sixt, Michael K"},{"full_name":"Schur, Florian KM","id":"48AD8942-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0003-4790-8078","first_name":"Florian KM","last_name":"Schur"}],"issue":"6","intvolume":"       223"},{"language":[{"iso":"eng"}],"external_id":{"isi":["001226893800001"],"arxiv":["2301.11615"]},"quality_controlled":"1","citation":{"mla":"Campbell, Rutger, et al. “Decompositions into Two Linear Forests of Bounded Lengths.” <i>Discrete Mathematics</i>, vol. 347, no. 6, 113962, Elsevier, 2024, doi:<a href=\"https://doi.org/10.1016/j.disc.2024.113962\">10.1016/j.disc.2024.113962</a>.","ista":"Campbell R, Hörsch F, Moore B. 2024. Decompositions into two linear forests of bounded lengths. Discrete Mathematics. 347(6), 113962.","apa":"Campbell, R., Hörsch, F., &#38; Moore, B. (2024). Decompositions into two linear forests of bounded lengths. <i>Discrete Mathematics</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.disc.2024.113962\">https://doi.org/10.1016/j.disc.2024.113962</a>","ieee":"R. Campbell, F. Hörsch, and B. Moore, “Decompositions into two linear forests of bounded lengths,” <i>Discrete Mathematics</i>, vol. 347, no. 6. Elsevier, 2024.","ama":"Campbell R, Hörsch F, Moore B. Decompositions into two linear forests of bounded lengths. <i>Discrete Mathematics</i>. 2024;347(6). doi:<a href=\"https://doi.org/10.1016/j.disc.2024.113962\">10.1016/j.disc.2024.113962</a>","chicago":"Campbell, Rutger, Florian Hörsch, and Benjamin Moore. “Decompositions into Two Linear Forests of Bounded Lengths.” <i>Discrete Mathematics</i>. Elsevier, 2024. <a href=\"https://doi.org/10.1016/j.disc.2024.113962\">https://doi.org/10.1016/j.disc.2024.113962</a>.","short":"R. Campbell, F. Hörsch, B. Moore, Discrete Mathematics 347 (2024)."},"corr_author":"1","publication_status":"published","status":"public","date_published":"2024-06-01T00:00:00Z","year":"2024","author":[{"first_name":"Rutger","full_name":"Campbell, Rutger","last_name":"Campbell"},{"first_name":"Florian","full_name":"Hörsch, Florian","last_name":"Hörsch"},{"first_name":"Benjamin","full_name":"Moore, Benjamin","id":"6dc1a1be-bf1c-11ed-8d2b-d044840f49d6","last_name":"Moore"}],"issue":"6","intvolume":"       347","abstract":[{"text":"For some k∈Z≥0∪{∞}, we call a linear forest k-bounded if each of its components has at most k edges. We will say a (k,ℓ)-bounded linear forest decomposition of a graph G is a partition of E(G) into the edge sets of two linear forests Fk,Fℓ where Fk is k-bounded and Fℓ is ℓ-bounded. We show that the problem of deciding whether a given graph has such a decomposition is NP-complete if both k and ℓ are at least 2, NP-complete if k≥9 and ℓ=1, and is in P for (k,ℓ)=(2,1). Before this, the only known NP-complete cases were the (2,2) and (3,3) cases. Our hardness result answers a question of Bermond et al. from 1984. We also show that planar graphs of girth at least nine decompose into a linear forest and a matching, which in particular is stronger than 3-edge-colouring such graphs.","lang":"eng"}],"oa":1,"publisher":"Elsevier","publication":"Discrete Mathematics","title":"Decompositions into two linear forests of bounded lengths","acknowledgement":"We wish to thank Dániel Marx and András Sebő for making us aware of the results in [8] and some clarifications on them.","date_created":"2024-03-24T23:00:58Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_updated":"2025-09-04T13:10:26Z","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2301.11615"}],"arxiv":1,"day":"01","doi":"10.1016/j.disc.2024.113962","publication_identifier":{"issn":["0012-365X"]},"volume":347,"_id":"15163","article_type":"original","article_number":"113962","department":[{"_id":"MaKw"}],"isi":1,"scopus_import":"1","article_processing_charge":"No","month":"06","type":"journal_article","oa_version":"Preprint"},{"article_number":"104143","article_type":"original","volume":126,"_id":"15164","day":"01","tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"doi":"10.1016/j.medengphy.2024.104143","publication_identifier":{"eissn":["1873-4030"],"issn":["1350-4533"]},"month":"04","type":"journal_article","oa_version":"Published Version","article_processing_charge":"Yes (in subscription journal)","department":[{"_id":"PreCl"}],"isi":1,"ddc":["610"],"scopus_import":"1","author":[{"last_name":"Silva-Henao","full_name":"Silva-Henao, Juan D.","first_name":"Juan D."},{"last_name":"Schober","first_name":"Sophie","id":"80b0a0ef-4b9f-11ec-b119-8d9d94c4a1d8","full_name":"Schober, Sophie"},{"first_name":"Dieter H.","full_name":"Pahr, Dieter H.","last_name":"Pahr"},{"first_name":"Andreas G.","full_name":"Reisinger, Andreas G.","last_name":"Reisinger"}],"intvolume":"       126","has_accepted_license":"1","citation":{"ieee":"J. D. Silva-Henao, S. Schober, D. H. Pahr, and A. G. Reisinger, “Critical loss of primary implant stability in osteosynthesis locking screws under cyclic overloading,” <i>Medical Engineering and Physics</i>, vol. 126. Elsevier, 2024.","apa":"Silva-Henao, J. D., Schober, S., Pahr, D. H., &#38; Reisinger, A. G. (2024). Critical loss of primary implant stability in osteosynthesis locking screws under cyclic overloading. <i>Medical Engineering and Physics</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.medengphy.2024.104143\">https://doi.org/10.1016/j.medengphy.2024.104143</a>","ama":"Silva-Henao JD, Schober S, Pahr DH, Reisinger AG. Critical loss of primary implant stability in osteosynthesis locking screws under cyclic overloading. <i>Medical Engineering and Physics</i>. 2024;126. doi:<a href=\"https://doi.org/10.1016/j.medengphy.2024.104143\">10.1016/j.medengphy.2024.104143</a>","ista":"Silva-Henao JD, Schober S, Pahr DH, Reisinger AG. 2024. Critical loss of primary implant stability in osteosynthesis locking screws under cyclic overloading. Medical Engineering and Physics. 126, 104143.","mla":"Silva-Henao, Juan D., et al. “Critical Loss of Primary Implant Stability in Osteosynthesis Locking Screws under Cyclic Overloading.” <i>Medical Engineering and Physics</i>, vol. 126, 104143, Elsevier, 2024, doi:<a href=\"https://doi.org/10.1016/j.medengphy.2024.104143\">10.1016/j.medengphy.2024.104143</a>.","short":"J.D. Silva-Henao, S. Schober, D.H. Pahr, A.G. Reisinger, Medical Engineering and Physics 126 (2024).","chicago":"Silva-Henao, Juan D., Sophie Schober, Dieter H. Pahr, and Andreas G. Reisinger. “Critical Loss of Primary Implant Stability in Osteosynthesis Locking Screws under Cyclic Overloading.” <i>Medical Engineering and Physics</i>. Elsevier, 2024. <a href=\"https://doi.org/10.1016/j.medengphy.2024.104143\">https://doi.org/10.1016/j.medengphy.2024.104143</a>."},"file_date_updated":"2024-03-25T08:29:52Z","status":"public","publication_status":"published","year":"2024","date_published":"2024-04-01T00:00:00Z","external_id":{"isi":["001219145400001"],"pmid":["38621845"]},"language":[{"iso":"eng"}],"quality_controlled":"1","date_updated":"2025-09-04T13:11:03Z","pmid":1,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publication":"Medical Engineering and Physics","title":"Critical loss of primary implant stability in osteosynthesis locking screws under cyclic overloading","acknowledgement":"The authors declare no conflict of interest related to this study. This project was funded by the Gesellschaft fuer Forschungsfoerderung Niederoesterreich m.b.H. Life Science Call 2017 Grant No. LS17004 and Science call 2019 Dissertationen Grant No. SC19014. No ethical approval was required for this study.","date_created":"2024-03-24T23:00:58Z","publisher":"Elsevier","abstract":[{"lang":"eng","text":"Primary implant stability, which refers to the stability of the implant during the initial healing period is a crucial factor in determining the long-term success of the implant and lays the foundation for secondary implant stability achieved through osseointegration. Factors affecting primary stability include implant design, surgical technique, and patient-specific factors like bone quality and morphology. In vivo, the cyclic nature of anatomical loading puts osteosynthesis locking screws under dynamic loads, which can lead to the formation of micro cracks and defects that slowly degrade the mechanical connection between the bone and screw, thus compromising the initial stability and secondary stability of the implant. Monotonic quasi-static loading used for testing the holding capacity of implanted screws is not well suited to capture this behavior since it cannot capture the progressive deterioration of peri‑implant bone at small displacements. In order to address this issue, this study aims to determine a critical point of loss of primary implant stability in osteosynthesis locking screws under cyclic overloading by investigating the evolution of damage, dissipated energy, and permanent deformation. A custom-made test setup was used to test implanted 2.5 mm locking screws under cyclic overloading test. For each loading cycle, maximum forces and displacement were recorded as well as initial and final cycle displacements and used to calculate damage and energy dissipation evolution. The results of this study demonstrate that for axial, shear, and mixed loading significant damage and energy dissipation can be observed at approximately 20 % of the failure force. Additionally, at this load level, permanent deformations on the screw-bone interface were found to be in the range of 50 to 150 mm which promotes osseointegration and secondary implant stability. This research can assist surgeons in making informed preoperative decisions by providing a better understanding of the critical point of loss of primary implant stability, thus improving the long-term success of the implant and overall patient satisfaction."}],"file":[{"checksum":"974acbf2731e7382dcf5920ac762e551","content_type":"application/pdf","relation":"main_file","file_name":"2024_MedEngineeringPhysics_SilvaHenao.pdf","file_size":10039402,"creator":"dernst","success":1,"date_created":"2024-03-25T08:29:52Z","file_id":"15177","access_level":"open_access","date_updated":"2024-03-25T08:29:52Z"}],"oa":1},{"year":"2024","date_published":"2024-03-16T00:00:00Z","publication_status":"published","status":"public","OA_type":"gold","citation":{"short":"B.B. GOSWAMI, Geophysical Research Letters 51 (2024).","chicago":"GOSWAMI, BIDYUT B. “A Pre-Monsoon Signal of False Alarms of Indian Monsoon Droughts.” <i>Geophysical Research Letters</i>. Wiley, 2024. <a href=\"https://doi.org/10.1029/2023GL106569\">https://doi.org/10.1029/2023GL106569</a>.","ieee":"B. B. GOSWAMI, “A pre-monsoon signal of false alarms of Indian monsoon droughts,” <i>Geophysical Research Letters</i>, vol. 51, no. 5. Wiley, 2024.","ama":"GOSWAMI BB. A pre-monsoon signal of false alarms of Indian monsoon droughts. <i>Geophysical Research Letters</i>. 2024;51(5). doi:<a href=\"https://doi.org/10.1029/2023GL106569\">10.1029/2023GL106569</a>","apa":"GOSWAMI, B. B. (2024). A pre-monsoon signal of false alarms of Indian monsoon droughts. <i>Geophysical Research Letters</i>. Wiley. <a href=\"https://doi.org/10.1029/2023GL106569\">https://doi.org/10.1029/2023GL106569</a>","ista":"GOSWAMI BB. 2024. A pre-monsoon signal of false alarms of Indian monsoon droughts. Geophysical Research Letters. 51(5), e2023GL106569.","mla":"GOSWAMI, BIDYUT B. “A Pre-Monsoon Signal of False Alarms of Indian Monsoon Droughts.” <i>Geophysical Research Letters</i>, vol. 51, no. 5, e2023GL106569, Wiley, 2024, doi:<a href=\"https://doi.org/10.1029/2023GL106569\">10.1029/2023GL106569</a>."},"corr_author":"1","file_date_updated":"2024-03-25T08:36:00Z","quality_controlled":"1","language":[{"iso":"eng"}],"external_id":{"isi":["001181635700001"]},"intvolume":"        51","issue":"5","author":[{"id":"3a4ac09c-6d61-11ec-bf66-884cde66b64b","full_name":"Goswami, Bidyut B","orcid":"0000-0001-8602-3083","first_name":"Bidyut B","last_name":"Goswami"}],"has_accepted_license":"1","ec_funded":1,"publisher":"Wiley","oa":1,"abstract":[{"text":"Current knowledge suggests a drought Indian monsoon (perhaps a severe one) when the El Nino Southern Oscillation and Pacific Decadal Oscillation each exhibit positive phases (a joint positive phase). For the monsoons, which are exceptions in this regard, we found northeast India often gets excess pre-monsoon rainfall. Further investigation reveals that this excess pre-monsoon rainfall is produced by the interaction of the large-scale circulation associated with the joint phase with the mountains in northeast India. We posit that a warmer troposphere, a consequence of excess rainfall over northeast India, drives a stronger monsoon circulation and enhances monsoon rainfall over central India. Hence, we argue that pre-monsoon rainfall over northeast India can be used for seasonal monsoon rainfall prediction over central India. Most importantly, its predictive value is at its peak when the Pacific Ocean exhibits a joint positive phase and the threat of extreme drought monsoon looms over India.","lang":"eng"}],"OA_place":"publisher","file":[{"creator":"dernst","file_name":"2024_GeophysResLetters_Goswami.pdf","file_size":2887134,"relation":"main_file","content_type":"application/pdf","checksum":"243bd966aca968ec7d9e474af8639f8d","access_level":"open_access","date_updated":"2024-03-25T08:36:00Z","date_created":"2024-03-25T08:36:00Z","file_id":"15178","success":1}],"date_updated":"2025-09-04T13:11:41Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_created":"2024-03-24T23:00:58Z","acknowledgement":"The author gratefully acknowledges ISTA for supporting this research through funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (Project CLUSTER, grant agreement No. 805041).","title":"A pre-monsoon signal of false alarms of Indian monsoon droughts","publication":"Geophysical Research Letters","_id":"15165","project":[{"grant_number":"805041","name":"Organization of CLoUdS, and implications of Tropical  cyclones and for the Energetics of the tropics, in current and waRming climate","_id":"629205d8-2b32-11ec-9570-e1356ff73576","call_identifier":"H2020"}],"volume":51,"publication_identifier":{"eissn":["1944-8007"],"issn":["0094-8276"]},"tmp":{"name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)","short":"CC BY-NC-ND (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","image":"/images/cc_by_nc_nd.png"},"day":"16","doi":"10.1029/2023GL106569","article_number":"e2023GL106569","article_type":"original","article_processing_charge":"Yes","scopus_import":"1","ddc":["550"],"isi":1,"department":[{"_id":"CaMu"}],"oa_version":"Published Version","APC_amount":"1470 EUR","DOAJ_listed":"1","type":"journal_article","month":"03"},{"date_created":"2024-03-24T23:00:58Z","acknowledgement":"The authors thank the Werner-Siemens-Stiftung and the Institute of Science and Technology Austria for financial support.","title":"Electron highways are cooler","publication":"Science","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_updated":"2025-09-04T13:12:19Z","pmid":1,"abstract":[{"text":"Reducing defects boosts room-temperature performance of a thermoelectric device","lang":"eng"}],"publisher":"American Association for the Advancement of Science","intvolume":"       383","issue":"6688","author":[{"first_name":"Navita","id":"6ebe278d-ba0b-11ee-8184-f34cdc671de4","full_name":"Navita, Navita","orcid":"0000-0001-7408-8197","last_name":"Navita"},{"orcid":"0000-0001-5013-2843","full_name":"Ibáñez, Maria","id":"43C61214-F248-11E8-B48F-1D18A9856A87","first_name":"Maria","last_name":"Ibáñez"}],"quality_controlled":"1","language":[{"iso":"eng"}],"external_id":{"pmid":["38484066"],"isi":["001273082800019"]},"date_published":"2024-03-14T00:00:00Z","year":"2024","status":"public","publication_status":"published","corr_author":"1","citation":{"ieee":"N. Jakhar and M. Ibáñez, “Electron highways are cooler,” <i>Science</i>, vol. 383, no. 6688. American Association for the Advancement of Science, p. 1184, 2024.","apa":"Jakhar, N., &#38; Ibáñez, M. (2024). Electron highways are cooler. <i>Science</i>. American Association for the Advancement of Science. <a href=\"https://doi.org/10.1126/science.ado4077\">https://doi.org/10.1126/science.ado4077</a>","ama":"Jakhar N, Ibáñez M. Electron highways are cooler. <i>Science</i>. 2024;383(6688):1184. doi:<a href=\"https://doi.org/10.1126/science.ado4077\">10.1126/science.ado4077</a>","ista":"Jakhar N, Ibáñez M. 2024. Electron highways are cooler. Science. 383(6688), 1184.","mla":"Jakhar, Navita, and Maria Ibáñez. “Electron Highways Are Cooler.” <i>Science</i>, vol. 383, no. 6688, American Association for the Advancement of Science, 2024, p. 1184, doi:<a href=\"https://doi.org/10.1126/science.ado4077\">10.1126/science.ado4077</a>.","short":"N. Jakhar, M. Ibáñez, Science 383 (2024) 1184.","chicago":"Jakhar, Navita, and Maria Ibáñez. “Electron Highways Are Cooler.” <i>Science</i>. American Association for the Advancement of Science, 2024. <a href=\"https://doi.org/10.1126/science.ado4077\">https://doi.org/10.1126/science.ado4077</a>."},"oa_version":"None","type":"journal_article","month":"03","scopus_import":"1","isi":1,"department":[{"_id":"MaIb"}],"page":"1184","article_processing_charge":"No","article_type":"letter_note","publication_identifier":{"issn":["0036-8075"],"eissn":["1095-9203"]},"doi":"10.1126/science.ado4077","day":"14","_id":"15166","project":[{"_id":"9B8F7476-BA93-11EA-9121-9846C619BF3A","name":"HighTE: The Werner Siemens Laboratory for the High Throughput Discovery of Semiconductors for Waste Heat Recovery"}],"volume":383},{"volume":109,"_id":"15167","publication_identifier":{"eissn":["2469-9934"],"issn":["2469-9926"]},"day":"19","doi":"10.1103/PhysRevA.109.033315","article_number":"033315","article_type":"original","article_processing_charge":"No","isi":1,"scopus_import":"1","department":[{"_id":"MiLe"}],"oa_version":"Preprint","month":"03","type":"journal_article","status":"public","publication_status":"published","date_published":"2024-03-19T00:00:00Z","year":"2024","citation":{"chicago":"Al Hyder, Ragheed, F. Chevy, and X. Leyronas. “Exploring Beyond-Mean-Field Logarithmic Divergences in Fermi-Polaron Energy.” <i>Physical Review A</i>. American Physical Society, 2024. <a href=\"https://doi.org/10.1103/PhysRevA.109.033315\">https://doi.org/10.1103/PhysRevA.109.033315</a>.","short":"R. Al Hyder, F. Chevy, X. Leyronas, Physical Review A 109 (2024).","mla":"Al Hyder, Ragheed, et al. “Exploring Beyond-Mean-Field Logarithmic Divergences in Fermi-Polaron Energy.” <i>Physical Review A</i>, vol. 109, no. 3, 033315, American Physical Society, 2024, doi:<a href=\"https://doi.org/10.1103/PhysRevA.109.033315\">10.1103/PhysRevA.109.033315</a>.","ama":"Al Hyder R, Chevy F, Leyronas X. Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy. <i>Physical Review A</i>. 2024;109(3). doi:<a href=\"https://doi.org/10.1103/PhysRevA.109.033315\">10.1103/PhysRevA.109.033315</a>","ieee":"R. Al Hyder, F. Chevy, and X. Leyronas, “Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy,” <i>Physical Review A</i>, vol. 109, no. 3. American Physical Society, 2024.","apa":"Al Hyder, R., Chevy, F., &#38; Leyronas, X. (2024). Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy. <i>Physical Review A</i>. American Physical Society. <a href=\"https://doi.org/10.1103/PhysRevA.109.033315\">https://doi.org/10.1103/PhysRevA.109.033315</a>","ista":"Al Hyder R, Chevy F, Leyronas X. 2024. Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy. Physical Review A. 109(3), 033315."},"corr_author":"1","quality_controlled":"1","external_id":{"isi":["001198511300017"],"arxiv":["2311.14536"]},"language":[{"iso":"eng"}],"issue":"3","intvolume":"       109","author":[{"last_name":"Al Hyder","full_name":"Al Hyder, Ragheed","id":"d1c405be-ae15-11ed-8510-ccf53278162e","first_name":"Ragheed"},{"first_name":"F.","full_name":"Chevy, F.","last_name":"Chevy"},{"full_name":"Leyronas, X.","first_name":"X.","last_name":"Leyronas"}],"publisher":"American Physical Society","oa":1,"abstract":[{"lang":"eng","text":"We perform a diagrammatic analysis of the energy of a mobile impurity immersed in a strongly interacting two-component Fermi gas to second order in the impurity-bath interaction. These corrections demonstrate divergent behavior in the limit of large impurity momentum. We show the fundamental processes responsible for these logarithmically divergent terms. We study the problem in the general case without any assumptions regarding the fermion-fermion interactions in the bath. We show that the divergent term can be summed up to all orders in the Fermi-Fermi interaction and that the resulting expression is equivalent to the one obtained in the few-body calculation. Finally, we provide a perturbative calculation to the second order in the Fermi-Fermi interaction, and we show the diagrams responsible for these terms."}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2311.14536"}],"arxiv":1,"date_updated":"2025-09-04T13:07:33Z","acknowledgement":"We thank Félix Werner and Kris Van Houcke for interesting discussions.","date_created":"2024-03-24T23:00:59Z","publication":"Physical Review A","title":"Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy"},{"date_created":"2024-03-24T23:00:59Z","acknowledgement":"The Python implementation of kCSD was started by Grzegorz Parka during Google Summer of Code project through the International Neuroinformatics Coordinating Facility. Jan Mąka implemented the first Python version of skCSD class. This work was supported by the Polish National Science Centre (2013/08/W/NZ4/00691 to DKW; 2015/17/B/ST7/04123 to DKW). ","title":"kCSD-python, reliable current source density estimation with quality control","publication":"PLoS Computational Biology","related_material":{"link":[{"url":"https://github.com/Neuroinflab/kCSD-python","relation":"software"}]},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_updated":"2025-09-04T13:08:54Z","pmid":1,"oa":1,"OA_place":"publisher","file":[{"file_name":"2024_PLoSCompBio_Chintaluri.pdf","file_size":2540277,"creator":"dernst","checksum":"c09718d0d09614642d877d0716ce32e8","relation":"main_file","content_type":"application/pdf","access_level":"open_access","date_updated":"2025-06-25T05:47:36Z","success":1,"file_id":"19897","date_created":"2025-06-25T05:47:36Z"}],"abstract":[{"lang":"eng","text":"Interpretation of extracellular recordings can be challenging due to the long range of electric field. This challenge can be mitigated by estimating the current source density (CSD). Here we introduce kCSD-python, an open Python package implementing Kernel Current Source Density (kCSD) method and related tools to facilitate CSD analysis of experimental data and the interpretation of results. We show how to counter the limitations imposed by noise and assumptions in the method itself. kCSD-python allows CSD estimation for an arbitrary distribution of electrodes in 1D, 2D, and 3D, assuming distributions of sources in tissue, a slice, or in a single cell, and includes a range of diagnostic aids. We demonstrate its features in a Jupyter Notebook tutorial which illustrates a typical analytical workflow and main functionalities useful in validating analysis results."}],"publisher":"Public Library of Science","has_accepted_license":"1","intvolume":"        20","issue":"3","author":[{"first_name":"Chaitanya","full_name":"Chintaluri, Chaitanya","id":"E4EDB536-3485-11EA-98D2-20AF3DDC885E","last_name":"Chintaluri"},{"first_name":"Marta","full_name":"Bejtka, Marta","last_name":"Bejtka"},{"last_name":"Sredniawa","full_name":"Sredniawa, Wladyslaw","first_name":"Wladyslaw"},{"last_name":"Czerwinski","first_name":"Michal","full_name":"Czerwinski, Michal"},{"first_name":"Jakub M.","full_name":"Dzik, Jakub M.","last_name":"Dzik"},{"last_name":"Jedrzejewska-Szmek","full_name":"Jedrzejewska-Szmek, Joanna","first_name":"Joanna"},{"last_name":"Wojciki","first_name":"Daniel K.","full_name":"Wojciki, Daniel K."}],"quality_controlled":"1","language":[{"iso":"eng"}],"external_id":{"isi":["001190689800001"],"pmid":["38484020"]},"date_published":"2024-03-14T00:00:00Z","year":"2024","publication_status":"published","status":"public","file_date_updated":"2025-06-25T05:47:36Z","corr_author":"1","citation":{"ista":"Chintaluri C, Bejtka M, Sredniawa W, Czerwinski M, Dzik JM, Jedrzejewska-Szmek J, Wojciki DK. 2024. kCSD-python, reliable current source density estimation with quality control. PLoS Computational Biology. 20(3), e1011941.","ama":"Chintaluri C, Bejtka M, Sredniawa W, et al. kCSD-python, reliable current source density estimation with quality control. <i>PLoS Computational Biology</i>. 2024;20(3). doi:<a href=\"https://doi.org/10.1371/journal.pcbi.1011941\">10.1371/journal.pcbi.1011941</a>","ieee":"C. Chintaluri <i>et al.</i>, “kCSD-python, reliable current source density estimation with quality control,” <i>PLoS Computational Biology</i>, vol. 20, no. 3. Public Library of Science, 2024.","apa":"Chintaluri, C., Bejtka, M., Sredniawa, W., Czerwinski, M., Dzik, J. M., Jedrzejewska-Szmek, J., &#38; Wojciki, D. K. (2024). kCSD-python, reliable current source density estimation with quality control. <i>PLoS Computational Biology</i>. Public Library of Science. <a href=\"https://doi.org/10.1371/journal.pcbi.1011941\">https://doi.org/10.1371/journal.pcbi.1011941</a>","mla":"Chintaluri, Chaitanya, et al. “KCSD-Python, Reliable Current Source Density Estimation with Quality Control.” <i>PLoS Computational Biology</i>, vol. 20, no. 3, e1011941, Public Library of Science, 2024, doi:<a href=\"https://doi.org/10.1371/journal.pcbi.1011941\">10.1371/journal.pcbi.1011941</a>.","short":"C. Chintaluri, M. Bejtka, W. Sredniawa, M. Czerwinski, J.M. Dzik, J. Jedrzejewska-Szmek, D.K. Wojciki, PLoS Computational Biology 20 (2024).","chicago":"Chintaluri, Chaitanya, Marta Bejtka, Wladyslaw Sredniawa, Michal Czerwinski, Jakub M. Dzik, Joanna Jedrzejewska-Szmek, and Daniel K. Wojciki. “KCSD-Python, Reliable Current Source Density Estimation with Quality Control.” <i>PLoS Computational Biology</i>. Public Library of Science, 2024. <a href=\"https://doi.org/10.1371/journal.pcbi.1011941\">https://doi.org/10.1371/journal.pcbi.1011941</a>."},"OA_type":"gold","oa_version":"Published Version","DOAJ_listed":"1","type":"journal_article","month":"03","scopus_import":"1","isi":1,"ddc":["000","570"],"department":[{"_id":"TiVo"}],"article_processing_charge":"Yes","article_type":"original","article_number":"e1011941","publication_identifier":{"issn":["1553-734X"],"eissn":["1553-7358"]},"tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"day":"14","doi":"10.1371/journal.pcbi.1011941","_id":"15169","volume":20},{"month":"03","type":"journal_article","DOAJ_listed":"1","oa_version":"Published Version","article_processing_charge":"Yes","department":[{"_id":"JoMa"}],"isi":1,"ddc":["550"],"scopus_import":"1","article_number":"39","article_type":"original","volume":964,"_id":"15170","tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"day":"01","doi":"10.3847/1538-4357/ad1e5f","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","arxiv":1,"date_updated":"2025-09-04T13:09:41Z","publication":"Astrophysical Journal","title":"UNCOVER spectroscopy confirms the surprising ubiquity of active galactic nuclei in red sources at z > 5","acknowledgement":"J.E.G. and A.D.G acknowledge support from NSF/AAG grant No. 1007094, and J.E.G. also acknowledges support from NSF/AAG grant No. 1007052. A.Z. acknowledges support by grant No. 2020750 from the United States-Israel Binational Science Foundation (BSF) and grant No. 2109066 from the United States National Science Foundation (NSF), and by the Ministry of Science & Technology of Israel. The Cosmic Dawn Center is funded by the Danish National Research Foundation (DNRF) under grant No. 140. This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI) under contract number MB22.00072, as well as from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. P.D. acknowledges support from the NWO grant 016.VIDI.189.162 (\"ODIN\") and from the European Commission's and University of Groningen's CO-FUND Rosalind Franklin program. K.G. and T.N. acknowledge support from Australian Research Council Laureate Fellowship FL180100060. H.A. and I.C. acknowledge support from CNES, focused on the JWST mission, and the Programme National Cosmology and Galaxies (PNCG) of CNRS/INSU with INP and IN2P3, cofunded by CEA and CNES. R.P.N. acknowledges funding from JWST programs GO-1933 and GO-2279. Support for this work was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. The research of C.C.W. is supported by NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. B.W. acknowledges support from JWST-GO-02561.022-A. A.J.B. acknowledges funding support from NASA/ADAP grant 21-ADAP21-0187. Support for this work was provided by The Brinson Foundation through a Brinson Prize Fellowship grant. R.P.N. acknowledges support for this work provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. C.P. thanks Marsha and Ralph Schilling for the generous support of this research.","date_created":"2024-03-24T23:00:59Z","publisher":"IOP Publishing","abstract":[{"text":"The James Webb Space Telescope is revealing a new population of dust-reddened broad-line active galactic nuclei (AGN) at redshifts z ≳ 5. Here we present deep NIRSpec/Prism spectroscopy from the Cycle 1 Treasury program Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) of 15 AGN candidates selected to be compact, with red continua in the rest-frame optical but with blue slopes in the UV. From NIRCam photometry alone, they could have been dominated by dusty star formation or an AGN. Here we show that the majority of the compact red sources in UNCOVER are dust-reddened AGN: 60% show definitive evidence for broad-line Hα with a FWHM > 2000 km s −1, 20% of the current data are inconclusive, and 20% are brown dwarf stars. We propose an updated photometric criterion to select red z > 5 AGN that excludes brown dwarfs and is expected to yield >80% AGN. Remarkably, among all zphot > 5 galaxies with F277W – F444W > 1 in UNCOVER at least 33% are AGN regardless of compactness, climbing to at least 80% AGN for sources with F277W – F444W > 1.6. The confirmed AGN have black hole masses of 107–109M⊙. While their UV luminosities (−16 > MUV > −20 AB mag) are low compared to UV-selected AGN at these epochs, consistent with percent-level scattered AGN light or low levels of unobscured star formation, the inferred bolometric luminosities are typical of 107–109M⊙ black holes radiating at ∼10%–40% the Eddington limit. The number densities are surprisingly high at ∼10−5 Mpc−3 mag−1, 100 times more common than the faintest UV-selected quasars, while accounting for ∼1% of the UV-selected galaxies. While their UV faintness suggests they may not contribute strongly to reionization, their ubiquity poses challenges to models of black hole growth.","lang":"eng"}],"file":[{"checksum":"389a880e176799d5c062ea7cb82d08c9","relation":"main_file","content_type":"application/pdf","file_name":"2024_AstrophysicalJourn_Greene.pdf","file_size":2700137,"creator":"dernst","success":1,"file_id":"15176","date_created":"2024-03-25T08:02:43Z","access_level":"open_access","date_updated":"2024-03-25T08:02:43Z"}],"oa":1,"author":[{"last_name":"Greene","full_name":"Greene, Jenny E.","first_name":"Jenny E."},{"last_name":"Labbe","full_name":"Labbe, Ivo","first_name":"Ivo"},{"last_name":"Goulding","full_name":"Goulding, Andy D.","first_name":"Andy D."},{"full_name":"Furtak, Lukas J.","first_name":"Lukas J.","last_name":"Furtak"},{"last_name":"Chemerynska","full_name":"Chemerynska, Iryna","first_name":"Iryna"},{"full_name":"Kokorev, Vasily","first_name":"Vasily","last_name":"Kokorev"},{"last_name":"Dayal","first_name":"Pratika","full_name":"Dayal, Pratika"},{"last_name":"Volonteri","full_name":"Volonteri, Marta","first_name":"Marta"},{"first_name":"Christina C.","full_name":"Williams, Christina C.","last_name":"Williams"},{"first_name":"Bingjie","full_name":"Wang, Bingjie","last_name":"Wang"},{"last_name":"Setton","full_name":"Setton, David J.","first_name":"David J."},{"full_name":"Burgasser, Adam J.","first_name":"Adam J.","last_name":"Burgasser"},{"full_name":"Bezanson, Rachel","first_name":"Rachel","last_name":"Bezanson"},{"first_name":"Hakim","full_name":"Atek, Hakim","last_name":"Atek"},{"last_name":"Brammer","full_name":"Brammer, Gabriel","first_name":"Gabriel"},{"last_name":"Cutler","full_name":"Cutler, Sam E.","first_name":"Sam E."},{"first_name":"Robert","full_name":"Feldmann, Robert","last_name":"Feldmann"},{"first_name":"Seiji","full_name":"Fujimoto, Seiji","last_name":"Fujimoto"},{"last_name":"Glazebrook","full_name":"Glazebrook, Karl","first_name":"Karl"},{"last_name":"De Graaff","full_name":"De Graaff, Anna","first_name":"Anna"},{"full_name":"Khullar, Gourav","first_name":"Gourav","last_name":"Khullar"},{"full_name":"Leja, Joel","first_name":"Joel","last_name":"Leja"},{"first_name":"Danilo","full_name":"Marchesini, Danilo","last_name":"Marchesini"},{"last_name":"Maseda","first_name":"Michael V.","full_name":"Maseda, Michael V."},{"last_name":"Matthee","first_name":"Jorryt J","orcid":"0000-0003-2871-127X","full_name":"Matthee, Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"last_name":"Miller","first_name":"Tim B.","full_name":"Miller, Tim B."},{"last_name":"Naidu","first_name":"Rohan P.","full_name":"Naidu, Rohan P."},{"last_name":"Nanayakkara","full_name":"Nanayakkara, Themiya","first_name":"Themiya"},{"last_name":"Oesch","first_name":"Pascal A.","full_name":"Oesch, Pascal A."},{"first_name":"Richard","full_name":"Pan, Richard","last_name":"Pan"},{"full_name":"Papovich, Casey","first_name":"Casey","last_name":"Papovich"},{"first_name":"Sedona H.","full_name":"Price, Sedona H.","last_name":"Price"},{"full_name":"Van Dokkum, Pieter","first_name":"Pieter","last_name":"Van Dokkum"},{"full_name":"Weaver, John R.","first_name":"John R.","last_name":"Weaver"},{"first_name":"Katherine E.","full_name":"Whitaker, Katherine E.","last_name":"Whitaker"},{"first_name":"Adi","full_name":"Zitrin, Adi","last_name":"Zitrin"}],"intvolume":"       964","has_accepted_license":"1","file_date_updated":"2024-03-25T08:02:43Z","citation":{"mla":"Greene, Jenny E., et al. “UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z &#62; 5.” <i>Astrophysical Journal</i>, vol. 964, 39, IOP Publishing, 2024, doi:<a href=\"https://doi.org/10.3847/1538-4357/ad1e5f\">10.3847/1538-4357/ad1e5f</a>.","ama":"Greene JE, Labbe I, Goulding AD, et al. UNCOVER spectroscopy confirms the surprising ubiquity of active galactic nuclei in red sources at z &#62; 5. <i>Astrophysical Journal</i>. 2024;964. doi:<a href=\"https://doi.org/10.3847/1538-4357/ad1e5f\">10.3847/1538-4357/ad1e5f</a>","apa":"Greene, J. E., Labbe, I., Goulding, A. D., Furtak, L. J., Chemerynska, I., Kokorev, V., … Zitrin, A. (2024). UNCOVER spectroscopy confirms the surprising ubiquity of active galactic nuclei in red sources at z &#62; 5. <i>Astrophysical Journal</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/1538-4357/ad1e5f\">https://doi.org/10.3847/1538-4357/ad1e5f</a>","ieee":"J. E. Greene <i>et al.</i>, “UNCOVER spectroscopy confirms the surprising ubiquity of active galactic nuclei in red sources at z &#62; 5,” <i>Astrophysical Journal</i>, vol. 964. IOP Publishing, 2024.","ista":"Greene JE, Labbe I, Goulding AD, Furtak LJ, Chemerynska I, Kokorev V, Dayal P, Volonteri M, Williams CC, Wang B, Setton DJ, Burgasser AJ, Bezanson R, Atek H, Brammer G, Cutler SE, Feldmann R, Fujimoto S, Glazebrook K, De Graaff A, Khullar G, Leja J, Marchesini D, Maseda MV, Matthee JJ, Miller TB, Naidu RP, Nanayakkara T, Oesch PA, Pan R, Papovich C, Price SH, Van Dokkum P, Weaver JR, Whitaker KE, Zitrin A. 2024. UNCOVER spectroscopy confirms the surprising ubiquity of active galactic nuclei in red sources at z &#62; 5. Astrophysical Journal. 964, 39.","chicago":"Greene, Jenny E., Ivo Labbe, Andy D. Goulding, Lukas J. Furtak, Iryna Chemerynska, Vasily Kokorev, Pratika Dayal, et al. “UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z &#62; 5.” <i>Astrophysical Journal</i>. IOP Publishing, 2024. <a href=\"https://doi.org/10.3847/1538-4357/ad1e5f\">https://doi.org/10.3847/1538-4357/ad1e5f</a>.","short":"J.E. Greene, I. Labbe, A.D. Goulding, L.J. Furtak, I. Chemerynska, V. Kokorev, P. Dayal, M. Volonteri, C.C. Williams, B. Wang, D.J. Setton, A.J. Burgasser, R. Bezanson, H. Atek, G. Brammer, S.E. Cutler, R. Feldmann, S. Fujimoto, K. Glazebrook, A. De Graaff, G. Khullar, J. Leja, D. Marchesini, M.V. Maseda, J.J. Matthee, T.B. Miller, R.P. Naidu, T. Nanayakkara, P.A. Oesch, R. Pan, C. Papovich, S.H. Price, P. Van Dokkum, J.R. Weaver, K.E. Whitaker, A. Zitrin, Astrophysical Journal 964 (2024)."},"status":"public","publication_status":"published","date_published":"2024-03-01T00:00:00Z","year":"2024","external_id":{"isi":["001184746500001"],"arxiv":["2309.05714"]},"language":[{"iso":"eng"}],"quality_controlled":"1"},{"publication_identifier":{"eissn":["1546-1726"],"issn":["1097-6256"]},"tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"doi":"10.1038/s41593-024-01597-4","day":"01","volume":27,"project":[{"call_identifier":"H2020","grant_number":"819603","name":"Learning the shape of synaptic plasticity rules for neuronal architectures and function through machine learning.","_id":"0aacfa84-070f-11eb-9043-d7eb2c709234"}],"_id":"15171","article_type":"original","ddc":["570"],"isi":1,"scopus_import":"1","page":"964-974","department":[{"_id":"TiVo"}],"article_processing_charge":"Yes (via OA deal)","oa_version":"Published Version","month":"05","type":"journal_article","quality_controlled":"1","external_id":{"isi":["001190081400001"],"pmid":["38509348 "]},"language":[{"iso":"eng"}],"status":"public","publication_status":"published","date_published":"2024-05-01T00:00:00Z","year":"2024","OA_type":"hybrid","citation":{"short":"E.J. Agnes, T.P. Vogels, Nature Neuroscience 27 (2024) 964–974.","chicago":"Agnes, Everton J., and Tim P Vogels. “Co-Dependent Excitatory and Inhibitory Plasticity Accounts for Quick, Stable and Long-Lasting Memories in Biological Networks.” <i>Nature Neuroscience</i>. Springer Nature, 2024. <a href=\"https://doi.org/10.1038/s41593-024-01597-4\">https://doi.org/10.1038/s41593-024-01597-4</a>.","ista":"Agnes EJ, Vogels TP. 2024. Co-dependent excitatory and inhibitory plasticity accounts for quick, stable and long-lasting memories in biological networks. Nature Neuroscience. 27, 964–974.","ama":"Agnes EJ, Vogels TP. Co-dependent excitatory and inhibitory plasticity accounts for quick, stable and long-lasting memories in biological networks. <i>Nature Neuroscience</i>. 2024;27:964-974. doi:<a href=\"https://doi.org/10.1038/s41593-024-01597-4\">10.1038/s41593-024-01597-4</a>","ieee":"E. J. Agnes and T. P. Vogels, “Co-dependent excitatory and inhibitory plasticity accounts for quick, stable and long-lasting memories in biological networks,” <i>Nature Neuroscience</i>, vol. 27. Springer Nature, pp. 964–974, 2024.","apa":"Agnes, E. J., &#38; Vogels, T. P. (2024). Co-dependent excitatory and inhibitory plasticity accounts for quick, stable and long-lasting memories in biological networks. <i>Nature Neuroscience</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41593-024-01597-4\">https://doi.org/10.1038/s41593-024-01597-4</a>","mla":"Agnes, Everton J., and Tim P. Vogels. “Co-Dependent Excitatory and Inhibitory Plasticity Accounts for Quick, Stable and Long-Lasting Memories in Biological Networks.” <i>Nature Neuroscience</i>, vol. 27, Springer Nature, 2024, pp. 964–74, doi:<a href=\"https://doi.org/10.1038/s41593-024-01597-4\">10.1038/s41593-024-01597-4</a>."},"file_date_updated":"2025-06-25T08:45:32Z","has_accepted_license":"1","intvolume":"        27","author":[{"last_name":"Agnes","full_name":"Agnes, Everton J.","first_name":"Everton J."},{"last_name":"Vogels","first_name":"Tim P","orcid":"0000-0003-3295-6181","id":"CB6FF8D2-008F-11EA-8E08-2637E6697425","full_name":"Vogels, Tim P"}],"oa":1,"OA_place":"publisher","abstract":[{"lang":"eng","text":"The brain’s functionality is developed and maintained through synaptic plasticity. As synapses undergo plasticity, they also affect each other. The nature of such ‘co-dependency’ is difficult to disentangle experimentally, because multiple synapses must be monitored simultaneously. To help understand the experimentally observed phenomena, we introduce a framework that formalizes synaptic co-dependency between different connection types. The resulting model explains how inhibition can gate excitatory plasticity while neighboring excitatory–excitatory interactions determine the strength of long-term potentiation. Furthermore, we show how the interplay between excitatory and inhibitory synapses can account for the quick rise and long-term stability of a variety of synaptic weight profiles, such as orientation tuning and dendritic clustering of co-active synapses. In recurrent neuronal networks, co-dependent plasticity produces rich and stable motor cortex-like dynamics with high input sensitivity. Our results suggest an essential role for the neighborly synaptic interaction during learning, connecting micro-level physiology with network-wide phenomena."}],"file":[{"relation":"main_file","content_type":"application/pdf","checksum":"dfca68a24749575b912b3a78a7de4516","creator":"dernst","file_size":10508018,"file_name":"2025_NatureNeuroscience_Agnes.pdf","date_created":"2025-06-25T08:45:32Z","success":1,"file_id":"19902","date_updated":"2025-06-25T08:45:32Z","access_level":"open_access"}],"ec_funded":1,"publisher":"Springer Nature","acknowledgement":"We thank C. Currin, B. Podlaski and the members of the Vogels group for fruitful discussions. E.J.A. and T.P.V. were supported by a Research Project Grant from the Leverhulme Trust (RPG-2016-446; TPV), a Sir Henry Dale Fellowship from the Wellcome Trust and the Royal Society (WT100000; T.P.V.), a Wellcome Trust Senior Research Fellowship (214316/Z/18/Z; T.P.V.) and a European Research Council Consolidator Grant (SYNAPSEEK, 819603; T.P.V.). For the purpose of open access, the authors have applied a CC BY public copyright license to any author accepted manuscript version arising from this submission. Open access funding provided by University of Basel.","date_created":"2024-03-24T23:01:00Z","publication":"Nature Neuroscience","title":"Co-dependent excitatory and inhibitory plasticity accounts for quick, stable and long-lasting memories in biological networks","date_updated":"2025-09-04T13:06:06Z","pmid":1,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345"},{"_id":"15172","project":[{"_id":"059876FA-7A3F-11EA-A408-12923DDC885E","name":"Prix Lopez-Loretta 2019 - Marco Mondelli"}],"volume":70,"publication_identifier":{"eissn":["1557-9654"],"issn":["0018-9448"]},"day":"01","doi":"10.1109/TIT.2024.3367767","article_type":"original","article_processing_charge":"No","scopus_import":"1","isi":1,"department":[{"_id":"MaMo"}],"page":"3823-3839","oa_version":"Preprint","type":"journal_article","month":"06","date_published":"2024-06-01T00:00:00Z","year":"2024","publication_status":"published","status":"public","citation":{"chicago":"Esposito, Amedeo Roberto, and Marco Mondelli. “Concentration without Independence via Information Measures.” <i>IEEE Transactions on Information Theory</i>. IEEE, 2024. <a href=\"https://doi.org/10.1109/TIT.2024.3367767\">https://doi.org/10.1109/TIT.2024.3367767</a>.","short":"A.R. Esposito, M. Mondelli, IEEE Transactions on Information Theory 70 (2024) 3823–3839.","mla":"Esposito, Amedeo Roberto, and Marco Mondelli. “Concentration without Independence via Information Measures.” <i>IEEE Transactions on Information Theory</i>, vol. 70, no. 6, IEEE, 2024, pp. 3823–39, doi:<a href=\"https://doi.org/10.1109/TIT.2024.3367767\">10.1109/TIT.2024.3367767</a>.","ista":"Esposito AR, Mondelli M. 2024. Concentration without independence via information measures. IEEE Transactions on Information Theory. 70(6), 3823–3839.","apa":"Esposito, A. R., &#38; Mondelli, M. (2024). Concentration without independence via information measures. <i>IEEE Transactions on Information Theory</i>. IEEE. <a href=\"https://doi.org/10.1109/TIT.2024.3367767\">https://doi.org/10.1109/TIT.2024.3367767</a>","ieee":"A. R. Esposito and M. Mondelli, “Concentration without independence via information measures,” <i>IEEE Transactions on Information Theory</i>, vol. 70, no. 6. IEEE, pp. 3823–3839, 2024.","ama":"Esposito AR, Mondelli M. Concentration without independence via information measures. <i>IEEE Transactions on Information Theory</i>. 2024;70(6):3823-3839. doi:<a href=\"https://doi.org/10.1109/TIT.2024.3367767\">10.1109/TIT.2024.3367767</a>"},"corr_author":"1","quality_controlled":"1","external_id":{"isi":["001230181100001"],"arxiv":["2303.07245"]},"language":[{"iso":"eng"}],"intvolume":"        70","issue":"6","author":[{"last_name":"Esposito","first_name":"Amedeo Roberto","id":"9583e921-e1ad-11ec-9862-cef099626dc9","full_name":"Esposito, Amedeo Roberto"},{"id":"27EB676C-8706-11E9-9510-7717E6697425","full_name":"Mondelli, Marco","orcid":"0000-0002-3242-7020","first_name":"Marco","last_name":"Mondelli"}],"publisher":"IEEE","oa":1,"abstract":[{"text":"We propose a novel approach to concentration for non-independent random variables. The main idea is to “pretend” that the random variables are independent and pay a multiplicative price measuring how far they are from actually being independent. This price is encapsulated in the Hellinger integral between the joint and the product of the marginals, which is then upper bounded leveraging tensorisation properties. Our bounds represent a natural generalisation of concentration inequalities in the presence of dependence: we recover exactly the classical bounds (McDiarmid’s inequality) when the random variables are independent. Furthermore, in a “large deviations” regime, we obtain the same decay in the probability as for the independent case, even when the random variables display non-trivial dependencies. To show this, we consider a number of applications of interest. First, we provide a bound for Markov chains with finite state space. Then, we consider the Simple Symmetric Random Walk, which is a non-contracting Markov chain, and a non-Markovian setting in which the stochastic process depends on its entire past. To conclude, we propose an application to Markov Chain Monte Carlo methods, where our approach leads to an improved lower bound on the minimum burn-in period required to reach a certain accuracy. In all of these settings, we provide a regime of parameters in which our bound fares better than what the state of the art can provide.","lang":"eng"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2303.07245","open_access":"1"}],"date_updated":"2025-09-04T13:06:53Z","arxiv":1,"date_created":"2024-03-24T23:01:00Z","title":"Concentration without independence via information measures","publication":"IEEE Transactions on Information Theory","related_material":{"record":[{"status":"public","relation":"earlier_version","id":"14922"}]}},{"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_updated":"2025-09-04T13:16:05Z","pmid":1,"title":"A hybrid pathway for self-sustained luminescence","publication":"Science Advances","date_created":"2024-03-25T08:54:33Z","acknowledgement":"We thank Milaboratory (milaboratory.com) for the access to computing and storage infrastructure. We thank J. Petrasek for providing the BY-2 cell culture line. We thank Konstantin Lukyanov laboratory and Sergey Deyev laboratory for assistance with experiments.\r\nThis study was partially funded by Light Bio and Planta. The Synthetic biology Group is funded by the MRC London Institute of Medical Sciences (UKRI MC-A658-5QEA0). Cloning and luminescent assays performed in BY-2 were partially supported by RSF, project number 22-14-00400, https://rscf.ru/project/22-14-00400/. Plant transformations were funded by RFBR and MOST, project number 21-54-52004. Plant imaging experiments were funded by RSF, project number 22-74-00124, https://rscf.ru/project/22-74-00124/. Viral delivery experiments were funded by the grant PID2019-108203RB-I00 Plan Nacional I + D from the Ministerio de Ciencia e Innovación (Spain) through the Agencia Estatal de Investigación (cofinanced by the European Regional Development Fund).","publisher":"American Association for the Advancement of Science","file":[{"checksum":"a19c43b260ea0bbaf895a29712e3153c","content_type":"application/pdf","relation":"main_file","file_name":"2024_ScienceAdv_Palkina.pdf","file_size":1499302,"creator":"dernst","file_id":"15185","date_created":"2024-03-25T09:42:10Z","success":1,"date_updated":"2024-03-25T09:42:10Z","access_level":"open_access"}],"OA_place":"publisher","abstract":[{"text":"The fungal bioluminescence pathway can be reconstituted in other organisms allowing luminescence imaging without exogenously supplied substrate. The pathway starts from hispidin biosynthesis—a step catalyzed by a large fungal polyketide synthase that requires a posttranslational modification for activity. Here, we report identification of alternative compact hispidin synthases encoded by a phylogenetically diverse group of plants. A hybrid bioluminescence pathway that combines plant and fungal genes is more compact, not dependent on availability of machinery for posttranslational modifications, and confers autonomous bioluminescence in yeast, mammalian, and plant hosts. The compact size of plant hispidin synthases enables additional modes of delivery of autoluminescence, such as delivery with viral vectors.","lang":"eng"}],"oa":1,"author":[{"last_name":"Palkina","full_name":"Palkina, Kseniia A.","first_name":"Kseniia A."},{"last_name":"Karataeva","full_name":"Karataeva, Tatiana A.","first_name":"Tatiana A."},{"full_name":"Perfilov, Maxim M.","first_name":"Maxim M.","last_name":"Perfilov"},{"last_name":"Fakhranurova","full_name":"Fakhranurova, Liliia I.","first_name":"Liliia I."},{"last_name":"Markina","full_name":"Markina, Nadezhda M.","first_name":"Nadezhda M."},{"orcid":"0000-0001-9139-5383","id":"4720D23C-F248-11E8-B48F-1D18A9856A87","full_name":"Gonzalez Somermeyer, Louisa","first_name":"Louisa","last_name":"Gonzalez Somermeyer"},{"last_name":"Garcia-Perez","first_name":"Elena","full_name":"Garcia-Perez, Elena"},{"last_name":"Vazquez-Vilar","first_name":"Marta","full_name":"Vazquez-Vilar, Marta"},{"last_name":"Rodriguez-Rodriguez","first_name":"Marta","full_name":"Rodriguez-Rodriguez, Marta"},{"last_name":"Vazquez-Vilriales","full_name":"Vazquez-Vilriales, Victor","first_name":"Victor"},{"first_name":"Ekaterina S.","full_name":"Shakhova, Ekaterina S.","last_name":"Shakhova"},{"last_name":"Mitiouchkina","first_name":"Tatiana","full_name":"Mitiouchkina, Tatiana"},{"last_name":"Belozerova","full_name":"Belozerova, Olga A.","first_name":"Olga A."},{"last_name":"Kovalchuk","full_name":"Kovalchuk, Sergey I.","first_name":"Sergey I."},{"full_name":"Alekberova, Anna","first_name":"Anna","last_name":"Alekberova"},{"first_name":"Alena K.","full_name":"Malyshevskaia, Alena K.","last_name":"Malyshevskaia"},{"full_name":"Bugaeva, Evgenia N.","first_name":"Evgenia N.","last_name":"Bugaeva"},{"last_name":"Guglya","first_name":"Elena B.","full_name":"Guglya, Elena B."},{"first_name":"Anastasia","full_name":"Balakireva, Anastasia","last_name":"Balakireva"},{"full_name":"Sytov, Nikita","first_name":"Nikita","last_name":"Sytov"},{"full_name":"Bezlikhotnova, Anastasia","first_name":"Anastasia","last_name":"Bezlikhotnova"},{"last_name":"Boldyreva","full_name":"Boldyreva, Daria I.","first_name":"Daria I."},{"last_name":"Babenko","first_name":"Vladislav V.","full_name":"Babenko, Vladislav V."},{"last_name":"Kondrashov","full_name":"Kondrashov, Fyodor","id":"44FDEF62-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8243-4694","first_name":"Fyodor"},{"last_name":"Choob","first_name":"Vladimir V.","full_name":"Choob, Vladimir V."},{"full_name":"Orzaez, Diego","first_name":"Diego","last_name":"Orzaez"},{"first_name":"Ilia V.","full_name":"Yampolsky, Ilia V.","last_name":"Yampolsky"},{"last_name":"Mishin","full_name":"Mishin, Alexander S.","first_name":"Alexander S."},{"full_name":"Sarkisyan, Karen S.","first_name":"Karen S.","last_name":"Sarkisyan"}],"intvolume":"        10","issue":"10","has_accepted_license":"1","file_date_updated":"2024-03-25T09:42:10Z","OA_type":"gold","citation":{"mla":"Palkina, Kseniia A., et al. “A Hybrid Pathway for Self-Sustained Luminescence.” <i>Science Advances</i>, vol. 10, no. 10, adk1992, American Association for the Advancement of Science, 2024, doi:<a href=\"https://doi.org/10.1126/sciadv.adk1992\">10.1126/sciadv.adk1992</a>.","ieee":"K. A. Palkina <i>et al.</i>, “A hybrid pathway for self-sustained luminescence,” <i>Science Advances</i>, vol. 10, no. 10. American Association for the Advancement of Science, 2024.","apa":"Palkina, K. A., Karataeva, T. A., Perfilov, M. M., Fakhranurova, L. I., Markina, N. M., Gonzalez Somermeyer, L., … Sarkisyan, K. S. (2024). A hybrid pathway for self-sustained luminescence. <i>Science Advances</i>. American Association for the Advancement of Science. <a href=\"https://doi.org/10.1126/sciadv.adk1992\">https://doi.org/10.1126/sciadv.adk1992</a>","ama":"Palkina KA, Karataeva TA, Perfilov MM, et al. A hybrid pathway for self-sustained luminescence. <i>Science Advances</i>. 2024;10(10). doi:<a href=\"https://doi.org/10.1126/sciadv.adk1992\">10.1126/sciadv.adk1992</a>","ista":"Palkina KA, Karataeva TA, Perfilov MM, Fakhranurova LI, Markina NM, Gonzalez Somermeyer L, Garcia-Perez E, Vazquez-Vilar M, Rodriguez-Rodriguez M, Vazquez-Vilriales V, Shakhova ES, Mitiouchkina T, Belozerova OA, Kovalchuk SI, Alekberova A, Malyshevskaia AK, Bugaeva EN, Guglya EB, Balakireva A, Sytov N, Bezlikhotnova A, Boldyreva DI, Babenko VV, Kondrashov F, Choob VV, Orzaez D, Yampolsky IV, Mishin AS, Sarkisyan KS. 2024. A hybrid pathway for self-sustained luminescence. Science Advances. 10(10), adk1992.","chicago":"Palkina, Kseniia A., Tatiana A. Karataeva, Maxim M. Perfilov, Liliia I. Fakhranurova, Nadezhda M. Markina, Louisa Gonzalez Somermeyer, Elena Garcia-Perez, et al. “A Hybrid Pathway for Self-Sustained Luminescence.” <i>Science Advances</i>. American Association for the Advancement of Science, 2024. <a href=\"https://doi.org/10.1126/sciadv.adk1992\">https://doi.org/10.1126/sciadv.adk1992</a>.","short":"K.A. Palkina, T.A. Karataeva, M.M. Perfilov, L.I. Fakhranurova, N.M. Markina, L. Gonzalez Somermeyer, E. Garcia-Perez, M. Vazquez-Vilar, M. Rodriguez-Rodriguez, V. Vazquez-Vilriales, E.S. Shakhova, T. Mitiouchkina, O.A. Belozerova, S.I. Kovalchuk, A. Alekberova, A.K. Malyshevskaia, E.N. Bugaeva, E.B. Guglya, A. Balakireva, N. Sytov, A. Bezlikhotnova, D.I. Boldyreva, V.V. Babenko, F. Kondrashov, V.V. Choob, D. Orzaez, I.V. Yampolsky, A.S. Mishin, K.S. Sarkisyan, Science Advances 10 (2024)."},"date_published":"2024-03-01T00:00:00Z","year":"2024","status":"public","publication_status":"published","language":[{"iso":"eng"}],"external_id":{"isi":["001187580500013"],"pmid":["38457503"]},"quality_controlled":"1","type":"journal_article","month":"03","oa_version":"Published Version","DOAJ_listed":"1","article_processing_charge":"Yes","department":[{"_id":"FyKo"}],"scopus_import":"1","ddc":["580"],"isi":1,"article_number":"adk1992","article_type":"original","_id":"15179","volume":10,"doi":"10.1126/sciadv.adk1992","tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"day":"01","publication_identifier":{"eissn":["2375-2548"]}},{"volume":963,"project":[{"name":"Young galaxies as tracers and agents of cosmic reionization","grant_number":"101076224","_id":"bd9b2118-d553-11ed-ba76-db24564edfea"}],"_id":"15180","doi":"10.3847/1538-4357/ad2345","tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"day":"07","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"article_number":"129","article_type":"original","article_processing_charge":"Yes","department":[{"_id":"JoMa"}],"ddc":["550"],"isi":1,"scopus_import":"1","month":"03","type":"journal_article","APC_amount":"5666,27 EUR","oa_version":"Published Version","OA_type":"gold","corr_author":"1","citation":{"short":"J.J. Matthee, R.P. Naidu, G. Brammer, J. Chisholm, A.-C. Eilers, A. Goulding, J. Greene, D. Kashino, I. Labbe, S.J. Lilly, R. Mackenzie, P.A. Oesch, A. Weibel, S. Wuyts, M. Xiao, R. Bordoloi, R. Bouwens, P. van Dokkum, G. Illingworth, I. Kramarenko, M.V. Maseda, C. Mason, R.A. Meyer, E.J. Nelson, N.A. Reddy, I. Shivaei, R.A. Simcoe, M. Yue, The Astrophysical Journal 963 (2024).","chicago":"Matthee, Jorryt J, Rohan P. Naidu, Gabriel Brammer, John Chisholm, Anna-Christina Eilers, Andy Goulding, Jenny Greene, et al. “Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2024. <a href=\"https://doi.org/10.3847/1538-4357/ad2345\">https://doi.org/10.3847/1538-4357/ad2345</a>.","ista":"Matthee JJ, Naidu RP, Brammer G, Chisholm J, Eilers A-C, Goulding A, Greene J, Kashino D, Labbe I, Lilly SJ, Mackenzie R, Oesch PA, Weibel A, Wuyts S, Xiao M, Bordoloi R, Bouwens R, van Dokkum P, Illingworth G, Kramarenko I, Maseda MV, Mason C, Meyer RA, Nelson EJ, Reddy NA, Shivaei I, Simcoe RA, Yue M. 2024. Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys. The Astrophysical Journal. 963(2), 129.","ieee":"J. J. Matthee <i>et al.</i>, “Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys,” <i>The Astrophysical Journal</i>, vol. 963, no. 2. American Astronomical Society, 2024.","apa":"Matthee, J. J., Naidu, R. P., Brammer, G., Chisholm, J., Eilers, A.-C., Goulding, A., … Yue, M. (2024). Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ad2345\">https://doi.org/10.3847/1538-4357/ad2345</a>","ama":"Matthee JJ, Naidu RP, Brammer G, et al. Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys. <i>The Astrophysical Journal</i>. 2024;963(2). doi:<a href=\"https://doi.org/10.3847/1538-4357/ad2345\">10.3847/1538-4357/ad2345</a>","mla":"Matthee, Jorryt J., et al. “Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys.” <i>The Astrophysical Journal</i>, vol. 963, no. 2, 129, American Astronomical Society, 2024, doi:<a href=\"https://doi.org/10.3847/1538-4357/ad2345\">10.3847/1538-4357/ad2345</a>."},"file_date_updated":"2024-03-25T09:31:58Z","status":"public","publication_status":"published","date_published":"2024-03-07T00:00:00Z","year":"2024","language":[{"iso":"eng"}],"external_id":{"isi":["001184703600001"]},"quality_controlled":"1","author":[{"first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X","full_name":"Matthee, Jorryt J","last_name":"Matthee"},{"last_name":"Naidu","full_name":"Naidu, Rohan P.","first_name":"Rohan P."},{"full_name":"Brammer, Gabriel","first_name":"Gabriel","last_name":"Brammer"},{"last_name":"Chisholm","full_name":"Chisholm, John","first_name":"John"},{"last_name":"Eilers","first_name":"Anna-Christina","full_name":"Eilers, Anna-Christina"},{"full_name":"Goulding, Andy","first_name":"Andy","last_name":"Goulding"},{"last_name":"Greene","full_name":"Greene, Jenny","first_name":"Jenny"},{"last_name":"Kashino","first_name":"Daichi","full_name":"Kashino, Daichi"},{"last_name":"Labbe","full_name":"Labbe, Ivo","first_name":"Ivo"},{"last_name":"Lilly","first_name":"Simon J.","full_name":"Lilly, Simon J."},{"last_name":"Mackenzie","first_name":"Ruari","full_name":"Mackenzie, Ruari"},{"last_name":"Oesch","full_name":"Oesch, Pascal A.","first_name":"Pascal A."},{"first_name":"Andrea","full_name":"Weibel, Andrea","last_name":"Weibel"},{"last_name":"Wuyts","full_name":"Wuyts, Stijn","first_name":"Stijn"},{"last_name":"Xiao","first_name":"Mengyuan","full_name":"Xiao, Mengyuan"},{"first_name":"Rongmon","full_name":"Bordoloi, Rongmon","last_name":"Bordoloi"},{"first_name":"Rychard","full_name":"Bouwens, Rychard","last_name":"Bouwens"},{"last_name":"van Dokkum","first_name":"Pieter","full_name":"van Dokkum, Pieter"},{"last_name":"Illingworth","first_name":"Garth","full_name":"Illingworth, Garth"},{"full_name":"Kramarenko, Ivan","first_name":"Ivan","last_name":"Kramarenko"},{"full_name":"Maseda, Michael V.","first_name":"Michael V.","last_name":"Maseda"},{"last_name":"Mason","full_name":"Mason, Charlotte","first_name":"Charlotte"},{"last_name":"Meyer","first_name":"Romain A.","full_name":"Meyer, Romain A."},{"full_name":"Nelson, Erica J.","first_name":"Erica J.","last_name":"Nelson"},{"first_name":"Naveen A.","full_name":"Reddy, Naveen A.","last_name":"Reddy"},{"full_name":"Shivaei, Irene","first_name":"Irene","last_name":"Shivaei"},{"last_name":"Simcoe","first_name":"Robert A.","full_name":"Simcoe, Robert A."},{"last_name":"Yue","full_name":"Yue, Minghao","first_name":"Minghao"}],"issue":"2","intvolume":"       963","has_accepted_license":"1","publisher":"American Astronomical Society","OA_place":"publisher","abstract":[{"lang":"eng","text":"Characterizing the prevalence and properties of faint active galactic nuclei (AGNs) in the early Universe is key for understanding the formation of supermassive black holes (SMBHs) and determining their role in cosmic reionization. We perform a spectroscopic search for broad Hα emitters at z ≈ 4–6 using deep JWST/NIRCam imaging and wide field slitless spectroscopy from the EIGER and FRESCO surveys. We identify 20 Hα lines at z = 4.2–5.5 that have broad components with line widths from ∼1200–3700 km s−1, contributing ∼30%–90% of the total line flux. We interpret these broad components as being powered by accretion onto SMBHs with implied masses ∼107–8M⊙. In the UV luminosity range MUV,AGN+host = −21 to −18, we measure number densities of ≈10−5 cMpc−3. This is an order of magnitude higher than expected from extrapolating quasar UV luminosity functions (LFs). Yet, such AGN are found in only <1% of star-forming galaxies at z ∼ 5. The number density discrepancy is much lower when compared to the broad Hα LF. The SMBH mass function agrees with large cosmological simulations. In two objects, we detect complex Hα profiles that we tentatively interpret as caused by absorption signatures from dense gas fueling SMBH growth and outflows. We may be witnessing early AGN feedback that will clear dust-free pathways through which more massive blue quasars are seen. We uncover a strong correlation between reddening and the fraction of total galaxy luminosity arising from faint AGN. This implies that early SMBH growth is highly obscured and that faint AGN are only minor contributors to cosmic reionization."}],"file":[{"relation":"main_file","content_type":"application/pdf","checksum":"dc7af4694f9f94a551417ab49fa43edf","creator":"dernst","file_name":"2024_AstrophysicalJourn_Matthee.pdf","file_size":6047536,"success":1,"date_created":"2024-03-25T09:31:58Z","file_id":"15184","date_updated":"2024-03-25T09:31:58Z","access_level":"open_access"}],"oa":1,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_updated":"2025-09-04T13:15:26Z","publication":"The Astrophysical Journal","related_material":{"link":[{"relation":"press_release","url":"https://ista.ac.at/en/news/baby-quasars-growing-supermassive-black-holes/","description":"News on ISTA website"}]},"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"title":"Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys","acknowledgement":"We thank the anonymous referee for constructive comments that helped improve the manuscript. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program Nos. 1243 and 1895. The specific observations analyzed can be accessed via doi:10.17909/4xx0-zj76. Funded by the European Union (ERC, AGENTS, 101076224). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. R.P.N. acknowledges funding from JWST programs GO-1933 and GO-2279. Support for this work for R.P.N. was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. Support for this work for G.I. was provided by NASA through grant JWST-GO-01895 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI) under contract No. MB22.00072, as well as from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant No. 140.\r\nFacility: JWST - James Webb Space Telescope, HST - Hubble Space Telescope satellite\r\nSoftware:​​​​​​​ Python, matplotlib (Hunter 2007), numpy (Harris et al. 2020), scipy (Virtanen et al. 2020), Astropy (Astropy Collaboration et al. 2013, 2018), Imfit (Erwin 2015).","date_created":"2024-03-25T08:54:47Z"},{"oa":1,"file":[{"file_name":"2024_PhysicalReviewResearch_Becker.pdf","file_size":2207067,"creator":"dernst","checksum":"4e0e58d1f58386fb016284c84db2a300","content_type":"application/pdf","relation":"main_file","access_level":"open_access","date_updated":"2024-03-25T09:24:55Z","date_created":"2024-03-25T09:24:55Z","success":1,"file_id":"15183"}],"abstract":[{"lang":"eng","text":"We demonstrate the failure of the adiabatic Born-Oppenheimer approximation to describe the ground state of a quantum impurity within an ultracold Fermi gas despite substantial mass differences between the bath and impurity species. Increasing repulsion leads to the appearance of nonadiabatic couplings between the fast bath and slow impurity degrees of freedom, which reduce the parity symmetry of the latter according to the pseudo Jahn-Teller effect. The presence of this mechanism is associated to a conical intersection involving the impurity position and the inverse of the interaction strength, which acts as a synthetic dimension. We elucidate the presence of these effects via a detailed ground-state analysis involving the comparison of ab initio fully correlated simulations with effective models. Our study suggests ultracold atomic ensembles as potent emulators of complex molecular phenomena."}],"ec_funded":1,"publisher":"American Physical Society","date_created":"2024-03-25T08:57:07Z","acknowledgement":"This work has been funded by the Cluster of Excellence “Advanced Imaging of Matter” of the Deutsche Forschungsgemeinschaft (DFG) - EXC 2056 - Project ID 390715994.\r\nG.M.K. gratefully acknowledges funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie Grant Agreement No. 101034413.","title":"Synthetic dimension-induced pseudo Jahn-Teller effect in one-dimensional confined fermions","publication":"Physical Review Research","date_updated":"2025-05-14T09:32:03Z","arxiv":1,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","quality_controlled":"1","language":[{"iso":"eng"}],"external_id":{"arxiv":["2310.17995"]},"date_published":"2024-03-01T00:00:00Z","year":"2024","status":"public","publication_status":"published","citation":{"mla":"Becker, A., et al. “Synthetic Dimension-Induced Pseudo Jahn-Teller Effect in One-Dimensional Confined Fermions.” <i>Physical Review Research</i>, vol. 6, no. 1, 013257, American Physical Society, 2024, doi:<a href=\"https://doi.org/10.1103/physrevresearch.6.013257\">10.1103/physrevresearch.6.013257</a>.","ieee":"A. Becker, G. Koutentakis, and P. Schmelcher, “Synthetic dimension-induced pseudo Jahn-Teller effect in one-dimensional confined fermions,” <i>Physical Review Research</i>, vol. 6, no. 1. American Physical Society, 2024.","ama":"Becker A, Koutentakis G, Schmelcher P. Synthetic dimension-induced pseudo Jahn-Teller effect in one-dimensional confined fermions. <i>Physical Review Research</i>. 2024;6(1). doi:<a href=\"https://doi.org/10.1103/physrevresearch.6.013257\">10.1103/physrevresearch.6.013257</a>","apa":"Becker, A., Koutentakis, G., &#38; Schmelcher, P. (2024). Synthetic dimension-induced pseudo Jahn-Teller effect in one-dimensional confined fermions. <i>Physical Review Research</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevresearch.6.013257\">https://doi.org/10.1103/physrevresearch.6.013257</a>","ista":"Becker A, Koutentakis G, Schmelcher P. 2024. Synthetic dimension-induced pseudo Jahn-Teller effect in one-dimensional confined fermions. Physical Review Research. 6(1), 013257.","chicago":"Becker, A., Georgios Koutentakis, and P. Schmelcher. “Synthetic Dimension-Induced Pseudo Jahn-Teller Effect in One-Dimensional Confined Fermions.” <i>Physical Review Research</i>. American Physical Society, 2024. <a href=\"https://doi.org/10.1103/physrevresearch.6.013257\">https://doi.org/10.1103/physrevresearch.6.013257</a>.","short":"A. Becker, G. Koutentakis, P. Schmelcher, Physical Review Research 6 (2024)."},"file_date_updated":"2024-03-25T09:24:55Z","has_accepted_license":"1","intvolume":"         6","issue":"1","author":[{"first_name":"A.","full_name":"Becker, A.","last_name":"Becker"},{"last_name":"Koutentakis","first_name":"Georgios","full_name":"Koutentakis, Georgios","id":"d7b23d3a-9e21-11ec-b482-f76739596b95"},{"first_name":"P.","full_name":"Schmelcher, P.","last_name":"Schmelcher"}],"scopus_import":"1","ddc":["530"],"department":[{"_id":"MiLe"}],"article_processing_charge":"Yes","oa_version":"Published Version","DOAJ_listed":"1","type":"journal_article","month":"03","publication_identifier":{"eissn":["2643-1564"]},"tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"day":"01","doi":"10.1103/physrevresearch.6.013257","project":[{"_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c","grant_number":"101034413","name":"IST-BRIDGE: International postdoctoral program","call_identifier":"H2020"}],"_id":"15181","volume":6,"article_type":"original","article_number":"013257"},{"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_updated":"2025-09-04T13:14:27Z","date_created":"2024-03-25T08:57:40Z","acknowledgement":"This work was supported by the Scientific Service Units (SSU) of ISTA through resources provided by the Electron Microscopy Facility (EMF), the Lab Support Facility (LSF), and the Nanofabrication Facility (NNF). This work was financially supported by ISTA and the Werner Siemens Foundation. The USTEM Service Unit of the Technical University of Vienna is acknowledged for EBSD sample preparation and analysis. R.L.B. acknowledges the National Science Foundation for funding the mass spectrometry analysis under award DMR 1904719. J.L. is a Serra Húnter Fellow and is grateful to the ICREA Academia program and projects MICINN/FEDER PID2021-124572OB-C31 and GC 2021 SGR 01061.","title":"A route to high thermoelectric performance: Solution‐based control of microstructure and composition in Ag2Se","publication":"Advanced Energy Materials","publisher":"Wiley","oa":1,"file":[{"checksum":"86b26430e00d5f43ea19e9b610692ab7","content_type":"application/pdf","relation":"main_file","file_name":"2024_AdvancedEnergyMaterials_Kleinhanns.pdf","file_size":8824301,"creator":"dernst","success":1,"date_created":"2024-07-22T12:07:56Z","file_id":"17314","access_level":"open_access","date_updated":"2024-07-22T12:07:56Z"}],"abstract":[{"lang":"eng","text":"Thermoelectric materials convert heat into electricity, with a broad range of applications near room temperature (RT). However, the library of RT high-performance materials is limited. Traditional high-temperature synthetic methods constrain the range of materials achievable, hindering the ability to surpass crystal structure limitations and engineer defects. Here, a solution-based synthetic approach is introduced, enabling RT synthesis of powders and exploration of densification at lower temperatures to influence the material's microstructure. The approach is exemplified by Ag2Se, an n-type alternative to bismuth telluride. It is demonstrated that the concentration of Ag interstitials, grain boundaries, and dislocations are directly correlated to the sintering temperature, and achieve a figure of merit of 1.1 from RT to 100 °C after optimization. Moreover, insights into and resolve Ag2Se's challenges are provided, including stoichiometry issues leading to irreproducible performances. This work highlights the potential of RT solution synthesis in expanding the repertoire of high-performance thermoelectric materials for practical applications."}],"intvolume":"        14","issue":"22","author":[{"last_name":"Kleinhanns","first_name":"Tobias","full_name":"Kleinhanns, Tobias","id":"8BD9DE16-AB3C-11E9-9C8C-2A03E6697425"},{"last_name":"Milillo","id":"38b830db-ea88-11ee-bf9b-929beaf79054","full_name":"Milillo, Francesco","first_name":"Francesco"},{"last_name":"Calcabrini","orcid":"0000-0003-4566-5877","id":"45D7531A-F248-11E8-B48F-1D18A9856A87","full_name":"Calcabrini, Mariano","first_name":"Mariano"},{"last_name":"Fiedler","full_name":"Fiedler, Christine","id":"bd3fceba-dc74-11ea-a0a7-c17f71817366","first_name":"Christine"},{"id":"03a7e858-01b1-11ec-8b71-99ae6c4a05bc","full_name":"Horta, Sharona","first_name":"Sharona","last_name":"Horta"},{"last_name":"Balazs","first_name":"Daniel","orcid":"0000-0001-7597-043X","id":"302BADF6-85FC-11EA-9E3B-B9493DDC885E","full_name":"Balazs, Daniel"},{"last_name":"Strumolo","full_name":"Strumolo, Marissa J.","first_name":"Marissa J."},{"full_name":"Hasler, Roger","first_name":"Roger","last_name":"Hasler"},{"full_name":"Llorca, Jordi","first_name":"Jordi","last_name":"Llorca"},{"full_name":"Tkadletz, Michael","first_name":"Michael","last_name":"Tkadletz"},{"full_name":"Brutchey, Richard L.","first_name":"Richard L.","last_name":"Brutchey"},{"id":"43C61214-F248-11E8-B48F-1D18A9856A87","full_name":"Ibáñez, Maria","orcid":"0000-0001-5013-2843","first_name":"Maria","last_name":"Ibáñez"}],"has_accepted_license":"1","date_published":"2024-06-12T00:00:00Z","year":"2024","publication_status":"published","status":"public","file_date_updated":"2024-07-22T12:07:56Z","corr_author":"1","citation":{"ista":"Kleinhanns T, Milillo F, Calcabrini M, Fiedler C, Horta S, Balazs D, Strumolo MJ, Hasler R, Llorca J, Tkadletz M, Brutchey RL, Ibáñez M. 2024. A route to high thermoelectric performance: Solution‐based control of microstructure and composition in Ag2Se. Advanced Energy Materials. 14(22), 2400408.","apa":"Kleinhanns, T., Milillo, F., Calcabrini, M., Fiedler, C., Horta, S., Balazs, D., … Ibáñez, M. (2024). A route to high thermoelectric performance: Solution‐based control of microstructure and composition in Ag2Se. <i>Advanced Energy Materials</i>. Wiley. <a href=\"https://doi.org/10.1002/aenm.202400408\">https://doi.org/10.1002/aenm.202400408</a>","ieee":"T. Kleinhanns <i>et al.</i>, “A route to high thermoelectric performance: Solution‐based control of microstructure and composition in Ag2Se,” <i>Advanced Energy Materials</i>, vol. 14, no. 22. Wiley, 2024.","ama":"Kleinhanns T, Milillo F, Calcabrini M, et al. A route to high thermoelectric performance: Solution‐based control of microstructure and composition in Ag2Se. <i>Advanced Energy Materials</i>. 2024;14(22). doi:<a href=\"https://doi.org/10.1002/aenm.202400408\">10.1002/aenm.202400408</a>","mla":"Kleinhanns, Tobias, et al. “A Route to High Thermoelectric Performance: Solution‐based Control of Microstructure and Composition in Ag2Se.” <i>Advanced Energy Materials</i>, vol. 14, no. 22, 2400408, Wiley, 2024, doi:<a href=\"https://doi.org/10.1002/aenm.202400408\">10.1002/aenm.202400408</a>.","short":"T. Kleinhanns, F. Milillo, M. Calcabrini, C. Fiedler, S. Horta, D. Balazs, M.J. Strumolo, R. Hasler, J. Llorca, M. Tkadletz, R.L. Brutchey, M. Ibáñez, Advanced Energy Materials 14 (2024).","chicago":"Kleinhanns, Tobias, Francesco Milillo, Mariano Calcabrini, Christine Fiedler, Sharona Horta, Daniel Balazs, Marissa J. Strumolo, et al. “A Route to High Thermoelectric Performance: Solution‐based Control of Microstructure and Composition in Ag2Se.” <i>Advanced Energy Materials</i>. Wiley, 2024. <a href=\"https://doi.org/10.1002/aenm.202400408\">https://doi.org/10.1002/aenm.202400408</a>."},"quality_controlled":"1","external_id":{"isi":["001184300200001"]},"language":[{"iso":"eng"}],"acknowledged_ssus":[{"_id":"EM-Fac"},{"_id":"LifeSc"},{"_id":"NanoFab"}],"oa_version":"Published Version","type":"journal_article","month":"06","article_processing_charge":"Yes (via OA deal)","scopus_import":"1","isi":1,"ddc":["530"],"department":[{"_id":"MaIb"},{"_id":"LifeSc"}],"article_number":"2400408","article_type":"original","_id":"15182","project":[{"name":"HighTE: The Werner Siemens Laboratory for the High Throughput Discovery of Semiconductors for Waste Heat Recovery","_id":"9B8F7476-BA93-11EA-9121-9846C619BF3A"}],"volume":14,"publication_identifier":{"issn":["1614-6832"],"eissn":["1614-6840"]},"doi":"10.1002/aenm.202400408","tmp":{"name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)","short":"CC BY-NC-ND (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","image":"/images/cc_by_nc_nd.png"},"day":"12"},{"quality_controlled":"1","external_id":{"isi":["001187002300001"]},"language":[{"iso":"eng"}],"publication_status":"published","status":"public","date_published":"2024-03-19T00:00:00Z","year":"2024","corr_author":"1","file_date_updated":"2024-03-25T11:28:25Z","citation":{"mla":"Hwong, Yi-Ling, and Caroline J. Muller. “The Unreasonable Efficiency of Total Rain Evaporation Removal in Triggering Convective Self‐aggregation.” <i>Geophysical Research Letters</i>, vol. 51, no. 6, e2023GL106523, Wiley, 2024, doi:<a href=\"https://doi.org/10.1029/2023gl106523\">10.1029/2023gl106523</a>.","apa":"Hwong, Y.-L., &#38; Muller, C. J. (2024). The unreasonable efficiency of total rain evaporation removal in triggering convective self‐aggregation. <i>Geophysical Research Letters</i>. Wiley. <a href=\"https://doi.org/10.1029/2023gl106523\">https://doi.org/10.1029/2023gl106523</a>","ieee":"Y.-L. Hwong and C. J. Muller, “The unreasonable efficiency of total rain evaporation removal in triggering convective self‐aggregation,” <i>Geophysical Research Letters</i>, vol. 51, no. 6. Wiley, 2024.","ama":"Hwong Y-L, Muller CJ. The unreasonable efficiency of total rain evaporation removal in triggering convective self‐aggregation. <i>Geophysical Research Letters</i>. 2024;51(6). doi:<a href=\"https://doi.org/10.1029/2023gl106523\">10.1029/2023gl106523</a>","ista":"Hwong Y-L, Muller CJ. 2024. The unreasonable efficiency of total rain evaporation removal in triggering convective self‐aggregation. Geophysical Research Letters. 51(6), e2023GL106523.","chicago":"Hwong, Yi-Ling, and Caroline J Muller. “The Unreasonable Efficiency of Total Rain Evaporation Removal in Triggering Convective Self‐aggregation.” <i>Geophysical Research Letters</i>. Wiley, 2024. <a href=\"https://doi.org/10.1029/2023gl106523\">https://doi.org/10.1029/2023gl106523</a>.","short":"Y.-L. Hwong, C.J. Muller, Geophysical Research Letters 51 (2024)."},"OA_type":"gold","has_accepted_license":"1","issue":"6","intvolume":"        51","author":[{"last_name":"Hwong","first_name":"Yi-Ling","orcid":"0000-0001-9281-3479","full_name":"Hwong, Yi-Ling","id":"1217aa61-4dd1-11ec-9ac3-f2ba3f17ee22"},{"last_name":"Muller","first_name":"Caroline J","id":"f978ccb0-3f7f-11eb-b193-b0e2bd13182b","orcid":"0000-0001-5836-5350","full_name":"Muller, Caroline J"}],"oa":1,"abstract":[{"lang":"eng","text":"The elimination of rain evaporation in the planetary boundary layer (PBL) has been found to lead to convective self‐aggregation (CSA) even without radiative feedback, but the precise mechanisms underlying this phenomenon remain unclear. We conducted cloud‐resolving simulations with two domain sizes and progressively reduced rain evaporation in the PBL. Surprisingly, CSA only occurred when rain evaporation was almost completely removed. The additional convective heating resulting from the reduction of evaporative cooling in the moist patch was found to be the trigger, thereafter a dry subsidence intrusion into the PBL in the dry patch takes over and sets CSA in motion. Temperature and moisture anomalies oppose each other in their buoyancy effects, hence explaining the need for almost total rain evaporation removal. We also found radiative cooling and not cold pools to be the leading cause for the comparative ease of CSA to take place in the larger domain."}],"OA_place":"publisher","file":[{"creator":"dernst","file_size":1280108,"file_name":"2024_GeophysResLetters_Hwong.pdf","content_type":"application/pdf","relation":"main_file","checksum":"eacb011091a503b9e7b748fef639ba4c","access_level":"open_access","date_updated":"2024-03-25T11:28:25Z","date_created":"2024-03-25T11:28:25Z","success":1,"file_id":"15187"}],"ec_funded":1,"publisher":"Wiley","acknowledgement":"YLH is supported by funding from the European Union's Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie Grant 101034413. CM gratefully acknowledges funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (Project CLUSTER, Grant 805041). The authors warmly thank Steven Sherwood, Jiawei Bao, Bidyut Goswami, and Martin Janssens for stimulating and helpful discussions. They also thank Christopher Holloway and an anonymous reviewer for providing helpful feedback that greatly improved this manuscript.\r\n","date_created":"2024-03-25T10:27:30Z","keyword":["General Earth and Planetary Sciences","Geophysics"],"publication":"Geophysical Research Letters","related_material":{"record":[{"relation":"research_data","id":"19307","status":"public"}]},"title":"The unreasonable efficiency of total rain evaporation removal in triggering convective self‐aggregation","date_updated":"2025-09-04T13:16:39Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publication_identifier":{"issn":["0094-8276"],"eissn":["1944-8007"]},"day":"19","tmp":{"name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)","short":"CC BY-NC-ND (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","image":"/images/cc_by_nc_nd.png"},"doi":"10.1029/2023gl106523","volume":51,"project":[{"name":"IST-BRIDGE: International postdoctoral program","grant_number":"101034413","_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c","call_identifier":"H2020"},{"grant_number":"805041","name":"Organization of CLoUdS, and implications of Tropical  cyclones and for the Energetics of the tropics, in current and waRming climate","_id":"629205d8-2b32-11ec-9570-e1356ff73576","call_identifier":"H2020"}],"_id":"15186","article_type":"original","article_number":" e2023GL106523","isi":1,"ddc":["550"],"scopus_import":"1","department":[{"_id":"CaMu"}],"article_processing_charge":"Yes","DOAJ_listed":"1","oa_version":"Published Version","APC_amount":"2940 EUR","month":"03","type":"journal_article"},{"tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"day":"04","doi":"10.1093/mnras/stae012","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"_id":"15189","volume":528,"article_type":"original","page":"676-692","scopus_import":"1","article_processing_charge":"No","type":"journal_article","month":"01","oa_version":"Published Version","language":[{"iso":"eng"}],"external_id":{"arxiv":["2401.04178"]},"quality_controlled":"1","citation":{"mla":"Galiullin, Ilkham, et al. “A Joint SRG/EROSITA + ZTF Search: Discovery of a 97-Min Period Eclipsing Cataclysmic Variable with Evidence of a Brown Dwarf Secondary.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 528, no. 1, Oxford University Press, 2024, pp. 676–92, doi:<a href=\"https://doi.org/10.1093/mnras/stae012\">10.1093/mnras/stae012</a>.","ieee":"I. Galiullin <i>et al.</i>, “A joint SRG/eROSITA + ZTF search: Discovery of a 97-min period eclipsing cataclysmic variable with evidence of a brown dwarf secondary,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 528, no. 1. Oxford University Press, pp. 676–692, 2024.","apa":"Galiullin, I., Rodriguez, A. C., Kulkarni, S. R., Sunyaev, R., Gilfanov, M., Bikmaev, I., … Vanderbosch, Z. P. (2024). A joint SRG/eROSITA + ZTF search: Discovery of a 97-min period eclipsing cataclysmic variable with evidence of a brown dwarf secondary. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stae012\">https://doi.org/10.1093/mnras/stae012</a>","ama":"Galiullin I, Rodriguez AC, Kulkarni SR, et al. A joint SRG/eROSITA + ZTF search: Discovery of a 97-min period eclipsing cataclysmic variable with evidence of a brown dwarf secondary. <i>Monthly Notices of the Royal Astronomical Society</i>. 2024;528(1):676-692. doi:<a href=\"https://doi.org/10.1093/mnras/stae012\">10.1093/mnras/stae012</a>","ista":"Galiullin I, Rodriguez AC, Kulkarni SR, Sunyaev R, Gilfanov M, Bikmaev I, Yungelson L, van Roestel J, Gänsicke BT, Khamitov I, Szkody P, El-Badry K, Suslikov M, Prince TA, Buntov M, Caiazzo I, Gorbachev M, Graham MJ, Gumerov R, Irtuganov E, Laher RR, Medvedev P, Riddle R, Rusholme B, Sakhibullin N, Sklyanov A, Vanderbosch ZP. 2024. A joint SRG/eROSITA + ZTF search: Discovery of a 97-min period eclipsing cataclysmic variable with evidence of a brown dwarf secondary. Monthly Notices of the Royal Astronomical Society. 528(1), 676–692.","chicago":"Galiullin, Ilkham, Antonio C Rodriguez, Shrinivas R Kulkarni, Rashid Sunyaev, Marat Gilfanov, Ilfan Bikmaev, Lev Yungelson, et al. “A Joint SRG/EROSITA + ZTF Search: Discovery of a 97-Min Period Eclipsing Cataclysmic Variable with Evidence of a Brown Dwarf Secondary.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2024. <a href=\"https://doi.org/10.1093/mnras/stae012\">https://doi.org/10.1093/mnras/stae012</a>.","short":"I. Galiullin, A.C. Rodriguez, S.R. Kulkarni, R. Sunyaev, M. Gilfanov, I. Bikmaev, L. Yungelson, J. van Roestel, B.T. Gänsicke, I. Khamitov, P. Szkody, K. El-Badry, M. Suslikov, T.A. Prince, M. Buntov, I. Caiazzo, M. Gorbachev, M.J. Graham, R. Gumerov, E. Irtuganov, R.R. Laher, P. Medvedev, R. Riddle, B. Rusholme, N. Sakhibullin, A. Sklyanov, Z.P. Vanderbosch, Monthly Notices of the Royal Astronomical Society 528 (2024) 676–692."},"date_published":"2024-01-04T00:00:00Z","year":"2024","status":"public","publication_status":"published","extern":"1","author":[{"first_name":"Ilkham","full_name":"Galiullin, Ilkham","last_name":"Galiullin"},{"full_name":"Rodriguez, Antonio C","first_name":"Antonio C","last_name":"Rodriguez"},{"full_name":"Kulkarni, Shrinivas R","first_name":"Shrinivas R","last_name":"Kulkarni"},{"full_name":"Sunyaev, Rashid","first_name":"Rashid","last_name":"Sunyaev"},{"last_name":"Gilfanov","full_name":"Gilfanov, Marat","first_name":"Marat"},{"first_name":"Ilfan","full_name":"Bikmaev, Ilfan","last_name":"Bikmaev"},{"full_name":"Yungelson, Lev","first_name":"Lev","last_name":"Yungelson"},{"first_name":"Jan","full_name":"van Roestel, Jan","last_name":"van Roestel"},{"full_name":"Gänsicke, Boris T","first_name":"Boris T","last_name":"Gänsicke"},{"last_name":"Khamitov","full_name":"Khamitov, Irek","first_name":"Irek"},{"last_name":"Szkody","first_name":"Paula","full_name":"Szkody, Paula"},{"last_name":"El-Badry","full_name":"El-Badry, Kareem","first_name":"Kareem"},{"last_name":"Suslikov","first_name":"Mikhail","full_name":"Suslikov, Mikhail"},{"last_name":"Prince","full_name":"Prince, Thomas A","first_name":"Thomas A"},{"first_name":"Mikhail","full_name":"Buntov, Mikhail","last_name":"Buntov"},{"last_name":"Caiazzo","first_name":"Ilaria","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","orcid":"0000-0002-4770-5388","full_name":"Caiazzo, Ilaria"},{"last_name":"Gorbachev","first_name":"Mark","full_name":"Gorbachev, Mark"},{"last_name":"Graham","full_name":"Graham, Matthew J","first_name":"Matthew J"},{"full_name":"Gumerov, Rustam","first_name":"Rustam","last_name":"Gumerov"},{"first_name":"Eldar","full_name":"Irtuganov, Eldar","last_name":"Irtuganov"},{"full_name":"Laher, Russ R","first_name":"Russ R","last_name":"Laher"},{"full_name":"Medvedev, Pavel","first_name":"Pavel","last_name":"Medvedev"},{"full_name":"Riddle, Reed","first_name":"Reed","last_name":"Riddle"},{"first_name":"Ben","full_name":"Rusholme, Ben","last_name":"Rusholme"},{"full_name":"Sakhibullin, Nail","first_name":"Nail","last_name":"Sakhibullin"},{"last_name":"Sklyanov","full_name":"Sklyanov, Alexander","first_name":"Alexander"},{"last_name":"Vanderbosch","first_name":"Zachary P","full_name":"Vanderbosch, Zachary P"}],"intvolume":"       528","issue":"1","abstract":[{"text":"Cataclysmic variables (CVs) that have evolved past the period minimum during their lifetimes are predicted to be systems with a brown dwarf donor. While population synthesis models predict that around 40–70 per cent of the Galactic CVs are post-period minimum systems referred to as ‘period bouncers’, only a few dozen confirmed systems are known. We report the study and characterization of a new eclipsing CV, SRGeJ041130.3+685350 (SRGeJ0411), discovered from a joint SRG/eROSITA and ZTF programme. The optical spectrum of SRGeJ0411 shows prominent hydrogen and helium emission lines, typical for CVs. We obtained optical high-speed photometry to confirm the eclipse of SRGeJ0411 and determine the orbital period to be Porb ≈ 97.530 min. The spectral energy distribution suggests that the donor has an effective temperature of ≲ 1800 K. We constrain the donor mass with the period–density relationship for Roche lobe-filling stars and find that Mdonor ≲ 0.04 M⊙. The binary parameters are consistent with evolutionary models for post-period minimum CVs, suggesting that SRGeJ0411 is a new period bouncer. The optical emission lines of SRGeJ0411 are single-peaked despite the system being eclipsing, which is typically only seen due to stream-fed accretion in polars. X-ray spectroscopy hints that the white dwarf in SRGeJ0411 could be magnetic, but verifying the magnetic nature of SRGeJ0411 requires further investigation. The lack of optical outbursts has made SRGeJ0411 elusive in previous surveys, and joint X-ray and optical surveys highlight the potential for discovering similar systems in the near future.","lang":"eng"}],"oa":1,"publisher":"Oxford University Press","title":"A joint SRG/eROSITA + ZTF search: Discovery of a 97-min period eclipsing cataclysmic variable with evidence of a brown dwarf secondary","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"publication":"Monthly Notices of the Royal Astronomical Society","date_created":"2024-03-26T09:43:55Z","arxiv":1,"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stae012"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2024-04-02T06:50:01Z"},{"article_number":"139","article_type":"original","_id":"15191","volume":961,"publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"doi":"10.3847/1538-4357/ad08bf","day":"22","oa_version":"Published Version","type":"journal_article","month":"01","article_processing_charge":"No","scopus_import":"1","intvolume":"       961","issue":"1","author":[{"last_name":"Gerasimov","full_name":"Gerasimov, Roman","first_name":"Roman"},{"last_name":"Burgasser","full_name":"Burgasser, Adam J.","first_name":"Adam J."},{"last_name":"Caiazzo","full_name":"Caiazzo, Ilaria","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","orcid":"0000-0002-4770-5388","first_name":"Ilaria"},{"full_name":"Homeier, Derek","first_name":"Derek","last_name":"Homeier"},{"last_name":"Richer","full_name":"Richer, Harvey B.","first_name":"Harvey B."},{"first_name":"Matteo","full_name":"Correnti, Matteo","last_name":"Correnti"},{"last_name":"Heyl","full_name":"Heyl, Jeremy","first_name":"Jeremy"}],"date_published":"2024-01-22T00:00:00Z","year":"2024","extern":"1","publication_status":"published","status":"public","citation":{"chicago":"Gerasimov, Roman, Adam J. Burgasser, Ilaria Caiazzo, Derek Homeier, Harvey B. Richer, Matteo Correnti, and Jeremy Heyl. “Exploring the Chemistry and Mass Function of the Globular Cluster 47 Tucanae with New Theoretical Color–Magnitude Diagrams.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2024. <a href=\"https://doi.org/10.3847/1538-4357/ad08bf\">https://doi.org/10.3847/1538-4357/ad08bf</a>.","short":"R. Gerasimov, A.J. Burgasser, I. Caiazzo, D. Homeier, H.B. Richer, M. Correnti, J. Heyl, The Astrophysical Journal 961 (2024).","mla":"Gerasimov, Roman, et al. “Exploring the Chemistry and Mass Function of the Globular Cluster 47 Tucanae with New Theoretical Color–Magnitude Diagrams.” <i>The Astrophysical Journal</i>, vol. 961, no. 1, 139, American Astronomical Society, 2024, doi:<a href=\"https://doi.org/10.3847/1538-4357/ad08bf\">10.3847/1538-4357/ad08bf</a>.","ieee":"R. Gerasimov <i>et al.</i>, “Exploring the chemistry and mass function of the globular cluster 47 Tucanae with new theoretical color–magnitude diagrams,” <i>The Astrophysical Journal</i>, vol. 961, no. 1. American Astronomical Society, 2024.","ama":"Gerasimov R, Burgasser AJ, Caiazzo I, et al. Exploring the chemistry and mass function of the globular cluster 47 Tucanae with new theoretical color–magnitude diagrams. <i>The Astrophysical Journal</i>. 2024;961(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/ad08bf\">10.3847/1538-4357/ad08bf</a>","apa":"Gerasimov, R., Burgasser, A. J., Caiazzo, I., Homeier, D., Richer, H. B., Correnti, M., &#38; Heyl, J. (2024). Exploring the chemistry and mass function of the globular cluster 47 Tucanae with new theoretical color–magnitude diagrams. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ad08bf\">https://doi.org/10.3847/1538-4357/ad08bf</a>","ista":"Gerasimov R, Burgasser AJ, Caiazzo I, Homeier D, Richer HB, Correnti M, Heyl J. 2024. Exploring the chemistry and mass function of the globular cluster 47 Tucanae with new theoretical color–magnitude diagrams. The Astrophysical Journal. 961(1), 139."},"quality_controlled":"1","language":[{"iso":"eng"}],"external_id":{"arxiv":["2310.11800"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","arxiv":1,"main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/ad08bf"}],"date_updated":"2024-04-02T06:52:43Z","date_created":"2024-03-26T09:44:50Z","title":"Exploring the chemistry and mass function of the globular cluster 47 Tucanae with new theoretical color–magnitude diagrams","publication":"The Astrophysical Journal","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"publisher":"American Astronomical Society","oa":1,"abstract":[{"text":"Despite their shared origin, members of globular clusters display star-to-star variations in composition. The observed pattern of element abundances is unique to these stellar environments and cannot be fully explained by any proposed mechanism. It remains unclear whether stars form with chemical heterogeneity or inherit it from interactions with other members. These scenarios may be differentiated by the dependence of chemical spread on stellar mass; however, obtaining a sufficiently large mass baseline requires abundance measurements on the lower main sequence, which is too faint for spectroscopy even in the nearest globular clusters. We developed a stellar modeling method to obtain precise chemical abundances for stars near the end of the main sequence from multiband photometry, and we applied it to the globular cluster 47 Tucanae. The computational efficiency is attained by matching chemical elements to the model components that are most sensitive to their abundance. We determined [O/Fe] for ∼5000 members below the main-sequence knee at the level of accuracy, comparable to the spectroscopic measurements of evolved members in the literature. The inferred distribution disfavors stellar interactions as the origin of chemical spread; however, an accurate theory of accretion is required to draw a more definitive conclusion. We anticipate that future observations of 47 Tucanae with the James Webb Space Telescope will extend the mass baseline of our analysis into the substellar regime. Therefore, we present predicted color–magnitude diagrams and mass–magnitude relations for the brown dwarf members of 47 Tucanae.","lang":"eng"}]},{"language":[{"iso":"eng"}],"external_id":{"isi":["001217739200001"],"arxiv":["2310.16701"]},"quality_controlled":"1","citation":{"short":"P. Frankl, J. Pach, D. Pálvölgyi, Journal of Combinatorial Theory, Series A 206 (2024).","chicago":"Frankl, Peter, János Pach, and Dömötör Pálvölgyi. “Odd-Sunflowers.” <i>Journal of Combinatorial Theory, Series A</i>. Elsevier, 2024. <a href=\"https://doi.org/10.1016/j.jcta.2024.105889\">https://doi.org/10.1016/j.jcta.2024.105889</a>.","apa":"Frankl, P., Pach, J., &#38; Pálvölgyi, D. (2024). Odd-sunflowers. <i>Journal of Combinatorial Theory, Series A</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.jcta.2024.105889\">https://doi.org/10.1016/j.jcta.2024.105889</a>","ama":"Frankl P, Pach J, Pálvölgyi D. Odd-sunflowers. <i>Journal of Combinatorial Theory, Series A</i>. 2024;206(8). doi:<a href=\"https://doi.org/10.1016/j.jcta.2024.105889\">10.1016/j.jcta.2024.105889</a>","ieee":"P. Frankl, J. Pach, and D. Pálvölgyi, “Odd-sunflowers,” <i>Journal of Combinatorial Theory, Series A</i>, vol. 206, no. 8. Elsevier, 2024.","ista":"Frankl P, Pach J, Pálvölgyi D. 2024. Odd-sunflowers. Journal of Combinatorial Theory, Series A. 206(8), 105889.","mla":"Frankl, Peter, et al. “Odd-Sunflowers.” <i>Journal of Combinatorial Theory, Series A</i>, vol. 206, no. 8, 105889, Elsevier, 2024, doi:<a href=\"https://doi.org/10.1016/j.jcta.2024.105889\">10.1016/j.jcta.2024.105889</a>."},"corr_author":"1","file_date_updated":"2025-01-09T08:37:20Z","OA_type":"hybrid","status":"public","publication_status":"published","date_published":"2024-08-01T00:00:00Z","year":"2024","has_accepted_license":"1","author":[{"last_name":"Frankl","first_name":"Peter","full_name":"Frankl, Peter"},{"last_name":"Pach","id":"E62E3130-B088-11EA-B919-BF823C25FEA4","full_name":"Pach, János","first_name":"János"},{"full_name":"Pálvölgyi, Dömötör","first_name":"Dömötör","last_name":"Pálvölgyi"}],"issue":"8","license":"https://creativecommons.org/licenses/by-nc/4.0/","intvolume":"       206","OA_place":"publisher","abstract":[{"text":"Extending the notion of sunflowers, we call a family of at least two sets an odd-sunflower if every element of the underlying set is contained in an odd number of sets or in none of them. It follows from the Erdős–Szemerédi conjecture, recently proved by Naslund and Sawin, that there is a constant <2 such that every family of subsets of an n-element set that contains no odd-sunflower consists of at most n sets. We construct such families of size at least 1.5021n. We also characterize minimal odd-sunflowers of triples.","lang":"eng"}],"file":[{"file_id":"18791","date_created":"2025-01-09T08:37:20Z","success":1,"access_level":"open_access","date_updated":"2025-01-09T08:37:20Z","content_type":"application/pdf","relation":"main_file","checksum":"ffc29d65e712849f0d31009271e06a63","creator":"dernst","file_size":366029,"file_name":"2024_JourCombiTheoryA_Frankl.pdf"}],"oa":1,"publisher":"Elsevier","publication":"Journal of Combinatorial Theory, Series A","title":"Odd-sunflowers","acknowledgement":"We are grateful to Balázs Keszegh, and to the members of the Miklós Schweitzer Competition committee of 2022 for valuable discussions, and Shira Zerbib for pointing out several important mathematical typos.","date_created":"2024-03-31T22:01:11Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_updated":"2025-09-04T13:20:39Z","arxiv":1,"doi":"10.1016/j.jcta.2024.105889","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by-nc/4.0/legalcode","image":"/images/cc_by_nc.png","name":"Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)","short":"CC BY-NC (4.0)"},"day":"01","publication_identifier":{"issn":["0097-3165"],"eissn":["1096-0899"]},"volume":206,"_id":"15247","article_type":"original","article_number":"105889","department":[{"_id":"HeEd"}],"isi":1,"ddc":["510"],"scopus_import":"1","article_processing_charge":"No","month":"08","type":"journal_article","oa_version":"Published Version"},{"article_processing_charge":"Yes (via OA deal)","department":[{"_id":"TaHa"}],"ddc":["510"],"isi":1,"scopus_import":"1","month":"05","type":"journal_article","oa_version":"Published Version","volume":443,"project":[{"call_identifier":"H2020","_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c","name":"IST-BRIDGE: International postdoctoral program","grant_number":"101034413"}],"_id":"15248","tmp":{"short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png"},"day":"01","doi":"10.1016/j.aim.2024.109616","publication_identifier":{"eissn":["1090-2082"],"issn":["0001-8708"]},"article_number":"109616","article_type":"original","publisher":"Elsevier","ec_funded":1,"OA_place":"publisher","abstract":[{"text":"Applying the technique of p-adic integration, we prove the topological mirror symmetry conjecture of Hausel-Thaddeus for the moduli spaces of (strongly) parabolic Higgs bundles for the structure groups SLn and PGLn, building on previous work of Groechenig-Wyss-Ziegler on the non-parabolic case. We also prove the E-polynomial of the smooth moduli space of parabolic GLn-Higgs bundles is independent of the degree of the underlying vector bundles.","lang":"eng"}],"file":[{"date_updated":"2024-07-22T12:10:03Z","access_level":"open_access","date_created":"2024-07-22T12:10:03Z","file_id":"17315","success":1,"file_size":702889,"file_name":"2024_AdvancesMath_Shen.pdf","creator":"dernst","checksum":"68f2f08136ccf547891a16a2c0621e97","relation":"main_file","content_type":"application/pdf"}],"oa":1,"arxiv":1,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","date_updated":"2025-09-04T13:21:18Z","publication":"Advances in Mathematics","title":"Mirror symmetry for parabolic Higgs bundles via p-adic integration","acknowledgement":"Shiyu Shen has received funding from the European Union's Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement No. 101034413.","date_created":"2024-03-31T22:01:11Z","corr_author":"1","file_date_updated":"2024-07-22T12:10:03Z","citation":{"mla":"Shen, Shiyu. “Mirror Symmetry for Parabolic Higgs Bundles via P-Adic Integration.” <i>Advances in Mathematics</i>, vol. 443, no. 5, 109616, Elsevier, 2024, doi:<a href=\"https://doi.org/10.1016/j.aim.2024.109616\">10.1016/j.aim.2024.109616</a>.","ama":"Shen S. Mirror symmetry for parabolic Higgs bundles via p-adic integration. <i>Advances in Mathematics</i>. 2024;443(5). doi:<a href=\"https://doi.org/10.1016/j.aim.2024.109616\">10.1016/j.aim.2024.109616</a>","ieee":"S. Shen, “Mirror symmetry for parabolic Higgs bundles via p-adic integration,” <i>Advances in Mathematics</i>, vol. 443, no. 5. Elsevier, 2024.","apa":"Shen, S. (2024). Mirror symmetry for parabolic Higgs bundles via p-adic integration. <i>Advances in Mathematics</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.aim.2024.109616\">https://doi.org/10.1016/j.aim.2024.109616</a>","ista":"Shen S. 2024. Mirror symmetry for parabolic Higgs bundles via p-adic integration. Advances in Mathematics. 443(5), 109616.","chicago":"Shen, Shiyu. “Mirror Symmetry for Parabolic Higgs Bundles via P-Adic Integration.” <i>Advances in Mathematics</i>. Elsevier, 2024. <a href=\"https://doi.org/10.1016/j.aim.2024.109616\">https://doi.org/10.1016/j.aim.2024.109616</a>.","short":"S. Shen, Advances in Mathematics 443 (2024)."},"OA_type":"hybrid","publication_status":"published","status":"public","date_published":"2024-05-01T00:00:00Z","year":"2024","language":[{"iso":"eng"}],"external_id":{"isi":["001216128200001"],"arxiv":["2302.02817"]},"quality_controlled":"1","author":[{"first_name":"Shiyu","full_name":"Shen, Shiyu","id":"544cccd3-9005-11ec-87bc-94aef1c5b814","orcid":"0000-0002-4444-8718","last_name":"Shen"}],"issue":"5","intvolume":"       443","has_accepted_license":"1"}]
