[{"year":"2024","issue":"5","type":"journal_article","corr_author":"1","publication":"Geophysical Research Letters","title":"A pre-monsoon signal of false alarms of Indian monsoon droughts","file":[{"creator":"dernst","access_level":"open_access","file_id":"15178","success":1,"date_updated":"2024-03-25T08:36:00Z","date_created":"2024-03-25T08:36:00Z","content_type":"application/pdf","relation":"main_file","file_size":2887134,"checksum":"243bd966aca968ec7d9e474af8639f8d","file_name":"2024_GeophysResLetters_Goswami.pdf"}],"language":[{"iso":"eng"}],"quality_controlled":"1","scopus_import":"1","date_created":"2024-03-24T23:00:58Z","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","short":"CC BY-NC-ND (4.0)","image":"/images/cc_by_nc_nd.png","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)"},"status":"public","volume":51,"APC_amount":"1470 EUR","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"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.","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>","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>.","ista":"GOSWAMI BB. 2024. A pre-monsoon signal of false alarms of Indian monsoon droughts. Geophysical Research Letters. 51(5), e2023GL106569.","short":"B.B. GOSWAMI, Geophysical Research Letters 51 (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>","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>."},"isi":1,"publication_identifier":{"issn":["0094-8276"],"eissn":["1944-8007"]},"department":[{"_id":"CaMu"}],"OA_place":"publisher","intvolume":"        51","DOAJ_listed":"1","date_published":"2024-03-16T00:00:00Z","article_number":"e2023GL106569","ddc":["550"],"ec_funded":1,"project":[{"call_identifier":"H2020","grant_number":"805041","_id":"629205d8-2b32-11ec-9570-e1356ff73576","name":"Organization of CLoUdS, and implications of Tropical  cyclones and for the Energetics of the tropics, in current and waRming climate"}],"day":"16","_id":"15165","author":[{"id":"3a4ac09c-6d61-11ec-bf66-884cde66b64b","last_name":"Goswami","full_name":"Goswami, Bidyut B","orcid":"0000-0001-8602-3083","first_name":"Bidyut B"}],"publication_status":"published","publisher":"Wiley","external_id":{"isi":["001181635700001"]},"doi":"10.1029/2023GL106569","article_processing_charge":"Yes","abstract":[{"lang":"eng","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."}],"oa":1,"article_type":"original","file_date_updated":"2024-03-25T08:36:00Z","oa_version":"Published Version","month":"03","has_accepted_license":"1","date_updated":"2025-09-04T13:11:41Z","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).","OA_type":"gold"},{"scopus_import":"1","quality_controlled":"1","date_created":"2024-03-24T23:00:58Z","status":"public","volume":383,"citation":{"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>","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.","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>.","ista":"Jakhar N, Ibáñez M. 2024. Electron highways are cooler. Science. 383(6688), 1184.","short":"N. Jakhar, M. Ibáñez, Science 383 (2024) 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>.","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>"},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","pmid":1,"year":"2024","type":"journal_article","issue":"6688","corr_author":"1","publication":"Science","title":"Electron highways are cooler","language":[{"iso":"eng"}],"intvolume":"       383","date_published":"2024-03-14T00:00:00Z","page":"1184","isi":1,"department":[{"_id":"MaIb"}],"publication_identifier":{"issn":["0036-8075"],"eissn":["1095-9203"]},"project":[{"_id":"9B8F7476-BA93-11EA-9121-9846C619BF3A","name":"HighTE: The Werner Siemens Laboratory for the High Throughput Discovery of Semiconductors for Waste Heat Recovery"}],"day":"14","_id":"15166","external_id":{"pmid":["38484066"],"isi":["001273082800019"]},"publisher":"American Association for the Advancement of Science","publication_status":"published","author":[{"full_name":"Navita, Navita","orcid":"0000-0001-7408-8197","first_name":"Navita","id":"6ebe278d-ba0b-11ee-8184-f34cdc671de4","last_name":"Navita"},{"first_name":"Maria","orcid":"0000-0001-5013-2843","full_name":"Ibáñez, Maria","last_name":"Ibáñez","id":"43C61214-F248-11E8-B48F-1D18A9856A87"}],"doi":"10.1126/science.ado4077","article_processing_charge":"No","abstract":[{"text":"Reducing defects boosts room-temperature performance of a thermoelectric device","lang":"eng"}],"month":"03","date_updated":"2025-09-04T13:12:19Z","acknowledgement":"The authors thank the Werner-Siemens-Stiftung and the Institute of Science and Technology Austria for financial support.","article_type":"letter_note","oa_version":"None"},{"date_updated":"2025-09-04T13:07:33Z","month":"03","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2311.14536","open_access":"1"}],"acknowledgement":"We thank Félix Werner and Kris Van Houcke for interesting discussions.","article_type":"original","oa":1,"oa_version":"Preprint","publication_status":"published","_id":"15167","external_id":{"arxiv":["2311.14536"],"isi":["001198511300017"]},"publisher":"American Physical Society","author":[{"last_name":"Al Hyder","id":"d1c405be-ae15-11ed-8510-ccf53278162e","first_name":"Ragheed","full_name":"Al Hyder, Ragheed"},{"last_name":"Chevy","first_name":"F.","full_name":"Chevy, F."},{"full_name":"Leyronas, X.","first_name":"X.","last_name":"Leyronas"}],"day":"19","abstract":[{"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.","lang":"eng"}],"article_processing_charge":"No","doi":"10.1103/PhysRevA.109.033315","intvolume":"       109","arxiv":1,"article_number":"033315","date_published":"2024-03-19T00:00:00Z","department":[{"_id":"MiLe"}],"publication_identifier":{"issn":["2469-9926"],"eissn":["2469-9934"]},"isi":1,"date_created":"2024-03-24T23:00:59Z","scopus_import":"1","quality_controlled":"1","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>.","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>","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.","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>","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.","short":"R. Al Hyder, F. Chevy, X. Leyronas, Physical Review A 109 (2024)."},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","volume":109,"status":"public","type":"journal_article","year":"2024","issue":"3","language":[{"iso":"eng"}],"title":"Exploring beyond-mean-field logarithmic divergences in Fermi-polaron energy","corr_author":"1","publication":"Physical Review A"},{"volume":289,"status":"public","citation":{"chicago":"Filakovský, Marek, Tamio Vesa Nakajima, Jakub Opršal, Gianluca Tasinato, and Uli Wagner. “Hardness of Linearly Ordered 4-Colouring of 3-Colourable 3-Uniform Hypergraphs.” In <i>41st International Symposium on Theoretical Aspects of Computer Science</i>, Vol. 289. Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2024. <a href=\"https://doi.org/10.4230/LIPIcs.STACS.2024.34\">https://doi.org/10.4230/LIPIcs.STACS.2024.34</a>.","ieee":"M. Filakovský, T. V. Nakajima, J. Opršal, G. Tasinato, and U. Wagner, “Hardness of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs,” in <i>41st International Symposium on Theoretical Aspects of Computer Science</i>, Clermont-Ferrand, France, 2024, vol. 289.","apa":"Filakovský, M., Nakajima, T. V., Opršal, J., Tasinato, G., &#38; Wagner, U. (2024). Hardness of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs. In <i>41st International Symposium on Theoretical Aspects of Computer Science</i> (Vol. 289). Clermont-Ferrand, France: Schloss Dagstuhl - Leibniz-Zentrum für Informatik. <a href=\"https://doi.org/10.4230/LIPIcs.STACS.2024.34\">https://doi.org/10.4230/LIPIcs.STACS.2024.34</a>","ama":"Filakovský M, Nakajima TV, Opršal J, Tasinato G, Wagner U. Hardness of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs. In: <i>41st International Symposium on Theoretical Aspects of Computer Science</i>. Vol 289. Schloss Dagstuhl - Leibniz-Zentrum für Informatik; 2024. doi:<a href=\"https://doi.org/10.4230/LIPIcs.STACS.2024.34\">10.4230/LIPIcs.STACS.2024.34</a>","mla":"Filakovský, Marek, et al. “Hardness of Linearly Ordered 4-Colouring of 3-Colourable 3-Uniform Hypergraphs.” <i>41st International Symposium on Theoretical Aspects of Computer Science</i>, vol. 289, 34, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2024, doi:<a href=\"https://doi.org/10.4230/LIPIcs.STACS.2024.34\">10.4230/LIPIcs.STACS.2024.34</a>.","short":"M. Filakovský, T.V. Nakajima, J. Opršal, G. Tasinato, U. Wagner, in:, 41st International Symposium on Theoretical Aspects of Computer Science, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2024.","ista":"Filakovský M, Nakajima TV, Opršal J, Tasinato G, Wagner U. 2024. Hardness of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs. 41st International Symposium on Theoretical Aspects of Computer Science. STACS: Symposium on Theoretical Aspects of Computer Science, LIPIcs, vol. 289, 34."},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","related_material":{"record":[{"status":"public","id":"20339","relation":"dissertation_contains"}]},"quality_controlled":"1","scopus_import":"1","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"date_created":"2024-03-24T23:00:59Z","title":"Hardness of linearly ordered 4-colouring of 3-colourable 3-uniform hypergraphs","corr_author":"1","publication":"41st International Symposium on Theoretical Aspects of Computer Science","language":[{"iso":"eng"}],"file":[{"creator":"dernst","file_id":"15175","access_level":"open_access","success":1,"date_updated":"2024-03-25T07:44:30Z","date_created":"2024-03-25T07:44:30Z","content_type":"application/pdf","file_size":927290,"relation":"main_file","checksum":"0524d4189fd1ed08989546511343edf3","file_name":"2024_LIPICs_Filakovsky.pdf"}],"type":"conference","year":"2024","date_published":"2024-03-01T00:00:00Z","article_number":"34","alternative_title":["LIPIcs"],"arxiv":1,"intvolume":"       289","department":[{"_id":"UlWa"}],"publication_identifier":{"eissn":["1868-8969"],"isbn":["9783959773119"]},"isi":1,"abstract":[{"lang":"eng","text":"A linearly ordered (LO) k-colouring of a hypergraph is a colouring of its vertices with colours 1, … , k such that each edge contains a unique maximal colour. Deciding whether an input hypergraph admits LO k-colouring with a fixed number of colours is NP-complete (and in the special case of graphs, LO colouring coincides with the usual graph colouring). Here, we investigate the complexity of approximating the \"linearly ordered chromatic number\" of a hypergraph. We prove that the following promise problem is NP-complete: Given a 3-uniform hypergraph, distinguish between the case that it is LO 3-colourable, and the case that it is not even LO 4-colourable. We prove this result by a combination of algebraic, topological, and combinatorial methods, building on and extending a topological approach for studying approximate graph colouring introduced by Krokhin, Opršal, Wrochna, and Živný (2023)."}],"article_processing_charge":"No","doi":"10.4230/LIPIcs.STACS.2024.34","conference":{"start_date":"2024-03-12","location":"Clermont-Ferrand, France","name":"STACS: Symposium on Theoretical Aspects of Computer Science","end_date":"2024-03-14"},"day":"01","project":[{"call_identifier":"FWF","grant_number":"P31312","_id":"26611F5C-B435-11E9-9278-68D0E5697425","name":"Algorithms for Embeddings and Homotopy Theory"},{"name":"IST-BRIDGE: International postdoctoral program","_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c","grant_number":"101034413","call_identifier":"H2020"}],"_id":"15168","publication_status":"published","external_id":{"isi":["001300393400034"],"arxiv":["2312.12981"]},"publisher":"Schloss Dagstuhl - Leibniz-Zentrum für Informatik","author":[{"first_name":"Marek","full_name":"Filakovský, Marek","id":"3E8AF77E-F248-11E8-B48F-1D18A9856A87","last_name":"Filakovský"},{"last_name":"Nakajima","first_name":"Tamio Vesa","full_name":"Nakajima, Tamio Vesa"},{"orcid":"0000-0003-1245-3456","full_name":"Opršal, Jakub","first_name":"Jakub","last_name":"Opršal","id":"ec596741-c539-11ec-b829-c79322a91242"},{"last_name":"Tasinato","id":"0433290C-AF8F-11E9-A4C7-F729E6697425","full_name":"Tasinato, Gianluca","first_name":"Gianluca"},{"last_name":"Wagner","id":"36690CA2-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-1494-0568","full_name":"Wagner, Uli","first_name":"Uli"}],"ec_funded":1,"ddc":["510"],"acknowledgement":"Marek Filakovský: This research was supported by Charles University (project PRIMUS/\r\n21/SCI/014), the Austrian Science Fund (FWF project P31312-N35), and MSCAfellow5_MUNI\r\n(CZ.02.01.01/00/22_010/0003229). Tamio-Vesa Nakajima: This research was funded by UKRI EP/X024431/1 and by a Clarendon Fund Scholarship. All data is provided in full in the results section of this paper. Jakub Opršal: This project has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie Grant Agreement No 101034413. Uli Wagner: This research was supported by the Austrian Science Fund (FWF project P31312-N35).","month":"03","date_updated":"2026-04-07T12:36:50Z","has_accepted_license":"1","file_date_updated":"2024-03-25T07:44:30Z","oa_version":"Published Version","oa":1},{"ddc":["000","570"],"_id":"15169","external_id":{"isi":["001190689800001"],"pmid":["38484020"]},"author":[{"first_name":"Chaitanya","full_name":"Chintaluri, Chaitanya","id":"E4EDB536-3485-11EA-98D2-20AF3DDC885E","last_name":"Chintaluri"},{"last_name":"Bejtka","full_name":"Bejtka, Marta","first_name":"Marta"},{"last_name":"Sredniawa","first_name":"Wladyslaw","full_name":"Sredniawa, Wladyslaw"},{"first_name":"Michal","full_name":"Czerwinski, Michal","last_name":"Czerwinski"},{"last_name":"Dzik","first_name":"Jakub M.","full_name":"Dzik, Jakub M."},{"full_name":"Jedrzejewska-Szmek, Joanna","first_name":"Joanna","last_name":"Jedrzejewska-Szmek"},{"last_name":"Wojciki","full_name":"Wojciki, Daniel K.","first_name":"Daniel K."}],"publisher":"Public Library of Science","publication_status":"published","day":"14","abstract":[{"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.","lang":"eng"}],"article_processing_charge":"Yes","doi":"10.1371/journal.pcbi.1011941","oa":1,"article_type":"original","file_date_updated":"2025-06-25T05:47:36Z","oa_version":"Published Version","date_updated":"2025-09-04T13:08:54Z","has_accepted_license":"1","month":"03","OA_type":"gold","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). ","issue":"3","year":"2024","type":"journal_article","pmid":1,"language":[{"iso":"eng"}],"file":[{"relation":"main_file","file_size":2540277,"file_name":"2024_PLoSCompBio_Chintaluri.pdf","checksum":"c09718d0d09614642d877d0716ce32e8","date_created":"2025-06-25T05:47:36Z","date_updated":"2025-06-25T05:47:36Z","content_type":"application/pdf","file_id":"19897","access_level":"open_access","success":1,"creator":"dernst"}],"title":"kCSD-python, reliable current source density estimation with quality control","publication":"PLoS Computational Biology","corr_author":"1","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"date_created":"2024-03-24T23:00:59Z","related_material":{"link":[{"url":"https://github.com/Neuroinflab/kCSD-python","relation":"software"}]},"scopus_import":"1","quality_controlled":"1","citation":{"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>.","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>","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.","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>.","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>","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."},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","volume":20,"status":"public","publication_identifier":{"issn":["1553-734X"],"eissn":["1553-7358"]},"department":[{"_id":"TiVo"}],"isi":1,"OA_place":"publisher","DOAJ_listed":"1","intvolume":"        20","date_published":"2024-03-14T00:00:00Z","article_number":"e1011941"},{"status":"public","volume":964,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"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.","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>.","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.","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).","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>"},"quality_controlled":"1","scopus_import":"1","date_created":"2024-03-24T23:00:59Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"publication":"Astrophysical Journal","title":"UNCOVER spectroscopy confirms the surprising ubiquity of active galactic nuclei in red sources at z > 5","file":[{"creator":"dernst","success":1,"access_level":"open_access","file_id":"15176","content_type":"application/pdf","date_updated":"2024-03-25T08:02:43Z","date_created":"2024-03-25T08:02:43Z","checksum":"389a880e176799d5c062ea7cb82d08c9","file_name":"2024_AstrophysicalJourn_Greene.pdf","relation":"main_file","file_size":2700137}],"language":[{"iso":"eng"}],"type":"journal_article","year":"2024","article_number":"39","date_published":"2024-03-01T00:00:00Z","arxiv":1,"intvolume":"       964","DOAJ_listed":"1","isi":1,"publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"department":[{"_id":"JoMa"}],"doi":"10.3847/1538-4357/ad1e5f","article_processing_charge":"Yes","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"}],"day":"01","_id":"15170","external_id":{"arxiv":["2309.05714"],"isi":["001184746500001"]},"publication_status":"published","publisher":"IOP Publishing","author":[{"last_name":"Greene","first_name":"Jenny E.","full_name":"Greene, Jenny E."},{"first_name":"Ivo","full_name":"Labbe, Ivo","last_name":"Labbe"},{"full_name":"Goulding, Andy D.","first_name":"Andy D.","last_name":"Goulding"},{"first_name":"Lukas J.","full_name":"Furtak, Lukas J.","last_name":"Furtak"},{"last_name":"Chemerynska","first_name":"Iryna","full_name":"Chemerynska, Iryna"},{"last_name":"Kokorev","full_name":"Kokorev, Vasily","first_name":"Vasily"},{"first_name":"Pratika","full_name":"Dayal, Pratika","last_name":"Dayal"},{"first_name":"Marta","full_name":"Volonteri, Marta","last_name":"Volonteri"},{"last_name":"Williams","full_name":"Williams, Christina C.","first_name":"Christina C."},{"first_name":"Bingjie","full_name":"Wang, Bingjie","last_name":"Wang"},{"full_name":"Setton, David J.","first_name":"David J.","last_name":"Setton"},{"first_name":"Adam J.","full_name":"Burgasser, Adam J.","last_name":"Burgasser"},{"full_name":"Bezanson, Rachel","first_name":"Rachel","last_name":"Bezanson"},{"last_name":"Atek","full_name":"Atek, Hakim","first_name":"Hakim"},{"full_name":"Brammer, Gabriel","first_name":"Gabriel","last_name":"Brammer"},{"last_name":"Cutler","full_name":"Cutler, Sam E.","first_name":"Sam E."},{"full_name":"Feldmann, Robert","first_name":"Robert","last_name":"Feldmann"},{"full_name":"Fujimoto, Seiji","first_name":"Seiji","last_name":"Fujimoto"},{"first_name":"Karl","full_name":"Glazebrook, Karl","last_name":"Glazebrook"},{"last_name":"De Graaff","first_name":"Anna","full_name":"De Graaff, Anna"},{"first_name":"Gourav","full_name":"Khullar, 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","full_name":"Maseda, Michael V.","first_name":"Michael V."},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","last_name":"Matthee","first_name":"Jorryt J","full_name":"Matthee, Jorryt J","orcid":"0000-0003-2871-127X"},{"last_name":"Miller","full_name":"Miller, Tim B.","first_name":"Tim B."},{"first_name":"Rohan P.","full_name":"Naidu, Rohan P.","last_name":"Naidu"},{"first_name":"Themiya","full_name":"Nanayakkara, Themiya","last_name":"Nanayakkara"},{"last_name":"Oesch","full_name":"Oesch, Pascal A.","first_name":"Pascal A."},{"full_name":"Pan, Richard","first_name":"Richard","last_name":"Pan"},{"first_name":"Casey","full_name":"Papovich, Casey","last_name":"Papovich"},{"last_name":"Price","first_name":"Sedona H.","full_name":"Price, Sedona H."},{"full_name":"Van Dokkum, Pieter","first_name":"Pieter","last_name":"Van Dokkum"},{"last_name":"Weaver","full_name":"Weaver, John R.","first_name":"John R."},{"full_name":"Whitaker, Katherine E.","first_name":"Katherine E.","last_name":"Whitaker"},{"last_name":"Zitrin","full_name":"Zitrin, Adi","first_name":"Adi"}],"ddc":["550"],"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.","month":"03","has_accepted_license":"1","date_updated":"2025-09-04T13:09:41Z","file_date_updated":"2024-03-25T08:02:43Z","oa_version":"Published Version","oa":1,"article_type":"original"},{"oa_version":"Published Version","file_date_updated":"2025-06-25T08:45:32Z","article_type":"original","oa":1,"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.","OA_type":"hybrid","month":"05","date_updated":"2025-09-04T13:06:06Z","has_accepted_license":"1","ec_funded":1,"ddc":["570"],"abstract":[{"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.","lang":"eng"}],"article_processing_charge":"Yes (via OA deal)","doi":"10.1038/s41593-024-01597-4","day":"01","project":[{"name":"Learning the shape of synaptic plasticity rules for neuronal architectures and function through machine learning.","_id":"0aacfa84-070f-11eb-9043-d7eb2c709234","grant_number":"819603","call_identifier":"H2020"}],"_id":"15171","publisher":"Springer Nature","publication_status":"published","author":[{"last_name":"Agnes","full_name":"Agnes, Everton J.","first_name":"Everton J."},{"full_name":"Vogels, Tim P","orcid":"0000-0003-3295-6181","first_name":"Tim P","id":"CB6FF8D2-008F-11EA-8E08-2637E6697425","last_name":"Vogels"}],"external_id":{"isi":["001190081400001"],"pmid":["38509348 "]},"OA_place":"publisher","publication_identifier":{"issn":["1097-6256"],"eissn":["1546-1726"]},"department":[{"_id":"TiVo"}],"isi":1,"date_published":"2024-05-01T00:00:00Z","page":"964-974","intvolume":"        27","title":"Co-dependent excitatory and inhibitory plasticity accounts for quick, stable and long-lasting memories in biological networks","publication":"Nature Neuroscience","language":[{"iso":"eng"}],"file":[{"creator":"dernst","success":1,"file_id":"19902","access_level":"open_access","content_type":"application/pdf","date_updated":"2025-06-25T08:45:32Z","date_created":"2025-06-25T08:45:32Z","checksum":"dfca68a24749575b912b3a78a7de4516","file_name":"2025_NatureNeuroscience_Agnes.pdf","file_size":10508018,"relation":"main_file"}],"pmid":1,"year":"2024","type":"journal_article","volume":27,"status":"public","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"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>.","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>","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.","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>.","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>","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.","short":"E.J. Agnes, T.P. Vogels, Nature Neuroscience 27 (2024) 964–974."},"quality_controlled":"1","scopus_import":"1","date_created":"2024-03-24T23:01:00Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"}},{"related_material":{"record":[{"relation":"earlier_version","status":"public","id":"14922"}]},"quality_controlled":"1","scopus_import":"1","date_created":"2024-03-24T23:01:00Z","volume":70,"status":"public","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"short":"A.R. Esposito, M. Mondelli, IEEE Transactions on Information Theory 70 (2024) 3823–3839.","ista":"Esposito AR, Mondelli M. 2024. Concentration without independence via information measures. IEEE Transactions on Information Theory. 70(6), 3823–3839.","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>","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>.","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.","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>","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>."},"type":"journal_article","year":"2024","issue":"6","title":"Concentration without independence via information measures","publication":"IEEE Transactions on Information Theory","corr_author":"1","language":[{"iso":"eng"}],"intvolume":"        70","date_published":"2024-06-01T00:00:00Z","page":"3823-3839","arxiv":1,"department":[{"_id":"MaMo"}],"publication_identifier":{"issn":["0018-9448"],"eissn":["1557-9654"]},"isi":1,"day":"01","project":[{"_id":"059876FA-7A3F-11EA-A408-12923DDC885E","name":"Prix Lopez-Loretta 2019 - Marco Mondelli"}],"publication_status":"published","_id":"15172","external_id":{"isi":["001230181100001"],"arxiv":["2303.07245"]},"publisher":"IEEE","author":[{"last_name":"Esposito","id":"9583e921-e1ad-11ec-9862-cef099626dc9","full_name":"Esposito, Amedeo Roberto","first_name":"Amedeo Roberto"},{"first_name":"Marco","full_name":"Mondelli, Marco","orcid":"0000-0002-3242-7020","id":"27EB676C-8706-11E9-9510-7717E6697425","last_name":"Mondelli"}],"abstract":[{"lang":"eng","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."}],"article_processing_charge":"No","doi":"10.1109/TIT.2024.3367767","month":"06","date_updated":"2025-09-04T13:06:53Z","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2303.07245"}],"oa":1,"article_type":"original","oa_version":"Preprint"},{"DOAJ_listed":"1","intvolume":"        10","date_published":"2024-03-01T00:00:00Z","article_number":"adk1992","publication_identifier":{"eissn":["2375-2548"]},"department":[{"_id":"FyKo"}],"isi":1,"OA_place":"publisher","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"date_created":"2024-03-25T08:54:33Z","quality_controlled":"1","scopus_import":"1","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","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>.","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.","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).","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>.","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>","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."},"volume":10,"status":"public","year":"2024","type":"journal_article","issue":"10","pmid":1,"language":[{"iso":"eng"}],"file":[{"creator":"dernst","success":1,"access_level":"open_access","file_id":"15185","content_type":"application/pdf","date_created":"2024-03-25T09:42:10Z","date_updated":"2024-03-25T09:42:10Z","file_name":"2024_ScienceAdv_Palkina.pdf","checksum":"a19c43b260ea0bbaf895a29712e3153c","relation":"main_file","file_size":1499302}],"title":"A hybrid pathway for self-sustained luminescence","publication":"Science Advances","date_updated":"2025-09-04T13:16:05Z","has_accepted_license":"1","month":"03","OA_type":"gold","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).","oa":1,"article_type":"original","oa_version":"Published Version","file_date_updated":"2024-03-25T09:42:10Z","author":[{"full_name":"Palkina, Kseniia A.","first_name":"Kseniia A.","last_name":"Palkina"},{"last_name":"Karataeva","full_name":"Karataeva, Tatiana A.","first_name":"Tatiana A."},{"last_name":"Perfilov","full_name":"Perfilov, Maxim M.","first_name":"Maxim M."},{"first_name":"Liliia I.","full_name":"Fakhranurova, Liliia I.","last_name":"Fakhranurova"},{"full_name":"Markina, Nadezhda M.","first_name":"Nadezhda M.","last_name":"Markina"},{"first_name":"Louisa","orcid":"0000-0001-9139-5383","full_name":"Gonzalez Somermeyer, Louisa","last_name":"Gonzalez Somermeyer","id":"4720D23C-F248-11E8-B48F-1D18A9856A87"},{"last_name":"Garcia-Perez","full_name":"Garcia-Perez, Elena","first_name":"Elena"},{"last_name":"Vazquez-Vilar","full_name":"Vazquez-Vilar, Marta","first_name":"Marta"},{"full_name":"Rodriguez-Rodriguez, Marta","first_name":"Marta","last_name":"Rodriguez-Rodriguez"},{"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","full_name":"Mitiouchkina, Tatiana","first_name":"Tatiana"},{"full_name":"Belozerova, Olga A.","first_name":"Olga A.","last_name":"Belozerova"},{"last_name":"Kovalchuk","first_name":"Sergey I.","full_name":"Kovalchuk, Sergey I."},{"full_name":"Alekberova, Anna","first_name":"Anna","last_name":"Alekberova"},{"last_name":"Malyshevskaia","full_name":"Malyshevskaia, Alena K.","first_name":"Alena K."},{"last_name":"Bugaeva","first_name":"Evgenia N.","full_name":"Bugaeva, Evgenia N."},{"last_name":"Guglya","full_name":"Guglya, Elena B.","first_name":"Elena B."},{"full_name":"Balakireva, Anastasia","first_name":"Anastasia","last_name":"Balakireva"},{"last_name":"Sytov","first_name":"Nikita","full_name":"Sytov, Nikita"},{"last_name":"Bezlikhotnova","first_name":"Anastasia","full_name":"Bezlikhotnova, Anastasia"},{"full_name":"Boldyreva, Daria I.","first_name":"Daria I.","last_name":"Boldyreva"},{"last_name":"Babenko","full_name":"Babenko, Vladislav V.","first_name":"Vladislav V."},{"first_name":"Fyodor","full_name":"Kondrashov, Fyodor","orcid":"0000-0001-8243-4694","id":"44FDEF62-F248-11E8-B48F-1D18A9856A87","last_name":"Kondrashov"},{"last_name":"Choob","full_name":"Choob, Vladimir V.","first_name":"Vladimir V."},{"last_name":"Orzaez","first_name":"Diego","full_name":"Orzaez, Diego"},{"first_name":"Ilia V.","full_name":"Yampolsky, Ilia V.","last_name":"Yampolsky"},{"last_name":"Mishin","full_name":"Mishin, Alexander S.","first_name":"Alexander S."},{"first_name":"Karen S.","full_name":"Sarkisyan, Karen S.","last_name":"Sarkisyan"}],"_id":"15179","external_id":{"isi":["001187580500013"],"pmid":["38457503"]},"publication_status":"published","publisher":"American Association for the Advancement of Science","day":"01","article_processing_charge":"Yes","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"}],"doi":"10.1126/sciadv.adk1992","ddc":["580"]},{"OA_place":"publisher","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"department":[{"_id":"JoMa"}],"isi":1,"article_number":"129","date_published":"2024-03-07T00:00:00Z","intvolume":"       963","language":[{"iso":"eng"}],"file":[{"checksum":"dc7af4694f9f94a551417ab49fa43edf","file_name":"2024_AstrophysicalJourn_Matthee.pdf","file_size":6047536,"relation":"main_file","content_type":"application/pdf","date_updated":"2024-03-25T09:31:58Z","date_created":"2024-03-25T09:31:58Z","success":1,"access_level":"open_access","file_id":"15184","creator":"dernst"}],"title":"Little Red Dots: An abundant population of faint active galactic nuclei at z ∼ 5 revealed by the EIGER and FRESCO JWST surveys","corr_author":"1","publication":"The Astrophysical Journal","year":"2024","type":"journal_article","issue":"2","citation":{"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>.","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>","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).","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.","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>.","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>","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."},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","APC_amount":"5666,27 EUR","volume":963,"status":"public","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"date_created":"2024-03-25T08:54:47Z","related_material":{"link":[{"description":"News on ISTA website","url":"https://ista.ac.at/en/news/baby-quasars-growing-supermassive-black-holes/","relation":"press_release"}]},"scopus_import":"1","quality_controlled":"1","oa_version":"Published Version","file_date_updated":"2024-03-25T09:31:58Z","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"article_type":"original","oa":1,"OA_type":"gold","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_updated":"2025-09-04T13:15:26Z","has_accepted_license":"1","month":"03","ddc":["550"],"article_processing_charge":"Yes","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."}],"doi":"10.3847/1538-4357/ad2345","_id":"15180","publisher":"American Astronomical Society","author":[{"first_name":"Jorryt J","full_name":"Matthee, Jorryt J","orcid":"0000-0003-2871-127X","id":"7439a258-f3c0-11ec-9501-9df22fe06720","last_name":"Matthee"},{"last_name":"Naidu","first_name":"Rohan P.","full_name":"Naidu, Rohan P."},{"last_name":"Brammer","full_name":"Brammer, Gabriel","first_name":"Gabriel"},{"last_name":"Chisholm","first_name":"John","full_name":"Chisholm, John"},{"last_name":"Eilers","full_name":"Eilers, Anna-Christina","first_name":"Anna-Christina"},{"full_name":"Goulding, Andy","first_name":"Andy","last_name":"Goulding"},{"full_name":"Greene, Jenny","first_name":"Jenny","last_name":"Greene"},{"first_name":"Daichi","full_name":"Kashino, Daichi","last_name":"Kashino"},{"first_name":"Ivo","full_name":"Labbe, Ivo","last_name":"Labbe"},{"last_name":"Lilly","full_name":"Lilly, Simon J.","first_name":"Simon J."},{"full_name":"Mackenzie, Ruari","first_name":"Ruari","last_name":"Mackenzie"},{"full_name":"Oesch, Pascal A.","first_name":"Pascal A.","last_name":"Oesch"},{"last_name":"Weibel","first_name":"Andrea","full_name":"Weibel, Andrea"},{"full_name":"Wuyts, Stijn","first_name":"Stijn","last_name":"Wuyts"},{"last_name":"Xiao","full_name":"Xiao, Mengyuan","first_name":"Mengyuan"},{"full_name":"Bordoloi, Rongmon","first_name":"Rongmon","last_name":"Bordoloi"},{"last_name":"Bouwens","full_name":"Bouwens, Rychard","first_name":"Rychard"},{"last_name":"van Dokkum","full_name":"van Dokkum, Pieter","first_name":"Pieter"},{"first_name":"Garth","full_name":"Illingworth, Garth","last_name":"Illingworth"},{"first_name":"Ivan","full_name":"Kramarenko, 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","full_name":"Meyer, Romain A.","first_name":"Romain A."},{"first_name":"Erica J.","full_name":"Nelson, Erica J.","last_name":"Nelson"},{"full_name":"Reddy, Naveen A.","first_name":"Naveen A.","last_name":"Reddy"},{"last_name":"Shivaei","first_name":"Irene","full_name":"Shivaei, Irene"},{"full_name":"Simcoe, Robert A.","first_name":"Robert A.","last_name":"Simcoe"},{"last_name":"Yue","first_name":"Minghao","full_name":"Yue, Minghao"}],"external_id":{"isi":["001184703600001"]},"publication_status":"published","day":"07","project":[{"name":"Young galaxies as tracers and agents of cosmic reionization","_id":"bd9b2118-d553-11ed-ba76-db24564edfea","grant_number":"101076224"}]},{"arxiv":1,"article_number":"013257","date_published":"2024-03-01T00:00:00Z","DOAJ_listed":"1","intvolume":"         6","publication_identifier":{"eissn":["2643-1564"]},"department":[{"_id":"MiLe"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"short":"A. Becker, G. Koutentakis, P. Schmelcher, Physical Review Research 6 (2024).","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.","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>.","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>","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.","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>."},"status":"public","volume":6,"date_created":"2024-03-25T08:57:07Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"quality_controlled":"1","scopus_import":"1","file":[{"success":1,"access_level":"open_access","file_id":"15183","creator":"dernst","file_name":"2024_PhysicalReviewResearch_Becker.pdf","checksum":"4e0e58d1f58386fb016284c84db2a300","relation":"main_file","file_size":2207067,"content_type":"application/pdf","date_created":"2024-03-25T09:24:55Z","date_updated":"2024-03-25T09:24:55Z"}],"language":[{"iso":"eng"}],"publication":"Physical Review Research","title":"Synthetic dimension-induced pseudo Jahn-Teller effect in one-dimensional confined fermions","issue":"1","year":"2024","type":"journal_article","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.","has_accepted_license":"1","date_updated":"2025-05-14T09:32:03Z","month":"03","file_date_updated":"2024-03-25T09:24:55Z","oa_version":"Published Version","oa":1,"article_type":"original","doi":"10.1103/physrevresearch.6.013257","article_processing_charge":"Yes","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."}],"_id":"15181","external_id":{"arxiv":["2310.17995"]},"publication_status":"published","publisher":"American Physical Society","author":[{"full_name":"Becker, A.","first_name":"A.","last_name":"Becker"},{"full_name":"Koutentakis, Georgios","first_name":"Georgios","last_name":"Koutentakis","id":"d7b23d3a-9e21-11ec-b482-f76739596b95"},{"full_name":"Schmelcher, P.","first_name":"P.","last_name":"Schmelcher"}],"project":[{"grant_number":"101034413","call_identifier":"H2020","_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c","name":"IST-BRIDGE: International postdoctoral program"}],"day":"01","ec_funded":1,"ddc":["530"]},{"oa_version":"Published Version","keyword":["General Earth and Planetary Sciences","Geophysics"],"file_date_updated":"2024-03-25T11:28:25Z","article_type":"original","oa":1,"OA_type":"gold","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","has_accepted_license":"1","date_updated":"2025-09-04T13:16:39Z","month":"03","ec_funded":1,"ddc":["550"],"doi":"10.1029/2023gl106523","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."}],"article_processing_charge":"Yes","_id":"15186","external_id":{"isi":["001187002300001"]},"publisher":"Wiley","publication_status":"published","author":[{"orcid":"0000-0001-9281-3479","full_name":"Hwong, Yi-Ling","first_name":"Yi-Ling","last_name":"Hwong","id":"1217aa61-4dd1-11ec-9ac3-f2ba3f17ee22"},{"id":"f978ccb0-3f7f-11eb-b193-b0e2bd13182b","last_name":"Muller","full_name":"Muller, Caroline J","orcid":"0000-0001-5836-5350","first_name":"Caroline J"}],"project":[{"call_identifier":"H2020","grant_number":"101034413","name":"IST-BRIDGE: International postdoctoral program","_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c"},{"call_identifier":"H2020","grant_number":"805041","_id":"629205d8-2b32-11ec-9570-e1356ff73576","name":"Organization of CLoUdS, and implications of Tropical  cyclones and for the Energetics of the tropics, in current and waRming climate"}],"day":"19","OA_place":"publisher","isi":1,"publication_identifier":{"issn":["0094-8276"],"eissn":["1944-8007"]},"department":[{"_id":"CaMu"}],"article_number":" e2023GL106523","date_published":"2024-03-19T00:00:00Z","DOAJ_listed":"1","intvolume":"        51","file":[{"success":1,"file_id":"15187","access_level":"open_access","creator":"dernst","file_name":"2024_GeophysResLetters_Hwong.pdf","checksum":"eacb011091a503b9e7b748fef639ba4c","file_size":1280108,"relation":"main_file","content_type":"application/pdf","date_created":"2024-03-25T11:28:25Z","date_updated":"2024-03-25T11:28:25Z"}],"language":[{"iso":"eng"}],"corr_author":"1","publication":"Geophysical Research Letters","title":"The unreasonable efficiency of total rain evaporation removal in triggering convective self‐aggregation","type":"journal_article","year":"2024","issue":"6","APC_amount":"2940 EUR","citation":{"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.","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>.","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.","short":"Y.-L. Hwong, C.J. Muller, Geophysical Research Letters 51 (2024).","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>.","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>"},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","status":"public","volume":51,"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","short":"CC BY-NC-ND (4.0)","image":"/images/cc_by_nc_nd.png","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)"},"date_created":"2024-03-25T10:27:30Z","scopus_import":"1","quality_controlled":"1","related_material":{"record":[{"id":"19307","status":"public","relation":"research_data"}]}},{"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>.","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>","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.","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>.","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>","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."},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","status":"public","volume":528,"date_created":"2024-03-26T09:43:55Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"scopus_import":"1","quality_controlled":"1","language":[{"iso":"eng"}],"publication":"Monthly Notices of the Royal Astronomical Society","title":"A joint SRG/eROSITA + ZTF search: Discovery of a 97-min period eclipsing cataclysmic variable with evidence of a brown dwarf secondary","year":"2024","issue":"1","type":"journal_article","arxiv":1,"page":"676-692","date_published":"2024-01-04T00:00:00Z","intvolume":"       528","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"doi":"10.1093/mnras/stae012","article_processing_charge":"No","abstract":[{"lang":"eng","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."}],"_id":"15189","author":[{"last_name":"Galiullin","full_name":"Galiullin, Ilkham","first_name":"Ilkham"},{"last_name":"Rodriguez","full_name":"Rodriguez, Antonio C","first_name":"Antonio C"},{"first_name":"Shrinivas R","full_name":"Kulkarni, Shrinivas R","last_name":"Kulkarni"},{"last_name":"Sunyaev","full_name":"Sunyaev, Rashid","first_name":"Rashid"},{"first_name":"Marat","full_name":"Gilfanov, Marat","last_name":"Gilfanov"},{"last_name":"Bikmaev","full_name":"Bikmaev, Ilfan","first_name":"Ilfan"},{"last_name":"Yungelson","first_name":"Lev","full_name":"Yungelson, Lev"},{"last_name":"van Roestel","first_name":"Jan","full_name":"van Roestel, Jan"},{"last_name":"Gänsicke","first_name":"Boris T","full_name":"Gänsicke, Boris T"},{"last_name":"Khamitov","full_name":"Khamitov, Irek","first_name":"Irek"},{"full_name":"Szkody, Paula","first_name":"Paula","last_name":"Szkody"},{"full_name":"El-Badry, Kareem","first_name":"Kareem","last_name":"El-Badry"},{"first_name":"Mikhail","full_name":"Suslikov, Mikhail","last_name":"Suslikov"},{"last_name":"Prince","full_name":"Prince, Thomas A","first_name":"Thomas A"},{"full_name":"Buntov, Mikhail","first_name":"Mikhail","last_name":"Buntov"},{"first_name":"Ilaria","orcid":"0000-0002-4770-5388","full_name":"Caiazzo, Ilaria","last_name":"Caiazzo","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d"},{"last_name":"Gorbachev","first_name":"Mark","full_name":"Gorbachev, Mark"},{"last_name":"Graham","full_name":"Graham, Matthew J","first_name":"Matthew J"},{"last_name":"Gumerov","full_name":"Gumerov, Rustam","first_name":"Rustam"},{"last_name":"Irtuganov","first_name":"Eldar","full_name":"Irtuganov, Eldar"},{"last_name":"Laher","first_name":"Russ R","full_name":"Laher, Russ R"},{"first_name":"Pavel","full_name":"Medvedev, Pavel","last_name":"Medvedev"},{"last_name":"Riddle","full_name":"Riddle, Reed","first_name":"Reed"},{"full_name":"Rusholme, Ben","first_name":"Ben","last_name":"Rusholme"},{"last_name":"Sakhibullin","first_name":"Nail","full_name":"Sakhibullin, Nail"},{"first_name":"Alexander","full_name":"Sklyanov, Alexander","last_name":"Sklyanov"},{"last_name":"Vanderbosch","first_name":"Zachary P","full_name":"Vanderbosch, Zachary P"}],"publisher":"Oxford University Press","publication_status":"published","external_id":{"arxiv":["2401.04178"]},"extern":"1","day":"04","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stae012","open_access":"1"}],"date_updated":"2024-04-02T06:50:01Z","month":"01","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"oa_version":"Published Version","article_type":"original","oa":1},{"quality_controlled":"1","scopus_import":"1","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"date_created":"2024-03-26T09:44:50Z","volume":961,"status":"public","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"short":"R. Gerasimov, A.J. Burgasser, I. Caiazzo, D. Homeier, H.B. Richer, M. Correnti, J. Heyl, The Astrophysical Journal 961 (2024).","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.","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>.","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>","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.","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>."},"issue":"1","type":"journal_article","year":"2024","title":"Exploring the chemistry and mass function of the globular cluster 47 Tucanae with new theoretical color–magnitude diagrams","publication":"The Astrophysical Journal","language":[{"iso":"eng"}],"intvolume":"       961","article_number":"139","date_published":"2024-01-22T00:00:00Z","arxiv":1,"publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"day":"22","extern":"1","_id":"15191","publisher":"American Astronomical Society","external_id":{"arxiv":["2310.11800"]},"author":[{"last_name":"Gerasimov","first_name":"Roman","full_name":"Gerasimov, Roman"},{"last_name":"Burgasser","first_name":"Adam J.","full_name":"Burgasser, Adam J."},{"id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","last_name":"Caiazzo","first_name":"Ilaria","full_name":"Caiazzo, Ilaria","orcid":"0000-0002-4770-5388"},{"last_name":"Homeier","full_name":"Homeier, Derek","first_name":"Derek"},{"first_name":"Harvey B.","full_name":"Richer, Harvey B.","last_name":"Richer"},{"full_name":"Correnti, Matteo","first_name":"Matteo","last_name":"Correnti"},{"last_name":"Heyl","first_name":"Jeremy","full_name":"Heyl, Jeremy"}],"publication_status":"published","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"}],"article_processing_charge":"No","doi":"10.3847/1538-4357/ad08bf","month":"01","date_updated":"2024-04-02T06:52:43Z","main_file_link":[{"url":"https://doi.org/10.3847/1538-4357/ad08bf","open_access":"1"}],"article_type":"original","oa":1,"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"oa_version":"Published Version"},{"title":"Odd-sunflowers","corr_author":"1","publication":"Journal of Combinatorial Theory, Series A","language":[{"iso":"eng"}],"file":[{"file_name":"2024_JourCombiTheoryA_Frankl.pdf","checksum":"ffc29d65e712849f0d31009271e06a63","relation":"main_file","file_size":366029,"content_type":"application/pdf","date_created":"2025-01-09T08:37:20Z","date_updated":"2025-01-09T08:37:20Z","success":1,"file_id":"18791","access_level":"open_access","creator":"dernst"}],"type":"journal_article","issue":"8","year":"2024","volume":206,"status":"public","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"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>","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>.","short":"P. Frankl, J. Pach, D. Pálvölgyi, Journal of Combinatorial Theory, Series A 206 (2024).","ista":"Frankl P, Pach J, Pálvölgyi D. 2024. Odd-sunflowers. Journal of Combinatorial Theory, Series A. 206(8), 105889.","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>.","ieee":"P. Frankl, J. Pach, and D. Pálvölgyi, “Odd-sunflowers,” <i>Journal of Combinatorial Theory, Series A</i>, vol. 206, no. 8. Elsevier, 2024.","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>"},"quality_controlled":"1","scopus_import":"1","date_created":"2024-03-31T22:01:11Z","tmp":{"short":"CC BY-NC (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc/4.0/legalcode","name":"Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)","image":"/images/cc_by_nc.png"},"OA_place":"publisher","department":[{"_id":"HeEd"}],"publication_identifier":{"eissn":["1096-0899"],"issn":["0097-3165"]},"isi":1,"date_published":"2024-08-01T00:00:00Z","article_number":"105889","arxiv":1,"intvolume":"       206","ddc":["510"],"abstract":[{"lang":"eng","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."}],"article_processing_charge":"No","doi":"10.1016/j.jcta.2024.105889","day":"01","author":[{"last_name":"Frankl","full_name":"Frankl, Peter","first_name":"Peter"},{"first_name":"János","full_name":"Pach, János","last_name":"Pach","id":"E62E3130-B088-11EA-B919-BF823C25FEA4"},{"first_name":"Dömötör","full_name":"Pálvölgyi, Dömötör","last_name":"Pálvölgyi"}],"_id":"15247","publication_status":"published","publisher":"Elsevier","external_id":{"isi":["001217739200001"],"arxiv":["2310.16701"]},"oa_version":"Published Version","file_date_updated":"2025-01-09T08:37:20Z","article_type":"original","oa":1,"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.","OA_type":"hybrid","month":"08","date_updated":"2025-09-04T13:20:39Z","has_accepted_license":"1"},{"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"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>","ieee":"S. Shen, “Mirror symmetry for parabolic Higgs bundles via p-adic integration,” <i>Advances in Mathematics</i>, vol. 443, no. 5. Elsevier, 2024.","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>.","ista":"Shen S. 2024. Mirror symmetry for parabolic Higgs bundles via p-adic integration. Advances in Mathematics. 443(5), 109616.","short":"S. Shen, Advances in Mathematics 443 (2024).","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>"},"status":"public","volume":443,"date_created":"2024-03-31T22:01:11Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"scopus_import":"1","quality_controlled":"1","file":[{"success":1,"file_id":"17315","access_level":"open_access","creator":"dernst","file_name":"2024_AdvancesMath_Shen.pdf","checksum":"68f2f08136ccf547891a16a2c0621e97","relation":"main_file","file_size":702889,"content_type":"application/pdf","date_created":"2024-07-22T12:10:03Z","date_updated":"2024-07-22T12:10:03Z"}],"language":[{"iso":"eng"}],"corr_author":"1","publication":"Advances in Mathematics","title":"Mirror symmetry for parabolic Higgs bundles via p-adic integration","issue":"5","year":"2024","type":"journal_article","arxiv":1,"date_published":"2024-05-01T00:00:00Z","article_number":"109616","intvolume":"       443","OA_place":"publisher","isi":1,"department":[{"_id":"TaHa"}],"publication_identifier":{"issn":["0001-8708"],"eissn":["1090-2082"]},"doi":"10.1016/j.aim.2024.109616","article_processing_charge":"Yes (via OA deal)","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"}],"_id":"15248","publication_status":"published","author":[{"orcid":"0000-0002-4444-8718","full_name":"Shen, Shiyu","first_name":"Shiyu","last_name":"Shen","id":"544cccd3-9005-11ec-87bc-94aef1c5b814"}],"publisher":"Elsevier","external_id":{"arxiv":["2302.02817"],"isi":["001216128200001"]},"project":[{"_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c","name":"IST-BRIDGE: International postdoctoral program","call_identifier":"H2020","grant_number":"101034413"}],"day":"01","ec_funded":1,"ddc":["510"],"OA_type":"hybrid","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.","has_accepted_license":"1","date_updated":"2025-09-04T13:21:18Z","month":"05","file_date_updated":"2024-07-22T12:10:03Z","oa_version":"Published Version","oa":1,"article_type":"original"},{"OA_place":"publisher","publication_identifier":{"issn":["0035-8711"],"eissn":["1365-2966"]},"department":[{"_id":"JoMa"}],"isi":1,"arxiv":1,"page":"2794-2806","date_published":"2024-04-01T00:00:00Z","DOAJ_listed":"1","intvolume":"       529","language":[{"iso":"eng"}],"file":[{"content_type":"application/pdf","date_updated":"2024-04-02T08:42:17Z","date_created":"2024-04-02T08:42:17Z","checksum":"1e65c40a71e565eebdc4c5ff11822ba2","file_name":"2024_MonthlyNRoyalAstronSoc_Matthee.pdf","relation":"main_file","file_size":2626735,"creator":"dernst","success":1,"file_id":"15255","access_level":"open_access"}],"title":"Large-scale excess H I absorption around z ≈ 4 galaxies detected in a background galaxy spectrum in the MUSE eXtremely deep field","corr_author":"1","publication":"Monthly Notices of the Royal Astronomical Society","issue":"3","type":"journal_article","year":"2024","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"apa":"Matthee, J. J., Golling, C., Mackenzie, R., Pezzulli, G., Lilly, S., Schaye, J., … Wisotzki, L. (2024). Large-scale excess H I absorption around z ≈ 4 galaxies detected in a background galaxy spectrum in the MUSE eXtremely deep field. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stae673\">https://doi.org/10.1093/mnras/stae673</a>","ieee":"J. J. Matthee <i>et al.</i>, “Large-scale excess H I absorption around z ≈ 4 galaxies detected in a background galaxy spectrum in the MUSE eXtremely deep field,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 529, no. 3. Oxford University Press, pp. 2794–2806, 2024.","chicago":"Matthee, Jorryt J, Christopher Golling, Ruari Mackenzie, Gabriele Pezzulli, Simon Lilly, Joop Schaye, Roland Bacon, et al. “Large-Scale Excess H I Absorption around z ≈ 4 Galaxies Detected in a Background Galaxy Spectrum in the MUSE EXtremely Deep Field.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2024. <a href=\"https://doi.org/10.1093/mnras/stae673\">https://doi.org/10.1093/mnras/stae673</a>.","short":"J.J. Matthee, C. Golling, R. Mackenzie, G. Pezzulli, S. Lilly, J. Schaye, R. Bacon, H. Kusakabe, T. Urrutia, L. Boogaard, J. Brinchmann, M.V. Maseda, T. Garel, N.F. Bouché, L. Wisotzki, Monthly Notices of the Royal Astronomical Society 529 (2024) 2794–2806.","ista":"Matthee JJ, Golling C, Mackenzie R, Pezzulli G, Lilly S, Schaye J, Bacon R, Kusakabe H, Urrutia T, Boogaard L, Brinchmann J, Maseda MV, Garel T, Bouché NF, Wisotzki L. 2024. Large-scale excess H I absorption around z ≈ 4 galaxies detected in a background galaxy spectrum in the MUSE eXtremely deep field. Monthly Notices of the Royal Astronomical Society. 529(3), 2794–2806.","mla":"Matthee, Jorryt J., et al. “Large-Scale Excess H I Absorption around z ≈ 4 Galaxies Detected in a Background Galaxy Spectrum in the MUSE EXtremely Deep Field.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 529, no. 3, Oxford University Press, 2024, pp. 2794–806, doi:<a href=\"https://doi.org/10.1093/mnras/stae673\">10.1093/mnras/stae673</a>.","ama":"Matthee JJ, Golling C, Mackenzie R, et al. Large-scale excess H I absorption around z ≈ 4 galaxies detected in a background galaxy spectrum in the MUSE eXtremely deep field. <i>Monthly Notices of the Royal Astronomical Society</i>. 2024;529(3):2794-2806. doi:<a href=\"https://doi.org/10.1093/mnras/stae673\">10.1093/mnras/stae673</a>"},"volume":529,"status":"public","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"date_created":"2024-03-31T22:01:12Z","quality_controlled":"1","scopus_import":"1","file_date_updated":"2024-04-02T08:42:17Z","oa_version":"Published Version","article_type":"original","oa":1,"OA_type":"gold","acknowledgement":"We thank the referee for constructive comments that helped improving the paper. Based on observations collected at the European Southern Observatory under ESO programme 1101.A-0127. 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. GP acknowledges support from the Netherlands Research School for Astronomy (Nederlandse Onderzoekschool Voor Astronomie, NOVA). JB acknowledges financial support from the Fundação para a Ciência e a Tecnologia (FCT) through national funds PTDC/FIS-AST/4862/2020, work contract 2020.03379.CEECIND, and research grants UIDB/04434/2020 and UIDP/04434/2020. TU and LW acknowledge funding by the European Research Council through ERC-AdG SPECMAP-CGM, GA 101020943. TG is supported by the ERC Starting grant 757258 ‘TRIPLE’.","date_updated":"2025-09-04T13:18:02Z","has_accepted_license":"1","month":"04","ddc":["520"],"article_processing_charge":"Yes","abstract":[{"text":"Observationally mapping the relation between galaxies and the intergalactic medium (IGM) is of key interest for studies of cosmic reionization. Diffuse hydrogen gas has typically been observed in H I Lyman-α (Lyα) absorption in the spectra of bright background quasars. However, it is important to extend these measurements to background galaxies as quasars become increasingly rare at high redshift and rarely probe closely separated sight lines. Here, we use deep integral field spectroscopy in the MUSE eXtremely Deep Field to demonstrate the measurement of the Lyα transmission at z ≈ 4 in absorption to a background galaxy at z = 4.77. The H I transmission is consistent with independent quasar sight lines at similar redshifts. Exploiting the high number of spectroscopic redshifts of faint galaxies (500 between z = 4.0–4.7 within a radius of 8 arcmin) that are tracers of the density field, we show that Lyα transmission is inversely correlated with galaxy density, i.e. transparent regions in the Lyα forest mark underdense regions at z ≈ 4. Due to large-scale clustering, galaxies are surrounded by excess H I absorption over the cosmic mean out to 4 cMpc/h70. We also find that redshifts from the peak of the Lyα line are typically offset from the systemic redshift by +170 km s−1. This work extends results from z ≈ 2–3 to higher redshifts and demonstrates the power of deep integral field spectroscopy to simultaneously measure the ionization structure of the IGM and the large-scale density field in the early Universe.","lang":"eng"}],"doi":"10.1093/mnras/stae673","publication_status":"published","_id":"15249","author":[{"orcid":"0000-0003-2871-127X","full_name":"Matthee, Jorryt J","first_name":"Jorryt J","last_name":"Matthee","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"last_name":"Golling","full_name":"Golling, Christopher","first_name":"Christopher"},{"first_name":"Ruari","full_name":"Mackenzie, Ruari","last_name":"Mackenzie"},{"full_name":"Pezzulli, Gabriele","first_name":"Gabriele","last_name":"Pezzulli"},{"last_name":"Lilly","full_name":"Lilly, Simon","first_name":"Simon"},{"full_name":"Schaye, Joop","first_name":"Joop","last_name":"Schaye"},{"first_name":"Roland","full_name":"Bacon, Roland","last_name":"Bacon"},{"first_name":"Haruka","full_name":"Kusakabe, Haruka","last_name":"Kusakabe"},{"last_name":"Urrutia","full_name":"Urrutia, Tanya","first_name":"Tanya"},{"full_name":"Boogaard, Leindert","first_name":"Leindert","last_name":"Boogaard"},{"first_name":"Jarle","full_name":"Brinchmann, Jarle","last_name":"Brinchmann"},{"last_name":"Maseda","first_name":"Michael V.","full_name":"Maseda, Michael V."},{"full_name":"Garel, Thibault","first_name":"Thibault","last_name":"Garel"},{"last_name":"Bouché","first_name":"Nicolas F.","full_name":"Bouché, Nicolas F."},{"first_name":"Lutz","full_name":"Wisotzki, Lutz","last_name":"Wisotzki"}],"publisher":"Oxford University Press","external_id":{"isi":["001188770300019"],"arxiv":["2305.15346"]},"day":"01","project":[{"name":"Young galaxies as tracers and agents of cosmic reionization","_id":"bd9b2118-d553-11ed-ba76-db24564edfea","grant_number":"101076224"}]},{"article_number":"e2319686121","date_published":"2024-03-26T00:00:00Z","intvolume":"       121","department":[{"_id":"DaSi"}],"publication_identifier":{"eissn":["1091-6490"]},"isi":1,"acknowledged_ssus":[{"_id":"Bio"}],"volume":121,"status":"public","citation":{"chicago":"Boytsov, Danila, Gregor M. Madej, Georg Horn, Nadine Blaha, Thomas Köcher, Harald H. Sitte, Daria E Siekhaus, Christine Ziegler, Walter Sandtner, and Marko Roblek. “Orphan Lysosomal Solute Carrier MFSD1 Facilitates Highly Selective Dipeptide Transport.” <i>Proceedings of the National Academy of Sciences of the United States of America</i>. National Academy of Sciences, 2024. <a href=\"https://doi.org/10.1073/pnas.2319686121\">https://doi.org/10.1073/pnas.2319686121</a>.","apa":"Boytsov, D., Madej, G. M., Horn, G., Blaha, N., Köcher, T., Sitte, H. H., … Roblek, M. (2024). Orphan lysosomal solute carrier MFSD1 facilitates highly selective dipeptide transport. <i>Proceedings of the National Academy of Sciences of the United States of America</i>. National Academy of Sciences. <a href=\"https://doi.org/10.1073/pnas.2319686121\">https://doi.org/10.1073/pnas.2319686121</a>","ieee":"D. Boytsov <i>et al.</i>, “Orphan lysosomal solute carrier MFSD1 facilitates highly selective dipeptide transport,” <i>Proceedings of the National Academy of Sciences of the United States of America</i>, vol. 121, no. 13. National Academy of Sciences, 2024.","mla":"Boytsov, Danila, et al. “Orphan Lysosomal Solute Carrier MFSD1 Facilitates Highly Selective Dipeptide Transport.” <i>Proceedings of the National Academy of Sciences of the United States of America</i>, vol. 121, no. 13, e2319686121, National Academy of Sciences, 2024, doi:<a href=\"https://doi.org/10.1073/pnas.2319686121\">10.1073/pnas.2319686121</a>.","ama":"Boytsov D, Madej GM, Horn G, et al. Orphan lysosomal solute carrier MFSD1 facilitates highly selective dipeptide transport. <i>Proceedings of the National Academy of Sciences of the United States of America</i>. 2024;121(13). doi:<a href=\"https://doi.org/10.1073/pnas.2319686121\">10.1073/pnas.2319686121</a>","short":"D. Boytsov, G.M. Madej, G. Horn, N. Blaha, T. Köcher, H.H. Sitte, D.E. Siekhaus, C. Ziegler, W. Sandtner, M. Roblek, Proceedings of the National Academy of Sciences of the United States of America 121 (2024).","ista":"Boytsov D, Madej GM, Horn G, Blaha N, Köcher T, Sitte HH, Siekhaus DE, Ziegler C, Sandtner W, Roblek M. 2024. Orphan lysosomal solute carrier MFSD1 facilitates highly selective dipeptide transport. Proceedings of the National Academy of Sciences of the United States of America. 121(13), e2319686121."},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","scopus_import":"1","quality_controlled":"1","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"date_created":"2024-03-31T22:01:12Z","title":"Orphan lysosomal solute carrier MFSD1 facilitates highly selective dipeptide transport","publication":"Proceedings of the National Academy of Sciences of the United States of America","corr_author":"1","language":[{"iso":"eng"}],"file":[{"content_type":"application/pdf","date_updated":"2024-04-02T08:54:28Z","date_created":"2024-04-02T08:54:28Z","checksum":"06f9e60b1146a685d58bf33999422fa8","file_name":"2024_PNAS_Boytsov.pdf","file_size":2483787,"relation":"main_file","creator":"dernst","success":1,"file_id":"15256","access_level":"open_access"}],"pmid":1,"year":"2024","issue":"13","type":"journal_article","acknowledgement":"We thank the Metabolomics Facility at Vienna BioCenter Core Facilities, which is a member of the Vienna BioCenter and funded by the City of Vienna through the Vienna Business Agency (shared research facility), for the LC–MS/MS analysis; and the BioImaging Facility at IST Austria for technical support and assistance. The authors want to thank N. Kastner for help with the live  cell  imaging  and  A.  Korošec  for  help  with  flow  cytometry.  This  work  was  supported by the Austrian Science Fund (FWF), grant P 36621- B (to M.R.), grant P 36667 (to W.S.), and core funding from IST Austria (to D.S.).","month":"03","date_updated":"2025-09-04T13:19:02Z","has_accepted_license":"1","oa_version":"Published Version","file_date_updated":"2024-04-02T08:54:28Z","oa":1,"article_type":"original","abstract":[{"text":"Orphan solute carrier (SLC) represents a group of membrane transporters whose exact functions and substrate specificities are not known. Elucidating the function and regulation of orphan SLC transporters is not only crucial for advancing our knowledge of cellular and molecular biology but can potentially lead to the development of new therapeutic strategies. Here, we provide evidence for the biological function of a ubiquitous orphan lysosomal SLC, the Major Facilitator Superfamily Domain-containing Protein 1 (MFSD1), which has remained phylogenetically unassigned. Targeted metabolomics revealed that dipeptides containing either lysine or arginine residues accumulate in lysosomes of cells lacking MFSD1. Whole-cell patch-clamp electrophysiological recordings of HEK293-cells expressing MFSD1 on the cell surface displayed transport affinities for positively charged dipeptides in the lower mM range, while dipeptides that carry a negative net charge were not transported. This was also true for single amino acids and tripeptides, which MFSD1 failed to transport. Our results identify MFSD1 as a highly selective lysosomal lysine/arginine/histidine-containing dipeptide exporter, which functions as a uniporter.","lang":"eng"}],"article_processing_charge":"Yes (in subscription journal)","doi":"10.1073/pnas.2319686121","day":"26","author":[{"first_name":"Danila","full_name":"Boytsov, Danila","last_name":"Boytsov"},{"last_name":"Madej","full_name":"Madej, Gregor M.","first_name":"Gregor M."},{"last_name":"Horn","full_name":"Horn, Georg","first_name":"Georg"},{"first_name":"Nadine","full_name":"Blaha, Nadine","last_name":"Blaha"},{"last_name":"Köcher","full_name":"Köcher, Thomas","first_name":"Thomas"},{"last_name":"Sitte","first_name":"Harald H.","full_name":"Sitte, Harald H."},{"first_name":"Daria E","orcid":"0000-0001-8323-8353","full_name":"Siekhaus, Daria E","last_name":"Siekhaus","id":"3D224B9E-F248-11E8-B48F-1D18A9856A87"},{"first_name":"Christine","full_name":"Ziegler, Christine","last_name":"Ziegler"},{"first_name":"Walter","full_name":"Sandtner, Walter","last_name":"Sandtner"},{"full_name":"Roblek, Marko","orcid":"0000-0001-9588-1389","first_name":"Marko","id":"3047D808-F248-11E8-B48F-1D18A9856A87","last_name":"Roblek"}],"_id":"15250","external_id":{"isi":["001206419000003"],"pmid":["38507452"]},"publication_status":"published","publisher":"National Academy of Sciences","ddc":["570"]},{"month":"03","date_updated":"2025-09-04T13:19:48Z","acknowledgement":"We thank the Cryo-EM Center of the University of Science and Technology of China for the EM facility support, Y. Yin (Iowa State University, Ames, IA, USA) for providing the anti-BES1 antibody, Y. Gao and all other staff members for their technical support on cryo-EM data collection, S. Vanneste (VIB, Ghent University, Ghent, Belgium) for useful discussions, and M. De Cock for help in preparing the manuscript.\r\nThis work was supported by the National Natural Science Foundation of China (grants 31870732 and 32322041 to L.S., grant 31900885 to X.L., and grant 32321001 to L.S.); the Strategic Priority Research Program of the Chinese Academy of Sciences (grant XDB37020103 to L.S.); the Natural Science Foundation of Anhui Province (grant 2008085MC90 to X.L. and grant 2008085J15 to L.S.); Fundamental Research Funds for the Central Universities (grant WK9100000031 to L.S.); USTC Research Funds of the Double First-Class Initiative (grant YD9100002004 to L.S. and grant YD9100002020 to X.L.); Research Foundation-Flanders (grant G002121N to E.R. and postdoctoral fellowships 12R7822N and 12R7819N to N.V.); and Chinese Scholarship Council predoctoral fellowships (Y.W. and H.Z.). L.S. is supported by an Outstanding Young Scholar Award from the Qiu Shi Science and Technologies Foundation and a Young Scholar Award from the Cyrus Tang Foundation.","main_file_link":[{"open_access":"1","url":"http://hdl.handle.net/1854/LU-01HTMBK3P3PPNB73YFCMFXP3ZZ"}],"OA_type":"green","oa":1,"article_type":"original","oa_version":"Submitted Version","day":"22","_id":"15251","external_id":{"isi":["001252955200028"],"pmid":["38513023"]},"publisher":"American Association for the Advancement of Science","author":[{"last_name":"Ying","full_name":"Ying, Wei","first_name":"Wei"},{"first_name":"Yaowei","full_name":"Wang, Yaowei","last_name":"Wang"},{"full_name":"Wei, Hong","first_name":"Hong","last_name":"Wei"},{"last_name":"Luo","full_name":"Luo, Yongming","first_name":"Yongming"},{"last_name":"Ma","first_name":"Qian","full_name":"Ma, Qian"},{"last_name":"Zhu","first_name":"Heyuan","full_name":"Zhu, Heyuan"},{"last_name":"Janssens","first_name":"Hilde","full_name":"Janssens, Hilde"},{"last_name":"Vukašinović","full_name":"Vukašinović, Nemanja","first_name":"Nemanja"},{"full_name":"Kvasnica, Miroslav","first_name":"Miroslav","last_name":"Kvasnica"},{"first_name":"Johan M.","full_name":"Winne, Johan M.","last_name":"Winne"},{"first_name":"Yongxiang","full_name":"Gao, Yongxiang","last_name":"Gao"},{"first_name":"Shutang","full_name":"Tan, Shutang","orcid":"0000-0002-0471-8285","id":"2DE75584-F248-11E8-B48F-1D18A9856A87","last_name":"Tan"},{"first_name":"Jiří","orcid":"0000-0002-8302-7596","full_name":"Friml, Jiří","last_name":"Friml","id":"4159519E-F248-11E8-B48F-1D18A9856A87"},{"last_name":"Liu","full_name":"Liu, Xin","first_name":"Xin"},{"first_name":"Eugenia","full_name":"Russinova, Eugenia","last_name":"Russinova"},{"first_name":"Linfeng","full_name":"Sun, Linfeng","last_name":"Sun"}],"publication_status":"published","article_processing_charge":"No","abstract":[{"lang":"eng","text":"Brassinosteroids are steroidal phytohormones that regulate plant development and physiology, including adaptation to environmental stresses. Brassinosteroids are synthesized in the cell interior but bind receptors at the cell surface, necessitating a yet to be identified export mechanism. Here, we show that a member of the ATP-binding cassette (ABC) transporter superfamily, ABCB19, functions as a brassinosteroid exporter. We present its structure in both the substrate-unbound and the brassinosteroid-bound states. Bioactive brassinosteroids are potent activators of ABCB19 ATP hydrolysis activity, and transport assays showed that ABCB19 transports brassinosteroids. In Arabidopsis thaliana, ABCB19 and its close homolog, ABCB1, positively regulate brassinosteroid responses. Our results uncover an elusive export mechanism for bioactive brassinosteroids that is tightly coordinated with brassinosteroid signaling."}],"doi":"10.1126/science.adj4591","intvolume":"       383","date_published":"2024-03-22T00:00:00Z","page":"eadj4591","department":[{"_id":"JiFr"}],"publication_identifier":{"eissn":["1095-9203"]},"isi":1,"OA_place":"repository","scopus_import":"1","quality_controlled":"1","date_created":"2024-03-31T22:01:12Z","volume":383,"status":"public","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"short":"W. Ying, Y. Wang, H. Wei, Y. Luo, Q. Ma, H. Zhu, H. Janssens, N. Vukašinović, M. Kvasnica, J.M. Winne, Y. Gao, S. Tan, J. Friml, X. Liu, E. Russinova, L. Sun, Science 383 (2024) eadj4591.","ista":"Ying W, Wang Y, Wei H, Luo Y, Ma Q, Zhu H, Janssens H, Vukašinović N, Kvasnica M, Winne JM, Gao Y, Tan S, Friml J, Liu X, Russinova E, Sun L. 2024. Structure and function of the Arabidopsis ABC transporter ABCB19 in brassinosteroid export. Science. 383(6689), eadj4591.","ama":"Ying W, Wang Y, Wei H, et al. Structure and function of the Arabidopsis ABC transporter ABCB19 in brassinosteroid export. <i>Science</i>. 2024;383(6689):eadj4591. doi:<a href=\"https://doi.org/10.1126/science.adj4591\">10.1126/science.adj4591</a>","mla":"Ying, Wei, et al. “Structure and Function of the Arabidopsis ABC Transporter ABCB19 in Brassinosteroid Export.” <i>Science</i>, vol. 383, no. 6689, American Association for the Advancement of Science, 2024, p. eadj4591, doi:<a href=\"https://doi.org/10.1126/science.adj4591\">10.1126/science.adj4591</a>.","ieee":"W. Ying <i>et al.</i>, “Structure and function of the Arabidopsis ABC transporter ABCB19 in brassinosteroid export,” <i>Science</i>, vol. 383, no. 6689. American Association for the Advancement of Science, p. eadj4591, 2024.","apa":"Ying, W., Wang, Y., Wei, H., Luo, Y., Ma, Q., Zhu, H., … Sun, L. (2024). Structure and function of the Arabidopsis ABC transporter ABCB19 in brassinosteroid export. <i>Science</i>. American Association for the Advancement of Science. <a href=\"https://doi.org/10.1126/science.adj4591\">https://doi.org/10.1126/science.adj4591</a>","chicago":"Ying, Wei, Yaowei Wang, Hong Wei, Yongming Luo, Qian Ma, Heyuan Zhu, Hilde Janssens, et al. “Structure and Function of the Arabidopsis ABC Transporter ABCB19 in Brassinosteroid Export.” <i>Science</i>. American Association for the Advancement of Science, 2024. <a href=\"https://doi.org/10.1126/science.adj4591\">https://doi.org/10.1126/science.adj4591</a>."},"pmid":1,"type":"journal_article","year":"2024","issue":"6689","title":"Structure and function of the Arabidopsis ABC transporter ABCB19 in brassinosteroid export","publication":"Science","language":[{"iso":"eng"}]},{"abstract":[{"lang":"eng","text":"A measurable map between measure spaces is shown to have bounded compression if and only if its image via the measure-algebra functor is Lipschitz-continuous w.r.t. the measure-algebra distances. This provides a natural interpretation of maps of bounded compression/deformation by means of the measure-algebra functor and corrobo-rates the assertion that maps of bounded deformation are a natural class of morphisms for the category of complete and separable metric measure spaces."}],"article_processing_charge":"No","project":[{"grant_number":"E208","_id":"34dbf174-11ca-11ed-8bc3-afe9d43d4b9c","name":"Configuration Spaces over Non-Smooth Spaces"}],"day":"01","_id":"15252","publication_status":"published","external_id":{"arxiv":["2304.11348"]},"author":[{"id":"ECEBF480-9E4F-11EA-B557-B0823DDC885E","last_name":"Dello Schiavo","full_name":"Dello Schiavo, Lorenzo","orcid":"0000-0002-9881-6870","first_name":"Lorenzo"}],"publisher":"Udruga Matematicara Osijek","oa_version":"Preprint","oa":1,"article_type":"original","acknowledgement":"The author gratefully acknowledges funding of his current position by the Austrian Science\r\nFund (FWF), grant ESPRIT208. He is grateful to Enrico Pasqualetto for pointing out some\r\nreferences on maps of bounded compression.","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2304.11348"}],"month":"01","date_updated":"2025-04-14T12:59:08Z","corr_author":"1","publication":"Mathematical Communications","title":"A characterization of maps of bounded compression","language":[{"iso":"eng"}],"type":"journal_article","year":"2024","issue":"1","status":"public","volume":29,"citation":{"ista":"Dello Schiavo L. 2024. A characterization of maps of bounded compression. Mathematical Communications. 29(1), 137–142.","short":"L. Dello Schiavo, Mathematical Communications 29 (2024) 137–142.","ama":"Dello Schiavo L. A characterization of maps of bounded compression. <i>Mathematical Communications</i>. 2024;29(1):137-142.","mla":"Dello Schiavo, Lorenzo. “A Characterization of Maps of Bounded Compression.” <i>Mathematical Communications</i>, vol. 29, no. 1, Udruga Matematicara Osijek, 2024, pp. 137–42.","ieee":"L. Dello Schiavo, “A characterization of maps of bounded compression,” <i>Mathematical Communications</i>, vol. 29, no. 1. Udruga Matematicara Osijek, pp. 137–142, 2024.","apa":"Dello Schiavo, L. (2024). A characterization of maps of bounded compression. <i>Mathematical Communications</i>. Udruga Matematicara Osijek.","chicago":"Dello Schiavo, Lorenzo. “A Characterization of Maps of Bounded Compression.” <i>Mathematical Communications</i>. Udruga Matematicara Osijek, 2024."},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","scopus_import":"1","quality_controlled":"1","date_created":"2024-03-31T22:01:12Z","department":[{"_id":"JaMa"}],"publication_identifier":{"eissn":["1848-8013"],"issn":["1331-0623"]},"date_published":"2024-01-01T00:00:00Z","page":"137-142","arxiv":1,"intvolume":"        29"}]