[{"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","author":[{"full_name":"Britavskiy, N.","last_name":"Britavskiy","first_name":"N."},{"full_name":"Mahy, L.","last_name":"Mahy","first_name":"L."},{"last_name":"Lennon","first_name":"D. J.","full_name":"Lennon, D. J."},{"first_name":"L. R.","last_name":"Patrick","full_name":"Patrick, L. R."},{"last_name":"Sana","first_name":"H.","full_name":"Sana, H."},{"first_name":"J. I.","last_name":"Villaseñor","full_name":"Villaseñor, J. I."},{"full_name":"Shenar, T.","last_name":"Shenar","first_name":"T."},{"first_name":"J.","last_name":"Bodensteiner","full_name":"Bodensteiner, J."},{"last_name":"Bernini-Peron","first_name":"M.","full_name":"Bernini-Peron, M."},{"first_name":"S. R.","last_name":"Berlanas","full_name":"Berlanas, S. R."},{"full_name":"Bowman, D. M.","last_name":"Bowman","first_name":"D. M."},{"full_name":"Crowther, P. A.","first_name":"P. A.","last_name":"Crowther"},{"last_name":"De Mink","first_name":"S. E.","full_name":"De Mink, S. E."},{"last_name":"Evans","first_name":"C. J.","full_name":"Evans, C. J."},{"orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","full_name":"Götberg, Ylva Louise Linsdotter","first_name":"Ylva Louise Linsdotter","last_name":"Götberg"},{"last_name":"Holgado","first_name":"G.","full_name":"Holgado, G."},{"last_name":"Johnston","first_name":"C.","full_name":"Johnston, C."},{"last_name":"Keszthelyi","first_name":"Z.","full_name":"Keszthelyi, Z."},{"full_name":"Klencki, J.","last_name":"Klencki","first_name":"J."},{"full_name":"Langer, N.","first_name":"N.","last_name":"Langer"},{"full_name":"Mandel, I.","last_name":"Mandel","first_name":"I."},{"first_name":"A.","last_name":"Menon","full_name":"Menon, A."},{"first_name":"M.","last_name":"Moe","full_name":"Moe, M."},{"full_name":"Oskinova, L. M.","last_name":"Oskinova","first_name":"L. M."},{"full_name":"Pauli, D.","first_name":"D.","last_name":"Pauli"},{"last_name":"Pawlak","first_name":"M.","full_name":"Pawlak, M."},{"last_name":"Ramachandran","first_name":"V.","full_name":"Ramachandran, V."},{"full_name":"Renzo, M.","first_name":"M.","last_name":"Renzo"},{"full_name":"Sander, A. A.C.","last_name":"Sander","first_name":"A. A.C."},{"full_name":"Schneider, F. R.N.","first_name":"F. R.N.","last_name":"Schneider"},{"first_name":"A.","last_name":"Schootemeijer","full_name":"Schootemeijer, A."},{"full_name":"Sen, K.","last_name":"Sen","first_name":"K."},{"first_name":"S.","last_name":"Simón-Díaz","full_name":"Simón-Díaz, S."},{"full_name":"Van Loon, J. T.","first_name":"J. T.","last_name":"Van Loon"},{"full_name":"Vink, J. S.","first_name":"J. S.","last_name":"Vink"}],"volume":698,"OA_place":"publisher","title":"Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud","article_processing_charge":"Yes","abstract":[{"text":"Context. The blue supergiant (BSG) domain contains a large variety of stars whose past and future evolutionary paths are still highly uncertain. Since binary interaction plays a crucial role in the fate of massive stars, investigating the multiplicity among BSGs helps shed light on the fate of such objects.\r\nAims. We aim to estimate the binary fraction of a large sample of BSGs in the Small Magellanic Cloud (SMC) within the Binarity at LOw Metallicity (BLOeM) survey. In total, we selected 262 targets with spectral types B0-B3 and luminosity classes I-II.\r\n\r\nMethods. This work is based on spectroscopic data collected by the FLAMES instrument, mounted on the Very Large Telescope, which gathered nine epochs over three months. Our spectroscopic analysis for each target includes the individual and peak-to-peak radial velocity measurements, an investigation of the line profile variability, and a periodogram analysis to search for possible short- and long-period binaries.\r\n\r\nResults. By applying a 20 km s−1 threshold on the peak-to-peak radial velocities above which we would consider the star to be binary, the resulting observed spectroscopic binary fraction for our BSG sample is 23 ± 3%. An independent analysis of line profile variability reveals 11 (plus 5 candidates) double-lined spectroscopic binaries and 32 (plus 41 candidates) single-lined spectroscopic binaries. Based on these results, we estimated the overall observed binary fraction in this sample to be 34 ± 3%, which is close to the computed intrinsic binary fraction of 40 ± 4%. In addition, we derived reliable orbital periods for 41 spectroscopic binaries and potential binary candidates, among which there are 17 eclipsing binaries, including 20 SB1 and SB2 systems with periods of less than 10 days. We reported a significant drop in the binary fraction of BSGs with spectral types later than B2 and effective temperatures less than 18 kK, which could indicate the end of the main sequence phase in this temperature regime. We found no metallicity dependence in the binary fraction of BSGs, compared to existing spectroscopic surveys of the Galaxy and Large Magellanic Cloud.","lang":"eng"}],"publication_status":"published","external_id":{"isi":["001497903100019"],"arxiv":["2502.12239"]},"doi":"10.1051/0004-6361/202452963","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"publication":"Astronomy & Astrophysics","year":"2025","date_created":"2025-06-15T22:01:29Z","article_number":"A40","has_accepted_license":"1","ddc":["520"],"quality_controlled":"1","file":[{"creator":"dernst","success":1,"date_created":"2025-06-25T08:38:02Z","content_type":"application/pdf","file_name":"2025_AstronomyAstrophysics_Britavskiy.pdf","checksum":"53a9f290cb1f468895e0d4446e0020f0","relation":"main_file","access_level":"open_access","file_size":7106568,"date_updated":"2025-06-25T08:38:02Z","file_id":"19901"}],"_id":"19841","scopus_import":"1","article_type":"original","intvolume":"       698","oa_version":"Published Version","type":"journal_article","acknowledgement":"We thank the anonymous referee for helpful comments that have improved the manuscript. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement 101164755/METAL) and was supported by the Israel Science Foundation (ISF) under grant number 2434/24. NB acknowledges support from the Belgian federal government grant for Ukrainian postdoctoral researchers (contract UF/2022/10). TS acknowledges support by the Israel Science Foundation (ISF) under grant number 0603225041. DP acknowledges financial support from the Deutsches Zentrum für Luft und Raumfahrt (DLR) grant FKZ 50OR2005 and the FWO junior postdoctoral fellowship No. 1256225N. DMB gratefully acknowledges UK Research and Innovation (UKRI) in the form of a Frontier Research grant under the UK government’s ERC Horizon Europe funding guarantee (SYMPHONY; PI Bowman; grant number: EP/Y031059/1), and a Royal Society University Research Fellowship (PI Bowman; grant number: URF\\R1\\231631). KS is funded by the National Science Center (NCN), Poland, under grant number OPUS 2021/41/B/ST9/00757. IM acknowledges support from the Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery (OzGav), through project number CE230100016. JIV acknowledges support from the European Research Council through ERC Advanced Grant No. 101054731. SS-D, and GH acknowledge support from the Spanish Ministry of Science and Innovation and Universities (MICIU) through the Spanish State Research Agency (AEI) through grants PID2021-122397NB-C21, and the Severo Ochoa Program 2020-2023 (CEX2019-000920-S).","month":"06","language":[{"iso":"eng"}],"date_published":"2025-06-01T00:00:00Z","publisher":"EDP Sciences","department":[{"_id":"YlGo"}],"arxiv":1,"date_updated":"2026-02-16T12:09:34Z","isi":1,"oa":1,"file_date_updated":"2025-06-25T08:38:02Z","status":"public","day":"01","OA_type":"diamond","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"citation":{"short":"N. Britavskiy, L. Mahy, D.J. Lennon, L.R. Patrick, H. Sana, J.I. Villaseñor, T. Shenar, J. Bodensteiner, M. Bernini-Peron, S.R. Berlanas, D.M. Bowman, P.A. Crowther, S.E. De Mink, C.J. Evans, Y.L.L. Götberg, G. Holgado, C. Johnston, Z. Keszthelyi, J. Klencki, N. Langer, I. Mandel, A. Menon, M. Moe, L.M. Oskinova, D. Pauli, M. Pawlak, V. Ramachandran, M. Renzo, A.A.C. Sander, F.R.N. Schneider, A. Schootemeijer, K. Sen, S. Simón-Díaz, J.T. Van Loon, J.S. Vink, Astronomy &#38; Astrophysics 698 (2025).","ieee":"N. Britavskiy <i>et al.</i>, “Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud,” <i>Astronomy &#38; Astrophysics</i>, vol. 698. EDP Sciences, 2025.","ista":"Britavskiy N, Mahy L, Lennon DJ, Patrick LR, Sana H, Villaseñor JI, Shenar T, Bodensteiner J, Bernini-Peron M, Berlanas SR, Bowman DM, Crowther PA, De Mink SE, Evans CJ, Götberg YLL, Holgado G, Johnston C, Keszthelyi Z, Klencki J, Langer N, Mandel I, Menon A, Moe M, Oskinova LM, Pauli D, Pawlak M, Ramachandran V, Renzo M, Sander AAC, Schneider FRN, Schootemeijer A, Sen K, Simón-Díaz S, Van Loon JT, Vink JS. 2025. Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud. Astronomy &#38; Astrophysics. 698, A40.","ama":"Britavskiy N, Mahy L, Lennon DJ, et al. Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud. <i>Astronomy &#38; Astrophysics</i>. 2025;698. doi:<a href=\"https://doi.org/10.1051/0004-6361/202452963\">10.1051/0004-6361/202452963</a>","chicago":"Britavskiy, N., L. Mahy, D. J. Lennon, L. R. Patrick, H. Sana, J. I. Villaseñor, T. Shenar, et al. “Binarity at LOw Metallicity (BLOeM): Multiplicity of Early B-Type Supergiants in the Small Magellanic Cloud.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2025. <a href=\"https://doi.org/10.1051/0004-6361/202452963\">https://doi.org/10.1051/0004-6361/202452963</a>.","apa":"Britavskiy, N., Mahy, L., Lennon, D. J., Patrick, L. R., Sana, H., Villaseñor, J. I., … Vink, J. S. (2025). Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202452963\">https://doi.org/10.1051/0004-6361/202452963</a>","mla":"Britavskiy, N., et al. “Binarity at LOw Metallicity (BLOeM): Multiplicity of Early B-Type Supergiants in the Small Magellanic Cloud.” <i>Astronomy &#38; Astrophysics</i>, vol. 698, A40, EDP Sciences, 2025, doi:<a href=\"https://doi.org/10.1051/0004-6361/202452963\">10.1051/0004-6361/202452963</a>."}},{"abstract":[{"lang":"eng","text":"Given the uncertain evolutionary status of blue supergiant stars, their multiplicity properties hold vital clues to better understand their origin and evolution. As part of The Binarity at LOw Metallicity (BLOeM) campaign in the Small Magellanic Cloud, we present a multi-epoch spectroscopic survey of 128 supergiant stars of spectral type B5–F5, which roughly correspond to initial masses in the 6–30 M⊙ range. The observed binary fraction for the B5–9 supergiants is 25 ± 6% (10 ± 4%) and 5 ± 2% (0%) for the A–F stars, which were found using a radial-velocity (RV) variability threshold of 5 km s−1 (10 km s−1) as a criterion for binarity. Accounting for observational biases, we find an intrinsic multiplicity fraction of less than 18% for the B5–9 stars and 8−7+9% for the AF stars, for the orbital periods up to 103.5 days and mass ratios (q) in the 0.1 < q < 1 range. The large stellar radii of these supergiant stars prevent short orbital periods, but we demonstrate that this effect alone cannot explain our results. We assessed the spectra and RV time series of the detected binary systems and find that only a small fraction display convincing solutions. We conclude that the multiplicity fractions are compromised by intrinsic stellar variability, such that the true multiplicity fraction may be significantly smaller. Our main conclusions from comparing the multiplicity properties of the B5–9- and AF-type supergiants to that of their less evolved counterparts is that such stars cannot be explained by a direct evolution from the main sequence. Furthermore, by comparing their multiplicity properties to red supergiant stars, we conclude that the AF supergiant stars are neither progenitors nor descendants of red supergiants."}],"external_id":{"isi":["001497903100028"],"arxiv":["2502.02644"]},"publication_status":"published","article_processing_charge":"Yes","title":"Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants","volume":698,"OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","author":[{"first_name":"L. R.","last_name":"Patrick","full_name":"Patrick, L. R."},{"full_name":"Lennon, D. J.","first_name":"D. J.","last_name":"Lennon"},{"last_name":"Najarro","first_name":"F.","full_name":"Najarro, F."},{"full_name":"Shenar, T.","last_name":"Shenar","first_name":"T."},{"full_name":"Bodensteiner, J.","first_name":"J.","last_name":"Bodensteiner"},{"full_name":"Sana, H.","last_name":"Sana","first_name":"H."},{"full_name":"Crowther, P. A.","last_name":"Crowther","first_name":"P. A."},{"full_name":"Britavskiy, N.","last_name":"Britavskiy","first_name":"N."},{"full_name":"Langer, N.","last_name":"Langer","first_name":"N."},{"full_name":"Schootemeijer, A.","last_name":"Schootemeijer","first_name":"A."},{"last_name":"Evans","first_name":"C. J.","full_name":"Evans, C. J."},{"full_name":"Mahy, L.","first_name":"L.","last_name":"Mahy"},{"orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","full_name":"Götberg, Ylva Louise Linsdotter","last_name":"Götberg","first_name":"Ylva Louise Linsdotter"},{"full_name":"De Mink, S. E.","last_name":"De Mink","first_name":"S. E."},{"full_name":"Schneider, F. R.N.","last_name":"Schneider","first_name":"F. R.N."},{"full_name":"O’Grady, A. J.G.","first_name":"A. J.G.","last_name":"O’Grady"},{"full_name":"Villaseñor, J. I.","last_name":"Villaseñor","first_name":"J. I."},{"first_name":"M.","last_name":"Bernini-Peron","full_name":"Bernini-Peron, M."},{"full_name":"Bowman, D. M.","first_name":"D. M.","last_name":"Bowman"},{"last_name":"De Koter","first_name":"A.","full_name":"De Koter, A."},{"last_name":"Deshmukh","first_name":"K.","full_name":"Deshmukh, K."},{"full_name":"Gilkis, A.","first_name":"A.","last_name":"Gilkis"},{"full_name":"González-Torà, G.","last_name":"González-Torà","first_name":"G."},{"full_name":"Kalari, V. M.","last_name":"Kalari","first_name":"V. M."},{"last_name":"K̃Eszthelyi","first_name":"Z.","full_name":"K̃Eszthelyi, Z."},{"first_name":"I.","last_name":"Mandel","full_name":"Mandel, I."},{"first_name":"A.","last_name":"Menon","full_name":"Menon, A."},{"first_name":"M.","last_name":"Moe","full_name":"Moe, M."},{"full_name":"Oskinova, L. M.","last_name":"Oskinova","first_name":"L. M."},{"last_name":"Pauli","first_name":"D.","full_name":"Pauli, D."},{"full_name":"Renzo, M.","last_name":"Renzo","first_name":"M."},{"first_name":"A. A.C.","last_name":"Sander","full_name":"Sander, A. A.C."},{"last_name":"Sen","first_name":"K.","full_name":"Sen, K."},{"full_name":"Stoop, M.","first_name":"M.","last_name":"Stoop"},{"last_name":"Van Loon","first_name":"J. T.","full_name":"Van Loon, J. T."},{"full_name":"Toonen, S.","first_name":"S.","last_name":"Toonen"},{"full_name":"Tramper, F.","last_name":"Tramper","first_name":"F."},{"first_name":"J. S.","last_name":"Vink","full_name":"Vink, J. S."},{"first_name":"C.","last_name":"Wang","full_name":"Wang, C."}],"file":[{"success":1,"creator":"dernst","date_created":"2025-06-23T07:09:38Z","content_type":"application/pdf","file_name":"2025_AstronomyAstrophysics_Patrick.pdf","access_level":"open_access","relation":"main_file","checksum":"93a907bf48da7e2ba7d75b53ea6011f5","date_updated":"2025-06-23T07:09:38Z","file_size":2130448,"file_id":"19863"}],"quality_controlled":"1","ddc":["520"],"has_accepted_license":"1","article_number":"A39","year":"2025","date_created":"2025-06-15T22:01:29Z","publication":"Astronomy & Astrophysics","doi":"10.1051/0004-6361/202452949","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"oa":1,"file_date_updated":"2025-06-23T07:09:38Z","isi":1,"publisher":"EDP Sciences","department":[{"_id":"YlGo"}],"arxiv":1,"date_updated":"2026-02-16T12:09:50Z","language":[{"iso":"eng"}],"month":"06","date_published":"2025-06-01T00:00:00Z","acknowledgement":"We thank Sipra Hota for kindly sharing the SMC UVIT catalogue prior to publication. LRP, FN. and FT acknowledge support by grants PID2019-105552RB-C41 and PID2022-137779OB-C41 funded by MCIN/AEI/10.13039/501100011033 by “ERDF A way of making Europe”. LRP acknowledges support from grant PID2022-140483NB-C22 funded by MCIN/AEI/10.13039/501100011033. TS acknowledges support by the Israel Science Foundation (ISF) under grant number 0603225041. The research leading to these results has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement numbers 772225: MULTIPLES). DMB gratefully acknowledges support from UK Research and Innovation (UKRI) in the form of a Frontier Research grant under the UK government’s ERC Horizon Europe funding guarantee (SYMPHONY; grant number: EP/Y031059/1), and a Royal Society University Research Fellowship (grant number: URF\\R1\\231631). GGT is supported by the German Deutsche Forschungsgemeinschaft (DFG) under Project-ID 496854903 (SA4064/2-1, PI Sander). AACS is funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) in the form of an Emmy Noether Research Group – Project-ID 445674056 (SA4064/1-1, PI Sander). GGT and AACS further acknowledges support from the Federal Ministry of Education and Research (BMBF) and the Baden-Württemberg Ministry of Science as part of the Excellence Strategy of the German Federal and State Governments. This paper benefited from discussions at the International Space Science Institute (ISSI) in Bern through ISSI International Team project 512 (Multiwavelength View on Massive Stars in the Era of Multimessenger Astronomy). DP acknowledges financial support by the Deutsches Zentrum für Luft und Raumfahrt (DLR) grant FKZ 50OR2005. JIV acknowledges support from the European Research Council for the ERC Advanced Grant 101054731. PAC is supported by the Science and Technology Facilities Council research grant ST/V000853/1 (PI. V. Dhillon). JSV is supported by Science and Technology Facilities Council funding under grant number ST/V000233/1. DFR is thankful for the support of the CAPES-Br and FAPERJ/DSC-10 (SEI-260003/001630/2023). This work has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (Grant agreement No. 945806) and is supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy EXC 2181/1-390900948 (the Heidelberg STRUCTURES Excellence Cluster).","type":"journal_article","article_type":"original","intvolume":"       698","oa_version":"Published Version","_id":"19842","scopus_import":"1","citation":{"apa":"Patrick, L. R., Lennon, D. J., Najarro, F., Shenar, T., Bodensteiner, J., Sana, H., … Wang, C. (2025). Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202452949\">https://doi.org/10.1051/0004-6361/202452949</a>","chicago":"Patrick, L. R., D. J. Lennon, F. Najarro, T. Shenar, J. Bodensteiner, H. Sana, P. A. Crowther, et al. “Binarity at LOw Metallicity (BLOeM): The Multiplicity Properties and Evolution of BAF-Type Supergiants.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2025. <a href=\"https://doi.org/10.1051/0004-6361/202452949\">https://doi.org/10.1051/0004-6361/202452949</a>.","mla":"Patrick, L. R., et al. “Binarity at LOw Metallicity (BLOeM): The Multiplicity Properties and Evolution of BAF-Type Supergiants.” <i>Astronomy &#38; Astrophysics</i>, vol. 698, A39, EDP Sciences, 2025, doi:<a href=\"https://doi.org/10.1051/0004-6361/202452949\">10.1051/0004-6361/202452949</a>.","ieee":"L. R. Patrick <i>et al.</i>, “Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants,” <i>Astronomy &#38; Astrophysics</i>, vol. 698. EDP Sciences, 2025.","short":"L.R. Patrick, D.J. Lennon, F. Najarro, T. Shenar, J. Bodensteiner, H. Sana, P.A. Crowther, N. Britavskiy, N. Langer, A. Schootemeijer, C.J. Evans, L. Mahy, Y.L.L. Götberg, S.E. De Mink, F.R.N. Schneider, A.J.G. O’Grady, J.I. Villaseñor, M. Bernini-Peron, D.M. Bowman, A. De Koter, K. Deshmukh, A. Gilkis, G. González-Torà, V.M. Kalari, Z. K̃Eszthelyi, I. Mandel, A. Menon, M. Moe, L.M. Oskinova, D. Pauli, M. Renzo, A.A.C. Sander, K. Sen, M. Stoop, J.T. Van Loon, S. Toonen, F. Tramper, J.S. Vink, C. Wang, Astronomy &#38; Astrophysics 698 (2025).","ama":"Patrick LR, Lennon DJ, Najarro F, et al. Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants. <i>Astronomy &#38; Astrophysics</i>. 2025;698. doi:<a href=\"https://doi.org/10.1051/0004-6361/202452949\">10.1051/0004-6361/202452949</a>","ista":"Patrick LR, Lennon DJ, Najarro F, Shenar T, Bodensteiner J, Sana H, Crowther PA, Britavskiy N, Langer N, Schootemeijer A, Evans CJ, Mahy L, Götberg YLL, De Mink SE, Schneider FRN, O’Grady AJG, Villaseñor JI, Bernini-Peron M, Bowman DM, De Koter A, Deshmukh K, Gilkis A, González-Torà G, Kalari VM, K̃Eszthelyi Z, Mandel I, Menon A, Moe M, Oskinova LM, Pauli D, Renzo M, Sander AAC, Sen K, Stoop M, Van Loon JT, Toonen S, Tramper F, Vink JS, Wang C. 2025. Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants. Astronomy &#38; Astrophysics. 698, A39."},"OA_type":"diamond","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"status":"public","day":"01"},{"scopus_import":"1","_id":"19843","oa_version":"Published Version","intvolume":"         4","article_type":"original","type":"journal_article","acknowledgement":"This work was supported by the European Research Council CoG 863818 (ForM-SMArt) (to K.C.) and the European Research Council Starting Grant 850529: E-DIRECT (to C.H.).","date_published":"2025-05-01T00:00:00Z","month":"05","language":[{"iso":"eng"}],"date_updated":"2026-04-07T12:30:56Z","publisher":"Oxford University Press","department":[{"_id":"KrCh"}],"file_date_updated":"2025-06-23T08:09:50Z","DOAJ_listed":"1","oa":1,"day":"01","status":"public","tmp":{"short":"CC BY-NC (4.0)","name":"Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)","image":"/images/cc_by_nc.png","legal_code_url":"https://creativecommons.org/licenses/by-nc/4.0/legalcode"},"OA_type":"gold","ec_funded":1,"citation":{"ista":"Hübner V, Schmid L, Hilbe C, Chatterjee K. 2025. Stable strategies of direct and indirect reciprocity across all social dilemmas. PNAS Nexus. 4(5), pgaf154.","ama":"Hübner V, Schmid L, Hilbe C, Chatterjee K. Stable strategies of direct and indirect reciprocity across all social dilemmas. <i>PNAS Nexus</i>. 2025;4(5). doi:<a href=\"https://doi.org/10.1093/pnasnexus/pgaf154\">10.1093/pnasnexus/pgaf154</a>","ieee":"V. Hübner, L. Schmid, C. Hilbe, and K. Chatterjee, “Stable strategies of direct and indirect reciprocity across all social dilemmas,” <i>PNAS Nexus</i>, vol. 4, no. 5. Oxford University Press, 2025.","short":"V. Hübner, L. Schmid, C. Hilbe, K. Chatterjee, PNAS Nexus 4 (2025).","mla":"Hübner, Valentin, et al. “Stable Strategies of Direct and Indirect Reciprocity across All Social Dilemmas.” <i>PNAS Nexus</i>, vol. 4, no. 5, pgaf154, Oxford University Press, 2025, doi:<a href=\"https://doi.org/10.1093/pnasnexus/pgaf154\">10.1093/pnasnexus/pgaf154</a>.","apa":"Hübner, V., Schmid, L., Hilbe, C., &#38; Chatterjee, K. (2025). Stable strategies of direct and indirect reciprocity across all social dilemmas. <i>PNAS Nexus</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/pnasnexus/pgaf154\">https://doi.org/10.1093/pnasnexus/pgaf154</a>","chicago":"Hübner, Valentin, Laura Schmid, Christian Hilbe, and Krishnendu Chatterjee. “Stable Strategies of Direct and Indirect Reciprocity across All Social Dilemmas.” <i>PNAS Nexus</i>. Oxford University Press, 2025. <a href=\"https://doi.org/10.1093/pnasnexus/pgaf154\">https://doi.org/10.1093/pnasnexus/pgaf154</a>."},"project":[{"call_identifier":"H2020","name":"Formal Methods for Stochastic Models: Algorithms and Applications","_id":"0599E47C-7A3F-11EA-A408-12923DDC885E","grant_number":"863818"}],"pmid":1,"related_material":{"record":[{"relation":"dissertation_contains","id":"19903","status":"public"}]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","author":[{"last_name":"Hübner","first_name":"Valentin","full_name":"Hübner, Valentin","id":"2c8aa207-dc7d-11ea-9b2f-f22972ecd910","orcid":"0009-0001-5009-4987"},{"first_name":"Laura","last_name":"Schmid","id":"38B437DE-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-6978-7329","full_name":"Schmid, Laura"},{"orcid":"0000-0001-5116-955X","id":"2FDF8F3C-F248-11E8-B48F-1D18A9856A87","full_name":"Hilbe, Christian","first_name":"Christian","last_name":"Hilbe"},{"first_name":"Krishnendu","last_name":"Chatterjee","full_name":"Chatterjee, Krishnendu","id":"2E5DCA20-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-4561-241X"}],"OA_place":"publisher","volume":4,"title":"Stable strategies of direct and indirect reciprocity across all social dilemmas","article_processing_charge":"Yes","external_id":{"pmid":["40417077"]},"publication_status":"published","abstract":[{"lang":"eng","text":"Social dilemmas are collective-action problems where individual interests are at odds with group interests. Such dilemmas occur frequently at all scales of human interactions. When dealing with collective-action problems, people often act reciprocally. They adjust their behavior to match the previous behavior of the recipient. The literature distinguishes two kinds of reciprocity. According to direct reciprocity, individuals react to their immediate experiences with the recipient. They are more likely to cooperate if the recipient previously cooperated with them. According to indirect reciprocity, individuals react to the recipient’s general behavior, irrespectively of whether or not they benefited directly. In practice, the two kinds of reciprocity are often intertwined; people typically base their decisions on both direct experiences and indirect observations. Yet only recently have researchers begun to explore how the two kinds of reciprocity interact. So far, this research only addresses a single type of social dilemma, the donation game, where the effects of individual behaviors are independent. Instead, here we allow for all pairwise social dilemmas. By applying novel techniques to generalize the theory of zero-determinant strategies, we establish an important proof of principle: In all social dilemmas, socially optimal outcomes can be sustained as an equilibrium, using either direct or indirect reciprocity, or arbitrary mixtures thereof. These results neither require games to be repeated infinitely often, nor that individual opinions are synchronized. In this way, we considerably generalize the scope of models of reciprocity, and we build further bridges between the literatures on direct and indirect reciprocity."}],"doi":"10.1093/pnasnexus/pgaf154","publication_identifier":{"eissn":["2752-6542"]},"issue":"5","publication":"PNAS Nexus","date_created":"2025-06-15T22:01:30Z","year":"2025","article_number":"pgaf154","has_accepted_license":"1","ddc":["000"],"corr_author":"1","file":[{"access_level":"open_access","relation":"main_file","checksum":"efd6648db3fc3ea0cdd7155d667e5f11","date_updated":"2025-06-23T08:09:50Z","file_size":2551195,"file_id":"19867","success":1,"creator":"dernst","date_created":"2025-06-23T08:09:50Z","content_type":"application/pdf","file_name":"2025_PNASNexus_Huebner.pdf"}],"quality_controlled":"1"},{"date_updated":"2026-04-16T08:17:17Z","department":[{"_id":"YlGo"}],"arxiv":1,"publisher":"EDP Sciences","date_published":"2025-06-01T00:00:00Z","month":"06","language":[{"iso":"eng"}],"file_date_updated":"2025-06-23T07:54:57Z","oa":1,"isi":1,"scopus_import":"1","_id":"19844","acknowledgement":"The research leading to these results has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 and Horizon Europe research and innovation programme (grant agreement numbers 772225: MULTIPLES, and 945806) and is supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy EXC 2181/1-390900948 (the Heidelberg STRUCTURES Excellence Cluster). DMB gratefully acknowledges funding from UK Research and Innovation (UKRI) in the form of a Frontier Research grant under the UK government’s ERC Horizon Europe funding guarantee (SYMPHONY; grant number: EP/Y031059/1), and a Royal Society University Research Fellowship (URF; grant number: URF\\R1\\231631). RGI is funded by STFC grant ST/Y002350/1 as part of the BRIDGCE UK network, and thanks IReNA colleagues for stimulating discussions. Z.K. acknowledges support from JSPS Kakenhi Grant-in-Aid for Scientific Research (23K19071). IM acknowledges support from the Australian Research Council (ARC) Centre of Excellence for GravitationalWave Discovery (OzGrav), through project number CE230100016. DP acknowledges financial support by the Deutsches Zentrum für Luft und Raumfahrt (DLR) grant FKZ 50OR2005. DFR is thankful for the support of CAPES-Br and FAPERJ/DSC-10 (SEI-260003/001630/2023). AACS and VR are supported by the German Deutsche Forschungsgemeinschaft (DFG) under Project-ID 445674056 (Emmy Noether Research Group SA4064/1-1, PI Sander). AACS and VR are further supported by funding from the Federal Ministry of Education and Research (BMBF) and the Baden-Württemberg Ministry of Science as part of the Excellence Strategy of the German Federal and State Governments. JIV acknowledges support from the European Research Council for the ERC Advanced Grant 101054731. LRP acknowledges support from grant PID2022-140483NB-C22 funded by MCIN/AEI/10.13039/501100011033. GH acknowledges support from grants PID2021-122397NB-C21/PID2022-136640NB-C22 funded by MCIN/AEI/FEDER/10.13039/501100011033. J.K. thanks for the support of a grant GA CR 22-34467S. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement 101164755/METAL) and was supported by the Israel Science Foundation (ISF) under grant number 2434/24.","type":"journal_article","intvolume":"       698","oa_version":"Published Version","article_type":"original","citation":{"short":"J. Bodensteiner, T. Shenar, H. Sana, N. Britavskiy, P.A. Crowther, N. Langer, D.J. Lennon, L. Mahy, L.R. Patrick, J.I. Villaseñor, M. Abdul-Masih, D.M. Bowman, A. De Koter, S.E. De Mink, K. Deshmukh, M. Fabry, A. Gilkis, Y.L.L. Götberg, G. Holgado, R.G. Izzard, S. Janssens, V.M. Kalari, Z. Keszthelyi, J. Kubát, I. Mandel, G. Maravelias, L.M. Oskinova, D. Pauli, V. Ramachandran, D.F. Rocha, M. Renzo, A.A.C. Sander, F.R.N. Schneider, A. Schootemeijer, K. Sen, M. Stoop, S. Toonen, J.T. Van Loon, R. Valli, A. Vigna-Gómez, J.S. Vink, C. Wang, X.T. Xu, Astronomy &#38; Astrophysics 698 (2025).","ieee":"J. Bodensteiner <i>et al.</i>, “Binarity at LOw Metallicity (BLOeM): Multiplicity properties of Oe and Be stars,” <i>Astronomy &#38; Astrophysics</i>, vol. 698. EDP Sciences, 2025.","ama":"Bodensteiner J, Shenar T, Sana H, et al. Binarity at LOw Metallicity (BLOeM): Multiplicity properties of Oe and Be stars. <i>Astronomy &#38; Astrophysics</i>. 2025;698. doi:<a href=\"https://doi.org/10.1051/0004-6361/202452623\">10.1051/0004-6361/202452623</a>","ista":"Bodensteiner J, Shenar T, Sana H, Britavskiy N, Crowther PA, Langer N, Lennon DJ, Mahy L, Patrick LR, Villaseñor JI, Abdul-Masih M, Bowman DM, De Koter A, De Mink SE, Deshmukh K, Fabry M, Gilkis A, Götberg YLL, Holgado G, Izzard RG, Janssens S, Kalari VM, Keszthelyi Z, Kubát J, Mandel I, Maravelias G, Oskinova LM, Pauli D, Ramachandran V, Rocha DF, Renzo M, Sander AAC, Schneider FRN, Schootemeijer A, Sen K, Stoop M, Toonen S, Van Loon JT, Valli R, Vigna-Gómez A, Vink JS, Wang C, Xu XT. 2025. Binarity at LOw Metallicity (BLOeM): Multiplicity properties of Oe and Be stars. Astronomy &#38; Astrophysics. 698, A38.","apa":"Bodensteiner, J., Shenar, T., Sana, H., Britavskiy, N., Crowther, P. A., Langer, N., … Xu, X. T. (2025). Binarity at LOw Metallicity (BLOeM): Multiplicity properties of Oe and Be stars. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202452623\">https://doi.org/10.1051/0004-6361/202452623</a>","chicago":"Bodensteiner, J., T. Shenar, H. Sana, N. Britavskiy, P. A. Crowther, N. Langer, D. J. Lennon, et al. “Binarity at LOw Metallicity (BLOeM): Multiplicity Properties of Oe and Be Stars.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2025. <a href=\"https://doi.org/10.1051/0004-6361/202452623\">https://doi.org/10.1051/0004-6361/202452623</a>.","mla":"Bodensteiner, J., et al. “Binarity at LOw Metallicity (BLOeM): Multiplicity Properties of Oe and Be Stars.” <i>Astronomy &#38; Astrophysics</i>, vol. 698, A38, EDP Sciences, 2025, doi:<a href=\"https://doi.org/10.1051/0004-6361/202452623\">10.1051/0004-6361/202452623</a>."},"status":"public","day":"01","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"OA_type":"diamond","title":"Binarity at LOw Metallicity (BLOeM): Multiplicity properties of Oe and Be stars","external_id":{"isi":["001497903100011"],"arxiv":["2502.02641"]},"publication_status":"published","abstract":[{"text":"Context. Rapidly rotating classical OBe stars have been proposed as the products of binary interactions, and the fraction of Be stars with compact companions implies that at least some are. However, to constrain the interaction physics spinning up the OBe stars, a large sample of homogeneously analyzed OBe stars with well-determined binary characteristics and orbital parameters are required.\r\n\r\nAims. We investigated the multiplicity properties of a sample of 18 Oe, 62 Be, and two Of?p stars observed within the BLOeM survey in the Small Magellanic Cloud. We analyzed the first nine epochs of spectroscopic observations obtained over approximately three months in 2023.\r\n\r\nMethods. Radial velocities (RVs) of all stars were measured using cross-correlation based on different sets of absorption and emission lines. Applying commonly used binarity criteria, we classified objects as binaries, binary candidates, and apparently single (RV stable) objects. We further inspected the spectra for double-lined spectroscopic binaries and cross-matched with catalogs of X-ray sources and photometric binaries.\r\n\r\nResults. We classify 14 OBe stars as binaries, and an additional 11 as binary candidates. The two Of?p stars are apparently single. We find two more objects that are most likely currently interacting binaries. Without those, the observed binary fraction for the remaining OBe sample of 78 stars is fobs+candOBe = 0.18 ± 0.04 (fobs+candOBe = 0.32±0.05 including candidates). This binary fraction is less than half of that measured for OB stars in BLOeM. Combined with the lower fraction of SB2s, this suggests that OBe stars do indeed have fundamentally different present-day binary properties than OB stars. We find no evidence for OBe binaries with massive compact companions, in contrast to expectations from binary population synthesis.\r\n\r\nConclusions. Our results support the binary scenario as an important formation channel for OBe stars, as post-interaction binaries may have been disrupted or the stripped companions of OBe stars are harder to detect. Further observations are required to characterize the detected binaries, their orbital parameters, and the nature of their companions.","lang":"eng"}],"article_processing_charge":"Yes","volume":698,"OA_place":"publisher","user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","author":[{"full_name":"Bodensteiner, J.","last_name":"Bodensteiner","first_name":"J."},{"full_name":"Shenar, T.","first_name":"T.","last_name":"Shenar"},{"full_name":"Sana, H.","last_name":"Sana","first_name":"H."},{"full_name":"Britavskiy, N.","last_name":"Britavskiy","first_name":"N."},{"full_name":"Crowther, P. A.","last_name":"Crowther","first_name":"P. A."},{"last_name":"Langer","first_name":"N.","full_name":"Langer, N."},{"first_name":"D. J.","last_name":"Lennon","full_name":"Lennon, D. J."},{"first_name":"L.","last_name":"Mahy","full_name":"Mahy, L."},{"full_name":"Patrick, L. R.","first_name":"L. R.","last_name":"Patrick"},{"full_name":"Villaseñor, J. I.","first_name":"J. I.","last_name":"Villaseñor"},{"first_name":"M.","last_name":"Abdul-Masih","full_name":"Abdul-Masih, M."},{"last_name":"Bowman","first_name":"D. M.","full_name":"Bowman, D. M."},{"first_name":"A.","last_name":"De Koter","full_name":"De Koter, A."},{"full_name":"De Mink, S. E.","first_name":"S. E.","last_name":"De Mink"},{"last_name":"Deshmukh","first_name":"K.","full_name":"Deshmukh, K."},{"full_name":"Fabry, M.","first_name":"M.","last_name":"Fabry"},{"last_name":"Gilkis","first_name":"A.","full_name":"Gilkis, A."},{"last_name":"Götberg","first_name":"Ylva Louise Linsdotter","full_name":"Götberg, Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d"},{"full_name":"Holgado, G.","first_name":"G.","last_name":"Holgado"},{"last_name":"Izzard","first_name":"R. G.","full_name":"Izzard, R. G."},{"full_name":"Janssens, S.","first_name":"S.","last_name":"Janssens"},{"full_name":"Kalari, V. M.","last_name":"Kalari","first_name":"V. M."},{"full_name":"Keszthelyi, Z.","last_name":"Keszthelyi","first_name":"Z."},{"full_name":"Kubát, J.","first_name":"J.","last_name":"Kubát"},{"first_name":"I.","last_name":"Mandel","full_name":"Mandel, I."},{"last_name":"Maravelias","first_name":"G.","full_name":"Maravelias, G."},{"full_name":"Oskinova, L. M.","first_name":"L. M.","last_name":"Oskinova"},{"full_name":"Pauli, D.","last_name":"Pauli","first_name":"D."},{"last_name":"Ramachandran","first_name":"V.","full_name":"Ramachandran, V."},{"full_name":"Rocha, D. F.","last_name":"Rocha","first_name":"D. F."},{"full_name":"Renzo, M.","first_name":"M.","last_name":"Renzo"},{"last_name":"Sander","first_name":"A. A.C.","full_name":"Sander, A. A.C."},{"full_name":"Schneider, F. R.N.","first_name":"F. R.N.","last_name":"Schneider"},{"first_name":"A.","last_name":"Schootemeijer","full_name":"Schootemeijer, A."},{"full_name":"Sen, K.","last_name":"Sen","first_name":"K."},{"full_name":"Stoop, M.","last_name":"Stoop","first_name":"M."},{"first_name":"S.","last_name":"Toonen","full_name":"Toonen, S."},{"last_name":"Van Loon","first_name":"J. T.","full_name":"Van Loon, J. T."},{"last_name":"Valli","first_name":"R.","full_name":"Valli, R."},{"full_name":"Vigna-Gómez, A.","first_name":"A.","last_name":"Vigna-Gómez"},{"last_name":"Vink","first_name":"J. S.","full_name":"Vink, J. S."},{"full_name":"Wang, C.","last_name":"Wang","first_name":"C."},{"full_name":"Xu, X. T.","last_name":"Xu","first_name":"X. T."}],"ddc":["520"],"has_accepted_license":"1","file":[{"file_id":"19866","relation":"main_file","checksum":"51d79c82f6030180fb7c5d7ba01b2da8","access_level":"open_access","file_size":2404827,"date_updated":"2025-06-23T07:54:57Z","date_created":"2025-06-23T07:54:57Z","content_type":"application/pdf","file_name":"2025_AstronomyAstrophysics_Bodensteiner.pdf","creator":"dernst","success":1}],"quality_controlled":"1","publication":"Astronomy & Astrophysics","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"doi":"10.1051/0004-6361/202452623","article_number":"A38","date_created":"2025-06-15T22:01:30Z","year":"2025"},{"citation":{"ieee":"G. Östlin <i>et al.</i>, “MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm,” <i>Astronomy &#38; Astrophysics</i>, vol. 696. EDP Sciences, 2025.","short":"G. Östlin, P.G. Pérez-González, J. Melinder, S. Gillman, E. Iani, L. Costantin, L.A. Boogaard, P. Rinaldi, L. Colina, H.U. Nørgaard-Nielsen, D. Dicken, T.R. Greve, G. Wright, A. Alonso-Herrero, J. Álvarez-Márquez, M. Annunziatella, A. Bik, S.E.I. Bosman, K.I. Caputi, A.C. Gomez, A. Eckart, M. Garcia-Marin, J. Hjorth, O. Ilbert, I. Jermann, S. Kendrew, A. Labiano, D. Langeroodi, O. Le Fevre, M. Libralato, R.A. Meyer, T. Moutard, F. Peissker, J.P. Pye, T.V. Tikkanen, M. Topinka, F. Walter, M. Ward, P. Van Der Werf, E.F. Van Dishoeck, M. Güdel, T. Henning, P.O. Lagage, T.P. Ray, B. Vandenbussche, Astronomy &#38; Astrophysics 696 (2025).","ista":"Östlin G, Pérez-González PG, Melinder J, Gillman S, Iani E, Costantin L, Boogaard LA, Rinaldi P, Colina L, Nørgaard-Nielsen HU, Dicken D, Greve TR, Wright G, Alonso-Herrero A, Álvarez-Márquez J, Annunziatella M, Bik A, Bosman SEI, Caputi KI, Gomez AC, Eckart A, Garcia-Marin M, Hjorth J, Ilbert O, Jermann I, Kendrew S, Labiano A, Langeroodi D, Le Fevre O, Libralato M, Meyer RA, Moutard T, Peissker F, Pye JP, Tikkanen TV, Topinka M, Walter F, Ward M, Van Der Werf P, Van Dishoeck EF, Güdel M, Henning T, Lagage PO, Ray TP, Vandenbussche B. 2025. MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm. Astronomy &#38; Astrophysics. 696, A57.","ama":"Östlin G, Pérez-González PG, Melinder J, et al. MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm. <i>Astronomy &#38; Astrophysics</i>. 2025;696. doi:<a href=\"https://doi.org/10.1051/0004-6361/202451723\">10.1051/0004-6361/202451723</a>","chicago":"Östlin, Göran, Pablo G. Pérez-González, Jens Melinder, Steven Gillman, Edoardo Iani, Luca Costantin, Leindert A. Boogaard, et al. “MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey Description and Early Results for the Galaxy Population Detected at 5.6 Μm.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2025. <a href=\"https://doi.org/10.1051/0004-6361/202451723\">https://doi.org/10.1051/0004-6361/202451723</a>.","apa":"Östlin, G., Pérez-González, P. G., Melinder, J., Gillman, S., Iani, E., Costantin, L., … Vandenbussche, B. (2025). MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202451723\">https://doi.org/10.1051/0004-6361/202451723</a>","mla":"Östlin, Göran, et al. “MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey Description and Early Results for the Galaxy Population Detected at 5.6 Μm.” <i>Astronomy &#38; Astrophysics</i>, vol. 696, A57, EDP Sciences, 2025, doi:<a href=\"https://doi.org/10.1051/0004-6361/202451723\">10.1051/0004-6361/202451723</a>."},"day":"01","status":"public","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"OA_type":"diamond","date_updated":"2026-02-16T12:10:36Z","arxiv":1,"publisher":"EDP Sciences","department":[{"_id":"JoMa"}],"date_published":"2025-04-01T00:00:00Z","month":"04","language":[{"iso":"eng"}],"file_date_updated":"2025-06-23T07:46:01Z","oa":1,"isi":1,"scopus_import":"1","_id":"19845","type":"journal_article","acknowledgement":"We dedicate this paper to the memory of our deceased and much valued MIRI-EC team members Hans Ulrik Nørgaard-Nielsen and Olivier Le Fèvre, both of whom played a central role in defining the MIDIS project. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The work presented is the effort of the entire MIRI team and the enthusiasm within the MIRI partnership is a significant factor in its success. The following National and International Funding Agencies funded and supported the MIRI development: NASA; ESA; Belgian Science Policy Office (BELSPO); Centre Nationale d’Etudes Spatiales (CNES); Danish National Space Centre; Deutsches Zentrum fur Luftund Raumfahrt (DLR); Enterprise Ireland; Ministerio De Economia y Competividad; Netherlands Research School for Astronomy (NOVA); Netherlands Organisation for Scientific Research (NWO); Science and Technology Facilities Council; Swiss Space Office; Swedish National Space Agency (SNSA); and UK Space Agency. MIRI drew on the scientific and technical expertise of the following organizations: Ames Research Center, USA; Airbus Defence and Space, UK; CEAIrfu, Saclay, France; Centre Spatial de Liège, Belgium; Consejo Superior de Investigaciones Cientficas, Spain; Carl Zeiss Optronics, Germany; Chalmers University of Technology, Sweden; Danish Space Research Institute, Denmark; Dublin Institute for Advanced Studies, Ireland; European Space Agency, Netherlands; ETCA, Belgium; ETH Zurich, Switzerland; Goddard Space Flight Center, USA; Institute d’Astrophysique Spatiale, France; Instituto Nacional de Técnica Aeroespacial,Spain; Institute for Astronomy, Edinburgh, UK; Jet Propulsion Laboratory, USA; Laboratoire d’Astrophysique de Marseille (LAM), France; Leiden University, Netherlands; Lockheed Advanced Technology Center (USA); NOVA Opt-IR group at Dwingeloo, Netherlands; Northrop Grumman, USA; Max Planck Institut f ür Astronomie (MPIA), Heidelberg, Germany; Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique (LESIA), France; Paul Scherrer Institut, Switzerland; Raytheon Vision Systems, USA; RUAG Aerospace, Switzerland; Rutherford Appleton Laboratory (RAL Space), UK; Space Telescope Science Institute, USA; Stockholm University, Sweden; Toegepast- Natuurwetenschappelijk Onderzoek (TNOTPD), Netherlands; UK Astronomy Technology Centre, UK; University College London, UK; University of Amsterdam, Netherlands; University of Arizona, USA; University of Cardiff, UK; University of Cologne, Germany; University of Ghent; University of Groningen, Netherlands; University of Leicester, UK; University of Leuven, Belgium; Utah State University, USA. Additional acknowledgements related to specific grants: G.Ö., J.M. and A.B. acknowledges funding from the Swedish National Space Administration (SNSA). P.G.P.-G. acknowledges support from grant PID2022-139567NB-I00 funded by Spanish Ministerio de Ciencia e Innovación MCIN/AEI/10.13039/501100011033, FEDER Una manera de hacer Europa. This work was supported by research grants (VIL16599,VIL54489) from VILLUM FONDEN. L.C. and J.A.-M. acknowledge support by grant PIB2021-127718NB-100 from the Spanish Ministry of Science and Innovation/State Agency of Research MCIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe”. M.A. acknowledges financial support from Comunidad de Madrid under Atracción de Talento grant 2020-T2/TIC-19971. J.P.P. and T.V.T. acknowledge financial support from the UK Science and Technology Facilities Council, and the UK Space Agency. A.A.-H. acknowledges financial support from grant PID2021-124665NB-I00 funded by MCIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe”. E.I. and K.I.C. acknowledge funding from the Netherlands Research School for Astronomy (NOVA). K.I.C. acknowledges funding from the Dutch Research Council (NWO) through the award of the Vici Grant VI.C.212.036. RAM acknowledges support from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. The paper uses JWST data from programme #1283, obtained from the Barbara Mikulski Archive for Space Telescopes at the Space Telescope Science Institute (STScI). For the purpose of open access, the authors have applied a Creative Commons Attribution (CC BY) licence to the Author Accepted Manuscript version arising from this submission.","intvolume":"       696","oa_version":"Published Version","article_type":"original","ddc":["520"],"has_accepted_license":"1","file":[{"file_size":15858045,"date_updated":"2025-06-23T07:46:01Z","checksum":"67600eba8bda24987a130ac334f10456","relation":"main_file","access_level":"open_access","file_id":"19865","creator":"dernst","success":1,"file_name":"2025_AstronomyAstrophysics_Oestlin.pdf","content_type":"application/pdf","date_created":"2025-06-23T07:46:01Z"}],"quality_controlled":"1","publication":"Astronomy & Astrophysics","doi":"10.1051/0004-6361/202451723","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"article_number":"A57","date_created":"2025-06-15T22:01:30Z","year":"2025","title":"MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm","publication_status":"published","external_id":{"arxiv":["2411.19686 "],"isi":["001459780300005"]},"abstract":[{"lang":"eng","text":"Context. The recently launched James Webb Space Telescope (JWST) is opening new observing windows on the distant Universe. Among JWST’s instruments, the Mid Infrared Instrument (MIRI) offers the unique capability of imaging observations at wavelengths of λ > 5 μm. This enables unique access to the rest frame near-infrared (NIR, λ ≥ 1 μm) emission from galaxies at redshifts of z > 4 and the visual (λ ≳ 5000 Å) rest frame for z > 9. We report here on the guaranteed time observations (GTO), from the MIRI European Consortium, of the Hubble Ultra Deep Field (HUDF), forming the MIRI Deep Imaging Survey (MIDIS), consisting of an on source integration time of ∼41 hours in the MIRI/F560W (5.6 μm) filter. The F560W filter was selected since it would produce the deepest data in terms of AB magnitudes in a given time. To our knowledge, this constitutes the longest single filter exposure obtained with JWST of an extragalactic field as of yet.\r\nAims. The HUDF is one of the most observed extragalactic fields, with extensive multi-wavelength coverage, where (before JWST) galaxies up to z ∼ 7 have been confirmed, and at z > 10 suggested, from HST photometry. We aim to characterise the galaxy population in HUDF at 5.6 μm, enabling studies such as: the rest frame NIR morphologies for galaxies at z ≲ 4.6, probing mature stellar populations and emission lines in z > 6 sources, intrinsically red and dusty galaxies, and active galactic nuclei (AGNs) and their host galaxies at intermediate redshifts.\r\n\r\nMethods. We reduced the MIRI data using the official JWST pipeline, augmented by in-house custom scripts. We measured the noise characteristics of the resulting image. Galaxy photometry was obtained, and photometric redshifts were estimated for sources with available multi-wavelength photometry (and compared to spectroscopic redshifts when available).\r\n\r\nResults. Over the deepest part of our image, the 5σ point source limit is 28.65 mag AB (12.6 nJy), ∼0.35 mag better than predicted by the JWST exposure time calculator. We find ∼2500 sources, the overwhelming majority of which are distant galaxies, but we note that spurious sources likely remain at faint magnitudes due to imperfect cosmic ray rejection in the JWST pipeline. More than 500 galaxies with available spectroscopic redshifts, up to z ≈ 11, have been identified, the majority of which are at z < 6. More than 1000 galaxies have reliable photometric redshift estimates, of which ∼25 are at 6 < z < 12. The point spread function in the F560W filter has a full width at half maximum (FWHM) of ≈0.2″ (corresponding to 1.4 kpc at z = 4), allowing the NIR rest frame morphologies and stellar mass distributions to be resolved for z < 4.5. Moreover, > 100 objects with very red NIRCam vs MIRI (3.6–5.6 μm > 1 mag) colours have been found, suggestive of dusty or old stellar populations at high redshifts.\r\n\r\nConclusions. We conclude that MIDIS surpasses preflight expectations and that deep MIRI imaging has great potential to characterise the galaxy population from cosmic noon to dawn."}],"article_processing_charge":"Yes","volume":696,"OA_place":"publisher","author":[{"first_name":"Göran","last_name":"Östlin","full_name":"Östlin, Göran"},{"first_name":"Pablo G.","last_name":"Pérez-González","full_name":"Pérez-González, Pablo G."},{"full_name":"Melinder, Jens","last_name":"Melinder","first_name":"Jens"},{"last_name":"Gillman","first_name":"Steven","full_name":"Gillman, Steven"},{"full_name":"Iani, Edoardo","orcid":"0000-0001-8386-3546","id":"4053390a-6b68-11ef-9828-a3b8adef8d0a","first_name":"Edoardo","last_name":"Iani"},{"last_name":"Costantin","first_name":"Luca","full_name":"Costantin, Luca"},{"first_name":"Leindert A.","last_name":"Boogaard","full_name":"Boogaard, Leindert A."},{"full_name":"Rinaldi, Pierluigi","first_name":"Pierluigi","last_name":"Rinaldi"},{"full_name":"Colina, Luis","last_name":"Colina","first_name":"Luis"},{"full_name":"Nørgaard-Nielsen, Hans Ulrik","last_name":"Nørgaard-Nielsen","first_name":"Hans Ulrik"},{"last_name":"Dicken","first_name":"Daniel","full_name":"Dicken, Daniel"},{"full_name":"Greve, Thomas R.","first_name":"Thomas R.","last_name":"Greve"},{"full_name":"Wright, Gillian","last_name":"Wright","first_name":"Gillian"},{"full_name":"Alonso-Herrero, Almudena","first_name":"Almudena","last_name":"Alonso-Herrero"},{"full_name":"Álvarez-Márquez, Javier","last_name":"Álvarez-Márquez","first_name":"Javier"},{"first_name":"Marianna","last_name":"Annunziatella","full_name":"Annunziatella, Marianna"},{"full_name":"Bik, Arjan","last_name":"Bik","first_name":"Arjan"},{"full_name":"Bosman, Sarah E.I.","last_name":"Bosman","first_name":"Sarah E.I."},{"first_name":"Karina I.","last_name":"Caputi","full_name":"Caputi, Karina I."},{"first_name":"Alejandro Crespo","last_name":"Gomez","full_name":"Gomez, Alejandro Crespo"},{"first_name":"Andreas","last_name":"Eckart","full_name":"Eckart, Andreas"},{"full_name":"Garcia-Marin, Macarena","last_name":"Garcia-Marin","first_name":"Macarena"},{"full_name":"Hjorth, Jens","first_name":"Jens","last_name":"Hjorth"},{"last_name":"Ilbert","first_name":"Olivier","full_name":"Ilbert, Olivier"},{"full_name":"Jermann, Iris","last_name":"Jermann","first_name":"Iris"},{"first_name":"Sarah","last_name":"Kendrew","full_name":"Kendrew, Sarah"},{"full_name":"Labiano, Alvaro","last_name":"Labiano","first_name":"Alvaro"},{"full_name":"Langeroodi, Danial","first_name":"Danial","last_name":"Langeroodi"},{"last_name":"Le Fevre","first_name":"Olivier","full_name":"Le Fevre, Olivier"},{"full_name":"Libralato, Mattia","first_name":"Mattia","last_name":"Libralato"},{"full_name":"Meyer, Romain A.","last_name":"Meyer","first_name":"Romain A."},{"last_name":"Moutard","first_name":"Thibaud","full_name":"Moutard, Thibaud"},{"full_name":"Peissker, Florian","last_name":"Peissker","first_name":"Florian"},{"first_name":"John P.","last_name":"Pye","full_name":"Pye, John P."},{"last_name":"Tikkanen","first_name":"Tuomo V.","full_name":"Tikkanen, Tuomo V."},{"full_name":"Topinka, Martin","first_name":"Martin","last_name":"Topinka"},{"first_name":"Fabian","last_name":"Walter","full_name":"Walter, Fabian"},{"full_name":"Ward, Martin","last_name":"Ward","first_name":"Martin"},{"first_name":"Paul","last_name":"Van Der Werf","full_name":"Van Der Werf, Paul"},{"first_name":"Ewine F.","last_name":"Van Dishoeck","full_name":"Van Dishoeck, Ewine F."},{"full_name":"Güdel, Manuel","last_name":"Güdel","first_name":"Manuel"},{"full_name":"Henning, Thomas","last_name":"Henning","first_name":"Thomas"},{"full_name":"Lagage, Pierre Olivier","last_name":"Lagage","first_name":"Pierre Olivier"},{"last_name":"Ray","first_name":"Tom P.","full_name":"Ray, Tom P."},{"first_name":"Bart","last_name":"Vandenbussche","full_name":"Vandenbussche, Bart"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87"},{"isi":1,"oa":1,"DOAJ_listed":"1","file_date_updated":"2025-06-23T10:20:22Z","month":"06","language":[{"iso":"eng"}],"date_published":"2025-06-18T00:00:00Z","publisher":"Elsevier","department":[{"_id":"AnSa"}],"date_updated":"2025-09-30T12:53:15Z","article_type":"original","oa_version":"Published Version","intvolume":"         6","acknowledgement":"We thank S. Buchegger for excellent technical assistance. This research was funded by the Austrian Science Fund (FWF) projects https://doi.org/10.55776/P32851, https://doi.org/10.55776/P35900, and https://doi.org/10.55776/P36202 to I.D. and https://doi.org/10.55776/PAT6871323 to A.T. N.M. is funded within the DOC program of the OeAW (Austrian Academy of Science). For open access purposes, the author has applied a CC BY public copyright license to any author-accepted manuscript version arising from this submission.","type":"journal_article","_id":"19846","scopus_import":"1","citation":{"short":"H. Najjar, S. Weiß, F. Horvath, V. Hopl, A. Tiffner, L. Höbarth, J. Söllner, M. Fröhlich, M. Prantl, N. Müller, Y. Nazarenko, S. Harant, L. Weissenböck, H. Grabmayr, M. Sallinger, L. Maltan, L.V. Echefu, T. Radiskovic, M. Leopold, S. Lindinger, C. Humer, C. Höglinger, H. Krobath, T. Renger, I. Derler, Cell Reports Physical Science 6 (2025).","ieee":"H. Najjar <i>et al.</i>, “STIM1-induced widening of non-pore-lining TM interfaces is crucial for Orai1 pore opening,” <i>Cell Reports Physical Science</i>, vol. 6, no. 6. Elsevier, 2025.","ista":"Najjar H, Weiß S, Horvath F, Hopl V, Tiffner A, Höbarth L, Söllner J, Fröhlich M, Prantl M, Müller N, Nazarenko Y, Harant S, Weissenböck L, Grabmayr H, Sallinger M, Maltan L, Echefu LV, Radiskovic T, Leopold M, Lindinger S, Humer C, Höglinger C, Krobath H, Renger T, Derler I. 2025. STIM1-induced widening of non-pore-lining TM interfaces is crucial for Orai1 pore opening. Cell Reports Physical Science. 6(6), 102623.","ama":"Najjar H, Weiß S, Horvath F, et al. STIM1-induced widening of non-pore-lining TM interfaces is crucial for Orai1 pore opening. <i>Cell Reports Physical Science</i>. 2025;6(6). doi:<a href=\"https://doi.org/10.1016/j.xcrp.2025.102623\">10.1016/j.xcrp.2025.102623</a>","apa":"Najjar, H., Weiß, S., Horvath, F., Hopl, V., Tiffner, A., Höbarth, L., … Derler, I. (2025). STIM1-induced widening of non-pore-lining TM interfaces is crucial for Orai1 pore opening. <i>Cell Reports Physical Science</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.xcrp.2025.102623\">https://doi.org/10.1016/j.xcrp.2025.102623</a>","chicago":"Najjar, Hadil, Sarah Weiß, Ferdinand Horvath, Valentina Hopl, Adéla Tiffner, Lorenz Höbarth, Julia Söllner, et al. “STIM1-Induced Widening of Non-Pore-Lining TM Interfaces Is Crucial for Orai1 Pore Opening.” <i>Cell Reports Physical Science</i>. Elsevier, 2025. <a href=\"https://doi.org/10.1016/j.xcrp.2025.102623\">https://doi.org/10.1016/j.xcrp.2025.102623</a>.","mla":"Najjar, Hadil, et al. “STIM1-Induced Widening of Non-Pore-Lining TM Interfaces Is Crucial for Orai1 Pore Opening.” <i>Cell Reports Physical Science</i>, vol. 6, no. 6, 102623, Elsevier, 2025, doi:<a href=\"https://doi.org/10.1016/j.xcrp.2025.102623\">10.1016/j.xcrp.2025.102623</a>."},"OA_type":"gold","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"day":"18","status":"public","article_processing_charge":"Yes","abstract":[{"lang":"eng","text":"The Ca2+-release-activated Ca2+ (CRAC) channel Orai1 is activated by interaction with the Ca2+ sensor Stromal Interaction Molecule 1 (STIM1). Owing to the lack of structurally resolved Orai1/STIM1 complexes, the impact of their coupling on individual Orai1 transmembrane domain (TM) movements is unclear. This study investigates STIM1-independent and STIM1-dependent Orai1-TM dynamics using photocrosslinking unnatural amino acids (UAAs) at each individual TM position. We primarily identify CRAC-channel-like currents directly after UAA incorporation or additional UV-light irradiation at TM3 sites that interface with non-pore-lining TMs. Using UAAs combined with conventional site-directed mutagenesis and molecular dynamics simulations, we discover that pore opening involves a widening of interfaces formed by TM3 with non-pore-lining TMs. Orai1 mutants with a UAA in TM3 exhibit weaker STIM1-induced activation after UV exposure, possibly caused by a restricted widening of non-pore-lining TM interfaces. We demonstrate that photocrosslinking UAAs are excellent tools for improving our understanding of key determinants and ion channel dynamics modulating pore opening."}],"publication_status":"published","external_id":{"isi":["001516570500009"]},"title":"STIM1-induced widening of non-pore-lining TM interfaces is crucial for Orai1 pore opening","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","author":[{"last_name":"Najjar","first_name":"Hadil","full_name":"Najjar, Hadil"},{"full_name":"Weiß, Sarah","first_name":"Sarah","last_name":"Weiß"},{"first_name":"Ferdinand","last_name":"Horvath","id":"b0dc7f61-21a3-11ef-a9b4-e6ab1aa6f21e","full_name":"Horvath, Ferdinand"},{"full_name":"Hopl, Valentina","last_name":"Hopl","first_name":"Valentina"},{"full_name":"Tiffner, Adéla","first_name":"Adéla","last_name":"Tiffner"},{"first_name":"Lorenz","last_name":"Höbarth","full_name":"Höbarth, Lorenz"},{"last_name":"Söllner","first_name":"Julia","full_name":"Söllner, Julia"},{"last_name":"Fröhlich","first_name":"Maximilian","full_name":"Fröhlich, Maximilian"},{"full_name":"Prantl, Magdalena","last_name":"Prantl","first_name":"Magdalena"},{"full_name":"Müller, Nora","first_name":"Nora","last_name":"Müller"},{"last_name":"Nazarenko","first_name":"Yuliia","full_name":"Nazarenko, Yuliia"},{"first_name":"Selina","last_name":"Harant","full_name":"Harant, Selina"},{"full_name":"Weissenböck, Lukas","first_name":"Lukas","last_name":"Weissenböck"},{"full_name":"Grabmayr, Herwig","last_name":"Grabmayr","first_name":"Herwig"},{"last_name":"Sallinger","first_name":"Matthias","full_name":"Sallinger, Matthias"},{"full_name":"Maltan, Lena","first_name":"Lena","last_name":"Maltan"},{"full_name":"Echefu, Linda V.","first_name":"Linda V.","last_name":"Echefu"},{"first_name":"Tamara","last_name":"Radiskovic","full_name":"Radiskovic, Tamara"},{"full_name":"Leopold, Melanie","last_name":"Leopold","first_name":"Melanie"},{"full_name":"Lindinger, Sonja","first_name":"Sonja","last_name":"Lindinger"},{"full_name":"Humer, Christina","first_name":"Christina","last_name":"Humer"},{"full_name":"Höglinger, Carmen","last_name":"Höglinger","first_name":"Carmen"},{"first_name":"Heinrich","last_name":"Krobath","full_name":"Krobath, Heinrich"},{"full_name":"Renger, Thomas","last_name":"Renger","first_name":"Thomas"},{"full_name":"Derler, Isabella","first_name":"Isabella","last_name":"Derler"}],"volume":6,"OA_place":"publisher","file":[{"file_id":"19868","file_size":9771117,"date_updated":"2025-06-23T10:20:22Z","access_level":"open_access","checksum":"37ff7c396f966d0ec363e4691d63d402","relation":"main_file","file_name":"2025_CellReportsPhysicalScience_Najjar.pdf","content_type":"application/pdf","date_created":"2025-06-23T10:20:22Z","success":1,"creator":"dernst"}],"quality_controlled":"1","has_accepted_license":"1","ddc":["570"],"year":"2025","date_created":"2025-06-15T22:01:31Z","article_number":"102623","issue":"6","doi":"10.1016/j.xcrp.2025.102623","publication_identifier":{"eissn":["2666-3864"]},"publication":"Cell Reports Physical Science"},{"title":"Prussian blue analogues as anode materials for battery applications: Complexities and horizons","abstract":[{"lang":"eng","text":"Prussian blue (PB) and Prussian blue analogues (PBAs) are a class of porous materials composed of transition metal cations, cyanide ligands, and alkali metal cations. Their ability to intercalate and deintercalate ions within their framework pores, coupled with the adaptability of their crystal structure to electrochemical changes, underpins their success in battery applications. PBAs with Fe or Co as the active site exhibit high redox potentials (vs SHE) and have been extensively explored as cathode materials, with well-documented chemistry, crystal structures, and electrochemical properties. In contrast, PBAs with Cr or Mn as the active site display lower redox potentials and remain significantly underexplored as anode materials. This gap has led to fewer reported compounds and a less comprehensive understanding of their structural and electrochemical behavior, leaving the field relatively opaque. In this perspective, we comprehensively analyze the challenges involved in producing and employing PBAs with low redox potentials as active battery materials. Conversely, we propose numerous horizons and ask fundamental questions that should pave the way for future research to advance the field."}],"external_id":{"isi":["001501830600001"]},"publication_status":"published","page":"4203-4226","article_processing_charge":"Yes (via OA deal)","OA_place":"publisher","volume":37,"author":[{"last_name":"Palacios Corella","first_name":"Mario","id":"452e82c6-803f-11ed-ab7e-ca0439e73a5d","full_name":"Palacios Corella, Mario"},{"last_name":"Echevarría","first_name":"Igor","id":"a623795e-21fb-11ed-b8a1-a0f51308eed7","full_name":"Echevarría, Igor"},{"last_name":"Santana Santos","first_name":"Carla","full_name":"Santana Santos, Carla"},{"last_name":"Schuhmann","first_name":"Wolfgang","full_name":"Schuhmann, Wolfgang"},{"first_name":"Edgar","last_name":"Ventosa","full_name":"Ventosa, Edgar"},{"first_name":"Maria","last_name":"Ibáñez","full_name":"Ibáñez, Maria","orcid":"0000-0001-5013-2843","id":"43C61214-F248-11E8-B48F-1D18A9856A87"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","ddc":["540"],"has_accepted_license":"1","quality_controlled":"1","file":[{"success":1,"creator":"dernst","file_name":"2025_ChemistryMaterials_PalaciosCorella.pdf","content_type":"application/pdf","date_created":"2025-12-30T08:40:55Z","file_size":8760757,"date_updated":"2025-12-30T08:40:55Z","access_level":"open_access","checksum":"902c52a2f52a028436e0acd8a5a4beac","relation":"main_file","file_id":"20897"}],"corr_author":"1","publication":"Chemistry of Materials","issue":"12","doi":"10.1021/acs.chemmater.5c00213","publication_identifier":{"issn":["0897-4756"],"eissn":["1520-5002"]},"year":"2025","date_created":"2025-06-15T22:01:31Z","publisher":"American Chemical Society","department":[{"_id":"MaIb"}],"date_updated":"2025-12-30T08:41:57Z","month":"06","language":[{"iso":"eng"}],"date_published":"2025-06-03T00:00:00Z","oa":1,"file_date_updated":"2025-12-30T08:40:55Z","isi":1,"_id":"19847","scopus_import":"1","acknowledgement":"All the authors acknowledge financial support by the MeBattery project. MeBattery has received funding from the European Innovation Council of the European Union under Grant Agreement No. 101046742. We acknowledge the valuable scientific discussions with Christine Fiedler. M.P.-C. acknowledges that the project that gave rise to these results received the support of a fellowship from the “la Caixa” Foundation (ID 100010434) with code LCF/BQ/PI24/12040015. E.V. also acknowledges financial support by the Spanish Ministry of Science and Innovation and NextGenerationEU (TED2021-131651B-C21) and Ramón y Cajal award (Ministry of Science and Innovation and European Social Funds, RYC2018-026086-I).","type":"journal_article","article_type":"original","oa_version":"Published Version","intvolume":"        37","project":[{"name":"MEDIATED BIPHASIC BATTERY","grant_number":"101046742","_id":"eb9fa02e-77a9-11ec-83b8-ab1143e5a30f"}],"PlanS_conform":"1","citation":{"mla":"Palacios Corella, Mario, et al. “Prussian Blue Analogues as Anode Materials for Battery Applications: Complexities and Horizons.” <i>Chemistry of Materials</i>, vol. 37, no. 12, American Chemical Society, 2025, pp. 4203–26, doi:<a href=\"https://doi.org/10.1021/acs.chemmater.5c00213\">10.1021/acs.chemmater.5c00213</a>.","apa":"Palacios Corella, M., Echevarría, I., Santana Santos, C., Schuhmann, W., Ventosa, E., &#38; Ibáñez, M. (2025). Prussian blue analogues as anode materials for battery applications: Complexities and horizons. <i>Chemistry of Materials</i>. American Chemical Society. <a href=\"https://doi.org/10.1021/acs.chemmater.5c00213\">https://doi.org/10.1021/acs.chemmater.5c00213</a>","chicago":"Palacios Corella, Mario, Igor Echevarría, Carla Santana Santos, Wolfgang Schuhmann, Edgar Ventosa, and Maria Ibáñez. “Prussian Blue Analogues as Anode Materials for Battery Applications: Complexities and Horizons.” <i>Chemistry of Materials</i>. American Chemical Society, 2025. <a href=\"https://doi.org/10.1021/acs.chemmater.5c00213\">https://doi.org/10.1021/acs.chemmater.5c00213</a>.","ista":"Palacios Corella M, Echevarría I, Santana Santos C, Schuhmann W, Ventosa E, Ibáñez M. 2025. Prussian blue analogues as anode materials for battery applications: Complexities and horizons. Chemistry of Materials. 37(12), 4203–4226.","ama":"Palacios Corella M, Echevarría I, Santana Santos C, Schuhmann W, Ventosa E, Ibáñez M. Prussian blue analogues as anode materials for battery applications: Complexities and horizons. <i>Chemistry of Materials</i>. 2025;37(12):4203-4226. doi:<a href=\"https://doi.org/10.1021/acs.chemmater.5c00213\">10.1021/acs.chemmater.5c00213</a>","ieee":"M. Palacios Corella, I. Echevarría, C. Santana Santos, W. Schuhmann, E. Ventosa, and M. Ibáñez, “Prussian blue analogues as anode materials for battery applications: Complexities and horizons,” <i>Chemistry of Materials</i>, vol. 37, no. 12. American Chemical Society, pp. 4203–4226, 2025.","short":"M. Palacios Corella, I. Echevarría, C. Santana Santos, W. Schuhmann, E. Ventosa, M. Ibáñez, Chemistry of Materials 37 (2025) 4203–4226."},"day":"03","status":"public","OA_type":"hybrid","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"}},{"oa":1,"isi":1,"date_updated":"2026-06-18T08:34:38Z","department":[{"_id":"UlWa"}],"arxiv":1,"publisher":"Springer Nature","date_published":"2025-05-26T00:00:00Z","language":[{"iso":"eng"}],"month":"05","type":"journal_article","acknowledgement":"Open access funding provided by Institute of Science and Technology (IST Austria).","oa_version":"Published Version","article_type":"original","scopus_import":"1","_id":"19848","citation":{"ista":"Tinarrage R, Ennes H, Resck L, Gomes LT, Ponciano JR, Poco J. 2025. Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification. Artificial Intelligence and Law.","ama":"Tinarrage R, Ennes H, Resck L, Gomes LT, Ponciano JR, Poco J. Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification. <i>Artificial Intelligence and Law</i>. 2025. doi:<a href=\"https://doi.org/10.1007/s10506-025-09458-6\">10.1007/s10506-025-09458-6</a>","short":"R. Tinarrage, H. Ennes, L. Resck, L.T. Gomes, J.R. Ponciano, J. Poco, Artificial Intelligence and Law (2025).","ieee":"R. Tinarrage, H. Ennes, L. Resck, L. T. Gomes, J. R. Ponciano, and J. Poco, “Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification,” <i>Artificial Intelligence and Law</i>. Springer Nature, 2025.","mla":"Tinarrage, Raphaël, et al. “Empirical Analysis of Binding Precedent Efficiency in Brazilian Supreme Court via Case Classification.” <i>Artificial Intelligence and Law</i>, Springer Nature, 2025, doi:<a href=\"https://doi.org/10.1007/s10506-025-09458-6\">10.1007/s10506-025-09458-6</a>.","apa":"Tinarrage, R., Ennes, H., Resck, L., Gomes, L. T., Ponciano, J. R., &#38; Poco, J. (2025). Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification. <i>Artificial Intelligence and Law</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s10506-025-09458-6\">https://doi.org/10.1007/s10506-025-09458-6</a>","chicago":"Tinarrage, Raphaël, Henrique Ennes, Lucas Resck, Lucas T. Gomes, Jean R. Ponciano, and Jorge Poco. “Empirical Analysis of Binding Precedent Efficiency in Brazilian Supreme Court via Case Classification.” <i>Artificial Intelligence and Law</i>. Springer Nature, 2025. <a href=\"https://doi.org/10.1007/s10506-025-09458-6\">https://doi.org/10.1007/s10506-025-09458-6</a>."},"OA_type":"hybrid","day":"26","status":"public","publication_status":"epub_ahead","external_id":{"isi":["001494836700001"],"arxiv":["2407.07004"]},"abstract":[{"lang":"eng","text":"Binding precedents (súmulas vinculantes) constitute a juridical instrument unique to the Brazilian legal system and whose objectives include the protection of the Federal Supreme Court against repetitive demands. Studies of the effectiveness of these instruments in decreasing the Court’s exposure to similar cases, however, indicate that they tend to fail in such a direction, with some of the binding precedents seemingly creating new demands. We empirically assess the legal impact of five binding precedents, 11, 14, 17, 26, and 37, at the highest Court level through their effects on the legal subjects they address. This analysis is only possible through the comparison of the Court’s ruling about the precedents’ themes before they are created, which means that these decisions should be detected through techniques of Similar Case Retrieval, which we tackle from the angle of Case Classification. The contributions of this article are therefore twofold: on the mathematical side, we compare the use of different methods of Natural Language Processing — TF-IDF, LSTM, Longformer, and regex — for Case Classification, whereas on the legal side, we contrast the inefficiency of these binding precedents with a set of hypotheses that may justify their repeated usage. We observe that the TF-IDF models performed slightly better than LSTM and Longformer when compared through common metrics; however, the deep learning models were able to detect certain important legal events that TF-IDF missed. On the legal side, we argue that the reasons for binding precedents to fail in responding to repetitive demand are heterogeneous and case-dependent, making it impossible to single out a specific cause. We identify five main hypotheses, which are found in different combinations in each of the precedents studied."}],"article_processing_charge":"Yes (via OA deal)","title":"Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification","OA_place":"publisher","author":[{"full_name":"Tinarrage, Raphaël","id":"40ebcc9d-905f-11ef-bf0a-dc475da8a04e","orcid":"0000-0002-1404-1095","last_name":"Tinarrage","first_name":"Raphaël"},{"last_name":"Ennes","first_name":"Henrique","full_name":"Ennes, Henrique"},{"full_name":"Resck, Lucas","first_name":"Lucas","last_name":"Resck"},{"full_name":"Gomes, Lucas T.","last_name":"Gomes","first_name":"Lucas T."},{"full_name":"Ponciano, Jean R.","first_name":"Jean R.","last_name":"Ponciano"},{"first_name":"Jorge","last_name":"Poco","full_name":"Poco, Jorge"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","quality_controlled":"1","corr_author":"1","ddc":["510"],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1007/s10506-025-09458-6"}],"date_created":"2025-06-15T22:01:31Z","year":"2025","publication":"Artificial Intelligence and Law","publication_identifier":{"eissn":["1572-8382"],"issn":["0924-8463"]},"doi":"10.1007/s10506-025-09458-6"},{"project":[{"name":"Center for Correlated Quantum Materials and Solid State Quantum Systems:  Probing topology in circuits and quantum materials","_id":"34a7f947-11ca-11ed-8bc3-c5dc2bbaae25","grant_number":"F8609"}],"citation":{"mla":"Babkin, Serafim, et al. “Superconducting Proximity Effect in Two-Dimensional Hole Gases.” <i>Physical Review B</i>, vol. 111, no. 21, 214518, American Physical Society, 2025, doi:<a href=\"https://doi.org/10.1103/k4jh-pnxy\">10.1103/k4jh-pnxy</a>.","apa":"Babkin, S., Joecker, B., Flensberg, K., Serbyn, M., &#38; Danon, J. (2025). Superconducting proximity effect in two-dimensional hole gases. <i>Physical Review B</i>. American Physical Society. <a href=\"https://doi.org/10.1103/k4jh-pnxy\">https://doi.org/10.1103/k4jh-pnxy</a>","chicago":"Babkin, Serafim, Benjamin Joecker, Karsten Flensberg, Maksym Serbyn, and Jeroen Danon. “Superconducting Proximity Effect in Two-Dimensional Hole Gases.” <i>Physical Review B</i>. American Physical Society, 2025. <a href=\"https://doi.org/10.1103/k4jh-pnxy\">https://doi.org/10.1103/k4jh-pnxy</a>.","ama":"Babkin S, Joecker B, Flensberg K, Serbyn M, Danon J. Superconducting proximity effect in two-dimensional hole gases. <i>Physical Review B</i>. 2025;111(21). doi:<a href=\"https://doi.org/10.1103/k4jh-pnxy\">10.1103/k4jh-pnxy</a>","ista":"Babkin S, Joecker B, Flensberg K, Serbyn M, Danon J. 2025. Superconducting proximity effect in two-dimensional hole gases. Physical Review B. 111(21), 214518.","ieee":"S. Babkin, B. Joecker, K. Flensberg, M. Serbyn, and J. Danon, “Superconducting proximity effect in two-dimensional hole gases,” <i>Physical Review B</i>, vol. 111, no. 21. American Physical Society, 2025.","short":"S. Babkin, B. Joecker, K. Flensberg, M. Serbyn, J. Danon, Physical Review B 111 (2025)."},"OA_type":"hybrid","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"status":"public","day":"18","oa":1,"file_date_updated":"2025-06-23T10:31:11Z","isi":1,"arxiv":1,"department":[{"_id":"MaSe"},{"_id":"GradSch"}],"publisher":"American Physical Society","date_updated":"2025-09-30T12:53:47Z","month":"06","language":[{"iso":"eng"}],"date_published":"2025-06-18T00:00:00Z","type":"journal_article","acknowledgement":"We acknowledge useful discussions with Georgios Katsaros, Andrew Higginbotham, and Oliver Schwarze. This research was funded in part by the Austrian Science Fund (FWF) F 86, the European Research Council (Grant Agreement No. 856526), and by the DFG Collaborative Research Center (CRC) 183 Project No. 277101999.","article_type":"original","oa_version":"Published Version","intvolume":"       111","_id":"19852","scopus_import":"1","file":[{"date_updated":"2025-06-23T10:31:11Z","file_size":1719489,"checksum":"fa8757f4780cfaeb51579c626284a8c1","relation":"main_file","access_level":"open_access","file_id":"19869","creator":"dernst","success":1,"file_name":"2025_PhysReviewB_Babkin.pdf","content_type":"application/pdf","date_created":"2025-06-23T10:31:11Z"}],"quality_controlled":"1","corr_author":"1","ddc":["530"],"has_accepted_license":"1","article_number":"214518","year":"2025","date_created":"2025-06-19T16:54:54Z","publication":"Physical Review B","issue":"21","doi":"10.1103/k4jh-pnxy","publication_identifier":{"issn":["2469-9950"],"eissn":["2469-9969"]},"abstract":[{"text":"Technology involving hybrid superconductor–semiconductor materials is a promising avenue for engineering quantum devices for information storage, manipulation, and transmission. Proximity-induced superconducting correlations are an essential part of such devices. While the proximity effect in the conduction band of common semiconductors is well understood, its manifestation in confined hole gases, realized for instance in germanium, is an active area of research. Lower-dimensional hole-based systems, particularly in germanium, are emerging as an attractive platform for a variety of solid-state quantum devices, due to their combination of efficient spin and charge control and long coherence times. The recent experimental realization of the proximity effect in germanium thus calls for a theoretical description that is tailored to hole gases. In this work, we propose a simple model to describe proximity-induced superconductivity in two-dimensional hole gases, incorporating both the heavy-hole (HH) and light-hole (LH) bands. We start from the Luttinger–Kohn model, introduce three parameters that characterize hopping across the superconductor–semiconductor interface, and derive explicit intraband and interband effective pairing terms for the HH and LH bands. Unlike previous approaches, our theory provides a quantitative relationship between induced pairings and interface properties. Restricting our general model to an experimentally relevant case where only the HH band crosses the chemical potential, we predict the coexistence of 𝑠-wave and 𝑑-wave singlet pairings, along with triplet-type pairings, and modified Zeeman and Rashba spin–orbit couplings. Our results thus present a starting point for theoretical modeling of quantum devices based on proximitized hole gases, fueling further progress in quantum technology.","lang":"eng"}],"publication_status":"published","external_id":{"isi":["001514328000004"],"arxiv":["2412.04084"]},"article_processing_charge":"Yes (via OA deal)","title":"Superconducting proximity effect in two-dimensional hole gases","OA_place":"publisher","volume":111,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","author":[{"first_name":"Serafim","last_name":"Babkin","id":"e63d75c3-72ef-11ef-b75a-e303e149911f","full_name":"Babkin, Serafim"},{"full_name":"Joecker, Benjamin","last_name":"Joecker","first_name":"Benjamin"},{"full_name":"Flensberg, Karsten","first_name":"Karsten","last_name":"Flensberg"},{"last_name":"Serbyn","first_name":"Maksym","full_name":"Serbyn, Maksym","orcid":"0000-0002-2399-5827","id":"47809E7E-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Danon, Jeroen","last_name":"Danon","first_name":"Jeroen"}]},{"day":"08","status":"public","alternative_title":["ISTA Master's Thesis"],"citation":{"apa":"Smith, K. (2025). <i>Exploring internal magnetism in partially suppressed red giant stars</i>. Institute of Science and Technology Austria. <a href=\"https://doi.org/10.15479/AT-ISTA-19853\">https://doi.org/10.15479/AT-ISTA-19853</a>","chicago":"Smith, Kanah. “Exploring Internal Magnetism in Partially Suppressed Red Giant Stars.” Institute of Science and Technology Austria, 2025. <a href=\"https://doi.org/10.15479/AT-ISTA-19853\">https://doi.org/10.15479/AT-ISTA-19853</a>.","mla":"Smith, Kanah. <i>Exploring Internal Magnetism in Partially Suppressed Red Giant Stars</i>. Institute of Science and Technology Austria, 2025, doi:<a href=\"https://doi.org/10.15479/AT-ISTA-19853\">10.15479/AT-ISTA-19853</a>.","ieee":"K. Smith, “Exploring internal magnetism in partially suppressed red giant stars,” Institute of Science and Technology Austria, 2025.","short":"K. Smith, Exploring Internal Magnetism in Partially Suppressed Red Giant Stars, Institute of Science and Technology Austria, 2025.","ama":"Smith K. Exploring internal magnetism in partially suppressed red giant stars. 2025. doi:<a href=\"https://doi.org/10.15479/AT-ISTA-19853\">10.15479/AT-ISTA-19853</a>","ista":"Smith K. 2025. Exploring internal magnetism in partially suppressed red giant stars. Institute of Science and Technology Austria."},"acknowledgement":"I would like to give thanks to myself for my hard work on this document. This paper includes data collected by the Kepler mission and obtained from the MAST data\r\narchive at the Space Telescope Science Institute (STScI). Funding for the Kepler mission is\r\nprovided by the NASA Science Mission Directorate. STScI is operated by the Association of\r\nUniversities for Research in Astronomy, Inc., under NASA contract NAS 5–26555.\r\n","type":"dissertation","oa_version":"Published Version","_id":"19853","file_date_updated":"2025-10-09T14:38:57Z","oa":1,"date_updated":"2026-04-07T12:01:37Z","department":[{"_id":"GradSch"},{"_id":"LiBu"}],"publisher":"Institute of Science and Technology Austria","date_published":"2025-10-08T00:00:00Z","month":"10","language":[{"iso":"eng"}],"date_created":"2025-06-20T13:27:08Z","year":"2025","publication_identifier":{"issn":["2791-4585"]},"doi":"10.15479/AT-ISTA-19853","file":[{"file_id":"20434","checksum":"80d241d11b69af771c1fab0998be4f19","relation":"source_file","access_level":"closed","date_updated":"2025-10-08T09:45:33Z","file_size":8263624,"date_created":"2025-10-08T08:01:42Z","file_name":"2025_Smith_Kanah_Thesis.zip","content_type":"application/zip","creator":"ksmith"},{"date_created":"2025-10-09T14:38:57Z","file_name":"2025_Smith_Kanah_Thesis.pdf","content_type":"application/pdf","success":1,"creator":"ksmith","file_id":"20439","access_level":"open_access","checksum":"13cb48cc98e00fdfe32f3ff66f17aa26","relation":"main_file","file_size":9748339,"date_updated":"2025-10-09T14:38:57Z"}],"corr_author":"1","ddc":["520"],"has_accepted_license":"1","OA_place":"publisher","user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","author":[{"last_name":"Smith","first_name":"Kanah","id":"7703505d-3211-11ee-a6a9-a2ab9d936c15","full_name":"Smith, Kanah"}],"publication_status":"published","abstract":[{"text":"The internal dynamical properties of red giant stars have been explored extensively in recent\r\nyears as a result of the increase in high precision data availability from the space missions\r\nKepler and TESS (Transiting Exoplanet Survey Satellite), and in this exploration, it has been\r\ndiscovered that some of these stars are not behaving as expected. Red giants are stars that have\r\nevolved off of the main sequence after having completed fusing hydrogen into helium in their\r\ncore. Observational data shows that the cores are rotating significantly slower than models can\r\nrecreate consistently across evolutionary stages. This discrepancy has prompted investigation\r\ninto the efficiency of angular momentum transport mechanisms and mixing processes including\r\nmeridional circulation, shear instability, internal gravity waves, Tayler-Spruit dynamo, fossil\r\nmagnetic fields etc., to explain this behavior.\r\nAnalyzing seismic oscillations in stars, via asteroseismology, is a powerful tool as it is the only\r\nway in which the deep stellar interior can be probed and subsequently characterized; this is\r\npossible as global oscillations modulating the stellar surface are effected by internal processes.\r\nFor red giants, p-modes (pressure modes; resonating through the entire star) and g-modes\r\n(gravity-modes; resonating in the radiative interior) couple to create mixed modes. These\r\nmixed modes give access to the otherwise hidden stellar interior as g-modes couple to p-modes,\r\ndelivering information from the interior to the surface.\r\nInternal magnetic signatures have been observationally confirmed in red giant stars via\r\nasteroseismology and characterized in two ways. One being that dipole mixed modes with\r\nℓ = 1 will display a global asymmetric frequency shift of its azimuthal components; where\r\nthe m = 0 and m = ±1 components of the ℓ = 1 dipole mode will be shifted by two\r\ndifferent power laws, respectively. And the other being a reduced visibility of dipole mixed\r\nmode amplitudes in the power spectra, where stars presenting with this feature are denoted as\r\nsuppressed.\r\nSeveral studies of the suppressed dipole mixed mode amplitudes have been carried out, but thus\r\nfar, no dedicated studies of the asymmetric frequency shifts of suppressed red giants have been\r\nconducted; one reason being that the asymmetric frequency shifts cannot be characterized\r\nwhen the dipole mixed mode amplitudes are severely reduced in many of the suppressed stars.\r\nSincefullysuppressedstarsdonothavedetectablemixed-modestoevaluate, partiallysuppressed\r\nstars, that is, red giant stars presenting with suppressed dipole mixed modes in select parts of\r\ntheir power spectra rather than across the entire spectra, will be the subject of this study as\r\nthe respective mode amplitudes are still visible at high frequencies.\r\nAs such, this study will search for asymmetric frequency shifts on the dipole mixed\r\nmodes of partially suppressed red giant stars; the aim here is to investigate if both\r\nmode suppression and magnetic shifting of dipole mixed modes occur simultaneously.\r\nThisstudywillbeconductedbycreatingapipelinetoestimatepriorsofasteroseismicparameters,\r\nuse the priors to model the power spectra with the stellar modeling code sloscillations_ISTA,\r\nand perform a Bayesian fit of the parameters with the simulated data on the star KIC 6975038,\r\na target with partially suppressed dipolar mode amplitudes identified in the literature, to fit its\r\nmagnetic parameters. I present a novel method to model the stellar power spectra of\r\npartially suppressed red giants by application of a sigmoid profile to the ℓ= 1 dipolar\r\nmode component of the spectra. With the results of this study I aim at constraining\r\nthe cause of this partial dipole mode amplitude suppression, allowing for more detailed\r\nstudies regarding their astrophysical nature. Furthermore, the long term hope for the method\r\nused in this study will be to expand the sample of partially suppressed red giants and fit their\r\nasteroseismic parameters accordingly.","lang":"eng"}],"article_processing_charge":"No","page":"38","keyword":["asteroseismology","stellar physics","red giant","magnetism","suppressed"],"supervisor":[{"orcid":"0000-0003-0142-4000","id":"d9edb345-f866-11ec-9b37-d119b5234501","full_name":"Bugnet, Lisa Annabelle","first_name":"Lisa Annabelle","last_name":"Bugnet"}],"degree_awarded":"MS","title":"Exploring internal magnetism in partially suppressed red giant stars"},{"volume":91,"OA_place":"publisher","author":[{"first_name":"Samuel","last_name":"Pastva","full_name":"Pastva, Samuel","orcid":"0000-0003-1993-0331","id":"07c5ea74-f61c-11ec-a664-aa7c5d957b2b"},{"last_name":"Park","first_name":"Kyu Hyong","full_name":"Park, Kyu Hyong"},{"first_name":"Ondřej","last_name":"Huvar","full_name":"Huvar, Ondřej"},{"full_name":"Rozum, Jordan C.","first_name":"Jordan C.","last_name":"Rozum"},{"full_name":"Albert, Réka","first_name":"Réka","last_name":"Albert"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","abstract":[{"text":"Asynchronous Boolean networks are a type of discrete dynamical system in which each variable can take one of two states, and a single variable state is updated in each time step according to pre-selected rules. Boolean networks are popular in systems biology due to their ability to model long-term biological phenotypes within a qualitative, predictive framework. Boolean networks model phenotypes as attractors, which are closely linked to minimal trap spaces (inescapable hypercubes in the system’s state space). In biological applications, attractors and minimal trap spaces are typically in one-to-one correspondence. However, this correspondence is not guaranteed: motif-avoidant attractors (MAAs) that lie outside minimal trap spaces are possible. MAAs are rare and poorly understood, despite recent efforts. In this contribution to the BMB & JMB Special Collection “Problems, Progress and Perspectives in Mathematical and Computational Biology”, we summarize the current state of knowledge regarding MAAs and present several novel observations regarding their response to node deletion reductions and linear extensions of edges. We conduct large-scale computational studies on an ensemble of 14 000 models derived from published Boolean models of biological systems, and more than 100 million Random Boolean Networks. Our findings quantify the rarity of MAAs; in particular, we only observed MAAs in biological models after applying standard simplification methods, highlighting the role of network reduction in introducing MAAs into the dynamics. We also show that MAAs are fragile to linear extensions: in sparse networks, even a single linear node can disrupt virtually all MAAs. Motivated by this observation, we improve the upper bound on the number of delays needed to disrupt a motif-avoidant attractor.","lang":"eng"}],"external_id":{"arxiv":["2410.03976"],"isi":["001507009300001"]},"publication_status":"published","article_processing_charge":"Yes (in subscription journal)","title":"An open problem: Why are motif-avoidant attractors so rare in asynchronous Boolean networks?","article_number":"11","year":"2025","date_created":"2025-06-22T22:02:05Z","publication":"Journal of Mathematical Biology","doi":"10.1007/s00285-025-02235-8","publication_identifier":{"issn":["0303-6812"],"eissn":["1432-1416"]},"quality_controlled":"1","file":[{"file_id":"19871","file_size":1243163,"date_updated":"2025-06-23T11:10:01Z","checksum":"a385ef2662f1d0c3497ed3f2721fe594","relation":"main_file","access_level":"open_access","content_type":"application/pdf","file_name":"2025_JourMathBiology_Pastva.pdf","date_created":"2025-06-23T11:10:01Z","creator":"dernst","success":1}],"corr_author":"1","ddc":["000"],"has_accepted_license":"1","type":"journal_article","acknowledgement":"Ondřej Huvar has been supported by the Czech Science Foundation grant No. GA22-10845S. Samuel Pastva received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grant Agreement No. 101034413. Kyu Hyong Park and Réka Albert have been supported by NSF grant MCB 1715826 and ARO grant 79961-SM-MUR. No funding bodies had any role in study design, analysis, decision to publish, or preparation of the manuscript.","article_type":"original","oa_version":"Published Version","intvolume":"        91","_id":"19854","scopus_import":"1","oa":1,"file_date_updated":"2025-06-23T11:10:01Z","isi":1,"department":[{"_id":"ToHe"}],"arxiv":1,"publisher":"Springer Nature","date_updated":"2025-09-30T13:36:46Z","language":[{"iso":"eng"}],"month":"06","date_published":"2025-06-12T00:00:00Z","ec_funded":1,"OA_type":"hybrid","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"status":"public","day":"12","project":[{"name":"IST-BRIDGE: International postdoctoral program","call_identifier":"H2020","grant_number":"101034413","_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c"}],"citation":{"ista":"Pastva S, Park KH, Huvar O, Rozum JC, Albert R. 2025. An open problem: Why are motif-avoidant attractors so rare in asynchronous Boolean networks? Journal of Mathematical Biology. 91, 11.","ama":"Pastva S, Park KH, Huvar O, Rozum JC, Albert R. An open problem: Why are motif-avoidant attractors so rare in asynchronous Boolean networks? <i>Journal of Mathematical Biology</i>. 2025;91. doi:<a href=\"https://doi.org/10.1007/s00285-025-02235-8\">10.1007/s00285-025-02235-8</a>","ieee":"S. Pastva, K. H. Park, O. Huvar, J. C. Rozum, and R. Albert, “An open problem: Why are motif-avoidant attractors so rare in asynchronous Boolean networks?,” <i>Journal of Mathematical Biology</i>, vol. 91. Springer Nature, 2025.","short":"S. Pastva, K.H. Park, O. Huvar, J.C. Rozum, R. Albert, Journal of Mathematical Biology 91 (2025).","mla":"Pastva, Samuel, et al. “An Open Problem: Why Are Motif-Avoidant Attractors so Rare in Asynchronous Boolean Networks?” <i>Journal of Mathematical Biology</i>, vol. 91, 11, Springer Nature, 2025, doi:<a href=\"https://doi.org/10.1007/s00285-025-02235-8\">10.1007/s00285-025-02235-8</a>.","chicago":"Pastva, Samuel, Kyu Hyong Park, Ondřej Huvar, Jordan C. Rozum, and Réka Albert. “An Open Problem: Why Are Motif-Avoidant Attractors so Rare in Asynchronous Boolean Networks?” <i>Journal of Mathematical Biology</i>. Springer Nature, 2025. <a href=\"https://doi.org/10.1007/s00285-025-02235-8\">https://doi.org/10.1007/s00285-025-02235-8</a>.","apa":"Pastva, S., Park, K. H., Huvar, O., Rozum, J. C., &#38; Albert, R. (2025). An open problem: Why are motif-avoidant attractors so rare in asynchronous Boolean networks? <i>Journal of Mathematical Biology</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s00285-025-02235-8\">https://doi.org/10.1007/s00285-025-02235-8</a>"}},{"title":"A negligible contribution of two luminous z ∼7.5 galaxies to the ionizing photon budget of reionization","article_processing_charge":"Yes","page":"2331-2348","publication_status":"published","external_id":{"arxiv":["2410.03337"],"isi":["001506103600001"]},"abstract":[{"lang":"eng","text":"We present indirect constraints on the absolute escape fraction of ionizing photons (f_{\\rm esc}^{\\rm LyC}) of the system GN 42912 which comprises two luminous galaxies (M_{\\rm UV} magnitudes of -20.89 and -20.37) at z\\sim7.5, GN 42912-NE and GN 42912-SW, to determine their contribution to the ionizing photon budget of the Epoch of Reionization (EoR). The high-resolution James Webb Space Telescope NIRSpec and NIRCam observations reveal the two galaxies are separated by only ~0.1\" (0.5 kpc) on the sky and have a 358 km s^{-1} velocity separation. GN 42912-NE and GN 42912-SW are relatively massive for this redshift (log(M_\\ast/M_\\odot) \\sim 8.4 and 8.9, respectively), with gas-phase metallicities of 18 per cent and 23 per cent solar, O_{32} ratios of 5.3 and >5.8, and \\beta slopes of -1.92 and -1.51, respectively. We use the Mg II\\lambda\\lambda2796,2803 doublet to constrain f_{\\rm esc}^{\\rm LyC}. Mg II has an ionization potential close to that of neutral hydrogen and, in the optically thin regime, can be used as an indirect tracer of the LyC leakage. We establish realistic conservative upper limits on f_{\\rm esc}^{\\rm LyC} of 8.5 per cent for GN 42912-NE and 14 per cent for GN 42912-SW. These estimates align with f_{\\rm esc}^{\\rm LyC} trends observed with \\beta, O_{32}, and the H\\beta equivalent width at z<4. The small inferred ionized region sizes (<0.3 pMpc) around both galaxies indicate they have not ionized a significant fraction of the surrounding neutral gas. While these z>7 f_{\\rm esc}^{\\rm LyC} constraints do not decisively determine a specific reionization model, they support a minor contribution from these two relatively luminous galaxies to the EoR."}],"author":[{"full_name":"Gazagnes, S.","first_name":"S.","last_name":"Gazagnes"},{"full_name":"Chisholm, J.","last_name":"Chisholm","first_name":"J."},{"last_name":"Endsley","first_name":"R.","full_name":"Endsley, R."},{"full_name":"Berg, D. A.","first_name":"D. A.","last_name":"Berg"},{"last_name":"Leclercq","first_name":"F.","full_name":"Leclercq, F."},{"full_name":"Jurlin, N.","last_name":"Jurlin","first_name":"N."},{"full_name":"Saldana-Lopez, A.","first_name":"A.","last_name":"Saldana-Lopez"},{"full_name":"Finkelstein, S. L.","last_name":"Finkelstein","first_name":"S. L."},{"last_name":"Flury","first_name":"S. R.","full_name":"Flury, S. R."},{"last_name":"Guseva","first_name":"N. G.","full_name":"Guseva, N. G."},{"first_name":"A.","last_name":"Henry","full_name":"Henry, A."},{"first_name":"Y. I.","last_name":"Izotov","full_name":"Izotov, Y. I."},{"first_name":"I.","last_name":"Jung","full_name":"Jung, I."},{"full_name":"Matthee, Jorryt J","orcid":"0000-0003-2871-127X","id":"7439a258-f3c0-11ec-9501-9df22fe06720","first_name":"Jorryt J","last_name":"Matthee"},{"full_name":"Schaerer, D.","first_name":"D.","last_name":"Schaerer"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","volume":540,"OA_place":"publisher","has_accepted_license":"1","ddc":["520"],"quality_controlled":"1","file":[{"date_updated":"2025-06-23T11:02:59Z","file_size":3111567,"access_level":"open_access","relation":"main_file","checksum":"f912c990a0474f1ddf9be6b8a89c7759","file_id":"19870","success":1,"creator":"dernst","file_name":"2025_MonthlyNoticesRAS_Gazagnes.pdf","content_type":"application/pdf","date_created":"2025-06-23T11:02:59Z"}],"doi":"10.1093/mnras/staf768","publication_identifier":{"issn":["0035-8711"],"eissn":["1365-2966"]},"issue":"3","publication":"Monthly Notices of the Royal Astronomical Society","date_created":"2025-06-22T22:02:05Z","year":"2025","date_published":"2025-07-01T00:00:00Z","month":"07","language":[{"iso":"eng"}],"date_updated":"2025-09-30T13:34:20Z","department":[{"_id":"JoMa"}],"arxiv":1,"publisher":"Oxford University Press","isi":1,"file_date_updated":"2025-06-23T11:02:59Z","oa":1,"scopus_import":"1","_id":"19855","intvolume":"       540","oa_version":"Published Version","article_type":"original","acknowledgement":"This work is based on observations made with the NASA/ESA/CSA JWST. 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 #01871. Support for program #01871 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–03127. SG is grateful for the support enabled by the Harlan J. Smith McDonald fellowship. YI and NG acknowledge support from the Simons Foundation and the National Academy of Sciences of Ukraine (Project 0121U109612). ASL acknowledges support from Knut and Alice Wallenberg Foundation.","type":"journal_article","citation":{"short":"S. Gazagnes, J. Chisholm, R. Endsley, D.A. Berg, F. Leclercq, N. Jurlin, A. Saldana-Lopez, S.L. Finkelstein, S.R. Flury, N.G. Guseva, A. Henry, Y.I. Izotov, I. Jung, J.J. Matthee, D. Schaerer, Monthly Notices of the Royal Astronomical Society 540 (2025) 2331–2348.","ieee":"S. Gazagnes <i>et al.</i>, “A negligible contribution of two luminous z ∼7.5 galaxies to the ionizing photon budget of reionization,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 540, no. 3. Oxford University Press, pp. 2331–2348, 2025.","ista":"Gazagnes S, Chisholm J, Endsley R, Berg DA, Leclercq F, Jurlin N, Saldana-Lopez A, Finkelstein SL, Flury SR, Guseva NG, Henry A, Izotov YI, Jung I, Matthee JJ, Schaerer D. 2025. A negligible contribution of two luminous z ∼7.5 galaxies to the ionizing photon budget of reionization. Monthly Notices of the Royal Astronomical Society. 540(3), 2331–2348.","ama":"Gazagnes S, Chisholm J, Endsley R, et al. A negligible contribution of two luminous z ∼7.5 galaxies to the ionizing photon budget of reionization. <i>Monthly Notices of the Royal Astronomical Society</i>. 2025;540(3):2331-2348. doi:<a href=\"https://doi.org/10.1093/mnras/staf768\">10.1093/mnras/staf768</a>","chicago":"Gazagnes, S., J. Chisholm, R. Endsley, D. A. Berg, F. Leclercq, N. Jurlin, A. Saldana-Lopez, et al. “A Negligible Contribution of Two Luminous z ∼7.5 Galaxies to the Ionizing Photon Budget of Reionization.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2025. <a href=\"https://doi.org/10.1093/mnras/staf768\">https://doi.org/10.1093/mnras/staf768</a>.","apa":"Gazagnes, S., Chisholm, J., Endsley, R., Berg, D. A., Leclercq, F., Jurlin, N., … Schaerer, D. (2025). A negligible contribution of two luminous z ∼7.5 galaxies to the ionizing photon budget of reionization. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/staf768\">https://doi.org/10.1093/mnras/staf768</a>","mla":"Gazagnes, S., et al. “A Negligible Contribution of Two Luminous z ∼7.5 Galaxies to the Ionizing Photon Budget of Reionization.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 540, no. 3, Oxford University Press, 2025, pp. 2331–48, doi:<a href=\"https://doi.org/10.1093/mnras/staf768\">10.1093/mnras/staf768</a>."},"status":"public","day":"01","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"OA_type":"gold"},{"external_id":{"isi":["001509005900006"],"arxiv":["2412.05031"]},"publication_status":"published","abstract":[{"text":"Unlike in crystals, it is difficult to trace emergent material properties of amorphous solids to their underlying structure. Nevertheless, one can tune features of a disordered spring network, ranging from bulk elastic constants to specific allosteric responses, through highly precise alterations of the structure. This has been understood through the notion of independent bond-level response—the observation that, in many cases, different springs have different effects on different properties. While this idea has motivated inverse design in numerous contexts, it has not been formalized and quantified in a general context that not just informs but enables and predicts inverse design. Here, we show how to quantify independent response by linearizing the simultaneous change in multiple emergent features, and introduce the much stronger notion of fully independent response. Remarkably, we find that the mechanical properties of disordered solids are always fully independent across a wide array of scenarios, regardless of the target features, tunable parameters, system size, dimensionality, and class of interactions. Furthermore, our formulation quantifies the susceptibility of features to parameter changes, which is correlated with the maximum linear tunability. We also demonstrate the implications for multifeature inverse design beyond the linear regime. These results formalize our understanding of a key fundamental difference between ordered and disordered solids while also creating a practical tool to both understand and perform inverse design.","lang":"eng"}],"article_processing_charge":"Yes (via OA deal)","title":"Fully independent response in disordered solids","volume":134,"OA_place":"publisher","user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","author":[{"first_name":"Mengjie","last_name":"Zu","id":"26dd9e7c-e86a-11eb-a854-82ac731c9ae2","full_name":"Zu, Mengjie"},{"last_name":"Desai","first_name":"Aayush A","full_name":"Desai, Aayush A","id":"502cfd30-32c1-11ee-a9a4-d8dad5c6739e"},{"last_name":"Goodrich","first_name":"Carl Peter","orcid":"0000-0002-1307-5074","id":"EB352CD2-F68A-11E9-89C5-A432E6697425","full_name":"Goodrich, Carl Peter"}],"related_material":{"link":[{"description":"News on ISTA website","url":"https://ista.ac.at/en/news/infinite-diversity-in-infinite-combinations/","relation":"press_release"}]},"file":[{"content_type":"application/pdf","file_name":"2025_PhysReviewLetters_Zu.pdf","date_created":"2025-06-23T11:41:08Z","creator":"dernst","success":1,"file_id":"19874","file_size":1132625,"date_updated":"2025-06-23T11:41:08Z","checksum":"040b6779c91aac62c15a9b2cc417b360","relation":"main_file","access_level":"open_access"}],"quality_controlled":"1","corr_author":"1","ddc":["530"],"has_accepted_license":"1","article_number":"238201","date_created":"2025-06-22T22:02:06Z","year":"2025","publication":"Physical Review Letters","doi":"10.1103/PhysRevLett.134.238201","publication_identifier":{"eissn":["1079-7114"],"issn":["0031-9007"]},"issue":"23","file_date_updated":"2025-06-23T11:41:08Z","oa":1,"isi":1,"date_updated":"2026-04-28T13:28:02Z","department":[{"_id":"CaGo"},{"_id":"IlCa"}],"arxiv":1,"publisher":"American Physical Society","date_published":"2025-06-13T00:00:00Z","month":"06","language":[{"iso":"eng"}],"acknowledgement":"We gratefully acknowledge Edouard Hannezo for helpful comments on the manuscript. The work was funded by the Institute of Science and Technology Austria.","type":"journal_article","intvolume":"       134","oa_version":"Published Version","article_type":"original","scopus_import":"1","_id":"19856","citation":{"short":"M. Zu, A.A. Desai, C.P. Goodrich, Physical Review Letters 134 (2025).","ieee":"M. Zu, A. A. Desai, and C. P. Goodrich, “Fully independent response in disordered solids,” <i>Physical Review Letters</i>, vol. 134, no. 23. American Physical Society, 2025.","ama":"Zu M, Desai AA, Goodrich CP. Fully independent response in disordered solids. <i>Physical Review Letters</i>. 2025;134(23). doi:<a href=\"https://doi.org/10.1103/PhysRevLett.134.238201\">10.1103/PhysRevLett.134.238201</a>","ista":"Zu M, Desai AA, Goodrich CP. 2025. Fully independent response in disordered solids. Physical Review Letters. 134(23), 238201.","apa":"Zu, M., Desai, A. A., &#38; Goodrich, C. P. (2025). Fully independent response in disordered solids. <i>Physical Review Letters</i>. American Physical Society. <a href=\"https://doi.org/10.1103/PhysRevLett.134.238201\">https://doi.org/10.1103/PhysRevLett.134.238201</a>","chicago":"Zu, Mengjie, Aayush A Desai, and Carl Peter Goodrich. “Fully Independent Response in Disordered Solids.” <i>Physical Review Letters</i>. American Physical Society, 2025. <a href=\"https://doi.org/10.1103/PhysRevLett.134.238201\">https://doi.org/10.1103/PhysRevLett.134.238201</a>.","mla":"Zu, Mengjie, et al. “Fully Independent Response in Disordered Solids.” <i>Physical Review Letters</i>, vol. 134, no. 23, 238201, American Physical Society, 2025, doi:<a href=\"https://doi.org/10.1103/PhysRevLett.134.238201\">10.1103/PhysRevLett.134.238201</a>."},"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"OA_type":"hybrid","status":"public","day":"13"},{"status":"public","day":"11","OA_type":"hybrid","ec_funded":1,"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"citation":{"ista":"Nikolic N, Pleska M, Bergmiller T, Guet CC. 2025. A bacterial toxin-antitoxin system as a native defence element against RNA phages. Biology Letters. 21(6), 20250080.","ama":"Nikolic N, Pleska M, Bergmiller T, Guet CC. A bacterial toxin-antitoxin system as a native defence element against RNA phages. <i>Biology Letters</i>. 2025;21(6). doi:<a href=\"https://doi.org/10.1098/rsbl.2025.0080\">10.1098/rsbl.2025.0080</a>","ieee":"N. Nikolic, M. Pleska, T. Bergmiller, and C. C. Guet, “A bacterial toxin-antitoxin system as a native defence element against RNA phages,” <i>Biology Letters</i>, vol. 21, no. 6. The Royal Society, 2025.","short":"N. Nikolic, M. Pleska, T. Bergmiller, C.C. Guet, Biology Letters 21 (2025).","mla":"Nikolic, Nela, et al. “A Bacterial Toxin-Antitoxin System as a Native Defence Element against RNA Phages.” <i>Biology Letters</i>, vol. 21, no. 6, 20250080, The Royal Society, 2025, doi:<a href=\"https://doi.org/10.1098/rsbl.2025.0080\">10.1098/rsbl.2025.0080</a>.","apa":"Nikolic, N., Pleska, M., Bergmiller, T., &#38; Guet, C. C. (2025). A bacterial toxin-antitoxin system as a native defence element against RNA phages. <i>Biology Letters</i>. The Royal Society. <a href=\"https://doi.org/10.1098/rsbl.2025.0080\">https://doi.org/10.1098/rsbl.2025.0080</a>","chicago":"Nikolic, Nela, Maros Pleska, Tobias Bergmiller, and Calin C Guet. “A Bacterial Toxin-Antitoxin System as a Native Defence Element against RNA Phages.” <i>Biology Letters</i>. The Royal Society, 2025. <a href=\"https://doi.org/10.1098/rsbl.2025.0080\">https://doi.org/10.1098/rsbl.2025.0080</a>."},"project":[{"name":"International IST Postdoc Fellowship Programme","call_identifier":"FP7","grant_number":"291734","_id":"25681D80-B435-11E9-9278-68D0E5697425"},{"_id":"26956E74-B435-11E9-9278-68D0E5697425","grant_number":"V00738","call_identifier":"FWF","name":"Bacterial toxin-antitoxin systems as antiphage defense mechanisms"}],"_id":"19857","scopus_import":"1","article_type":"original","intvolume":"        21","oa_version":"Published Version","type":"journal_article","acknowledgement":"This work was supported by ISTFELLOW (People Program – Marie Curie Actions of the European Union’s Seventh Framework Program FP7 under REA grant agreement 291734), the FWF (Austrian Science Fund) Elise Richter Program project number V 738 and the Wellcome Trust Institutional Strategic Support Award (WT105618MA), to N.N. M.P. was a Simons Foundation Fellow of the Life Sciences Research Foundation. We are grateful to Kathrin Tomasek, Lisa Butt, Chris Estell, Alys Jepson, Franklin Nobrega, Stefano Pagliara, Remy Chait, Steve West, Vicki Gold, Josh Eaton, Ivana Gudelj and Rob Beardmore for useful discussions and technical support, as well as to Robin Wright, Christian Fitch and Ben Temperton for sharing equipment. We thank Laurence Van Melderen for sharing the strains. We acknowledge the IST Austria Lab Support Facility, LSI Technical Services Team at the University of Exeter and the Translational Research Exchange @ Exeter (TREE) network. N.N. is grateful to Fabrice Gielen for his support.","month":"06","language":[{"iso":"eng"}],"date_published":"2025-06-11T00:00:00Z","publisher":"The Royal Society","department":[{"_id":"CaGu"}],"date_updated":"2025-09-30T13:38:08Z","isi":1,"oa":1,"file_date_updated":"2025-06-23T11:34:39Z","issue":"6","publication_identifier":{"eissn":["1744-957X"],"issn":["1744-9561"]},"doi":"10.1098/rsbl.2025.0080","publication":"Biology Letters","year":"2025","date_created":"2025-06-22T22:02:06Z","article_number":"20250080","has_accepted_license":"1","ddc":["570"],"corr_author":"1","quality_controlled":"1","file":[{"creator":"dernst","success":1,"date_created":"2025-06-23T11:34:39Z","file_name":"2025_BiologyLetters_Nikolic.pdf","content_type":"application/pdf","checksum":"016f644ed068f8609ded306ad26dbd3f","relation":"main_file","access_level":"open_access","file_size":1850797,"date_updated":"2025-06-23T11:34:39Z","file_id":"19873"}],"acknowledged_ssus":[{"_id":"LifeSc"}],"pmid":1,"author":[{"first_name":"Nela","last_name":"Nikolic","id":"42D9CABC-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-9068-6090","full_name":"Nikolic, Nela"},{"last_name":"Pleska","first_name":"Maros","orcid":"0000-0001-7460-7479","id":"4569785E-F248-11E8-B48F-1D18A9856A87","full_name":"Pleska, Maros"},{"full_name":"Bergmiller, Tobias","id":"2C471CFA-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-5396-4346","last_name":"Bergmiller","first_name":"Tobias"},{"first_name":"Calin C","last_name":"Guet","full_name":"Guet, Calin C","orcid":"0000-0001-6220-2052","id":"47F8433E-F248-11E8-B48F-1D18A9856A87"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","volume":21,"OA_place":"publisher","title":"A bacterial toxin-antitoxin system as a native defence element against RNA phages","article_processing_charge":"Yes (via OA deal)","abstract":[{"lang":"eng","text":"Bacteria have evolved a wide range of defence strategies to protect themselves against bacterial viruses (phages). Most known bacterial antiphage defence systems target phages with DNA genomes, which raises the question of how bacteria defend against phages with RNA genomes. Bacterial toxin–antitoxin systems that cleave intracellular RNA could potentially protect bacteria against RNA phages, but this has not been explored experimentally. In this study, we investigated the role of a model toxin–antitoxin system, MazEF, in protecting Escherichia coli against two RNA phage species. When challenged with these phages, the native presence of mazEF moderately reduced population susceptibility and increased the survival of individual E. coli cells. Genomic analysis further revealed an underrepresentation of the MazF cleavage site in genomes of RNA phages infecting E. coli, indicating selection against cleavage. These results show that, in addition to other physiological roles, RNA-degrading toxin–antitoxin systems may also help defend against RNA phages."}],"external_id":{"pmid":["40494395"],"isi":["001505019800001"]},"publication_status":"published"},{"intvolume":"       330","oa_version":"Published Version","acknowledgement":"This project has received funding from the European Research Council (ERC) under the\r\nEuropean Union’s Horizon 2020 research and innovation programme (MoDynStruct, No. 101019564) and the Austrian Science Fund (FWF) grant DOI 10.55776/Z422, grant DOI 10.55776/I5982, and grant DOI 10.55776/P33775 with additional funding from the netidee SCIENCE Stiftung, 2020–2024. This work was further supported by the Federal Ministry of Education and Research (BMBF) project, 6G-RIC: 6G Research and Innovation Cluster, grant 16KISK020K.","type":"conference","_id":"19858","scopus_import":"1","isi":1,"oa":1,"file_date_updated":"2025-06-23T11:23:29Z","language":[{"iso":"eng"}],"month":"06","date_published":"2025-06-02T00:00:00Z","department":[{"_id":"MoHe"}],"arxiv":1,"publisher":"Schloss Dagstuhl - Leibniz-Zentrum für Informatik","date_updated":"2025-09-30T13:37:28Z","OA_type":"gold","ec_funded":1,"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"alternative_title":["LIPIcs"],"day":"02","status":"public","citation":{"mla":"El-Hayek, Antoine, et al. “On B-Matching and Fully-Dynamic Maximum k-Edge Coloring.” <i>4th Symposium on Algorithmic Foundations of Dynamic Networks</i>, vol. 330, 4, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2025, doi:<a href=\"https://doi.org/10.4230/LIPIcs.SAND.2025.4\">10.4230/LIPIcs.SAND.2025.4</a>.","chicago":"El-Hayek, Antoine, Kathrin Hanauer, and Monika Henzinger. “On B-Matching and Fully-Dynamic Maximum k-Edge Coloring.” In <i>4th Symposium on Algorithmic Foundations of Dynamic Networks</i>, Vol. 330. Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2025. <a href=\"https://doi.org/10.4230/LIPIcs.SAND.2025.4\">https://doi.org/10.4230/LIPIcs.SAND.2025.4</a>.","apa":"El-Hayek, A., Hanauer, K., &#38; Henzinger, M. (2025). On b-matching and fully-dynamic maximum k-edge coloring. In <i>4th Symposium on Algorithmic Foundations of Dynamic Networks</i> (Vol. 330). Liverpool, United Kingdom: Schloss Dagstuhl - Leibniz-Zentrum für Informatik. <a href=\"https://doi.org/10.4230/LIPIcs.SAND.2025.4\">https://doi.org/10.4230/LIPIcs.SAND.2025.4</a>","ama":"El-Hayek A, Hanauer K, Henzinger M. On b-matching and fully-dynamic maximum k-edge coloring. In: <i>4th Symposium on Algorithmic Foundations of Dynamic Networks</i>. Vol 330. Schloss Dagstuhl - Leibniz-Zentrum für Informatik; 2025. doi:<a href=\"https://doi.org/10.4230/LIPIcs.SAND.2025.4\">10.4230/LIPIcs.SAND.2025.4</a>","ista":"El-Hayek A, Hanauer K, Henzinger M. 2025. On b-matching and fully-dynamic maximum k-edge coloring. 4th Symposium on Algorithmic Foundations of Dynamic Networks. SAND: Symposium on Algorithmic Foundations of Dynamic Networks, LIPIcs, vol. 330, 4.","ieee":"A. El-Hayek, K. Hanauer, and M. Henzinger, “On b-matching and fully-dynamic maximum k-edge coloring,” in <i>4th Symposium on Algorithmic Foundations of Dynamic Networks</i>, Liverpool, United Kingdom, 2025, vol. 330.","short":"A. El-Hayek, K. Hanauer, M. Henzinger, in:, 4th Symposium on Algorithmic Foundations of Dynamic Networks, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2025."},"project":[{"name":"The design and evaluation of modern fully dynamic data structures","call_identifier":"H2020","grant_number":"101019564","_id":"bd9ca328-d553-11ed-ba76-dc4f890cfe62"},{"name":"Efficient algorithms","_id":"34def286-11ca-11ed-8bc3-da5948e1613c","grant_number":"Z00422"},{"name":"Static and Dynamic Hierarchical Graph Decompositions","grant_number":"I05982","_id":"bda196b2-d553-11ed-ba76-8e8ee6c21103"},{"name":"Fast Algorithms for a Reactive Network Layer","grant_number":"P33775","_id":"bd9e3a2e-d553-11ed-ba76-8aa684ce17fe"}],"author":[{"full_name":"El-Hayek, Antoine","orcid":"0000-0003-4268-7368","id":"888a098e-fcac-11ee-aff7-d347be57b725","first_name":"Antoine","last_name":"El-Hayek"},{"full_name":"Hanauer, Kathrin","first_name":"Kathrin","last_name":"Hanauer"},{"full_name":"Henzinger, Monika H","id":"540c9bbd-f2de-11ec-812d-d04a5be85630","orcid":"0000-0002-5008-6530","last_name":"Henzinger","first_name":"Monika H"}],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","OA_place":"publisher","volume":330,"article_processing_charge":"No","abstract":[{"lang":"eng","text":"Given a graph G that undergoes a sequence of edge insertions and deletions, we study the Maximum k-Edge Coloring problem (MkEC): Having access to k different colors, color as many edges of G as possible such that no two adjacent edges share the same color. While this problem is different from simply maintaining a b-matching with b = k, the two problems are related. However, maximum b-matching can be solved efficiently in the static setting, whereas MkEC is NP-hard and even APX-hard for k ≥ 2. \r\nWe present new results on both problems: For b-matching, we show a new integrality gap result and we adapt Wajc’s matching sparsification scheme [David Wajc, 2020] for the case where b is a constant.\r\nUsing these as basis, we give three new algorithms for the dynamic MkEC problem: Our MatchO algorithm builds on the dynamic (2+ε)-approximation algorithm of Bhattacharya, Gupta, and Mohan [Sayan Bhattacharya et al., 2017] for b-matching and achieves a (2+ε)(k+1)/k-approximation in O(poly(log n, ε^-1)) update time against an oblivious adversary. Our MatchA algorithm builds on the dynamic (7+ε)-approximation algorithm by Bhattacharya, Henzinger, and Italiano [Sayan Bhattacharya et al., 2015] for fractional b-matching and achieves a (7+ε)(3k+3)/(3k-1)-approximation in O(poly(log n, ε^-1)) update time against an adaptive adversary. Moreover, our reductions use the dynamic b-matching algorithm as a black box, so any future improvement in the approximation ratio for dynamic b-matching will automatically translate into a better approximation ratio for our algorithms. Finally, we present a greedy algorithm with O(Δ+k) update time, which guarantees a 2.16 approximation factor."}],"external_id":{"arxiv":["2310.01149"],"isi":["001532136900004"]},"publication_status":"published","title":"On b-matching and fully-dynamic maximum k-edge coloring","year":"2025","date_created":"2025-06-22T22:02:06Z","article_number":"4","doi":"10.4230/LIPIcs.SAND.2025.4","publication_identifier":{"isbn":["9783959773683"],"issn":["1868-8969"]},"publication":"4th Symposium on Algorithmic Foundations of Dynamic Networks","corr_author":"1","file":[{"date_updated":"2025-06-23T11:23:29Z","file_size":995666,"checksum":"ad93a1e052adb29d7bfe8bd551bab193","relation":"main_file","access_level":"open_access","file_id":"19872","creator":"dernst","success":1,"content_type":"application/pdf","file_name":"2025_LIPIcs_ElHayek.pdf","date_created":"2025-06-23T11:23:29Z"}],"quality_controlled":"1","has_accepted_license":"1","conference":{"name":"SAND: Symposium on Algorithmic Foundations of Dynamic Networks","start_date":"2025-06-09","end_date":"2025-06-11","location":"Liverpool, United Kingdom"},"ddc":["000"]},{"author":[{"id":"9aa8388e-d003-11ee-8458-c4c1d7447977","full_name":"Lichev, Lyuben","first_name":"Lyuben","last_name":"Lichev"},{"full_name":"Schapira, Bruno","first_name":"Bruno","last_name":"Schapira"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","volume":8,"OA_place":"publisher","page":"35-65","article_processing_charge":"Yes","abstract":[{"text":"We consider a recently introduced model of color-avoiding percolation (abbreviated CA-percolation) defined as follows. Every edge in a graph G is colored in some of k>=2 colors. Two vertices u and v in G are said to be CA-connected if u and v may be connected using any subset of k-1 colors. CA-connectivity defines an equivalence relation on the vertex set of G whose classes are called CA-components.\r\nWe study the component structure of a randomly colored Erdős–Rényi random graph of constant average degree. We distinguish three regimes for the size of the largest component: a supercritical regime, a so-called intermediate regime, and a subcritical regime, in which the largest CA-component has respectively linear, logarithmic, and bounded size. Interestingly, in the subcritical regime, the bound is deterministic and given by the number of colors.","lang":"eng"}],"publication_status":"published","external_id":{"arxiv":["2211.16086 "]},"title":"Color-avoiding percolation on the Erdős–Rényi random graph","year":"2025","date_created":"2025-06-22T22:02:07Z","publication_identifier":{"eissn":["2644-9463"]},"doi":"10.5802/ahl.228","publication":"Annales Henri Lebesgue","corr_author":"1","file":[{"content_type":"application/pdf","file_name":"2025_AnnalesHenriLebesgue_Lichev.pdf","date_created":"2025-06-23T11:59:22Z","success":1,"creator":"dernst","file_id":"19875","date_updated":"2025-06-23T11:59:22Z","file_size":746588,"access_level":"open_access","relation":"main_file","checksum":"cca22d171b7affa010d17f5e793b0045"}],"quality_controlled":"1","has_accepted_license":"1","ddc":["510"],"article_type":"original","intvolume":"         8","oa_version":"Published Version","type":"journal_article","acknowledgement":"We thank Dieter Mitsche for enlightening discussions, Balázs Ráth for a number of comments\r\nand corrections on a first version of this paper, and an anonymous referee for several useful remarks.","_id":"19859","scopus_import":"1","oa":1,"file_date_updated":"2025-06-23T11:59:22Z","DOAJ_listed":"1","language":[{"iso":"eng"}],"month":"06","date_published":"2025-06-01T00:00:00Z","arxiv":1,"publisher":"École normale supérieure de Rennes","department":[{"_id":"MaKw"}],"date_updated":"2025-06-23T12:01:36Z","OA_type":"gold","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"day":"01","status":"public","citation":{"ista":"Lichev L, Schapira B. 2025. Color-avoiding percolation on the Erdős–Rényi random graph. Annales Henri Lebesgue. 8, 35–65.","ama":"Lichev L, Schapira B. Color-avoiding percolation on the Erdős–Rényi random graph. <i>Annales Henri Lebesgue</i>. 2025;8:35-65. doi:<a href=\"https://doi.org/10.5802/ahl.228\">10.5802/ahl.228</a>","short":"L. Lichev, B. Schapira, Annales Henri Lebesgue 8 (2025) 35–65.","ieee":"L. Lichev and B. Schapira, “Color-avoiding percolation on the Erdős–Rényi random graph,” <i>Annales Henri Lebesgue</i>, vol. 8. École normale supérieure de Rennes, pp. 35–65, 2025.","mla":"Lichev, Lyuben, and Bruno Schapira. “Color-Avoiding Percolation on the Erdős–Rényi Random Graph.” <i>Annales Henri Lebesgue</i>, vol. 8, École normale supérieure de Rennes, 2025, pp. 35–65, doi:<a href=\"https://doi.org/10.5802/ahl.228\">10.5802/ahl.228</a>.","chicago":"Lichev, Lyuben, and Bruno Schapira. “Color-Avoiding Percolation on the Erdős–Rényi Random Graph.” <i>Annales Henri Lebesgue</i>. École normale supérieure de Rennes, 2025. <a href=\"https://doi.org/10.5802/ahl.228\">https://doi.org/10.5802/ahl.228</a>.","apa":"Lichev, L., &#38; Schapira, B. (2025). Color-avoiding percolation on the Erdős–Rényi random graph. <i>Annales Henri Lebesgue</i>. École normale supérieure de Rennes. <a href=\"https://doi.org/10.5802/ahl.228\">https://doi.org/10.5802/ahl.228</a>"}},{"type":"journal_article","acknowledgement":"We thank Nick Barton for useful comments on the manuscript. This research was supported by the Scientific Service Units (SSU) of Institute of Science and Technology Austria (ISTA) through resources provided by Scientific Computing (SciComp).","article_type":"original","intvolume":"        79","oa_version":"Published Version","_id":"19876","scopus_import":"1","oa":1,"file_date_updated":"2025-12-30T08:43:33Z","isi":1,"publisher":"Oxford University Press","department":[{"_id":"NiBa"}],"date_updated":"2025-12-30T08:44:13Z","month":"07","language":[{"iso":"eng"}],"date_published":"2025-07-01T00:00:00Z","OA_type":"hybrid","tmp":{"short":"CC BY-NC-ND (4.0)","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","image":"/images/cc_by_nc_nd.png"},"status":"public","day":"01","citation":{"ieee":"P. Surendranadh and H. Sachdeva, “Effect of assortative mating and sexual selection on polygenic barriers to gene flow,” <i>Evolution</i>, vol. 79, no. 7. Oxford University Press, pp. 1185–1198, 2025.","short":"P. Surendranadh, H. Sachdeva, Evolution 79 (2025) 1185–1198.","ama":"Surendranadh P, Sachdeva H. Effect of assortative mating and sexual selection on polygenic barriers to gene flow. <i>Evolution</i>. 2025;79(7):1185-1198. doi:<a href=\"https://doi.org/10.1093/evolut/qpaf047\">10.1093/evolut/qpaf047</a>","ista":"Surendranadh P, Sachdeva H. 2025. Effect of assortative mating and sexual selection on polygenic barriers to gene flow. Evolution. 79(7), 1185–1198.","apa":"Surendranadh, P., &#38; Sachdeva, H. (2025). Effect of assortative mating and sexual selection on polygenic barriers to gene flow. <i>Evolution</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/evolut/qpaf047\">https://doi.org/10.1093/evolut/qpaf047</a>","chicago":"Surendranadh, Parvathy, and Himani Sachdeva. “Effect of Assortative Mating and Sexual Selection on Polygenic Barriers to Gene Flow.” <i>Evolution</i>. Oxford University Press, 2025. <a href=\"https://doi.org/10.1093/evolut/qpaf047\">https://doi.org/10.1093/evolut/qpaf047</a>.","mla":"Surendranadh, Parvathy, and Himani Sachdeva. “Effect of Assortative Mating and Sexual Selection on Polygenic Barriers to Gene Flow.” <i>Evolution</i>, vol. 79, no. 7, Oxford University Press, 2025, pp. 1185–98, doi:<a href=\"https://doi.org/10.1093/evolut/qpaf047\">10.1093/evolut/qpaf047</a>."},"OA_place":"publisher","volume":79,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","author":[{"first_name":"Parvathy","last_name":"Surendranadh","id":"455235B8-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-6395-386X","full_name":"Surendranadh, Parvathy"},{"last_name":"Sachdeva","first_name":"Himani","full_name":"Sachdeva, Himani"}],"related_material":{"record":[{"relation":"research_data","id":"18712","status":"public"}]},"acknowledged_ssus":[{"_id":"ScienComp"}],"abstract":[{"lang":"eng","text":"Assortative mating and sexual selection are widespread in nature and can play an important role in speciation by facilitating the buildup and maintenance of reproductive isolation (RI). However, their contribution to genome-wide suppression of gene flow during RI is rarely quantified.\r\nHere, we consider a polygenic “magic” trait that is divergently selected across two populations connected by migration, while also serving as the basis of assortative mating, thus generating sexual selection on one or both sexes. We obtain theoretical predictions for divergence at\r\nindividual trait loci by assuming that the effect of all other loci on any locus can be encapsulated via an effective migration rate, which bears a simple relationship to measurable fitness components of migrants and various early-generation hybrids. Our analysis clarifies how “tipping\r\npoints” (characterized by an abrupt collapse of adaptive divergence) arise, and when assortative mating can shift the critical level of migration beyond which divergence collapses. We quantify the relative contributions of viability and sexual selection to genome-wide barriers to gene\r\nflow and discuss how these depend on existing divergence levels. Our results suggest that effective migration rates provide a useful way of understanding genomic divergence, even in scenarios involving multiple, interacting mechanisms of RI. "}],"publication_status":"published","external_id":{"isi":["001490646300001"]},"page":"1185-1198","article_processing_charge":"Yes (via OA deal)","title":"Effect of assortative mating and sexual selection on polygenic barriers to gene flow","year":"2025","date_created":"2025-06-23T13:51:00Z","publication":"Evolution","issue":"7","doi":"10.1093/evolut/qpaf047","publication_identifier":{"issn":["0014-3820"],"eissn":["1558-5646"]},"file":[{"success":1,"creator":"dernst","date_created":"2025-12-30T08:43:33Z","content_type":"application/pdf","file_name":"2025_Evolution_Surendranadh.pdf","access_level":"open_access","checksum":"288ca936cef794d68a55356e70671846","relation":"main_file","date_updated":"2025-12-30T08:43:33Z","file_size":2784295,"file_id":"20898"}],"quality_controlled":"1","corr_author":"1","ddc":["570"],"has_accepted_license":"1"},{"oa_version":"Published Version","acknowledgement":"The authors would like to thank the Neural Magic team, in particular Michael Goin, Alexander Matveev, and Rob Shaw, for support with the vLLM integration. This research was supported in part by generous grants from NVIDIA and Google.","type":"conference","scopus_import":"1","_id":"19877","isi":1,"file_date_updated":"2025-06-24T06:04:17Z","oa":1,"date_published":"2025-02-28T00:00:00Z","language":[{"iso":"eng"}],"month":"02","date_updated":"2025-09-30T13:41:57Z","department":[{"_id":"DaAl"}],"arxiv":1,"publisher":"Association for Computing Machinery","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"OA_type":"hybrid","day":"28","status":"public","citation":{"apa":"Frantar, E., Castro, R. L., Chen, J., Hoefler, T., &#38; Alistarh, D.-A. (2025). MARLIN: Mixed-precision auto-regressive parallel inference on Large Language Models. In <i>Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel Programming</i> (pp. 239–251). Las Vegas, NV, United States: Association for Computing Machinery. <a href=\"https://doi.org/10.1145/3710848.3710871\">https://doi.org/10.1145/3710848.3710871</a>","chicago":"Frantar, Elias, Roberto L. Castro, Jiale Chen, Torsten Hoefler, and Dan-Adrian Alistarh. “MARLIN: Mixed-Precision Auto-Regressive Parallel Inference on Large Language Models.” In <i>Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel Programming</i>, 239–51. Association for Computing Machinery, 2025. <a href=\"https://doi.org/10.1145/3710848.3710871\">https://doi.org/10.1145/3710848.3710871</a>.","mla":"Frantar, Elias, et al. “MARLIN: Mixed-Precision Auto-Regressive Parallel Inference on Large Language Models.” <i>Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel Programming</i>, Association for Computing Machinery, 2025, pp. 239–51, doi:<a href=\"https://doi.org/10.1145/3710848.3710871\">10.1145/3710848.3710871</a>.","short":"E. Frantar, R.L. Castro, J. Chen, T. Hoefler, D.-A. Alistarh, in:, Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel Programming, Association for Computing Machinery, 2025, pp. 239–251.","ieee":"E. Frantar, R. L. Castro, J. Chen, T. Hoefler, and D.-A. Alistarh, “MARLIN: Mixed-precision auto-regressive parallel inference on Large Language Models,” in <i>Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel Programming</i>, Las Vegas, NV, United States, 2025, pp. 239–251.","ista":"Frantar E, Castro RL, Chen J, Hoefler T, Alistarh D-A. 2025. MARLIN: Mixed-precision auto-regressive parallel inference on Large Language Models. Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel Programming. PPoPP: Symposium on Principles and Practice of Parallel Programming, 239–251.","ama":"Frantar E, Castro RL, Chen J, Hoefler T, Alistarh D-A. MARLIN: Mixed-precision auto-regressive parallel inference on Large Language Models. In: <i>Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel Programming</i>. Association for Computing Machinery; 2025:239-251. doi:<a href=\"https://doi.org/10.1145/3710848.3710871\">10.1145/3710848.3710871</a>"},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","author":[{"last_name":"Frantar","first_name":"Elias","full_name":"Frantar, Elias","id":"09a8f98d-ec99-11ea-ae11-c063a7b7fe5f"},{"full_name":"Castro, Roberto L.","first_name":"Roberto L.","last_name":"Castro"},{"full_name":"Chen, Jiale","orcid":"0000-0001-5337-5875","id":"4d0a9064-1ff6-11ee-9fa6-ec046c604785","first_name":"Jiale","last_name":"Chen"},{"last_name":"Hoefler","first_name":"Torsten","full_name":"Hoefler, Torsten"},{"last_name":"Alistarh","first_name":"Dan-Adrian","id":"4A899BFC-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0003-3650-940X","full_name":"Alistarh, Dan-Adrian"}],"OA_place":"publisher","related_material":{"record":[{"status":"public","id":"19884","relation":"software"}]},"article_processing_charge":"Yes (via OA deal)","page":"239-251","external_id":{"isi":["001437826500019"],"arxiv":["2408.11743"]},"publication_status":"published","abstract":[{"text":"As inference on Large Language Models (LLMs) emerges as an important workload in machine learning applications, model weight quantization has become a standard technique for efficient GPU deployment. Quantization not only reduces model size, but has also been shown to yield substantial speedups for single-user inference, due to reduced memory movement, with low accuracy impact. Yet, it remains a key open question whether speedups are achievable also in batched settings with multiple parallel clients, which are highly relevant for practical serving. It is unclear whether GPU kernels can be designed to remain practically memory-bound, while supporting the substantially increased compute requirements of batched workloads.\r\nIn this paper, we resolve this question positively by introducing a new design for Mixed-precision Auto-Regressive LINear kernels, called MARLIN. Concretely, given a model whose weights are compressed via quantization to, e.g., 4 bits per element, MARLIN shows that batchsizes up to 16-32 can be practically supported with close to maximum (4×) quantization speedup, and larger batchsizes up to 64-128 with gradually decreasing, but still significant, acceleration. MARLIN accomplishes this via a combination of techniques, such as asynchronous memory access, complex task scheduling and pipelining, and bespoke quantization support. Our experiments show that MARLIN's near-optimal performance on individual LLM layers across different scenarios can also lead to significant end-to-end LLM inference speedups (of up to 2.8×) when integrated with the popular vLLM open-source serving engine. Finally, we show that MARLIN is extensible to further compression techniques, like NVIDIA 2:4 sparsity, leading to additional speedups.","lang":"eng"}],"title":"MARLIN: Mixed-precision auto-regressive parallel inference on Large Language Models","date_created":"2025-06-23T13:51:58Z","year":"2025","doi":"10.1145/3710848.3710871","publication_identifier":{"isbn":["9798400714436"]},"publication":"Proceedings of the 30th ACM SIGPLAN Annual Symposium on Principles and Practice of Parallel Programming","corr_author":"1","file":[{"file_id":"19883","date_updated":"2025-06-24T06:04:17Z","file_size":1330044,"checksum":"a0566ea3c168e8273501a5eb7d767cf8","relation":"main_file","access_level":"open_access","content_type":"application/pdf","file_name":"2025_PPoPP_Frantar.pdf","date_created":"2025-06-24T06:04:17Z","creator":"dernst","success":1}],"quality_controlled":"1","has_accepted_license":"1","ddc":["000"],"conference":{"end_date":"2025-03-05","location":"Las Vegas, NV, United States","name":"PPoPP: Symposium on Principles and Practice of Parallel Programming","start_date":"2025-03-01"}},{"OA_place":"publisher","volume":130,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","author":[{"first_name":"Juan Vicente","last_name":"Melo Velasco","full_name":"Melo Velasco, Juan Vicente","id":"2611dec0-b9c6-11ed-9bea-a81c2b17a549"},{"last_name":"Miles","first_name":"Evan","full_name":"Miles, Evan"},{"last_name":"McCarthy","first_name":"Michael","full_name":"McCarthy, Michael","id":"22a2674a-61ce-11ee-94b5-d18813baf16f"},{"last_name":"Shaw","first_name":"Thomas","orcid":"0000-0001-7640-6152","id":"3caa3f91-1f03-11ee-96ce-e0e553054d6e","full_name":"Shaw, Thomas"},{"id":"001b0422-8d15-11ed-bc51-cab6c037a228","full_name":"Fyffe, Catriona Louise","first_name":"Catriona Louise","last_name":"Fyffe"},{"first_name":"Adrià","last_name":"Fontrodona-Bach","full_name":"Fontrodona-Bach, Adrià","id":"f06891fd-9f42-11ee-8632-a20971c43046"},{"full_name":"Pellicciotti, Francesca","orcid":"0000-0002-5554-8087","id":"b28f055a-81ea-11ed-b70c-a9fe7f7b0e70","first_name":"Francesca","last_name":"Pellicciotti"}],"title":"Method dependence in thermal conductivity and aerodynamic roughness length estimates on a debris‐covered glacier","abstract":[{"text":"Rock debris partially covers glaciers worldwide, with varying extents and distributions, and controls sub‐debris melt rates by modifying energy transfer from the atmosphere to the ice. Two key physical properties controlling this energy exchange are thermal conductivity (k) and aerodynamic roughness length (z0). Accurate representation of these properties in energy‐balance models is critical for understanding climate‐glacier interactions and predicting the behavior of debris‐covered glaciers. However, k and z0 have been derived at very few sites from limited local measurements, using different approaches, and most model applications rely on values reported from these few sites and studies. We derive k and z0 using established and modified approaches from data at three locations on Pirámide Glacier in the central Chilean Andes. By comparing methods and evaluating melt simulated with an energy‐balance model, we reveal substantial differences between approaches. These lead to discrepancies between ice melt from energy‐balance simulations and observed data, and highlight the impact of method choice on calculated ice melt. Optimizing k against measured melt appears a viable approach to constrain melt simulations. Determining z0 seems less critical, as it has a smaller impact on total melt. Profile aerodynamic method measurements for estimating z0, despite higher costs, are independent of ice melt calculations. The large, unexpected differences between methods indicate a substantial knowledge gap. The fact that field‐derived k and z0 fail to work well in energy‐balance models, suggests that model values represent bulk properties distinct from theoretical field measurements. Addressing this gap is essential for improving glacier melt predictions.","lang":"eng"}],"external_id":{"isi":["001508794200001"]},"publication_status":"published","article_processing_charge":"Yes (via OA deal)","publication":"Journal of Geophysical Research: Earth Surface","issue":"6","doi":"10.1029/2025jf008360","publication_identifier":{"eissn":["2169-9011"],"issn":["2169-9003"]},"article_number":"e2025JF008360","year":"2025","date_created":"2025-06-23T13:54:01Z","ddc":["550"],"has_accepted_license":"1","quality_controlled":"1","file":[{"file_id":"19886","file_size":3949928,"date_updated":"2025-06-24T06:27:34Z","checksum":"ca91541516c71d240321630ca42b4dc4","relation":"main_file","access_level":"open_access","content_type":"application/pdf","file_name":"2025_JGREarthSurface_MeloVelasco.pdf","date_created":"2025-06-24T06:27:34Z","creator":"dernst","success":1}],"corr_author":"1","_id":"19878","scopus_import":"1","type":"journal_article","acknowledgement":"This project received funding from the Swiss National Science Foundation (Grant 204322, project “REsolving the thickNess Of debris on Earth's glacIers and its Rate of change,” RENOIR). We thank Lars Groeneveld, Diego Hernández, Alonso Mejías, Gabriela Reyes and Gabriela Tala for their support during fieldwork. Open access funding provided by Institute of Science and Technology Austria/KEMÖ.","article_type":"original","intvolume":"       130","oa_version":"Published Version","publisher":"Wiley","department":[{"_id":"FrPe"}],"date_updated":"2025-09-30T13:42:28Z","language":[{"iso":"eng"}],"month":"06","date_published":"2025-06-15T00:00:00Z","oa":1,"file_date_updated":"2025-06-24T06:27:34Z","isi":1,"day":"15","status":"public","OA_type":"hybrid","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"citation":{"ieee":"J. V. Melo Velasco <i>et al.</i>, “Method dependence in thermal conductivity and aerodynamic roughness length estimates on a debris‐covered glacier,” <i>Journal of Geophysical Research: Earth Surface</i>, vol. 130, no. 6. Wiley, 2025.","short":"J.V. Melo Velasco, E. Miles, M. McCarthy, T. Shaw, C.L. Fyffe, A. Fontrodona-Bach, F. Pellicciotti, Journal of Geophysical Research: Earth Surface 130 (2025).","ama":"Melo Velasco JV, Miles E, McCarthy M, et al. Method dependence in thermal conductivity and aerodynamic roughness length estimates on a debris‐covered glacier. <i>Journal of Geophysical Research: Earth Surface</i>. 2025;130(6). doi:<a href=\"https://doi.org/10.1029/2025jf008360\">10.1029/2025jf008360</a>","ista":"Melo Velasco JV, Miles E, McCarthy M, Shaw T, Fyffe CL, Fontrodona-Bach A, Pellicciotti F. 2025. Method dependence in thermal conductivity and aerodynamic roughness length estimates on a debris‐covered glacier. Journal of Geophysical Research: Earth Surface. 130(6), e2025JF008360.","apa":"Melo Velasco, J. V., Miles, E., McCarthy, M., Shaw, T., Fyffe, C. L., Fontrodona-Bach, A., &#38; Pellicciotti, F. (2025). Method dependence in thermal conductivity and aerodynamic roughness length estimates on a debris‐covered glacier. <i>Journal of Geophysical Research: Earth Surface</i>. Wiley. <a href=\"https://doi.org/10.1029/2025jf008360\">https://doi.org/10.1029/2025jf008360</a>","chicago":"Melo Velasco, Juan Vicente, Evan Miles, Michael McCarthy, Thomas Shaw, Catriona Louise Fyffe, Adrià Fontrodona-Bach, and Francesca Pellicciotti. “Method Dependence in Thermal Conductivity and Aerodynamic Roughness Length Estimates on a Debris‐covered Glacier.” <i>Journal of Geophysical Research: Earth Surface</i>. Wiley, 2025. <a href=\"https://doi.org/10.1029/2025jf008360\">https://doi.org/10.1029/2025jf008360</a>.","mla":"Melo Velasco, Juan Vicente, et al. “Method Dependence in Thermal Conductivity and Aerodynamic Roughness Length Estimates on a Debris‐covered Glacier.” <i>Journal of Geophysical Research: Earth Surface</i>, vol. 130, no. 6, e2025JF008360, Wiley, 2025, doi:<a href=\"https://doi.org/10.1029/2025jf008360\">10.1029/2025jf008360</a>."}},{"date_created":"2025-06-23T13:54:46Z","year":"2025","article_number":"104138","publication_identifier":{"issn":["0195-6698"]},"doi":"10.1016/j.ejc.2025.104138","publication":"European Journal of Combinatorics","corr_author":"1","file":[{"creator":"dernst","success":1,"date_created":"2025-06-24T06:33:30Z","content_type":"application/pdf","file_name":"2025_EuropJournCombinatorics_Dvorak.pdf","checksum":"8b3585df45b25091fba9bee9854b7d01","relation":"main_file","access_level":"open_access","file_size":564203,"date_updated":"2025-06-24T06:33:30Z","file_id":"19887"}],"quality_controlled":"1","has_accepted_license":"1","ddc":["510"],"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","author":[{"first_name":"Zdeněk","last_name":"Dvořák","full_name":"Dvořák, Zdeněk"},{"last_name":"Moore","first_name":"Benjamin","id":"6dc1a1be-bf1c-11ed-8d2b-d044840f49d6","full_name":"Moore, Benjamin"},{"first_name":"Michaela","last_name":"Seifrtová","full_name":"Seifrtová, Michaela"},{"full_name":"Šámal, Robert","last_name":"Šámal","first_name":"Robert"}],"volume":127,"OA_place":"publisher","article_processing_charge":"Yes (via OA deal)","publication_status":"published","external_id":{"isi":["001443061400001"],"arxiv":["2312.13061"]},"abstract":[{"lang":"eng","text":"We consider the 4-precoloring extension problem in planar near-Eulerian- triangulations, i.e., plane graphs where all faces except possibly for the outer one have length three, all vertices not incident with the outer face have even degree, and exactly the vertices incident with the outer face are precolored. We give a necessary topological condition for the precoloring to extend, and give a complete characterization when the outer face has length at most five and when all vertices of the outer face have odd degree and are colored using only three colors."}],"title":"Precoloring extension in planar near-Eulerian-triangulations","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","short":"CC BY (4.0)"},"OA_type":"hybrid","day":"01","status":"public","citation":{"ieee":"Z. Dvořák, B. Moore, M. Seifrtová, and R. Šámal, “Precoloring extension in planar near-Eulerian-triangulations,” <i>European Journal of Combinatorics</i>, vol. 127. Elsevier, 2025.","short":"Z. Dvořák, B. Moore, M. Seifrtová, R. Šámal, European Journal of Combinatorics 127 (2025).","ista":"Dvořák Z, Moore B, Seifrtová M, Šámal R. 2025. Precoloring extension in planar near-Eulerian-triangulations. European Journal of Combinatorics. 127, 104138.","ama":"Dvořák Z, Moore B, Seifrtová M, Šámal R. Precoloring extension in planar near-Eulerian-triangulations. <i>European Journal of Combinatorics</i>. 2025;127. doi:<a href=\"https://doi.org/10.1016/j.ejc.2025.104138\">10.1016/j.ejc.2025.104138</a>","chicago":"Dvořák, Zdeněk, Benjamin Moore, Michaela Seifrtová, and Robert Šámal. “Precoloring Extension in Planar Near-Eulerian-Triangulations.” <i>European Journal of Combinatorics</i>. Elsevier, 2025. <a href=\"https://doi.org/10.1016/j.ejc.2025.104138\">https://doi.org/10.1016/j.ejc.2025.104138</a>.","apa":"Dvořák, Z., Moore, B., Seifrtová, M., &#38; Šámal, R. (2025). Precoloring extension in planar near-Eulerian-triangulations. <i>European Journal of Combinatorics</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.ejc.2025.104138\">https://doi.org/10.1016/j.ejc.2025.104138</a>","mla":"Dvořák, Zdeněk, et al. “Precoloring Extension in Planar Near-Eulerian-Triangulations.” <i>European Journal of Combinatorics</i>, vol. 127, 104138, Elsevier, 2025, doi:<a href=\"https://doi.org/10.1016/j.ejc.2025.104138\">10.1016/j.ejc.2025.104138</a>."},"oa_version":"Published Version","intvolume":"       127","article_type":"original","type":"journal_article","acknowledgement":"Supported by project 22-17398S (Flows and cycles in graphs on surfaces) of Czech Science Foundation. An extended abstract appeared in Proceedings of the 12th European Conference on Combinatorics, Graph Theory and Applications (EUROCOMB’23)","scopus_import":"1","_id":"19879","isi":1,"file_date_updated":"2025-06-24T06:33:30Z","oa":1,"date_published":"2025-06-01T00:00:00Z","month":"06","language":[{"iso":"eng"}],"date_updated":"2025-09-30T13:42:59Z","department":[{"_id":"MaKw"}],"arxiv":1,"publisher":"Elsevier"}]