[{"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"OA_type":"gold","file":[{"file_id":"21789","relation":"main_file","file_name":"2026_AstrophysicalJour_Lin.pdf","date_created":"2026-05-04T10:24:49Z","date_updated":"2026-05-04T10:24:49Z","success":1,"creator":"dernst","content_type":"application/pdf","access_level":"open_access","checksum":"5162d1539ef7d10927ef73d8b4500017","file_size":2619679}],"oa_version":"Published Version","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"publisher","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"has_accepted_license":"1","year":"2026","status":"public","issue":"2","publisher":"IOP Publishing","date_published":"2026-02-01T00:00:00Z","month":"02","article_type":"original","publication_status":"published","date_updated":"2026-05-04T10:26:59Z","department":[{"_id":"ZoHa"}],"article_number":"316","article_processing_charge":"Yes","oa":1,"intvolume":"       997","acknowledgement":"M.C. acknowledges support by the European Union (ERC; MMMonsters, 101117624). This work was also supported in part by NASA grants 80NSSC24K0440 and 80NSSC22K0822. This research used the resources of the Center for Institutional Research Computing at Washington State University.","citation":{"mla":"Lin, Allison, et al. “Lomb-Scargle Periodogram Struggles with Non-Sinusoidal Supermassive Black Hole Binary Signatures in Quasar Lightcurves.” <i>The Astrophysical Journal</i>, vol. 997, no. 2, 316, IOP Publishing, 2026, doi:<a href=\"https://doi.org/10.3847/1538-4357/ae29a7\">10.3847/1538-4357/ae29a7</a>.","ieee":"A. Lin, M. Charisi, and Z. Haiman, “Lomb-scargle periodogram struggles with non-sinusoidal supermassive Black Hole binary signatures in quasar lightcurves,” <i>The Astrophysical Journal</i>, vol. 997, no. 2. IOP Publishing, 2026.","ama":"Lin A, Charisi M, Haiman Z. Lomb-scargle periodogram struggles with non-sinusoidal supermassive Black Hole binary signatures in quasar lightcurves. <i>The Astrophysical Journal</i>. 2026;997(2). doi:<a href=\"https://doi.org/10.3847/1538-4357/ae29a7\">10.3847/1538-4357/ae29a7</a>","apa":"Lin, A., Charisi, M., &#38; Haiman, Z. (2026). Lomb-scargle periodogram struggles with non-sinusoidal supermassive Black Hole binary signatures in quasar lightcurves. <i>The Astrophysical Journal</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/1538-4357/ae29a7\">https://doi.org/10.3847/1538-4357/ae29a7</a>","ista":"Lin A, Charisi M, Haiman Z. 2026. Lomb-scargle periodogram struggles with non-sinusoidal supermassive Black Hole binary signatures in quasar lightcurves. The Astrophysical Journal. 997(2), 316.","short":"A. Lin, M. Charisi, Z. Haiman, The Astrophysical Journal 997 (2026).","chicago":"Lin, Allison, Maria Charisi, and Zoltán Haiman. “Lomb-Scargle Periodogram Struggles with Non-Sinusoidal Supermassive Black Hole Binary Signatures in Quasar Lightcurves.” <i>The Astrophysical Journal</i>. IOP Publishing, 2026. <a href=\"https://doi.org/10.3847/1538-4357/ae29a7\">https://doi.org/10.3847/1538-4357/ae29a7</a>."},"ddc":["520"],"publication":"The Astrophysical Journal","type":"journal_article","doi":"10.3847/1538-4357/ae29a7","_id":"21712","author":[{"last_name":"Lin","first_name":"Allison","full_name":"Lin, Allison"},{"first_name":"Maria","full_name":"Charisi, Maria","last_name":"Charisi"},{"last_name":"Haiman","orcid":"0000-0003-3633-5403","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán"}],"quality_controlled":"1","scopus_import":"1","abstract":[{"lang":"eng","text":"Supermassive black hole binary (SMBHB) systems are expected to form as a consequence of galaxy mergers. At subparsec separations, SMBHBs can be identified as quasars with periodic variability, with previous periodicity searches uncovering significant candidates. However, these searches focused primarily on sinusoidal signals, while theoretical models and hydrodynamical simulations predict that binaries produce more complex non-sinusoidal pulse shapes. Here we examine the efficacy of the Lomb–Scargle periodogram (LSP; one of the most popular tools for periodicity searches in unevenly sampled lightcurves) to detect periodicities with a sawtooth shape mimicking results of hydrodynamical simulations. We simulate idealized well-sampled lightcurves, lightcurves that mimic the data in the Palomar Transient Factory (PTF) analyzed in M. Charisi et al. (2016), and lightcurves that resemble our expectations for single-band data in the upcoming Legacy Survey of Space and Time (LSST) of the Rubin Observatory. We approximate quasar variability with a damped random walk (DRW) model, inject sinusoidal and sawtooth pulse shapes, and assess their statistical significance. We find that in the presence of red noise, the LSP detects a relatively low fraction of the sinusoidal signals (∼45%, ∼24%, and ∼23%, in the PTF-like, idealized, and LSST-like lightcurves, respectively). The fraction is significantly reduced for sawtooth periodicity (with only ∼9% in PTF-like and ∼1% in idealized and LSST-like lightcurves). These low recovery rates imply that previous searches have missed the large majority of binaries. They also have significant implications for the detection of SMBHBs in upcoming LSST necessitating the development of advanced tools that go beyond the simple LSP."}],"day":"01","date_created":"2026-04-12T22:01:49Z","file_date_updated":"2026-05-04T10:24:49Z","volume":997,"title":"Lomb-scargle periodogram struggles with non-sinusoidal supermassive Black Hole binary signatures in quasar lightcurves","DOAJ_listed":"1","language":[{"iso":"eng"}]},{"OA_type":"gold","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"oa_version":"Published Version","file":[{"date_created":"2026-05-04T09:49:53Z","file_name":"2026_AstrophysicalJourLetters_Bartos.pdf","relation":"main_file","file_id":"21788","file_size":866725,"access_level":"open_access","content_type":"application/pdf","checksum":"ac46ba3d13f0150ccbc42665bed3ae47","creator":"dernst","success":1,"date_updated":"2026-05-04T09:49:53Z"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["2041-8213"],"issn":["2041-8205"]},"OA_place":"publisher","corr_author":"1","has_accepted_license":"1","issue":"2","year":"2026","status":"public","publisher":"IOP Publishing","publication_status":"published","date_updated":"2026-05-04T09:54:18Z","article_type":"original","date_published":"2026-01-10T00:00:00Z","month":"01","department":[{"_id":"ZoHa"}],"article_number":"L44","article_processing_charge":"Yes","oa":1,"intvolume":"       996","arxiv":1,"external_id":{"arxiv":["2508.08558"]},"ddc":["520"],"acknowledgement":"The authors thank Davide Gerosa and Matthew Mould for valuable suggestions. We are grateful for support by the National Science Foundation under grant No. PHY-2309024 (I.B.) and by NASA under grants 80NSSC22K0822 and 80NSSC24K0440 (Z.H.). We used OpenAI’s ChatGPT (OpenAI 2025) during the preparation of this manuscript. This material is based upon work supported by NSF’s LIGO Laboratory, which is a major facility fully funded by the National Science Foundation.","citation":{"ama":"Bartos I, Haiman Z. Accretion is all you need: Black Hole spin alignment in merger GW231123 indicates accretion pathway. <i>The Astrophysical Journal Letters</i>. 2026;996(2). doi:<a href=\"https://doi.org/10.3847/2041-8213/ae2bff\">10.3847/2041-8213/ae2bff</a>","apa":"Bartos, I., &#38; Haiman, Z. (2026). Accretion is all you need: Black Hole spin alignment in merger GW231123 indicates accretion pathway. <i>The Astrophysical Journal Letters</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/2041-8213/ae2bff\">https://doi.org/10.3847/2041-8213/ae2bff</a>","ieee":"I. Bartos and Z. Haiman, “Accretion is all you need: Black Hole spin alignment in merger GW231123 indicates accretion pathway,” <i>The Astrophysical Journal Letters</i>, vol. 996, no. 2. IOP Publishing, 2026.","mla":"Bartos, Imre, and Zoltán Haiman. “Accretion Is All You Need: Black Hole Spin Alignment in Merger GW231123 Indicates Accretion Pathway.” <i>The Astrophysical Journal Letters</i>, vol. 996, no. 2, L44, IOP Publishing, 2026, doi:<a href=\"https://doi.org/10.3847/2041-8213/ae2bff\">10.3847/2041-8213/ae2bff</a>.","short":"I. Bartos, Z. Haiman, The Astrophysical Journal Letters 996 (2026).","chicago":"Bartos, Imre, and Zoltán Haiman. “Accretion Is All You Need: Black Hole Spin Alignment in Merger GW231123 Indicates Accretion Pathway.” <i>The Astrophysical Journal Letters</i>. IOP Publishing, 2026. <a href=\"https://doi.org/10.3847/2041-8213/ae2bff\">https://doi.org/10.3847/2041-8213/ae2bff</a>.","ista":"Bartos I, Haiman Z. 2026. Accretion is all you need: Black Hole spin alignment in merger GW231123 indicates accretion pathway. The Astrophysical Journal Letters. 996(2), L44."},"publication":"The Astrophysical Journal Letters","type":"journal_article","_id":"21713","doi":"10.3847/2041-8213/ae2bff","author":[{"last_name":"Bartos","full_name":"Bartos, Imre","first_name":"Imre"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman","orcid":"0000-0003-3633-5403"}],"quality_controlled":"1","scopus_import":"1","date_created":"2026-04-12T22:01:49Z","day":"10","abstract":[{"lang":"eng","text":"GW231123 represents the most massive binary–black hole merger detected to date, lying firmly within, or even above, the pair-instability mass gap. The component spins are both exceptionally high (a1 = 0.90 +0.10/-0.19, a2 = 0.80 +0.20/-0.51), which is difficult to explain with repeated mergers. Here we show that the black hole spin vectors are closely aligned with each other while significantly tilted relative to the binary’s orbital angular momentum, pointing to a common accretion-driven origin. We examine astrophysical formation channels capable of producing near-equal, high-mass, and mutually aligned spins consistent with GW231123—particularly binaries embedded in AGN disks and Population III remnants, which grew via coherent misaligned gas accretion. We further argue that other high-mass, high-spin events, e.g., GW190521, may share a similar evolutionary pathway. These findings underscore the critical role of sustained, coherent accretion in shaping the most extreme black hole binaries."}],"volume":996,"file_date_updated":"2026-05-04T09:49:53Z","language":[{"iso":"eng"}],"title":"Accretion is all you need: Black Hole spin alignment in merger GW231123 indicates accretion pathway","DOAJ_listed":"1"},{"language":[{"iso":"eng"}],"DOAJ_listed":"1","title":"Formation of Be stars via wind accretion: Case study on Black Hole + Be star binaries","volume":996,"file_date_updated":"2026-04-16T06:24:30Z","date_created":"2026-04-12T22:01:50Z","day":"10","abstract":[{"lang":"eng","text":"Be stars are rapidly rotating main-sequence stars that play a crucial role in understanding stellar evolution and binary interactions. In this Letter, we propose a new formation scenario for black hole (BH) + Be star binaries (hereafter BHBe binaries), where the Be star is produced through the wind Roche lobe overflow (WRLOF) mechanism. Our analysis is based on numerical simulations of the WRLOF process in massive binaries, building on recent theoretical work. We demonstrate that the WRLOF model can efficiently form BHBe binaries under reasonable assumptions on stellar wind velocities. Using rapid binary population synthesis, we estimate the population of such systems in the Milky Way, predicting ∼1800−3200 currently existing BHBe binaries originating from the WRLOF channel. These systems are characterized by high eccentricities and exceptionally wide orbits, with typical orbital periods exceeding 1000 days and a peak distribution around ∼10,000 days. Due to their long orbital separations, these BHBe binaries are promising targets for future detection via astrometric and interferometric observations."}],"scopus_import":"1","quality_controlled":"1","author":[{"first_name":"Zhenwei","full_name":"Li, Zhenwei","last_name":"Li"},{"last_name":"Jia","first_name":"Shi","full_name":"Jia, Shi"},{"full_name":"Wei, Dandan","first_name":"Dandan","id":"5dd129bd-0601-11ef-b325-833284687b76","last_name":"Wei"},{"last_name":"Ge","first_name":"Hongwei","full_name":"Ge, Hongwei"},{"first_name":"Hailiang","full_name":"Chen, Hailiang","last_name":"Chen"},{"last_name":"Zhang","first_name":"Yangyang","full_name":"Zhang, Yangyang"},{"first_name":"Xuefei","full_name":"Chen, Xuefei","last_name":"Chen"},{"full_name":"Han, Zhanwen","first_name":"Zhanwen","last_name":"Han"}],"_id":"21714","doi":"10.3847/2041-8213/ae3008","type":"journal_article","publication":"The Astrophysical Journal Letters","external_id":{"arxiv":["2512.18565"]},"ddc":["520"],"citation":{"ieee":"Z. Li <i>et al.</i>, “Formation of Be stars via wind accretion: Case study on Black Hole + Be star binaries,” <i>The Astrophysical Journal Letters</i>, vol. 996, no. 2. IOP Publishing, 2026.","mla":"Li, Zhenwei, et al. “Formation of Be Stars via Wind Accretion: Case Study on Black Hole + Be Star Binaries.” <i>The Astrophysical Journal Letters</i>, vol. 996, no. 2, L42, IOP Publishing, 2026, doi:<a href=\"https://doi.org/10.3847/2041-8213/ae3008\">10.3847/2041-8213/ae3008</a>.","apa":"Li, Z., Jia, S., Wei, D., Ge, H., Chen, H., Zhang, Y., … Han, Z. (2026). Formation of Be stars via wind accretion: Case study on Black Hole + Be star binaries. <i>The Astrophysical Journal Letters</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/2041-8213/ae3008\">https://doi.org/10.3847/2041-8213/ae3008</a>","ama":"Li Z, Jia S, Wei D, et al. Formation of Be stars via wind accretion: Case study on Black Hole + Be star binaries. <i>The Astrophysical Journal Letters</i>. 2026;996(2). doi:<a href=\"https://doi.org/10.3847/2041-8213/ae3008\">10.3847/2041-8213/ae3008</a>","ista":"Li Z, Jia S, Wei D, Ge H, Chen H, Zhang Y, Chen X, Han Z. 2026. Formation of Be stars via wind accretion: Case study on Black Hole + Be star binaries. The Astrophysical Journal Letters. 996(2), L42.","chicago":"Li, Zhenwei, Shi Jia, Dandan Wei, Hongwei Ge, Hailiang Chen, Yangyang Zhang, Xuefei Chen, and Zhanwen Han. “Formation of Be Stars via Wind Accretion: Case Study on Black Hole + Be Star Binaries.” <i>The Astrophysical Journal Letters</i>. IOP Publishing, 2026. <a href=\"https://doi.org/10.3847/2041-8213/ae3008\">https://doi.org/10.3847/2041-8213/ae3008</a>.","short":"Z. Li, S. Jia, D. Wei, H. Ge, H. Chen, Y. Zhang, X. Chen, Z. Han, The Astrophysical Journal Letters 996 (2026)."},"acknowledgement":"We are deeply grateful to the anonymous referee for the insightful comments, which have significantly improved the quality of this work. The authors express their gratitude to Zhaoyu Zuo and I. El Mellah for sharing the grids of wind accretion efficiencies. Z.L. thanks Matthias U. Kruckow for detailed discussions about the BH formation. This work is supported by the Natural Science Foundation of China (grant Nos. 12125303, 12525304, 12288102, 12090040/3, 12473034, 12503044, 12333008, 12433009, 12422305, 12273105, 12073070, 12173081), the Strategic Priority Research Program of the Chinese Academy of Sciences (grant Nos. XDB1160303, XDB1160201, XDB1160000), the National Key R&D Program of China (grant Nos. 2021YFA1600403 and 2021YFA1600400), the CAS “Light of West China,” the Yunnan Revitalization Talent Support Program-Science & Technology Champion Project (No. 202305AB350003) and Young Talent project, the International Centre of Supernovae (ICESUN), Yunnan Key Laboratory of Supernova Research (Nos. 202302AN360001 and 202201BC070003), Yunnan Fundamental Research Projects (No. 202401AT070139), and the Natural Science Foundation of Henan Province (No. 242300420944). X.C. acknowledges the New Cornerstone Science Foundation through the XPLORER PRIZE. The authors gratefully acknowledge the “PHOENIX Supercomputing Platform” jointly operated by the Binary Population Synthesis Group and the Stellar Astrophysics Group at Yunnan Observatories, Chinese Academy of Sciences.","intvolume":"       996","arxiv":1,"oa":1,"article_processing_charge":"Yes","article_number":"L42","department":[{"_id":"YlGo"}],"date_updated":"2026-04-16T06:26:18Z","publication_status":"published","date_published":"2026-01-10T00:00:00Z","month":"01","article_type":"original","publisher":"IOP Publishing","status":"public","year":"2026","issue":"2","has_accepted_license":"1","publication_identifier":{"issn":["2041-8205"],"eissn":["2041-8213"]},"OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Published Version","file":[{"relation":"main_file","file_name":"2026_AstrophysicalJourLetters_Li.pdf","date_created":"2026-04-16T06:24:30Z","file_id":"21741","success":1,"creator":"dernst","content_type":"application/pdf","access_level":"open_access","checksum":"09200c1cf405101abdd298ce80c9a90d","file_size":5202345,"date_updated":"2026-04-16T06:24:30Z"}],"OA_type":"gold","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"}},{"ddc":["520"],"external_id":{"arxiv":["2509.05434"]},"citation":{"ama":"Greene JE, Setton DJ, Furtak LJ, et al. What you see is what you get: Empirically measured bolometric luminosities of Little Red Dots. <i>The Astrophysical Journal</i>. 2026;996(2). doi:<a href=\"https://doi.org/10.3847/1538-4357/ae1836\">10.3847/1538-4357/ae1836</a>","apa":"Greene, J. E., Setton, D. J., Furtak, L. J., Naidu, R. P., Volonteri, M., Dayal, P., … Zitrin, A. (2026). What you see is what you get: Empirically measured bolometric luminosities of Little Red Dots. <i>The Astrophysical Journal</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/1538-4357/ae1836\">https://doi.org/10.3847/1538-4357/ae1836</a>","mla":"Greene, Jenny E., et al. “What You See Is What You Get: Empirically Measured Bolometric Luminosities of Little Red Dots.” <i>The Astrophysical Journal</i>, vol. 996, no. 2, 129, IOP Publishing, 2026, doi:<a href=\"https://doi.org/10.3847/1538-4357/ae1836\">10.3847/1538-4357/ae1836</a>.","ieee":"J. E. Greene <i>et al.</i>, “What you see is what you get: Empirically measured bolometric luminosities of Little Red Dots,” <i>The Astrophysical Journal</i>, vol. 996, no. 2. IOP Publishing, 2026.","short":"J.E. Greene, D.J. Setton, L.J. Furtak, R.P. Naidu, M. Volonteri, P. Dayal, I. Labbe, P. Van Dokkum, R. Bezanson, G. Brammer, S.E. Cutler, K. Glazebrook, A. De Graaff, M. Hirschmann, R.E. Hviding, V. Kokorev, J. Leja, H. Liu, Y. Ma, J.J. Matthee, T. Nanayakkara, P.A. Oesch, R. Pan, S.H. Price, J.S. Spilker, B. Wang, J.R. Weaver, K.E. Whitaker, C.C. Williams, A. Zitrin, The Astrophysical Journal 996 (2026).","chicago":"Greene, Jenny E., David J. Setton, Lukas J. Furtak, Rohan P. Naidu, Marta Volonteri, Pratika Dayal, Ivo Labbe, et al. “What You See Is What You Get: Empirically Measured Bolometric Luminosities of Little Red Dots.” <i>The Astrophysical Journal</i>. IOP Publishing, 2026. <a href=\"https://doi.org/10.3847/1538-4357/ae1836\">https://doi.org/10.3847/1538-4357/ae1836</a>.","ista":"Greene JE, Setton DJ, Furtak LJ, Naidu RP, Volonteri M, Dayal P, Labbe I, Van Dokkum P, Bezanson R, Brammer G, Cutler SE, Glazebrook K, De Graaff A, Hirschmann M, Hviding RE, Kokorev V, Leja J, Liu H, Ma Y, Matthee JJ, Nanayakkara T, Oesch PA, Pan R, Price SH, Spilker JS, Wang B, Weaver JR, Whitaker KE, Williams CC, Zitrin A. 2026. What you see is what you get: Empirically measured bolometric luminosities of Little Red Dots. The Astrophysical Journal. 996(2), 129."},"acknowledgement":"We benefit from the following JWST programs: UNCOVER (JWST/GO #2561; Labbé & Bezanson); ALT (JWST-GO #3516; Naidu & Matthee); MegaScience (JWST-GO #4111; Suess); RUBIES (JWST-GO #4233; de Graaff & Brammer); PRIMER (JWST/GO #1837; Dunlop).\r\n\r\nWe acknowledge funding from NSF/AAG #2306950, JWST-GO-02561, JWST-GO-03516, and JWST-GO-04111, provided through a grant from the STScI under NASA contract NAS5-03127. I.L. acknowledges support from Australian Research Council Future Fellowship FT220100798. K.G. and T.N. acknowledge support from Australian Research Council Laureate Fellowship FL180100060. A.Z. acknowledges support by grant No. 2020750 from the United States-Israel Binational Science Foundation (BSF) and grant No. 2109066 from the United States National Science Foundation (NSF); by the Ministry of Science & Technology, Israel; and by the Israel Science Foundation grant No. 864/23. J.M. and I.K. are funded by the European Union (ERC, AGENTS, 101076224). Views and opinions expressed are, however, those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. Y.F. acknowledges support from JSPS KAKENHI grant No. JSPS KAKENHI grant Nos. JP22K21349 and JP23K13149. This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI) under contract No. MB22.00072, as well as from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant DNRF140. Support for this work for RPN was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. The work of CCW is supported by NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. J.M. acknowledges funding by the European Union (ERC, AGENTS, 101076224). R.E.H. acknowledges support by the German Aerospace Center (DLR) and the Federal Ministry for Economic Affairs and Energy (BMWi) through program 50OR2403 “RUBIES.”","intvolume":"       996","arxiv":1,"type":"journal_article","publication":"The Astrophysical Journal","_id":"21715","doi":"10.3847/1538-4357/ae1836","project":[{"_id":"bd9b2118-d553-11ed-ba76-db24564edfea","name":"Young galaxies as tracers and agents of cosmic reionization","grant_number":"101076224"}],"quality_controlled":"1","author":[{"full_name":"Greene, Jenny E.","first_name":"Jenny E.","last_name":"Greene"},{"last_name":"Setton","first_name":"David J.","full_name":"Setton, David J."},{"last_name":"Furtak","full_name":"Furtak, Lukas J.","first_name":"Lukas J."},{"full_name":"Naidu, Rohan P.","first_name":"Rohan P.","last_name":"Naidu"},{"first_name":"Marta","full_name":"Volonteri, Marta","last_name":"Volonteri"},{"last_name":"Dayal","full_name":"Dayal, Pratika","first_name":"Pratika"},{"first_name":"Ivo","full_name":"Labbe, Ivo","last_name":"Labbe"},{"last_name":"Van Dokkum","first_name":"Pieter","full_name":"Van Dokkum, Pieter"},{"full_name":"Bezanson, Rachel","first_name":"Rachel","last_name":"Bezanson"},{"last_name":"Brammer","full_name":"Brammer, Gabriel","first_name":"Gabriel"},{"last_name":"Cutler","full_name":"Cutler, Sam E.","first_name":"Sam E."},{"last_name":"Glazebrook","full_name":"Glazebrook, Karl","first_name":"Karl"},{"last_name":"De Graaff","full_name":"De Graaff, Anna","first_name":"Anna"},{"last_name":"Hirschmann","first_name":"Michaela","full_name":"Hirschmann, Michaela"},{"full_name":"Hviding, Raphael E.","first_name":"Raphael E.","last_name":"Hviding"},{"first_name":"Vasily","full_name":"Kokorev, Vasily","last_name":"Kokorev"},{"last_name":"Leja","full_name":"Leja, Joel","first_name":"Joel"},{"first_name":"Hanpu","full_name":"Liu, Hanpu","last_name":"Liu"},{"last_name":"Ma","full_name":"Ma, Yilun","first_name":"Yilun"},{"first_name":"Jorryt J","full_name":"Matthee, Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X","last_name":"Matthee"},{"full_name":"Nanayakkara, Themiya","first_name":"Themiya","last_name":"Nanayakkara"},{"full_name":"Oesch, Pascal A.","first_name":"Pascal A.","last_name":"Oesch"},{"full_name":"Pan, Richard","first_name":"Richard","last_name":"Pan"},{"first_name":"Sedona H.","full_name":"Price, Sedona H.","last_name":"Price"},{"first_name":"Justin S.","full_name":"Spilker, Justin S.","last_name":"Spilker"},{"full_name":"Wang, Bingjie","first_name":"Bingjie","last_name":"Wang"},{"last_name":"Weaver","first_name":"John R.","full_name":"Weaver, John R."},{"last_name":"Whitaker","first_name":"Katherine E.","full_name":"Whitaker, Katherine E."},{"full_name":"Williams, Christina C.","first_name":"Christina C.","last_name":"Williams"},{"last_name":"Zitrin","full_name":"Zitrin, Adi","first_name":"Adi"}],"scopus_import":"1","date_created":"2026-04-12T22:01:50Z","day":"10","abstract":[{"text":"New populations of red active galactic nuclei (known as “little red dots”) discovered by JWST exhibit remarkable spectral energy distributions. Leveraging X-ray through far-infrared observations of two of the most luminous known little red dots, we directly measure their bolometric luminosities. We find evidence that more than half of the bolometric luminosity likely emerges in the rest-frame optical, with Lbol/L5100 = 5, roughly half the value for “standard” active galactic nuclei. Meanwhile, the X-ray emitting corona, UV-emitting blackbody, and reprocessed mid to far-infrared emission are all considerably subdominant, assuming that the far-infrared luminosity is well below current measured limits. We present new bolometric corrections that dramatically lower inferred bolometric luminosities by a factor of 10 compared to published values in the literature. These bolometric corrections are in accord with expectations from models in which gas absorption and reprocessing are responsible for the red rest-frame optical colors of little red dots. We discuss how this lowered luminosity scale suggests a lower mass scale for the population by at least an order of magnitude (e.g., ∼105–107 M⊙ black holes, and ∼108 M⊙ galaxies), alleviating tensions with clustering, overmassive black holes, and the integrated black hole mass density in the Universe.","lang":"eng"}],"language":[{"iso":"eng"}],"title":"What you see is what you get: Empirically measured bolometric luminosities of Little Red Dots","DOAJ_listed":"1","volume":996,"file_date_updated":"2026-05-04T11:19:48Z","oa_version":"Published Version","file":[{"date_updated":"2026-05-04T11:19:48Z","access_level":"open_access","content_type":"application/pdf","file_size":684400,"checksum":"7b3cb025d4bcaa35c6e52bd0c8fb6cf4","creator":"dernst","success":1,"file_id":"21792","date_created":"2026-05-04T11:19:48Z","file_name":"2026_AstrophysicalJour_Greene.pdf","relation":"main_file"}],"OA_type":"gold","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","has_accepted_license":"1","issue":"2","status":"public","year":"2026","publisher":"IOP Publishing","date_updated":"2026-05-04T11:20:42Z","publication_status":"published","month":"01","article_type":"original","date_published":"2026-01-10T00:00:00Z","PlanS_conform":"1","article_processing_charge":"Yes","article_number":"129","department":[{"_id":"JoMa"}],"oa":1},{"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["1879-0356"],"issn":["1369-5266"]},"OA_place":"publisher","OA_type":"hybrid","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"oa_version":"Published Version","issue":"6","status":"public","year":"2026","has_accepted_license":"1","corr_author":"1","PlanS_conform":"1","publication_status":"epub_ahead","date_updated":"2026-05-04T11:15:57Z","date_published":"2026-04-01T00:00:00Z","article_type":"original","month":"04","publisher":"Elsevier","oa":1,"department":[{"_id":"XiFe"}],"article_number":"102881","article_processing_charge":"Yes (via OA deal)","publication":"Current Opinion in Plant Biology","type":"journal_article","intvolume":"        91","ddc":["580"],"acknowledgement":"This work was supported by JSPS KAKENHI (grant number JP22J01430) and the Osamu Hayaishi Memorial Scholarship for Study Abroad for H.N.","citation":{"ieee":"H. NAGAI and X. Feng, “Genetic and epigenetic mechanisms underlying male reproductive thermotolerance,” <i>Current Opinion in Plant Biology</i>, vol. 91, no. 6. Elsevier, 2026.","mla":"NAGAI, HIROKI, and Xiaoqi Feng. “Genetic and Epigenetic Mechanisms Underlying Male Reproductive Thermotolerance.” <i>Current Opinion in Plant Biology</i>, vol. 91, no. 6, 102881, Elsevier, 2026, doi:<a href=\"https://doi.org/10.1016/j.pbi.2026.102881\">10.1016/j.pbi.2026.102881</a>.","apa":"NAGAI, H., &#38; Feng, X. (2026). Genetic and epigenetic mechanisms underlying male reproductive thermotolerance. <i>Current Opinion in Plant Biology</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.pbi.2026.102881\">https://doi.org/10.1016/j.pbi.2026.102881</a>","ama":"NAGAI H, Feng X. Genetic and epigenetic mechanisms underlying male reproductive thermotolerance. <i>Current Opinion in Plant Biology</i>. 2026;91(6). doi:<a href=\"https://doi.org/10.1016/j.pbi.2026.102881\">10.1016/j.pbi.2026.102881</a>","ista":"NAGAI H, Feng X. 2026. Genetic and epigenetic mechanisms underlying male reproductive thermotolerance. Current Opinion in Plant Biology. 91(6), 102881.","chicago":"NAGAI, HIROKI, and Xiaoqi Feng. “Genetic and Epigenetic Mechanisms Underlying Male Reproductive Thermotolerance.” <i>Current Opinion in Plant Biology</i>. Elsevier, 2026. <a href=\"https://doi.org/10.1016/j.pbi.2026.102881\">https://doi.org/10.1016/j.pbi.2026.102881</a>.","short":"H. NAGAI, X. Feng, Current Opinion in Plant Biology 91 (2026)."},"author":[{"last_name":"Nagai","orcid":"0000-0003-1671-9434","id":"608df3e6-e2ab-11ed-8890-c9318cec7da4","full_name":"Nagai, Hiroki","first_name":"Hiroki"},{"orcid":"0000-0002-4008-1234","last_name":"Feng","first_name":"Xiaoqi","full_name":"Feng, Xiaoqi","id":"e0164712-22ee-11ed-b12a-d80fcdf35958"}],"quality_controlled":"1","_id":"21716","doi":"10.1016/j.pbi.2026.102881","scopus_import":"1","volume":91,"language":[{"iso":"eng"}],"main_file_link":[{"url":"https://doi.org/10.1016/j.pbi.2026.102881","open_access":"1"}],"title":"Genetic and epigenetic mechanisms underlying male reproductive thermotolerance","date_created":"2026-04-12T22:01:50Z","day":"01","abstract":[{"text":"Male germline development in plants is highly sensitive to heat stress, with elevated temperatures frequently impairing male fertility and consequently reducing seed production. Indeed, recent global warming has decreased major crop yields, emphasizing the urgent need to elucidate the molecular and cellular mechanisms underlying heat-induced male sterility. This review synthesizes current knowledge on how heat stress disrupts microsporogenesis and microgametogenesis, and how plants counteract these stresses through diverse thermotolerance mechanisms. We emphasize temperature-sensitive processes, including meiotic progression in male germ cells, programmed cell death of somatic tapetal nurse cells, and post-meiotic pollen tube development. We further discuss how epigenetic regulators enhance thermotolerance by reprogramming DNA methylation landscapes and modulating histone variant distribution. Finally, we propose future directions aimed at understanding the mechanisms of reproductive thermotolerance from the epigenetic perspective.","lang":"eng"}]},{"volume":40,"main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2505.04539"}],"language":[{"iso":"eng"}],"title":"Qualitative analysis of ω-regular objectives on robust MDPs","date_created":"2026-04-12T22:01:50Z","day":"14","abstract":[{"lang":"eng","text":"Robust Markov Decision Processes (RMDPs) generalize classical MDPs that consider uncertainties in transition probabilities by defining a set of possible transition functions. An objective is a set of runs (or infinite trajectories) of the RMDP, and the value for an objective is the maximal probability that the agent can guarantee against the adversarial environment. We consider (a) reachability objectives, where given a target set of states, the goal is to eventually arrive at one of them; and (b) parity objectives, which are a canonical representation for ω-regular objectives. The qualitative analysis problem asks whether the objective can be ensured with probability 1. In this work, we study the qualitative problem for reachability and parity objectives on RMDPs without making any assumption over the structures of the RMDPs, e.g., unichain or aperiodic. Our contributions are twofold. We first present efficient algorithms with oracle access to uncertainty sets that solve qualitative problems of reachability and parity objectives. We then report experimental results demonstrating the effectiveness of our oracle-based approach on classical RMDP examples from the literature scaling up to thousands of states."}],"scopus_import":"1","author":[{"full_name":"Asadi, Ali","first_name":"Ali","id":"02d96aae-000e-11ec-b801-cadd0a5eefbb","last_name":"Asadi"},{"last_name":"Chatterjee","orcid":"0000-0002-4561-241X","id":"2E5DCA20-F248-11E8-B48F-1D18A9856A87","first_name":"Krishnendu","full_name":"Chatterjee, Krishnendu"},{"last_name":"Kafshdar Goharshadi","orcid":"0000-0002-8595-0587","id":"103b4fa0-896a-11ed-bdf8-87b697bef40d","full_name":"Kafshdar Goharshadi, Ehsan","first_name":"Ehsan"},{"orcid":"0009-0007-5253-9170","last_name":"Karrabi","full_name":"Karrabi, Mehrdad","first_name":"Mehrdad","id":"67638922-f394-11eb-9cf6-f20423e08757"},{"last_name":"Shafiee","full_name":"Shafiee, Ali","first_name":"Ali","id":"2783031a-7378-11f0-b2d0-f17f1db2ebad"}],"page":"36137-36145","quality_controlled":"1","project":[{"grant_number":"863818","call_identifier":"H2020","name":"Formal Methods for Stochastic Models: Algorithms and Applications","_id":"0599E47C-7A3F-11EA-A408-12923DDC885E"}],"_id":"21717","doi":"10.1609/aaai.v40i43.40931","publication":"Proceedings of the 40th AAAI Conference on Artificial Intelligence","type":"conference","intvolume":"        40","arxiv":1,"external_id":{"arxiv":["2505.04539"]},"citation":{"short":"A. Asadi, K. Chatterjee, E. Goharshady, M. Karrabi, A. Shafiee, in:, Proceedings of the 40th AAAI Conference on Artificial Intelligence, Association for the Advancement of Artificial Intelligence, 2026, pp. 36137–36145.","chicago":"Asadi, Ali, Krishnendu Chatterjee, Ehsan Goharshady, Mehrdad Karrabi, and Ali Shafiee. “Qualitative Analysis of ω-Regular Objectives on Robust MDPs.” In <i>Proceedings of the 40th AAAI Conference on Artificial Intelligence</i>, 40:36137–45. Association for the Advancement of Artificial Intelligence, 2026. <a href=\"https://doi.org/10.1609/aaai.v40i43.40931\">https://doi.org/10.1609/aaai.v40i43.40931</a>.","ista":"Asadi A, Chatterjee K, Goharshady E, Karrabi M, Shafiee A. 2026. Qualitative analysis of ω-regular objectives on robust MDPs. Proceedings of the 40th AAAI Conference on Artificial Intelligence. AAAI: Conference on Artificial Intelligence vol. 40, 36137–36145.","ama":"Asadi A, Chatterjee K, Goharshady E, Karrabi M, Shafiee A. Qualitative analysis of ω-regular objectives on robust MDPs. In: <i>Proceedings of the 40th AAAI Conference on Artificial Intelligence</i>. Vol 40. Association for the Advancement of Artificial Intelligence; 2026:36137-36145. doi:<a href=\"https://doi.org/10.1609/aaai.v40i43.40931\">10.1609/aaai.v40i43.40931</a>","apa":"Asadi, A., Chatterjee, K., Goharshady, E., Karrabi, M., &#38; Shafiee, A. (2026). Qualitative analysis of ω-regular objectives on robust MDPs. In <i>Proceedings of the 40th AAAI Conference on Artificial Intelligence</i> (Vol. 40, pp. 36137–36145). Singapore, Singapore: Association for the Advancement of Artificial Intelligence. <a href=\"https://doi.org/10.1609/aaai.v40i43.40931\">https://doi.org/10.1609/aaai.v40i43.40931</a>","mla":"Asadi, Ali, et al. “Qualitative Analysis of ω-Regular Objectives on Robust MDPs.” <i>Proceedings of the 40th AAAI Conference on Artificial Intelligence</i>, vol. 40, no. 43, Association for the Advancement of Artificial Intelligence, 2026, pp. 36137–45, doi:<a href=\"https://doi.org/10.1609/aaai.v40i43.40931\">10.1609/aaai.v40i43.40931</a>.","ieee":"A. Asadi, K. Chatterjee, E. Goharshady, M. Karrabi, and A. Shafiee, “Qualitative analysis of ω-regular objectives on robust MDPs,” in <i>Proceedings of the 40th AAAI Conference on Artificial Intelligence</i>, Singapore, Singapore, 2026, vol. 40, no. 43, pp. 36137–36145."},"acknowledgement":"This work was supported by ERC CoG 863818 (ForMSMArt) and Austrian Science Fund (FWF) 10.55776/COE12. We also thank Hossein Zakerinia for his helpful feedback.","oa":1,"department":[{"_id":"KrCh"},{"_id":"GradSch"}],"conference":{"end_date":"2026-01-27","location":"Singapore, Singapore","start_date":"2026-01-20","name":"AAAI: Conference on Artificial Intelligence"},"article_processing_charge":"No","date_updated":"2026-05-04T11:38:56Z","publication_status":"published","month":"03","date_published":"2026-03-14T00:00:00Z","ec_funded":1,"publisher":"Association for the Advancement of Artificial Intelligence","status":"public","issue":"43","year":"2026","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["2374-3468"],"issn":["2159-5399"]},"OA_place":"repository","OA_type":"green","oa_version":"Preprint"},{"_id":"21718","doi":"10.3842/SIGMA.2026.024","project":[{"name":"Geometry of the tip of the global nilpotent cone","grant_number":"P35847","_id":"34b2c9cb-11ca-11ed-8bc3-a50ba74ca4a3"},{"_id":"e6c64f42-ab3c-11f0-94c7-a95658059ccc","name":"Big algebras in classical types","grant_number":"27483"}],"quality_controlled":"1","author":[{"last_name":"Ngo","first_name":"Nhok T","full_name":"Ngo, Nhok T","id":"28e53c8c-896a-11ed-bdf8-f809043ce2f0"}],"external_id":{"arxiv":["2501.04605"]},"ddc":["510"],"citation":{"ama":"Ngo NT. Big algebra in type A for the coordinate ring of the matrix space. <i>Symmetry, Integrability and Geometry: Methods and Applications</i>. 2026;22. doi:<a href=\"https://doi.org/10.3842/SIGMA.2026.024\">10.3842/SIGMA.2026.024</a>","apa":"Ngo, N. T. (2026). Big algebra in type A for the coordinate ring of the matrix space. <i>Symmetry, Integrability and Geometry: Methods and Applications</i>. National Academy of Science of Ukraine. <a href=\"https://doi.org/10.3842/SIGMA.2026.024\">https://doi.org/10.3842/SIGMA.2026.024</a>","ieee":"N. T. Ngo, “Big algebra in type A for the coordinate ring of the matrix space,” <i>Symmetry, Integrability and Geometry: Methods and Applications</i>, vol. 22. National Academy of Science of Ukraine, 2026.","mla":"Ngo, Nhok T. “Big Algebra in Type A for the Coordinate Ring of the Matrix Space.” <i>Symmetry, Integrability and Geometry: Methods and Applications</i>, vol. 22, 024, National Academy of Science of Ukraine, 2026, doi:<a href=\"https://doi.org/10.3842/SIGMA.2026.024\">10.3842/SIGMA.2026.024</a>.","short":"N.T. Ngo, Symmetry, Integrability and Geometry: Methods and Applications 22 (2026).","chicago":"Ngo, Nhok T. “Big Algebra in Type A for the Coordinate Ring of the Matrix Space.” <i>Symmetry, Integrability and Geometry: Methods and Applications</i>. National Academy of Science of Ukraine, 2026. <a href=\"https://doi.org/10.3842/SIGMA.2026.024\">https://doi.org/10.3842/SIGMA.2026.024</a>.","ista":"Ngo NT. 2026. Big algebra in type A for the coordinate ring of the matrix space. Symmetry, Integrability and Geometry: Methods and Applications. 22, 024."},"acknowledgement":"I would like to express my gratitude to Tam´as Hausel for introducing me to the subject and\r\nfor his constant guidance throughout this work. I would also like to thank Tam´as Hausel,\r\nMischa Elkner, Jakub L¨owit, Anton Mellit, Marino Romero, Leonid Rybnikov for many fruitful\r\ndiscussions and feedback on earlier drafts of this paper. We are grateful to the anonymous\r\nreferees for many useful comments and suggestions that improved the manuscript. This work was done during the author’s PhD studies at the Institute of Science and Technology Austria (ISTA). The author was supported by the Austrian Science Fund (FWF) grant\r\n“Geometry of the tip of the global nilpotent cone” no. 10.55776/P35847 and the DOC Fellowship of the Austrian Academy of Sciences. The author also acknowledges the long-term program\r\nof support of the Ukrainian research teams at the Polish Academy of Sciences carried out in\r\ncollaboration with the U.S. National Academy of Sciences with the financial support of external\r\npartners. For open access purposes, the author has applied a CC BY public copyright license\r\nto any author-accepted manuscript version arising from this submission.","intvolume":"        22","arxiv":1,"type":"journal_article","publication":"Symmetry, Integrability and Geometry: Methods and Applications","date_created":"2026-04-12T22:01:51Z","abstract":[{"lang":"eng","text":"In this paper, we consider the big algebra recently introduced by Hausel for the GLn-action on the coordinate ring of the matrix space Mat(n,r). In particular, we obtain explicit formulas for the big algebra generators in terms of differential operators with polynomial coefficients. We show that big algebras in type A are commutative and relate them to the Bethe subalgebra in the Yangian Y(gln). We apply these results to big algebras of symmetric powers of the standard representation of GLn.\r\n."}],"day":"14","language":[{"iso":"eng"}],"title":"Big algebra in type A for the coordinate ring of the matrix space","DOAJ_listed":"1","volume":22,"file_date_updated":"2026-04-16T06:06:54Z","scopus_import":"1","corr_author":"1","has_accepted_license":"1","status":"public","year":"2026","oa_version":"Published Version","file":[{"success":1,"creator":"dernst","content_type":"application/pdf","file_size":975460,"access_level":"open_access","checksum":"29b28b5f8717ed1a084a2b551d0fd284","date_updated":"2026-04-16T06:06:54Z","relation":"main_file","file_name":"2026_SIGMA_Ngo.pdf","date_created":"2026-04-16T06:06:54Z","file_id":"21740"}],"OA_type":"diamond","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"publication_identifier":{"eissn":["1815-0659"]},"OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","article_number":"024","department":[{"_id":"TaHa"}],"oa":1,"publisher":"National Academy of Science of Ukraine","date_updated":"2026-04-16T06:11:12Z","publication_status":"published","date_published":"2026-03-14T00:00:00Z","month":"03","article_type":"original"},{"publication_identifier":{"isbn":["9781611978971"],"issn":["10719040"],"eissn":["15579468"]},"OA_place":"repository","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Preprint","OA_type":"green","year":"2026","status":"public","date_updated":"2026-05-04T11:54:09Z","publication_status":"published","month":"01","date_published":"2026-01-07T00:00:00Z","publisher":"Society for Industrial and Applied Mathematics","ec_funded":1,"oa":1,"article_processing_charge":"No","department":[{"_id":"MoHe"}],"conference":{"name":"SODA: Symposium on Discrete Algorithms"},"publication":"Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms","type":"conference","external_id":{"arxiv":["2601.09139"]},"acknowledgement":"Monika Henzinger: Funded by the European union. Views and opinions expressed\r\nare however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council Executive Agency. Neither the European Union nor the granting authority can be held responsible for them. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (MoDynStruct, No. 101019564) and the Austrian Science Fund (FWF) grant DOI 10.55776/I5982. For open access purposes, the author has applied a CC BY public copyright license to any author accepted manuscript version arising from this submission.\r\nPeter Kiss: This research was funded in whole or in part by the Austrian Science Fund (FWF)\r\n10.55776/ESP6088024.","citation":{"ama":"Goranci G, Henzinger M, Kiss P, Momeni A, Zöcklein G. Dynamic hierarchical j-tree decomposition and its applications. In: <i>Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms</i>. Vol 2026-January. Society for Industrial and Applied Mathematics; 2026:1128-1180. doi:<a href=\"https://doi.org/10.1137/1.9781611978971.45\">10.1137/1.9781611978971.45</a>","apa":"Goranci, G., Henzinger, M., Kiss, P., Momeni, A., &#38; Zöcklein, G. (2026). Dynamic hierarchical j-tree decomposition and its applications. In <i>Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms</i> (Vol. 2026–January, pp. 1128–1180). Society for Industrial and Applied Mathematics. <a href=\"https://doi.org/10.1137/1.9781611978971.45\">https://doi.org/10.1137/1.9781611978971.45</a>","ieee":"G. Goranci, M. Henzinger, P. Kiss, A. Momeni, and G. Zöcklein, “Dynamic hierarchical j-tree decomposition and its applications,” in <i>Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms</i>, 2026, vol. 2026–January, pp. 1128–1180.","mla":"Goranci, Gramoz, et al. “Dynamic Hierarchical J-Tree Decomposition and Its Applications.” <i>Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms</i>, vol. 2026–January, Society for Industrial and Applied Mathematics, 2026, pp. 1128–80, doi:<a href=\"https://doi.org/10.1137/1.9781611978971.45\">10.1137/1.9781611978971.45</a>.","short":"G. Goranci, M. Henzinger, P. Kiss, A. Momeni, G. Zöcklein, in:, Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms, Society for Industrial and Applied Mathematics, 2026, pp. 1128–1180.","chicago":"Goranci, Gramoz, Monika Henzinger, Peter Kiss, Ali Momeni, and Gernot Zöcklein. “Dynamic Hierarchical J-Tree Decomposition and Its Applications.” In <i>Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms</i>, 2026–January:1128–80. Society for Industrial and Applied Mathematics, 2026. <a href=\"https://doi.org/10.1137/1.9781611978971.45\">https://doi.org/10.1137/1.9781611978971.45</a>.","ista":"Goranci G, Henzinger M, Kiss P, Momeni A, Zöcklein G. 2026. Dynamic hierarchical j-tree decomposition and its applications. Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms. SODA: Symposium on Discrete Algorithms vol. 2026–January, 1128–1180."},"arxiv":1,"quality_controlled":"1","author":[{"last_name":"Goranci","first_name":"Gramoz","full_name":"Goranci, Gramoz"},{"full_name":"Henzinger, Monika H","first_name":"Monika H","id":"540c9bbd-f2de-11ec-812d-d04a5be85630","orcid":"0000-0002-5008-6530","last_name":"Henzinger"},{"last_name":"Kiss","first_name":"Peter","full_name":"Kiss, Peter"},{"last_name":"Momeni","full_name":"Momeni, Ali","first_name":"Ali"},{"last_name":"Zöcklein","id":"45d5e826-47af-11f1-84e5-ba87c23fe681","full_name":"Zöcklein, Gernot","first_name":"Gernot"}],"page":"1128-1180","_id":"21719","doi":"10.1137/1.9781611978971.45","project":[{"_id":"bd9ca328-d553-11ed-ba76-dc4f890cfe62","call_identifier":"H2020","grant_number":"101019564","name":"The design and evaluation of modern fully dynamic data structures"},{"name":"Static and Dynamic Hierarchical Graph Decompositions","grant_number":"I05982","_id":"bda196b2-d553-11ed-ba76-8e8ee6c21103"}],"scopus_import":"1","language":[{"iso":"eng"}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2601.09139"}],"title":"Dynamic hierarchical j-tree decomposition and its applications","volume":"2026-January","date_created":"2026-04-12T22:01:51Z","abstract":[{"lang":"eng","text":"We develop a new algorithmic framework for designing approximation algorithms for cut-based optimization problems on capacitated undirected graphs that undergo edge insertions and deletions. Specifically, our framework dynamically maintains a variant of the hierarchical 𝑗-tree decomposition of [Madry FOCS’10], achieving a poly-logarithmic approximation factor to the graph’s cut structure and supporting edge updates in 𝑂⁡(𝑛𝜀) amortized update time, for any arbitrarily small constant 𝜀 ∈(0,1).\r\nConsequently, we obtain new trade-offs between approximation and update/query time for fundamental cut-based optimization problems in the fully dynamic setting, including all-pairs minimum cuts, sparsest cut, multi-way cut, and multi-cut. For the last three problems, these trade-offs give the first fully-dynamic algorithms achieving poly-logarithmic approximation in sub-linear time per operation.\r\nThe main technical ingredient behind our dynamic hierarchy is a dynamic cut-sparsifier algorithm that can handle vertex splits with low recourse. This is achieved by white-boxing the dynamic cut sparsifier construction of [Abraham et al. FOCS’16], based on forest packing, together with new structural insights about the maintenance of these forests under vertex splits. Given the versatility of cut sparsification in both the static and dynamic graph algorithms literature, we believe this construction may be of independent interest."}],"day":"07"},{"article_processing_charge":"No","conference":{"name":"SODA: Symposium on Discrete Algorithms","start_date":"2026-01-11","location":"Vancouver, Canada","end_date":"2026-01-14"},"department":[{"_id":"MoHe"},{"_id":"GradSch"}],"oa":1,"publisher":"Society for Industrial and Applied Mathematics","ec_funded":1,"date_updated":"2026-05-04T11:36:47Z","publication_status":"published","date_published":"2026-01-07T00:00:00Z","month":"01","status":"public","year":"2026","oa_version":"Preprint","OA_type":"green","publication_identifier":{"issn":["1071-9040"],"eissn":["1557-9468"],"eisbn":["9781611978971"]},"OA_place":"repository","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_created":"2026-04-12T22:01:51Z","abstract":[{"text":"We present an exact fully-dynamic minimum cut algorithm that runs in 𝑛𝑜⁡(1) deterministic update time when the minimum cut size is at most 2Θ⁡(log3/4−𝑐⁡𝑛) for any 𝑐 >0, improving on the previous algorithm of Jin, Sun, and Thorup (SODA 2024) whose minimum cut size limit is (log⁡𝑛)𝑜⁡(1). Combined with graph sparsification, we obtain the first (1 +𝜖)-approximate fully-dynamic minimum cut algorithm on weighted graphs, for any 𝜖 ≥2−Θ⁡(log3/4−𝑐⁡𝑛), in 𝑛𝑜⁡(1) randomized update time.\r\nOur main technical contribution is a deterministic local minimum cut algorithm, which replaces the randomized LocalKCut procedure from El-Hayek, Henzinger, and Li (SODA 2025).","lang":"eng"}],"day":"07","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2512.13105"}],"language":[{"iso":"eng"}],"title":"Deterministic and exact fully-dynamic minimum cut of superpolylogarithmic size in subpolynomial time","volume":2026,"scopus_import":"1","_id":"21720","doi":"10.1137/1.9781611978971.25","project":[{"name":"The design and evaluation of modern fully dynamic data structures","grant_number":"101019564","call_identifier":"H2020","_id":"bd9ca328-d553-11ed-ba76-dc4f890cfe62"},{"_id":"bda196b2-d553-11ed-ba76-8e8ee6c21103","name":"Static and Dynamic Hierarchical Graph Decompositions","grant_number":"I05982"}],"quality_controlled":"1","page":"613-663","author":[{"first_name":"Antoine","full_name":"El-Hayek, Antoine","id":"888a098e-fcac-11ee-aff7-d347be57b725","orcid":"0000-0003-4268-7368","last_name":"El-Hayek"},{"last_name":"Henzinger","orcid":"0000-0002-5008-6530","id":"540c9bbd-f2de-11ec-812d-d04a5be85630","full_name":"Henzinger, Monika H","first_name":"Monika H"},{"last_name":"Li","full_name":"Li, Jason","first_name":"Jason"}],"external_id":{"arxiv":["2512.13105"]},"acknowledgement":"Funded by the European union. Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council Executive Agency. Neither the European Union nor the granting authority can be held responsible for them. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (MoDynStruct, No. 101019564) and the Austrian Science Fund (FWF) grant DOI 10.55776/I5982. For open access purposes, the author has applied a CC BY public copyright license to any author-accepted manuscript version arising from this submission.","citation":{"chicago":"El-Hayek, Antoine, Monika Henzinger, and Jason Li. “Deterministic and Exact Fully-Dynamic Minimum Cut of Superpolylogarithmic Size in Subpolynomial Time.” In <i>Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms</i>, 2026:613–63. Society for Industrial and Applied Mathematics, 2026. <a href=\"https://doi.org/10.1137/1.9781611978971.25\">https://doi.org/10.1137/1.9781611978971.25</a>.","short":"A. El-Hayek, M. Henzinger, J. Li, in:, Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms, Society for Industrial and Applied Mathematics, 2026, pp. 613–663.","ista":"El-Hayek A, Henzinger M, Li J. 2026. Deterministic and exact fully-dynamic minimum cut of superpolylogarithmic size in subpolynomial time. Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms. SODA: Symposium on Discrete Algorithms vol. 2026, 613–663.","apa":"El-Hayek, A., Henzinger, M., &#38; Li, J. (2026). Deterministic and exact fully-dynamic minimum cut of superpolylogarithmic size in subpolynomial time. In <i>Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms</i> (Vol. 2026, pp. 613–663). Vancouver, Canada: Society for Industrial and Applied Mathematics. <a href=\"https://doi.org/10.1137/1.9781611978971.25\">https://doi.org/10.1137/1.9781611978971.25</a>","ama":"El-Hayek A, Henzinger M, Li J. Deterministic and exact fully-dynamic minimum cut of superpolylogarithmic size in subpolynomial time. In: <i>Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms</i>. Vol 2026. Society for Industrial and Applied Mathematics; 2026:613-663. doi:<a href=\"https://doi.org/10.1137/1.9781611978971.25\">10.1137/1.9781611978971.25</a>","mla":"El-Hayek, Antoine, et al. “Deterministic and Exact Fully-Dynamic Minimum Cut of Superpolylogarithmic Size in Subpolynomial Time.” <i>Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms</i>, vol. 2026, Society for Industrial and Applied Mathematics, 2026, pp. 613–63, doi:<a href=\"https://doi.org/10.1137/1.9781611978971.25\">10.1137/1.9781611978971.25</a>.","ieee":"A. El-Hayek, M. Henzinger, and J. Li, “Deterministic and exact fully-dynamic minimum cut of superpolylogarithmic size in subpolynomial time,” in <i>Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms</i>, Vancouver, Canada, 2026, vol. 2026, pp. 613–663."},"intvolume":"      2026","arxiv":1,"type":"conference","publication":"Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms"},{"abstract":[{"text":"Swimming bacteria move through a fluid by actuating their moving body parts. They are force-free and can be described as hydrodynamic force dipoles: pushers or pullers. This modelling description is broadly used in biological physics and active matter research, and it has successfully predicted, for example, the superfluid behaviour of suspensions of pushers or the bend instability and emergence of turbulent flows in active nematics. However, this description accounts only for the translational motion of the swimming body and neglects the effects of hydrodynamic torque dipoles, which are relevant to bacteria with rotary motor-driven flagella, such as swimming Escherichia coli. Here we show that the torque dipole of confined swimming E. coli can power the persistent rotation of symmetric discs. The torque dipole leads to a traction force on the discs, an additive mechanism that is both contactless and independent of the orientation of the bacteria. Our results indicate that the torque dipole of swimming E. coli is notable in confined geometries, which is relevant to bacterial transport through porous materials, biofilms and the development of chiral fluids.","lang":"eng"}],"day":"27","date_created":"2026-04-12T22:01:51Z","title":"The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs","language":[{"iso":"eng"}],"main_file_link":[{"url":"https://doi.org/10.1038/s41567-026-03189-4","open_access":"1"}],"scopus_import":"1","doi":"10.1038/s41567-026-03189-4","_id":"21721","project":[{"_id":"bdac72da-d553-11ed-ba76-eae56e802b74","name":"VULCAN: matter, powered from within","grant_number":"101086998"}],"quality_controlled":"1","author":[{"first_name":"Daniel B","full_name":"Grober, Daniel B","id":"c692f879-718d-11ee-81f0-da7caa79c783","last_name":"Grober"},{"first_name":"Tanumoy","full_name":"Dhar, Tanumoy","last_name":"Dhar"},{"full_name":"Saintillan, David","first_name":"David","last_name":"Saintillan"},{"id":"8fb92548-2b22-11eb-b7c1-a3f0d08d7c7d","first_name":"Jérémie A","full_name":"Palacci, Jérémie A","last_name":"Palacci","orcid":"0000-0002-7253-9465"}],"acknowledgement":"We thank E. Krasnopeeva for help with the bacterial culture, motility and genetic engineering. We thank Q. Martinet for help with the experimental design, F. Pertl for atomic force microscopy measurements and S. Hajek for the scanning electron microscopy imaging. This project has received funding from the European Research Council under the European Union’s Horizon Europe research and innovation programme (VULCAN, 101086998). The views and opinions expressed are, however, those of the authors only and do not necessarily reflect those of the European Union or the European Research Council Executive Agency. Neither the European Union nor the granting authority can be held responsible for them. J.P. thanks the Nanofabrication and Electron Microscopy Shared Scientific Units of ISTA for support. Open access funding provided by Institute of Science and Technology (IST Austria).","citation":{"ista":"Grober DB, Dhar T, Saintillan D, Palacci JA. 2026. The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs. Nature Physics.","chicago":"Grober, Daniel B, Tanumoy Dhar, David Saintillan, and Jérémie A Palacci. “The Hydrodynamic Torque Dipole from Rotary Bacterial Flagella Powers Symmetric Discs.” <i>Nature Physics</i>. Springer Nature, 2026. <a href=\"https://doi.org/10.1038/s41567-026-03189-4\">https://doi.org/10.1038/s41567-026-03189-4</a>.","short":"D.B. Grober, T. Dhar, D. Saintillan, J.A. Palacci, Nature Physics (2026).","mla":"Grober, Daniel B., et al. “The Hydrodynamic Torque Dipole from Rotary Bacterial Flagella Powers Symmetric Discs.” <i>Nature Physics</i>, Springer Nature, 2026, doi:<a href=\"https://doi.org/10.1038/s41567-026-03189-4\">10.1038/s41567-026-03189-4</a>.","ieee":"D. B. Grober, T. Dhar, D. Saintillan, and J. A. Palacci, “The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs,” <i>Nature Physics</i>. Springer Nature, 2026.","apa":"Grober, D. B., Dhar, T., Saintillan, D., &#38; Palacci, J. A. (2026). The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs. <i>Nature Physics</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41567-026-03189-4\">https://doi.org/10.1038/s41567-026-03189-4</a>","ama":"Grober DB, Dhar T, Saintillan D, Palacci JA. The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs. <i>Nature Physics</i>. 2026. doi:<a href=\"https://doi.org/10.1038/s41567-026-03189-4\">10.1038/s41567-026-03189-4</a>"},"ddc":["570"],"publication":"Nature Physics","type":"journal_article","article_processing_charge":"Yes (via OA deal)","department":[{"_id":"JePa"}],"oa":1,"publisher":"Springer Nature","acknowledged_ssus":[{"_id":"NanoFab"},{"_id":"EM-Fac"}],"article_type":"original","date_published":"2026-03-27T00:00:00Z","month":"03","publication_status":"epub_ahead","date_updated":"2026-04-16T06:20:23Z","PlanS_conform":"1","corr_author":"1","has_accepted_license":"1","status":"public","year":"2026","oa_version":"Published Version","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"OA_type":"hybrid","OA_place":"publisher","publication_identifier":{"eissn":["1745-2481"],"issn":["1745-2473"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87"},{"corr_author":"1","year":"2026","status":"public","issue":"43","OA_type":"green","oa_version":"Preprint","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["2374-3468"],"issn":["2159-5399"]},"OA_place":"repository","department":[{"_id":"KrCh"}],"conference":{"location":"Singapore, Singapore","end_date":"2026-01-27","name":"AAAI: Conference on Artificial Intelligence","start_date":"2026-01-20"},"article_processing_charge":"No","ec_funded":1,"publisher":"Association for the Advancement of Artificial Intelligence","date_updated":"2026-05-04T11:44:14Z","publication_status":"published","date_published":"2026-03-14T00:00:00Z","month":"03","project":[{"_id":"0599E47C-7A3F-11EA-A408-12923DDC885E","call_identifier":"H2020","grant_number":"863818","name":"Formal Methods for Stochastic Models: Algorithms and Applications"}],"_id":"21722","doi":"10.1609/aaai.v40i43.40932","page":"36146-36154","author":[{"id":"02d96aae-000e-11ec-b801-cadd0a5eefbb","full_name":"Asadi, Ali","first_name":"Ali","last_name":"Asadi"},{"id":"2E5DCA20-F248-11E8-B48F-1D18A9856A87","full_name":"Chatterjee, Krishnendu","first_name":"Krishnendu","last_name":"Chatterjee","orcid":"0000-0002-4561-241X"},{"id":"579a6c20-34cf-11f1-acbd-8c2f19cdb4da","first_name":"David","full_name":"Lurie, David","last_name":"Lurie"},{"orcid":"0000-0001-5103-038X","last_name":"Saona Urmeneta","full_name":"Saona Urmeneta, Raimundo J","first_name":"Raimundo J","id":"BD1DF4C4-D767-11E9-B658-BC13E6697425"}],"quality_controlled":"1","intvolume":"        40","arxiv":1,"external_id":{"arxiv":["2511.13134"]},"acknowledgement":"This work was partially supported by the ANRT under the French CIFRE Ph.D program in collaboration between NyxAir and Paris-Dauphine University (Contract: CIFRE N° 2022/0513), by the French Agence Nationale de la Recherche (ANR) under reference ANR-21-CE40-\r\n0020 (CONVERGENCE project), by Austrian Science Fund (FWF) 10.55776/COE12, and by the ERC CoG 863818 (ForM-SMArt) grant.","citation":{"apa":"Asadi, A., Chatterjee, K., Lurie, D., &#38; Saona Urmeneta, R. J. (2026). Revealing POMDPs: Qualitative and quantitative analysis for parity objectives. In <i>Proceedings of the AAAI Conference on Artificial Intelligence</i> (Vol. 40, pp. 36146–36154). Singapore, Singapore: Association for the Advancement of Artificial Intelligence. <a href=\"https://doi.org/10.1609/aaai.v40i43.40932\">https://doi.org/10.1609/aaai.v40i43.40932</a>","ama":"Asadi A, Chatterjee K, Lurie D, Saona Urmeneta RJ. Revealing POMDPs: Qualitative and quantitative analysis for parity objectives. In: <i>Proceedings of the AAAI Conference on Artificial Intelligence</i>. Vol 40. Association for the Advancement of Artificial Intelligence; 2026:36146-36154. doi:<a href=\"https://doi.org/10.1609/aaai.v40i43.40932\">10.1609/aaai.v40i43.40932</a>","ieee":"A. Asadi, K. Chatterjee, D. Lurie, and R. J. Saona Urmeneta, “Revealing POMDPs: Qualitative and quantitative analysis for parity objectives,” in <i>Proceedings of the AAAI Conference on Artificial Intelligence</i>, Singapore, Singapore, 2026, vol. 40, no. 43, pp. 36146–36154.","mla":"Asadi, Ali, et al. “Revealing POMDPs: Qualitative and Quantitative Analysis for Parity Objectives.” <i>Proceedings of the AAAI Conference on Artificial Intelligence</i>, vol. 40, no. 43, Association for the Advancement of Artificial Intelligence, 2026, pp. 36146–54, doi:<a href=\"https://doi.org/10.1609/aaai.v40i43.40932\">10.1609/aaai.v40i43.40932</a>.","chicago":"Asadi, Ali, Krishnendu Chatterjee, David Lurie, and Raimundo J Saona Urmeneta. “Revealing POMDPs: Qualitative and Quantitative Analysis for Parity Objectives.” In <i>Proceedings of the AAAI Conference on Artificial Intelligence</i>, 40:36146–54. Association for the Advancement of Artificial Intelligence, 2026. <a href=\"https://doi.org/10.1609/aaai.v40i43.40932\">https://doi.org/10.1609/aaai.v40i43.40932</a>.","short":"A. Asadi, K. Chatterjee, D. Lurie, R.J. Saona Urmeneta, in:, Proceedings of the AAAI Conference on Artificial Intelligence, Association for the Advancement of Artificial Intelligence, 2026, pp. 36146–36154.","ista":"Asadi A, Chatterjee K, Lurie D, Saona Urmeneta RJ. 2026. Revealing POMDPs: Qualitative and quantitative analysis for parity objectives. Proceedings of the AAAI Conference on Artificial Intelligence. AAAI: Conference on Artificial Intelligence vol. 40, 36146–36154."},"type":"conference","publication":"Proceedings of the AAAI Conference on Artificial Intelligence","date_created":"2026-04-12T22:01:52Z","abstract":[{"lang":"eng","text":"Partially observable Markov decision processes (POMDPs) are a central model for uncertainty in sequential decision making. The most basic objective is the reachability objective, where a target set must be eventually visited, and the more general parity objectives can model all omega-regular specifications. For such objectives, the computational analysis problems are the following: (a) qualitative analysis that asks whether the objective can be satisfied with probability 1 (almost-sure winning) or probability arbitrarily close to 1 (limit-sure winning); and (b) quantitative analysis that asks for the approximation of the optimal probability of satisfying the objective. For general POMDPs, almost-sure analysis for reachability objectives is EXPTIME-complete, but limit-sure and quantitative analyses for reachability objectives are undecidable; almost-sure, limit-sure, and quantitative analyses for parity objectives are all undecidable. A special class of POMDPs, called revealing POMDPs, has been studied recently in several works, and for this subclass the almost-sure analysis for parity objectives was shown to be EXPTIME-complete. In this work, we show that for revealing POMDPs the limit-sure analysis for parity objectives is EXPTIME-complete, and even the quantitative analysis for parity objectives can be achieved in EXPTIME."}],"day":"14","volume":40,"language":[{"iso":"eng"}],"main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2511.13134"}],"title":"Revealing POMDPs: Qualitative and quantitative analysis for parity objectives","scopus_import":"1"},{"issue":"1","status":"public","year":"2026","has_accepted_license":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"publisher","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"OA_type":"gold","file":[{"file_size":19310053,"checksum":"65a8237a519188af83b6dc4d47ad85fa","access_level":"open_access","content_type":"application/pdf","creator":"dernst","success":1,"date_updated":"2026-04-13T08:36:50Z","date_created":"2026-04-13T08:36:50Z","file_name":"2026_AstrophysicalJournal_Miller.pdf","relation":"main_file","file_id":"21733"}],"oa_version":"Published Version","oa":1,"department":[{"_id":"IlCa"}],"article_number":"69","article_processing_charge":"Yes","PlanS_conform":"1","month":"01","article_type":"original","date_published":"2026-01-01T00:00:00Z","date_updated":"2026-04-13T08:39:39Z","publication_status":"published","publisher":"IOP Publishing","author":[{"last_name":"Miller","full_name":"Miller, David R.","first_name":"David R."},{"orcid":"0000-0002-4770-5388","last_name":"Caiazzo","first_name":"Ilaria","full_name":"Caiazzo, Ilaria","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d"},{"first_name":"Jeremy","full_name":"Heyl, Jeremy","last_name":"Heyl"},{"last_name":"Richer","first_name":"Harvey B.","full_name":"Richer, Harvey B."},{"first_name":"Mark A.","full_name":"Hollands, Mark A.","last_name":"Hollands"},{"last_name":"Tremblay","first_name":"Pier Emmanuel","full_name":"Tremblay, Pier Emmanuel"},{"first_name":"Kareem","full_name":"El-Badry, Kareem","last_name":"El-Badry"},{"last_name":"Rodriguez","first_name":"Antonio C.","full_name":"Rodriguez, Antonio C."},{"last_name":"Vanderbosch","full_name":"Vanderbosch, Zachary P.","first_name":"Zachary P."}],"quality_controlled":"1","doi":"10.3847/1538-4357/ae18c8","_id":"21725","publication":"The Astrophysical Journal","type":"journal_article","arxiv":1,"intvolume":"       996","citation":{"short":"D.R. Miller, I. Caiazzo, J. Heyl, H.B. Richer, M.A. Hollands, P.E. Tremblay, K. El-Badry, A.C. Rodriguez, Z.P. Vanderbosch, The Astrophysical Journal 996 (2026).","chicago":"Miller, David R., Ilaria Caiazzo, Jeremy Heyl, Harvey B. Richer, Mark A. Hollands, Pier Emmanuel Tremblay, Kareem El-Badry, Antonio C. Rodriguez, and Zachary P. Vanderbosch. “The White Dwarf Initial–Final Mass Relation from Open Clusters in Gaia DR3.” <i>The Astrophysical Journal</i>. IOP Publishing, 2026. <a href=\"https://doi.org/10.3847/1538-4357/ae18c8\">https://doi.org/10.3847/1538-4357/ae18c8</a>.","ista":"Miller DR, Caiazzo I, Heyl J, Richer HB, Hollands MA, Tremblay PE, El-Badry K, Rodriguez AC, Vanderbosch ZP. 2026. The White Dwarf initial–final mass relation from open clusters in Gaia DR3. The Astrophysical Journal. 996(1), 69.","ama":"Miller DR, Caiazzo I, Heyl J, et al. The White Dwarf initial–final mass relation from open clusters in Gaia DR3. <i>The Astrophysical Journal</i>. 2026;996(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/ae18c8\">10.3847/1538-4357/ae18c8</a>","apa":"Miller, D. R., Caiazzo, I., Heyl, J., Richer, H. B., Hollands, M. A., Tremblay, P. E., … Vanderbosch, Z. P. (2026). The White Dwarf initial–final mass relation from open clusters in Gaia DR3. <i>The Astrophysical Journal</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/1538-4357/ae18c8\">https://doi.org/10.3847/1538-4357/ae18c8</a>","mla":"Miller, David R., et al. “The White Dwarf Initial–Final Mass Relation from Open Clusters in Gaia DR3.” <i>The Astrophysical Journal</i>, vol. 996, no. 1, 69, IOP Publishing, 2026, doi:<a href=\"https://doi.org/10.3847/1538-4357/ae18c8\">10.3847/1538-4357/ae18c8</a>.","ieee":"D. R. Miller <i>et al.</i>, “The White Dwarf initial–final mass relation from open clusters in Gaia DR3,” <i>The Astrophysical Journal</i>, vol. 996, no. 1. IOP Publishing, 2026."},"acknowledgement":"The authors would like to thank the anonymous referee for their constructive feedback, which helped improve the clarify of the manuscript. This work was supported in part by the Natural Sciences and Engineering Research Council of Canada Discovery grants Nos. DG-RGPIN-2022-03051 and DG-RGPIN-2023-04486. This research received funding from the European Research Council under the European Union’s Horizon 2020 research and innovation program number 101002408 (MOS100PC). This work includes results based on observations obtained at the international Gemini Observatory, a program of NSF’s NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation on behalf of the Gemini Observatory partnership: the National Science Foundation (United States), National Research Council (Canada), Agencia Nacional de Investigación y Desarrollo (Chile), Ministerio de Ciencia, Tecnología e Innovación (Argentina), Ministério da Ciência, Tecnologia, Inovações e Comunicações (Brazil), and Korea Astronomy and Space Science Institute (Republic of Korea). This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. Gemini spectra were processed using the DRAGONS package (K. Labrie et al. 2023). LRIS spectra were reduced using the Lpipe pipeline (D. A. Perley 2019).\r\n\r\nFacilities: Gaia - (DR2 & DR3), Gemini:Gillett - Gillett Gemini North Telescope (GMOS-N), Gemini:South - Gemini South Telescope (GMOS-S), Keck:I - KECK I Telescope (LRIS).\r\n\r\nSoftware: Astropy (Astropy Collaboration et al. 2013,2018, 2022), emcee (D. Foreman-Mackey et al. 2013).","external_id":{"arxiv":["2510.24877"]},"ddc":["520"],"file_date_updated":"2026-04-13T08:36:50Z","volume":996,"keyword":["White dwarf stars","Open star clusters","Compact objects","Stellar evolution"],"DOAJ_listed":"1","title":"The White Dwarf initial–final mass relation from open clusters in Gaia DR3","language":[{"iso":"eng"}],"abstract":[{"text":"The initial–final mass relation (IFMR) links a star’s birth mass to the mass of its white dwarf (WD) remnant, providing key constraints on stellar evolution. Open clusters offer the most straightforward way to empirically determine the IFMR, as their well-defined ages allow for direct progenitor lifetime estimates. We construct the most comprehensive open cluster WD IFMR to date by combining new spectroscopy of 22 WDs with an extensive literature review of WDs with strong cluster associations. To minimize systematics, we restrict our analysis to spectroscopically confirmed hydrogen-atmosphere (DA) WDs consistent with single-stellar origins. We separately analyze a subset with reliable Gaia-based astrometric membership assessments, as well as a full sample that adds WDs with strong cluster associations whose membership cannot be reliably assessed with Gaia. The Gaia-based sample includes 69 spectroscopically confirmed DA WDs, more than doubling the sample size of previous Gaia-based open cluster IFMRs. The full sample, which includes 53 additional literature WDs,\r\nincreases the total number of cluster WDs by over 50% relative to earlier works. We provide functional forms for both the Gaia-based and full-sample IFMRs. The Gaia-based result useful for Mi � 2.67 M⊙ is Mf = [0.179 0.100H (Mi 3.84 M )] × (Mi 3.84 M ) + 0.628 M , where H(x) is the Heaviside step function. Comparing our IFMR to recent literature, we identify significant deviations from best-fit IFMRs derived from both Gaia-based volume-limited samples of field WDs and double WD binaries, with the largest discrepancy occurring for initial masses of about 5 M⊙.","lang":"eng"}],"day":"01","date_created":"2026-04-12T22:01:52Z","scopus_import":"1"},{"publication":"Nature Materials","type":"journal_article","citation":{"chicago":"Baykusheva, Denitsa Rangelova, Deven Carmichael, Clara S. Weber, I. Te Lu, Filippo Glerean, Tepie Meng, Pedro B.M. De Oliveira, et al. “Quantum Control of Hubbard Excitons.” <i>Nature Materials</i>. Springer Nature, 2026. <a href=\"https://doi.org/10.1038/s41563-026-02517-6\">https://doi.org/10.1038/s41563-026-02517-6</a>.","short":"D.R. Baykusheva, D. Carmichael, C.S. Weber, I.T. Lu, F. Glerean, T. Meng, P.B.M. De Oliveira, C.C. Homes, I.A. Zaliznyak, G.D. Gu, M.P.M. Dean, A. Rubio, D.M. Kennes, M. Claassen, M. Mitrano, Nature Materials (2026).","ista":"Baykusheva DR, Carmichael D, Weber CS, Lu IT, Glerean F, Meng T, De Oliveira PBM, Homes CC, Zaliznyak IA, Gu GD, Dean MPM, Rubio A, Kennes DM, Claassen M, Mitrano M. 2026. Quantum control of Hubbard excitons. Nature Materials.","apa":"Baykusheva, D. R., Carmichael, D., Weber, C. S., Lu, I. T., Glerean, F., Meng, T., … Mitrano, M. (2026). Quantum control of Hubbard excitons. <i>Nature Materials</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41563-026-02517-6\">https://doi.org/10.1038/s41563-026-02517-6</a>","ama":"Baykusheva DR, Carmichael D, Weber CS, et al. Quantum control of Hubbard excitons. <i>Nature Materials</i>. 2026. doi:<a href=\"https://doi.org/10.1038/s41563-026-02517-6\">10.1038/s41563-026-02517-6</a>","mla":"Baykusheva, Denitsa Rangelova, et al. “Quantum Control of Hubbard Excitons.” <i>Nature Materials</i>, Springer Nature, 2026, doi:<a href=\"https://doi.org/10.1038/s41563-026-02517-6\">10.1038/s41563-026-02517-6</a>.","ieee":"D. R. Baykusheva <i>et al.</i>, “Quantum control of Hubbard excitons,” <i>Nature Materials</i>. Springer Nature, 2026."},"acknowledgement":"We thank K. Burch, M. Buzzi, P. Cappellaro, A. Cavalleri, E. Demler, M. Eckstein, T. Giamarchi, D. Hsieh, H. Okamoto, D. Reis, T. Tohyama, P. Werner and A. Yacoby for insightful discussions. We thank B. Baxley for assistance with graphics. This work was primarily supported by the US Department of Energy, Office of Basic Energy Sciences, Early Career Award Program, under award no. DE-SC0022883 (D.R.B., F.G., T.M. and M.M.) and award no. DE-SC0024494 (D.C. and M.C.). D.C. and P.B.M.D.O. acknowledge funding from the NSF GRFP under grant nos. DGE-1845298 and DGE 2140743, respectively. The work performed at Brookhaven National Laboratory was supported by the US Department of Energy, Division of Materials Science, under contract no. DE-SC0012704. We acknowledge funding from the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – 531215165 (Research Unit “OPTIMAL’). This work was supported by the Cluster of Excellence ‘Advanced Imaging of Matter’ (AIM) and the Max Planck-New York City Center for Non-Equilibrium Quantum Phenomena. The Flatiron Institute is a division of the Simons Foundation. Simulations were performed with computing resources granted by RWTH Aachen University under projects rwth0752 and rwth1258. We acknowledge computing time on the supercomputer JURECA52 at Forschungszentrum Jülich under the project ID enhancerg.","external_id":{"arxiv":["2601.20695 "]},"arxiv":1,"quality_controlled":"1","author":[{"last_name":"Baykusheva","orcid":"0000-0002-7438-1139","id":"71b4d059-2a03-11ee-914d-dfa3beed6530","first_name":"Denitsa Rangelova","full_name":"Baykusheva, Denitsa Rangelova"},{"full_name":"Carmichael, Deven","first_name":"Deven","last_name":"Carmichael"},{"last_name":"Weber","first_name":"Clara S.","full_name":"Weber, Clara S."},{"last_name":"Lu","first_name":"I. Te","full_name":"Lu, I. Te"},{"last_name":"Glerean","full_name":"Glerean, Filippo","first_name":"Filippo"},{"last_name":"Meng","first_name":"Tepie","full_name":"Meng, Tepie"},{"first_name":"Pedro B.M.","full_name":"De Oliveira, Pedro B.M.","last_name":"De Oliveira"},{"last_name":"Homes","first_name":"Christopher C.","full_name":"Homes, Christopher C."},{"last_name":"Zaliznyak","full_name":"Zaliznyak, Igor A.","first_name":"Igor A."},{"first_name":"G. D.","full_name":"Gu, G. D.","last_name":"Gu"},{"full_name":"Dean, Mark P.M.","first_name":"Mark P.M.","last_name":"Dean"},{"last_name":"Rubio","full_name":"Rubio, Angel","first_name":"Angel"},{"last_name":"Kennes","full_name":"Kennes, Dante M.","first_name":"Dante M."},{"full_name":"Claassen, Martin","first_name":"Martin","last_name":"Claassen"},{"last_name":"Mitrano","full_name":"Mitrano, Matteo","first_name":"Matteo"}],"doi":"10.1038/s41563-026-02517-6","_id":"21726","scopus_import":"1","title":"Quantum control of Hubbard excitons","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2601.20695","open_access":"1"}],"language":[{"iso":"eng"}],"abstract":[{"text":"Quantum control of the many-body wavefunction is a central challenge in quantum materials research, as it could yield a precise control knob to manipulate emergent phenomena. Floquet engineering, the coherent dressing of quantum states with periodic non-resonant optical fields, has become an important strategy for quantum control. Most applications to solid-state systems have targeted weakly interacting or single-ion states, leaving the manipulation of many-body wavefunctions largely unexplored. Here we use Floquet engineering to achieve quantum control of a strongly correlated Hubbard exciton in the one-dimensional Mott insulator Sr2CuO3. A non-resonant mid-infrared optical field coherently dresses the exciton wavefunction, driving its rotation between bright and dark states. We use resonant third-harmonic generation to quantify ultrafast π/2 rotations on the Bloch sphere spanned by these exciton states. Our work advances the quest towards programmable control of correlated states and exciton-based quantum sensing.","lang":"eng"}],"day":"09","date_created":"2026-04-12T22:01:53Z","OA_place":"repository","publication_identifier":{"eissn":["1476-4660"],"issn":["1476-1122"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Preprint","OA_type":"green","year":"2026","status":"public","corr_author":"1","month":"03","date_published":"2026-03-09T00:00:00Z","article_type":"original","date_updated":"2026-04-13T07:29:34Z","publication_status":"epub_ahead","publisher":"Springer Nature","oa":1,"article_processing_charge":"No","department":[{"_id":"DeBa"}]},{"acknowledged_ssus":[{"_id":"LifeSc"}],"publisher":"Royal Society of Chemistry","date_published":"2026-04-10T00:00:00Z","month":"04","article_type":"original","publication_status":"epub_ahead","date_updated":"2026-04-16T05:44:49Z","department":[{"_id":"StFr"}],"article_processing_charge":"No","OA_type":"closed access","oa_version":"None","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"issn":["2050-750X"],"eissn":["2050-7518"]},"corr_author":"1","year":"2026","status":"public","pmid":1,"scopus_import":"1","abstract":[{"lang":"eng","text":"Hydrogen peroxide (H2O2) is a crucial member of the reactive oxygen species (ROS) family, playing roles in cellular signalling and immune responses in human health. Moreover, it is a potential biomarker of diabetes when present in aberrant concentrations. Therefore, monitoring trace levels of H2O2 has become a research hotspot for analytical and sensor chemists. In this context, we report a rhodamine-based fluorescent probe (RN), which shows excellent fluorescent enhancement at 555 nm upon the addition of H2O2 along with a low limit of detection (LOD) of 0.67 ppm and fast response (∼2 min). The probe is highly selective for H2O2, showing no fluorescence enhancement with other ROS. RN is synthesised in a one-pot chemical reaction using rhodamine 6G (R6G) and 4,7,10-trioxa-1,13-tridecanediamine (TTDA). H2O2 detection in pre-treated milk samples proves its real-world viability. We found that RN shows low cytotoxicity, which allowed us to successfully explore its potential to monitor H2O2 generation in a diabetic L929 skin cell line and diabetic mice liver tissue. This result demonstrates promising features for assessing early diabetic progression through fluorescence imaging."}],"day":"10","date_created":"2026-04-13T07:45:26Z","title":"H2O2 responsive rhodamine-based probe for monitoring early-stage diabetes diagnosis","language":[{"iso":"eng"}],"acknowledgement":"MM acknowledges the Government of India for DST-INSPIRE\r\nfellowship [IF200389] and Federal Ministry of Education, Science and Research (BMBWF) and the OeAD – Austria’s Agency for Education and Internationalisation for an Ernst Mach Grant, weltweit (grant number MPC-2024-01518) for research internship at ISTA. The Scientific Service Units of ISTA supported this research through resources provided by the Lab Support Facility. PG acknowledges the ANRF, India, for his NPDF fellowship (File no. PDF/2022/001960). PB acknowledges ANRF, India, for the SERB-CRG sponsored project GAP-240712 (vide reference no. CRG/2022/001679).","citation":{"apa":"Mondal, M., Ghorai, P., Samadder, A., Freunberger, S. A., &#38; Banerjee, P. (2026). H2O2 responsive rhodamine-based probe for monitoring early-stage diabetes diagnosis. <i>Journal of Materials Chemistry B</i>. Royal Society of Chemistry. <a href=\"https://doi.org/10.1039/d5tb02687c\">https://doi.org/10.1039/d5tb02687c</a>","ama":"Mondal M, Ghorai P, Samadder A, Freunberger SA, Banerjee P. H2O2 responsive rhodamine-based probe for monitoring early-stage diabetes diagnosis. <i>Journal of Materials Chemistry B</i>. 2026. doi:<a href=\"https://doi.org/10.1039/d5tb02687c\">10.1039/d5tb02687c</a>","ieee":"M. Mondal, P. Ghorai, A. Samadder, S. A. Freunberger, and P. Banerjee, “H2O2 responsive rhodamine-based probe for monitoring early-stage diabetes diagnosis,” <i>Journal of Materials Chemistry B</i>. Royal Society of Chemistry, 2026.","mla":"Mondal, Moumita, et al. “H2O2 Responsive Rhodamine-Based Probe for Monitoring Early-Stage Diabetes Diagnosis.” <i>Journal of Materials Chemistry B</i>, Royal Society of Chemistry, 2026, doi:<a href=\"https://doi.org/10.1039/d5tb02687c\">10.1039/d5tb02687c</a>.","chicago":"Mondal, Moumita, Pravat Ghorai, Asmita Samadder, Stefan Alexander Freunberger, and Priyabrata Banerjee. “H2O2 Responsive Rhodamine-Based Probe for Monitoring Early-Stage Diabetes Diagnosis.” <i>Journal of Materials Chemistry B</i>. Royal Society of Chemistry, 2026. <a href=\"https://doi.org/10.1039/d5tb02687c\">https://doi.org/10.1039/d5tb02687c</a>.","short":"M. Mondal, P. Ghorai, A. Samadder, S.A. Freunberger, P. Banerjee, Journal of Materials Chemistry B (2026).","ista":"Mondal M, Ghorai P, Samadder A, Freunberger SA, Banerjee P. 2026. H2O2 responsive rhodamine-based probe for monitoring early-stage diabetes diagnosis. Journal of Materials Chemistry B."},"external_id":{"pmid":["41958432"]},"type":"journal_article","publication":"Journal of Materials Chemistry B","doi":"10.1039/d5tb02687c","_id":"21730","author":[{"first_name":"Moumita","full_name":"Mondal, Moumita","last_name":"Mondal"},{"last_name":"Ghorai","full_name":"Ghorai, Pravat","first_name":"Pravat"},{"first_name":"Asmita","full_name":"Samadder, Asmita","last_name":"Samadder"},{"id":"A8CA28E6-CE23-11E9-AD2D-EC27E6697425","full_name":"Freunberger, Stefan Alexander","first_name":"Stefan Alexander","last_name":"Freunberger","orcid":"0000-0003-2902-5319"},{"last_name":"Banerjee","first_name":"Priyabrata","full_name":"Banerjee, Priyabrata"}],"quality_controlled":"1"},{"type":"preprint","publication":"arXiv","acknowledgement":"This project was funded in part by the European Research Council (ERC Consolidator Grant 101045083 CoDiNA) and the National Science Foundation CAREER Award 2239062.\r\n","citation":{"ista":"Chern A, Ishida S. L’Hopital rules for complex-valued functions in higher dimensions. arXiv, 2602.09958.","chicago":"Chern, Albert, and Sadashige Ishida. “L’Hopital Rules for Complex-Valued Functions in Higher Dimensions.” <i>ArXiv</i>, n.d. <a href=\"https://doi.org/10.48550/ARXIV.2602.09958\">https://doi.org/10.48550/ARXIV.2602.09958</a>.","short":"A. Chern, S. Ishida, ArXiv (n.d.).","mla":"Chern, Albert, and Sadashige Ishida. “L’Hopital Rules for Complex-Valued Functions in Higher Dimensions.” <i>ArXiv</i>, 2602.09958, doi:<a href=\"https://doi.org/10.48550/ARXIV.2602.09958\">10.48550/ARXIV.2602.09958</a>.","ieee":"A. Chern and S. Ishida, “L’Hopital rules for complex-valued functions in higher dimensions,” <i>arXiv</i>. .","apa":"Chern, A., &#38; Ishida, S. (n.d.). L’Hopital rules for complex-valued functions in higher dimensions. <i>arXiv</i>. <a href=\"https://doi.org/10.48550/ARXIV.2602.09958\">https://doi.org/10.48550/ARXIV.2602.09958</a>","ama":"Chern A, Ishida S. L’Hopital rules for complex-valued functions in higher dimensions. <i>arXiv</i>. doi:<a href=\"https://doi.org/10.48550/ARXIV.2602.09958\">10.48550/ARXIV.2602.09958</a>"},"ddc":["510"],"external_id":{"arxiv":["2602.09958"]},"arxiv":1,"author":[{"last_name":"Chern","full_name":"Chern, Albert","first_name":"Albert"},{"orcid":"0000-0002-3121-3100","last_name":"Ishida","first_name":"Sadashige","full_name":"Ishida, Sadashige","id":"6F7C4B96-A8E9-11E9-A7CA-09ECE5697425"}],"doi":"10.48550/ARXIV.2602.09958","_id":"21737","project":[{"_id":"34bc2376-11ca-11ed-8bc3-9a3b3961a088","grant_number":"101045083","name":"Computational Discovery of Numerical Algorithms for Animation and Simulation of Natural Phenomena"}],"title":"L'Hopital rules for complex-valued functions in higher dimensions","language":[{"iso":"eng"}],"file_date_updated":"2026-04-28T10:53:27Z","keyword":["l’Hopital theorem","complex functions"],"day":"10","abstract":[{"text":"In calculus, l'Hopital's rule provides a simple way to evaluate the limits of quotient functions when both the numerator and denominator vanish. But what happens when we move beyond real functions on a real interval? In this article, we study when the quotient of two complex-valued functions in higher dimension can be defined continuously at the points where both functions vanish. Surprisingly, the answer is far subtler than in the real-valued setting. We provide a complete characterization for the continuity of the quotient function. We also point out why extending this result to smoother quotients remains an intriguing challenge.","lang":"eng"}],"date_created":"2026-04-15T16:28:24Z","OA_place":"repository","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","file":[{"file_id":"21771","relation":"main_file","file_name":"2026_arXiv_2602.09958.pdf","date_created":"2026-04-28T10:53:27Z","date_updated":"2026-04-28T10:53:27Z","success":1,"creator":"dernst","content_type":"application/pdf","file_size":867109,"access_level":"open_access","checksum":"6a76591c723d3e949ad5afa9f7dbb2ee"}],"oa_version":"Preprint","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"OA_type":"green","year":"2026","status":"public","corr_author":"1","has_accepted_license":"1","month":"02","date_published":"2026-02-10T00:00:00Z","date_updated":"2026-04-28T10:56:30Z","publication_status":"submitted","oa":1,"article_processing_charge":"No","article_number":"2602.09958","department":[{"_id":"GradSch"},{"_id":"ChWo"}]},{"oa":1,"department":[{"_id":"GradSch"},{"_id":"ChWo"}],"article_number":"45","article_processing_charge":"Yes (via OA deal)","PlanS_conform":"1","publication_status":"published","date_updated":"2026-04-28T09:59:01Z","date_published":"2026-04-15T00:00:00Z","article_type":"original","month":"04","publisher":"Springer Nature","year":"2026","issue":"2","status":"public","has_accepted_license":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"issn":["0938-8974"],"eissn":["1432-1467"]},"OA_place":"publisher","OA_type":"hybrid","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"oa_version":"Published Version","file":[{"relation":"main_file","file_name":"2026_JourNonlinearScience_Bauer.pdf","date_created":"2026-04-28T09:55:32Z","file_id":"21770","success":1,"creator":"dernst","checksum":"760de2631b6fd7d57bcd5115ed36c0a2","access_level":"open_access","file_size":1108518,"content_type":"application/pdf","date_updated":"2026-04-28T09:55:32Z"}],"volume":36,"file_date_updated":"2026-04-28T09:55:32Z","language":[{"iso":"eng"}],"related_material":{"record":[{"status":"public","relation":"earlier_version","id":"17361"}]},"title":"Symplectic structures on the space of space curves","date_created":"2026-04-16T07:29:17Z","abstract":[{"text":"We present symplectic structures on the shape space of unparameterized space curves that generalize the classical Marsden–Weinstein structure. Our method integrates the Liouville 1-form of the Marsden–Weinstein structure with Riemannian structures that have been introduced in mathematical shape analysis. We also derive Hamiltonian vector fields for several classical Hamiltonian functions with respect to these new symplectic structures.","lang":"eng"}],"day":"15","scopus_import":"1","author":[{"full_name":"Bauer, Martin","first_name":"Martin","last_name":"Bauer"},{"first_name":"Sadashige","full_name":"Ishida, Sadashige","id":"6F7C4B96-A8E9-11E9-A7CA-09ECE5697425","orcid":"0000-0002-3121-3100","last_name":"Ishida"},{"full_name":"Michor, Peter W.","first_name":"Peter W.","last_name":"Michor"}],"quality_controlled":"1","project":[{"grant_number":"101045083","name":"Computational Discovery of Numerical Algorithms for Animation and Simulation of Natural Phenomena","_id":"34bc2376-11ca-11ed-8bc3-9a3b3961a088"}],"_id":"21743","doi":"10.1007/s00332-026-10266-8","type":"journal_article","publication":"Journal of Nonlinear Science","intvolume":"        36","arxiv":1,"external_id":{"arxiv":["2407.19908"]},"ddc":["510"],"citation":{"chicago":"Bauer, Martin, Sadashige Ishida, and Peter W. Michor. “Symplectic Structures on the Space of Space Curves.” <i>Journal of Nonlinear Science</i>. Springer Nature, 2026. <a href=\"https://doi.org/10.1007/s00332-026-10266-8\">https://doi.org/10.1007/s00332-026-10266-8</a>.","short":"M. Bauer, S. Ishida, P.W. Michor, Journal of Nonlinear Science 36 (2026).","ista":"Bauer M, Ishida S, Michor PW. 2026. Symplectic structures on the space of space curves. Journal of Nonlinear Science. 36(2), 45.","apa":"Bauer, M., Ishida, S., &#38; Michor, P. W. (2026). Symplectic structures on the space of space curves. <i>Journal of Nonlinear Science</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s00332-026-10266-8\">https://doi.org/10.1007/s00332-026-10266-8</a>","ama":"Bauer M, Ishida S, Michor PW. Symplectic structures on the space of space curves. <i>Journal of Nonlinear Science</i>. 2026;36(2). doi:<a href=\"https://doi.org/10.1007/s00332-026-10266-8\">10.1007/s00332-026-10266-8</a>","ieee":"M. Bauer, S. Ishida, and P. W. Michor, “Symplectic structures on the space of space curves,” <i>Journal of Nonlinear Science</i>, vol. 36, no. 2. Springer Nature, 2026.","mla":"Bauer, Martin, et al. “Symplectic Structures on the Space of Space Curves.” <i>Journal of Nonlinear Science</i>, vol. 36, no. 2, 45, Springer Nature, 2026, doi:<a href=\"https://doi.org/10.1007/s00332-026-10266-8\">10.1007/s00332-026-10266-8</a>."},"acknowledgement":"The authors are grateful to Boris Khesin for valuable comments on the MW symplectic structure and S. Ishida thanks Albert Chern for insightful discussions on space curves and Chris Wojtan for his continuous support. M. Bauer was partially supported by NSF grant DMS-1953244 and by the Binational Science Foundation (BSF). S. Ishida was partially supported by ERC Consolidator Grant 101045083 “CoDiNA” funded by the European Research Council. Some figures were generated by the software Houdini and its education license was provided by SideFX. Open access funding provided by University of Vienna."},{"pmid":1,"scopus_import":"1","date_created":"2026-04-16T13:51:29Z","abstract":[{"lang":"eng","text":"The paraventricular hypothalamus (PVH) controls behavioral and physiologic processes, including appetite, social behavior, autonomic outflow, and pituitary hormone secretion. However, molecular markers for centrally projecting PVH neuron populations remain largely undefined, and a complete census of PVH cell types has not been established. Therefore, we performed extensive single-cell/nucleus RNA sequencing to catalog PVH neuron subtypes and multiplexed error-robust fluorescence in situ hybridization (MERFISH) to map them spatially. Our spatial transcriptomic atlas resolves 26 Sim1+ and 29 GABAergic neuron populations from the PVH and surrounding areas. Additionally, projection-based profiling identified neurons that project to the parabrachial region (PB) and spinal cord, helping to determine PVH populations that regulate satiety and sympathetic nervous system activity, respectively. Notably, activation of PB-projecting PVH neurons expressing Brs3 reduces food intake, and silencing them causes obesity. Together, this atlas contributes high-resolution PVH spatial and circuit-based gene expression profiles, representing a valuable resource for the field of homeostasis."}],"day":"24","language":[{"iso":"eng"}],"DOAJ_listed":"1","title":"A spatial and projection-based transcriptomic atlas of paraventricular hypothalamic cell types","volume":45,"file_date_updated":"2026-05-04T11:58:51Z","external_id":{"pmid":["41581146"]},"ddc":["570"],"citation":{"short":"Y. Li, T.C. Butler, S. Nardone, C.L. Jacobs, A.M. Douglass, J.C. Madara, M.C. McDonough, J. Tao, E.D. Lowenstein, L. Wang, D. Pant, S.J. Walker, A. Wang, H. Srinivasan, Z. Yang, J.N. Campbell, L.T. Tsai, B.B. Lowell, J.M. Resch, Cell Reports 45 (2026).","chicago":"Li, Yuxi, Trevor C. Butler, Stefano Nardone, Christopher L. Jacobs, Amelia M. Douglass, Joseph C. Madara, Miriam C. McDonough, et al. “A Spatial and Projection-Based Transcriptomic Atlas of Paraventricular Hypothalamic Cell Types.” <i>Cell Reports</i>. Elsevier, 2026. <a href=\"https://doi.org/10.1016/j.celrep.2025.116904\">https://doi.org/10.1016/j.celrep.2025.116904</a>.","ista":"Li Y, Butler TC, Nardone S, Jacobs CL, Douglass AM, Madara JC, McDonough MC, Tao J, Lowenstein ED, Wang L, Pant D, Walker SJ, Wang A, Srinivasan H, Yang Z, Campbell JN, Tsai LT, Lowell BB, Resch JM. 2026. A spatial and projection-based transcriptomic atlas of paraventricular hypothalamic cell types. Cell Reports. 45(2), 116904.","ama":"Li Y, Butler TC, Nardone S, et al. A spatial and projection-based transcriptomic atlas of paraventricular hypothalamic cell types. <i>Cell Reports</i>. 2026;45(2). doi:<a href=\"https://doi.org/10.1016/j.celrep.2025.116904\">10.1016/j.celrep.2025.116904</a>","apa":"Li, Y., Butler, T. C., Nardone, S., Jacobs, C. L., Douglass, A. M., Madara, J. C., … Resch, J. M. (2026). A spatial and projection-based transcriptomic atlas of paraventricular hypothalamic cell types. <i>Cell Reports</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.celrep.2025.116904\">https://doi.org/10.1016/j.celrep.2025.116904</a>","mla":"Li, Yuxi, et al. “A Spatial and Projection-Based Transcriptomic Atlas of Paraventricular Hypothalamic Cell Types.” <i>Cell Reports</i>, vol. 45, no. 2, 116904, Elsevier, 2026, doi:<a href=\"https://doi.org/10.1016/j.celrep.2025.116904\">10.1016/j.celrep.2025.116904</a>.","ieee":"Y. Li <i>et al.</i>, “A spatial and projection-based transcriptomic atlas of paraventricular hypothalamic cell types,” <i>Cell Reports</i>, vol. 45, no. 2. Elsevier, 2026."},"acknowledgement":"We would like to thank Drs. Mark Andermann, Joel Geerling, and Clifford\r\nSaper, as well as the Lowell, Tsai, and Resch laboratories for helpful discussions;\r\nAlysia Berns, Jia Yu, and Yanfang Li for technical support; the BNORC\r\nFunctional Genomics and Bioinformatics Core (P30DK046200) and the Iowa\r\nInstitute for Human Genetics Genomics Division (IIHG, RRID: SCR_023422)\r\nfor helpful discussions and technical assistance with sc/snRNA-seq; Zachary\r\nNiziolek and the Bauer Core Facility at Harvard University, the BIDMC Flow Cytometry\r\nCore, and Heath Vignes, Michael Shey, and Thomas Kaufman of the\r\nFlow Cytometry Facility at the University of Iowa Carver College of Medicine\r\nfor helpful discussions and technical support; the ICCB-Longwood Screening\r\nFacility of Harvard Medical School for assistance with the snRNA-seq\r\nexperiments; Dr. Sayak Mitter and Vizgen support for technical assistance\r\nwith the MERSCOPE platform; and Mara Jendro and Li-Chun (Queena) Lin\r\nfor their assistance with MERSCOPE experiments within the Iowa\r\nNeuroBank Core in the Iowa Neuroscience Institute at the University of Iowa\r\nCarver College of Medicine. This research was funded by the following NIH\r\ngrants to L.T.T.: R01DK128406; to B.B.L.: R01DK075632, R01DK134427,\r\nand R01DK096010; to J.M.R.: R00HL144923 and R01NS141072; and to M.C.M.: F31HL170784; T.C.B. and M.C.M. were supported by a pharmacological\r\nsciences predoctoral training grant T32GM144636. Additional funding\r\nto J.M.R. came from the American Heart Association (AHA 935362), a University\r\nof Iowa Fraternal Order of Eagles Diabetes Research Center Pilot and\r\nFeasibility Catalyst Grant, and an Iowa Neuroscience Institute Early Stage\r\nInvestigator award from the Carver Trust. Y.L. was supported by a predoctoral\r\nfellowship from the American Heart Association (AHA 25PRE1372983). A.M.D.\r\nwas supported by a postdoctoral fellowship from the Charles A. King Trust.","intvolume":"        45","type":"journal_article","publication":"Cell Reports","_id":"21744","doi":"10.1016/j.celrep.2025.116904","quality_controlled":"1","author":[{"full_name":"Li, Yuxi","first_name":"Yuxi","last_name":"Li"},{"first_name":"Trevor C.","full_name":"Butler, Trevor C.","last_name":"Butler"},{"last_name":"Nardone","first_name":"Stefano","full_name":"Nardone, Stefano"},{"last_name":"Jacobs","first_name":"Christopher L.","full_name":"Jacobs, Christopher L."},{"last_name":"Douglass","orcid":"0000-0001-5398-6473","id":"de5f6fda-80fb-11ef-996f-a8c4ecd8e289","first_name":"Amelia May Barnett","full_name":"Douglass, Amelia May Barnett"},{"last_name":"Madara","full_name":"Madara, Joseph C.","first_name":"Joseph C."},{"last_name":"McDonough","first_name":"Miriam C.","full_name":"McDonough, Miriam C."},{"last_name":"Tao","first_name":"Jenkang","full_name":"Tao, Jenkang"},{"first_name":"Elijah D.","full_name":"Lowenstein, Elijah D.","last_name":"Lowenstein"},{"first_name":"Luhong","full_name":"Wang, Luhong","last_name":"Wang"},{"last_name":"Pant","full_name":"Pant, Deepti","first_name":"Deepti"},{"first_name":"Samuel J.","full_name":"Walker, Samuel J.","last_name":"Walker"},{"full_name":"Wang, Annette","first_name":"Annette","last_name":"Wang"},{"full_name":"Srinivasan, Harini","first_name":"Harini","last_name":"Srinivasan"},{"full_name":"Yang, Zongfang","first_name":"Zongfang","last_name":"Yang"},{"last_name":"Campbell","first_name":"John N.","full_name":"Campbell, John N."},{"first_name":"Linus T.","full_name":"Tsai, Linus T.","last_name":"Tsai"},{"last_name":"Lowell","first_name":"Bradford B.","full_name":"Lowell, Bradford B."},{"first_name":"Jon M.","full_name":"Resch, Jon M.","last_name":"Resch"}],"publisher":"Elsevier","publication_status":"published","date_updated":"2026-05-04T12:00:31Z","article_type":"original","date_published":"2026-02-24T00:00:00Z","month":"02","article_processing_charge":"Yes","department":[{"_id":"AmDo"}],"article_number":"116904","oa":1,"oa_version":"Published Version","file":[{"file_id":"21793","file_name":"2026_CellReports_Li.pdf","date_created":"2026-05-04T11:58:51Z","relation":"main_file","date_updated":"2026-05-04T11:58:51Z","creator":"dernst","checksum":"82098dd9d0ca609119f9f2c6beb4fc1e","content_type":"application/pdf","access_level":"open_access","file_size":38532865,"success":1}],"OA_type":"gold","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","short":"CC BY-NC-ND (4.0)","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)","image":"/images/cc_by_nc_nd.png"},"publication_identifier":{"issn":["2639-1856"],"eissn":["2211-1247"]},"OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","has_accepted_license":"1","status":"public","year":"2026","issue":"2"},{"quality_controlled":"1","author":[{"full_name":"Elms, Abbigail K.","first_name":"Abbigail K.","last_name":"Elms"},{"full_name":"Bagnulo, Stefano","first_name":"Stefano","last_name":"Bagnulo"},{"first_name":"Pier Emmanuel","full_name":"Tremblay, Pier Emmanuel","last_name":"Tremblay"},{"last_name":"Cunningham","first_name":"Tim","full_name":"Cunningham, Tim"},{"first_name":"James","full_name":"Munday, James","last_name":"Munday"},{"first_name":"John","full_name":"Landstreet, John","last_name":"Landstreet"},{"first_name":"Kareem","full_name":"El-Badry, Kareem","last_name":"El-Badry"},{"last_name":"Caiazzo","orcid":"0000-0002-4770-5388","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","full_name":"Caiazzo, Ilaria","first_name":"Ilaria"},{"full_name":"Melis, Carl","first_name":"Carl","last_name":"Melis"},{"full_name":"Pinter, Viktoria","first_name":"Viktoria","last_name":"Pinter"},{"last_name":"Weinberger","full_name":"Weinberger, Alycia","first_name":"Alycia"}],"_id":"21745","doi":"10.1093/mnras/stag505","publication":"Monthly Notices of the Royal Astronomical Society","type":"journal_article","ddc":["520"],"external_id":{"arxiv":["2603.12048"]},"acknowledgement":"This project has received funding from the European Research Council under the European Union’s Horizon 2020 research and innovation programme (Grant agreement numbers 101002408). The observationsfrom the FOcal Reducer/low dispersion Spectrograph 2 (FORS2) instrument were collected at the European Southern Observatory (ESO) under ESO programme(s) 113.26ES.001. This work has made use of data from the European Space\r\nAgency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/conso\r\nrtium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grants No. AST-1440341 and AST-2034437 and a collaboration including current partners Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and\r\nHumboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, IN2P3, University\r\nof Warwick, Ruhr University Bochum, Northwestern University and former partners the University of Washington, Los Alamos National Laboratories, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW. This work has made use of data from the Asteroid Terrestrialimpact Last Alert System (ATLAS) project. The Asteroid Terrestrial-impact Last Alert System (ATLAS) project is primarily funded to search for near earth asteroids through NASA grants NN12AR55G, 80NSSC18K0284, and 80NSSC18K1575; byproducts of the NEO search include images and catalogs from the survey area. This work was partially funded by Kepler/K2 grant J1944/80NSSC19K0112 and HST GO-15889, and STFC grants ST/T000198/1 and ST/S006109/1. The ATLAS science products have been made possible through the contributions of the University of Hawaii Institute for Astronomy, the Queen’s University Belfast, the Space Telescope Science Institute, the South African\r\nAstronomical Observatory, and The Millennium Institute of Astrophysics (MAS), Chile.\r\nThis work makes use of observations from the Las Cumbres Observatory global telescope network. Research at Lick Observatory is partially supported by a generous gift from Google. A major upgrade of the Kast spectrograph on the Shane 3 m telescope at Lick Observatory was made possible through generous gifts from William and Marina Kast as well as the Heising–Simons Foundation. The Isaac Newton Telescope is operated on the island of La Palma by the Isaac Newton Group of Telescopes in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias.This paper includes data gathered with the 6.5 meter Magellan Telescopes located at Las Campanas Observatory, Chile. Observations reported here were obtained at the Multiple Mirror Telescope (MMT) Observatory, a joint facility of the Smithsonian Institution and the University of Arizona. Based on observations collected at Centro Astronómico Hispano en Andalucía (CAHA) at Calar Alto, operated jointly by Junta de Andalucía and Consejo Superior de Investigaciones Científicas (IAA-CSIC).","citation":{"short":"A.K. Elms, S. Bagnulo, P.E. Tremblay, T. Cunningham, J. Munday, J. Landstreet, K. El-Badry, I. Caiazzo, C. Melis, V. Pinter, A. Weinberger, Monthly Notices of the Royal Astronomical Society 548 (2026).","chicago":"Elms, Abbigail K., Stefano Bagnulo, Pier Emmanuel Tremblay, Tim Cunningham, James Munday, John Landstreet, Kareem El-Badry, et al. “Detection of a Weak Magnetic Field in the Balmer Emission Line White Dwarf WDJ1653−1001.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2026. <a href=\"https://doi.org/10.1093/mnras/stag505\">https://doi.org/10.1093/mnras/stag505</a>.","ista":"Elms AK, Bagnulo S, Tremblay PE, Cunningham T, Munday J, Landstreet J, El-Badry K, Caiazzo I, Melis C, Pinter V, Weinberger A. 2026. Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653−1001. Monthly Notices of the Royal Astronomical Society. 548(1), stag505.","ama":"Elms AK, Bagnulo S, Tremblay PE, et al. Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653−1001. <i>Monthly Notices of the Royal Astronomical Society</i>. 2026;548(1). doi:<a href=\"https://doi.org/10.1093/mnras/stag505\">10.1093/mnras/stag505</a>","apa":"Elms, A. K., Bagnulo, S., Tremblay, P. E., Cunningham, T., Munday, J., Landstreet, J., … Weinberger, A. (2026). Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653−1001. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stag505\">https://doi.org/10.1093/mnras/stag505</a>","mla":"Elms, Abbigail K., et al. “Detection of a Weak Magnetic Field in the Balmer Emission Line White Dwarf WDJ1653−1001.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 548, no. 1, stag505, Oxford University Press, 2026, doi:<a href=\"https://doi.org/10.1093/mnras/stag505\">10.1093/mnras/stag505</a>.","ieee":"A. K. Elms <i>et al.</i>, “Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653−1001,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 548, no. 1. Oxford University Press, 2026."},"intvolume":"       548","arxiv":1,"language":[{"iso":"eng"}],"DOAJ_listed":"1","title":"Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653−1001","volume":548,"file_date_updated":"2026-05-04T12:10:40Z","date_created":"2026-04-19T22:07:42Z","day":"01","abstract":[{"text":"The small DAHe and DAe spectral classes comprise isolated, hydrogen-dominated atmosphere white dwarfs that exhibit variable photometric flux and Balmer line emission. These mysterious systems offer unique insight into the complex interplay between magnetic fields, stellar rotation and atmospheric activity in single white dwarfs. DAHe stars have detectable magnetic fields through Zeeman-split spectral lines, whereas DAe stars lack such splitting. We report the first discovery and characterization of magnetism in the DAe white dwarf WD J165335.21−100116.33 with new time-resolved spectropolarimetry from FORS2. We detect a weak but variable longitudinal magnetic field with values Bz > −9.2 ± 2.4 kG and Bz < −2.2 ± 1.0 kG. Independent ZTF and ATLAS photometry reveal a consistent period of P = 80.3070 ± 0.0007 h. Time-resolved optical spectroscopy obtained with six ground-based instruments demonstrates strong modulation in the strength of the Hα and Hβ Balmer line emission with P = 80.2922 ± 0.0108 h. The photometric flux and Balmer emission strength vary in antiphase, with the strongest magnetic detections coinciding with phases of low photometric flux and strong line emission. These characteristicssupport the theory that a magnetically active, temperature-inverted spot/region is producing an optically thin chromospheric emission region. Comparison with other DAe and DAHe white dwarfsreveals all systems have a strikingly similar antiphase phenomenology, reinforcing the theory that they are subject to a unified physical mechanism. With the detection of a weak magnetic field, we reclassify WD J165335.21−100116.33 as a low-field DAHe white dwarf. ","lang":"eng"}],"scopus_import":"1","issue":"1","status":"public","year":"2026","has_accepted_license":"1","publication_identifier":{"issn":["0035-8711"],"eissn":["1365-2966"]},"OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Published Version","file":[{"file_name":"2026_MNRAS_Elms.pdf","date_created":"2026-05-04T12:10:40Z","relation":"main_file","file_id":"21794","creator":"dernst","content_type":"application/pdf","access_level":"open_access","file_size":4991495,"checksum":"75c48d70d10a9a48875f577e04da80bc","success":1,"date_updated":"2026-05-04T12:10:40Z"}],"OA_type":"gold","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"oa":1,"article_processing_charge":"Yes","department":[{"_id":"IlCa"}],"article_number":"stag505","date_updated":"2026-05-04T12:11:53Z","publication_status":"published","article_type":"original","date_published":"2026-05-01T00:00:00Z","month":"05","publisher":"Oxford University Press"},{"article_processing_charge":"Yes","department":[{"_id":"LoSw"},{"_id":"GradSch"},{"_id":"TiVo"},{"_id":"Bio"},{"_id":"NiBa"}],"article_number":"117227","oa":1,"acknowledged_ssus":[{"_id":"Bio"},{"_id":"LifeSc"}],"publisher":"Elsevier","month":"04","article_type":"original","date_published":"2026-04-28T00:00:00Z","publication_status":"published","date_updated":"2026-05-04T12:27:06Z","PlanS_conform":"1","corr_author":"1","has_accepted_license":"1","year":"2026","issue":"4","status":"public","file":[{"access_level":"open_access","checksum":"0d26cdb5b8d8dec3a911d8261a65cdef","file_size":14925958,"content_type":"application/pdf","creator":"dernst","success":1,"date_updated":"2026-05-04T12:20:10Z","date_created":"2026-05-04T12:20:10Z","file_name":"2026_CellReports_Vijatovic.pdf","relation":"main_file","file_id":"21795"}],"oa_version":"Published Version","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"OA_type":"gold","OA_place":"publisher","publication_identifier":{"eissn":["2211-1247"],"issn":["2639-1856"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","day":"28","abstract":[{"text":"As vertebrates transitioned from water to land, locomotion shifted from undulatory swimming to limb-based movement. How spinal circuits and their cell types evolved to support this transition remains unclear. We leverage frog metamorphosis, which recapitulates this transition within a single organism, to define how spinal circuits generate aquatic versus terrestrial motor patterns. At swim stages, spinal architecture is uniform, with a transcriptionally and anatomically homogeneous motor and interneurons. As limbs develop and their movement complexifies, spinal circuits expand in neuron number and subtype diversity. This expansion is most pronounced for V1 inhibitory neurons, which increase ∼70-fold and diversify into transcriptionally distinct subtypes. Disrupting transcription factors defining emerging motor and V1 populations reveals molecular segregation between swim and limb circuits, highlighting the role of subtype diversity in motor coordination. A multifold increase in inhibitory neuron diversity thus underlies the tail-to-limb locomotor transition, providing a framework for spinal circuit adaptation during vertebrate evolution.","lang":"eng"}],"date_created":"2026-04-19T22:07:43Z","DOAJ_listed":"1","title":"Multifold increase in spinal inhibitory cell types with emergence of limb movement","language":[{"iso":"eng"}],"file_date_updated":"2026-05-04T12:20:10Z","volume":45,"pmid":1,"scopus_import":"1","doi":"10.1016/j.celrep.2026.117227","_id":"21746","project":[{"_id":"ebb66355-77a9-11ec-83b8-b8ac210a4dae","grant_number":"101041551","name":"Development and Evolution of Tetrapod Motor Circuits"},{"name":"Stem Cell Modulation in Neural Development and Regeneration/ P14-Swim-to-limb transition: cell type to connection diversity","grant_number":"F7814","_id":"8da85f50-16d5-11f0-9cad-eab8b0ff6c9e"},{"name":"Tools for automation and feedback microscopy","grant_number":"CZI01","_id":"c08e9ad1-5a5b-11eb-8a69-9d1cf3b07473"},{"_id":"bd73af52-d553-11ed-ba76-912049f0ac7a","grant_number":"FTI21-D-046","name":"Development of V1 interneuron diversity during swim-to-walk transition of Xenopus metamorphosis"}],"quality_controlled":"1","author":[{"last_name":"Vijatovic","id":"cf391e77-ec3c-11ea-a124-d69323410b58","full_name":"Vijatovic, David","first_name":"David"},{"last_name":"Toma","id":"2f73f876-f128-11eb-9611-b96b5a30cb0e","first_name":"Florina Alexandra ","full_name":"Toma, Florina Alexandra "},{"full_name":"Ignatyev, Y","first_name":"Y","last_name":"Ignatyev"},{"last_name":"Harrington","orcid":"0009-0008-0158-4032","id":"a8144562-32c9-11ee-b5ce-d9800628bda2","first_name":"Zoe P","full_name":"Harrington, Zoe P"},{"last_name":"Sommer","orcid":"0000-0003-1216-9105","id":"4DF26D8C-F248-11E8-B48F-1D18A9856A87","first_name":"Christoph M","full_name":"Sommer, Christoph M"},{"last_name":"Hauschild","orcid":"0000-0001-9843-3522","id":"4E01D6B4-F248-11E8-B48F-1D18A9856A87","first_name":"Robert","full_name":"Hauschild, Robert"},{"id":"7a231d52-e216-11ee-a0bb-8acd55f8f1f0","first_name":"Matthijs Geert","full_name":"Smits, Matthijs Geert","last_name":"Smits"},{"last_name":"Dalla Vecchia","id":"02a7a869-ff06-11ed-a87f-86649d6077e5","first_name":"Marco","full_name":"Dalla Vecchia, Marco"},{"last_name":"Trevisan","full_name":"Trevisan, Alexandra J.","first_name":"Alexandra J."},{"first_name":"Phillip","full_name":"Chapman, Phillip","last_name":"Chapman"},{"id":"1cf464b2-dc7d-11ea-9b2f-f9b1aa9417d1","full_name":"Julseth, Mara","first_name":"Mara","last_name":"Julseth"},{"full_name":"Brenner-Morton, Susan","first_name":"Susan","last_name":"Brenner-Morton"},{"full_name":"Gabitto, Mariano I.","first_name":"Mariano I.","last_name":"Gabitto"},{"last_name":"Dasen","first_name":"Jeremy S.","full_name":"Dasen, Jeremy S."},{"first_name":"Jay B.","full_name":"Bikoff, Jay B.","last_name":"Bikoff"},{"last_name":"Sweeney","orcid":"0000-0001-9242-5601","id":"56BE8254-C4F0-11E9-8E45-0B23E6697425","full_name":"Sweeney, Lora Beatrice Jaeger","first_name":"Lora Beatrice Jaeger"}],"citation":{"chicago":"Vijatovic, David, Florina Alexandra  Toma, Y Ignatyev, Zoe P Harrington, Christoph M Sommer, Robert Hauschild, Matthijs Geert Smits, et al. “Multifold Increase in Spinal Inhibitory Cell Types with Emergence of Limb Movement.” <i>Cell Reports</i>. Elsevier, 2026. <a href=\"https://doi.org/10.1016/j.celrep.2026.117227\">https://doi.org/10.1016/j.celrep.2026.117227</a>.","short":"D. Vijatovic, F.A. Toma, Y. Ignatyev, Z.P. Harrington, C.M. Sommer, R. Hauschild, M.G. Smits, M. Dalla Vecchia, A.J. Trevisan, P. Chapman, M. Julseth, S. Brenner-Morton, M.I. Gabitto, J.S. Dasen, J.B. Bikoff, L.B. Sweeney, Cell Reports 45 (2026).","ista":"Vijatovic D, Toma FA, Ignatyev Y, Harrington ZP, Sommer CM, Hauschild R, Smits MG, Dalla Vecchia M, Trevisan AJ, Chapman P, Julseth M, Brenner-Morton S, Gabitto MI, Dasen JS, Bikoff JB, Sweeney LB. 2026. Multifold increase in spinal inhibitory cell types with emergence of limb movement. Cell Reports. 45(4), 117227.","apa":"Vijatovic, D., Toma, F. A., Ignatyev, Y., Harrington, Z. P., Sommer, C. M., Hauschild, R., … Sweeney, L. B. (2026). Multifold increase in spinal inhibitory cell types with emergence of limb movement. <i>Cell Reports</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.celrep.2026.117227\">https://doi.org/10.1016/j.celrep.2026.117227</a>","ama":"Vijatovic D, Toma FA, Ignatyev Y, et al. Multifold increase in spinal inhibitory cell types with emergence of limb movement. <i>Cell Reports</i>. 2026;45(4). doi:<a href=\"https://doi.org/10.1016/j.celrep.2026.117227\">10.1016/j.celrep.2026.117227</a>","mla":"Vijatovic, David, et al. “Multifold Increase in Spinal Inhibitory Cell Types with Emergence of Limb Movement.” <i>Cell Reports</i>, vol. 45, no. 4, 117227, Elsevier, 2026, doi:<a href=\"https://doi.org/10.1016/j.celrep.2026.117227\">10.1016/j.celrep.2026.117227</a>.","ieee":"D. Vijatovic <i>et al.</i>, “Multifold increase in spinal inhibitory cell types with emergence of limb movement,” <i>Cell Reports</i>, vol. 45, no. 4. Elsevier, 2026."},"acknowledgement":"We would like to thank the members of the Sweeney Lab, Mario de Bono, Michael Forsthofer, Katharina Lust, and Meital Oren, for comments on the manuscript. We are also grateful to Tom Jessell and Chris Kintner for their scientific insight and mentorship during the conception of this project. It would also have not been possible without the technical support of the Aquatics and Imaging and Optics Facility support teams (ISTA). We thank Martin Estermann for preparing the initial draft of the graphical abstract and Niki Barolini for the final version. In addition, we thank our funding sources for providing the resources to do these experiments: GFF NÖ FTI Strategy Lower Austria dissertation grant FT121-D-046 (to D.V.), Horizon Europe ERC starting grant 101041551 (to Y.I., L.B.S., F.A.T., and D.V.), Special Research Program (SFB) of the Austrian Science Fund (FWF) project F7814-B (to L.B.S.), Austrian Science Fund (FWF) 10.55776/COE16 (to Y.I. and L.B.S.), NINDS 5R35NS116858 (to J.S.D.), CZI grant DAF2020-225401 (DOI) 10.37921/120055ratwvi (to R.H.), NIH grant R01NS123116 (to J.B.B.), American Lebanese Syrian Associated Charities (ALSAC) (to J.B.B.), German Academic Exchange Service (DAAD) IFI grant 57515251-91853472 (to Z.H.), and Project A.L.S. (to S.B.-M.).","ddc":["570"],"external_id":{"pmid":["41964955 "]},"intvolume":"        45","type":"journal_article","publication":"Cell Reports"},{"scopus_import":"1","file_date_updated":"2026-05-05T12:01:08Z","volume":13,"DOAJ_listed":"1","title":"Testing single-photon entanglement using self-referential measurements","language":[{"iso":"eng"}],"abstract":[{"lang":"eng","text":"Entanglement does not always require one particle per party. It was predicted some 30 years ago that a single photon traversing a beam splitter could violate a Bell inequality. Although initially debated, single-photon nonlocality was eventually demonstrated via homodyne measurements. Here, we present an alternate realization that avoids the complexity of homodyne measurements and potential loopholes in their implementation. We violate a Bell inequality by performing joint measurements on two copies of the same single-photon entangled state, where one photon acts as a phase reference for the other, making it self-referential. We observe CHSH parameters of 2.71 = 0.09 and 2.23 = 0.07, depending on the joint measurements implemented. This offers a perspective on single-photon nonlocality and a more accessible experimental route, potentially applicable to general mode-entangled states in diverse platforms."}],"day":"20","date_created":"2026-04-19T22:07:44Z","publication":"Optica","type":"journal_article","arxiv":1,"intvolume":"        13","acknowledgement":"European Union ERC (101071779 (GRAVITES)); European Union Horizon 2020 Research and Innovation Programme (899368 (EPIQUS)); European Union Horizon 2020 Research and Innovation Programme Marie Sklodowska-Curie (956071 (AppQInfo)); European Union HORIZON Europe Research and Innovation Programme (101135288 (EPIQUE)); FWF Austrian Science Fund (10.55776/COE1 (Quantum Science Austria), 10.55776/F71 (BeyondC), 10.55776/FG5 (Research Group 5)); United States Air Force Office of Scientific Research (FA9550-21-1-0355 (Q-Trust), FA8655-23-1-7063 (TIQI)).","citation":{"ieee":"D. Kun, K. T. Strömberg, B. Dakić, P. Walther, and L. A. Rozema, “Testing single-photon entanglement using self-referential measurements,” <i>Optica</i>, vol. 13, no. 4. Optica Publishing Group, pp. 745–751, 2026.","mla":"Kun, Daniel, et al. “Testing Single-Photon Entanglement Using Self-Referential Measurements.” <i>Optica</i>, vol. 13, no. 4, Optica Publishing Group, 2026, pp. 745–51, doi:<a href=\"https://doi.org/10.1364/OPTICA.586172\">10.1364/OPTICA.586172</a>.","apa":"Kun, D., Strömberg, K. T., Dakić, B., Walther, P., &#38; Rozema, L. A. (2026). Testing single-photon entanglement using self-referential measurements. <i>Optica</i>. Optica Publishing Group. <a href=\"https://doi.org/10.1364/OPTICA.586172\">https://doi.org/10.1364/OPTICA.586172</a>","ama":"Kun D, Strömberg KT, Dakić B, Walther P, Rozema LA. Testing single-photon entanglement using self-referential measurements. <i>Optica</i>. 2026;13(4):745-751. doi:<a href=\"https://doi.org/10.1364/OPTICA.586172\">10.1364/OPTICA.586172</a>","ista":"Kun D, Strömberg KT, Dakić B, Walther P, Rozema LA. 2026. Testing single-photon entanglement using self-referential measurements. Optica. 13(4), 745–751.","chicago":"Kun, Daniel, Karl T Strömberg, Borivoje Dakić, Philip Walther, and Lee A. Rozema. “Testing Single-Photon Entanglement Using Self-Referential Measurements.” <i>Optica</i>. Optica Publishing Group, 2026. <a href=\"https://doi.org/10.1364/OPTICA.586172\">https://doi.org/10.1364/OPTICA.586172</a>.","short":"D. Kun, K.T. Strömberg, B. Dakić, P. Walther, L.A. Rozema, Optica 13 (2026) 745–751."},"external_id":{"arxiv":["2511.21819"]},"ddc":["530"],"author":[{"first_name":"Daniel","full_name":"Kun, Daniel","last_name":"Kun"},{"full_name":"Strömberg, Karl T","first_name":"Karl T","id":"68011cd2-da32-11ee-a930-b2774c7aba5f","last_name":"Strömberg"},{"last_name":"Dakić","first_name":"Borivoje","full_name":"Dakić, Borivoje"},{"first_name":"Philip","full_name":"Walther, Philip","last_name":"Walther"},{"last_name":"Rozema","first_name":"Lee A.","full_name":"Rozema, Lee A."}],"page":"745-751","quality_controlled":"1","project":[{"name":"QUANTUM INFORMATION SYSTEMS BEYOND CLASSICAL CAPABILITIES / P5- Integration of Superconducting Quantum Circuits","grant_number":"F07105","_id":"bdb108fd-d553-11ed-ba76-83dc74a9864f"}],"doi":"10.1364/OPTICA.586172","_id":"21747","PlanS_conform":"1","date_published":"2026-04-20T00:00:00Z","month":"04","article_type":"original","publication_status":"published","date_updated":"2026-05-05T12:05:47Z","publisher":"Optica Publishing Group","oa":1,"department":[{"_id":"OnHo"}],"article_processing_charge":"Yes","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"publisher","publication_identifier":{"eissn":["2334-2536"]},"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"OA_type":"gold","file":[{"date_updated":"2026-05-05T12:01:08Z","success":1,"content_type":"application/pdf","file_size":858539,"access_level":"open_access","checksum":"f6e62a93f274e0c07197bf4e457eff31","creator":"dernst","file_id":"21799","relation":"main_file","date_created":"2026-05-05T12:01:08Z","file_name":"2026_Optica_Kun.pdf"}],"oa_version":"Published Version","status":"public","year":"2026","issue":"4","has_accepted_license":"1"}]
