--- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '21707' abstract: - lang: eng text: Structural and functional differences between brain hemispheres are a common feature of animal nervous systems with reduced bilateral asymmetry often linked to impaired cognitive performance. How neuronal left-right asymmetry is initiated and integrated into a bilaterally symmetrical ground pattern is poorly understood. Here, we show that the directional asymmetry of a Drosophila central brain circuit originates from axonal interactions of two types of bilateral pioneer neurons. Subsequent recruitment of neighboring neurons into the asymmetric neuropil primordium results in hemisphere-specific microcircuits. Circuit lateralization requires dynamic expression of the cell adhesion molecule Fasciclin 2 to maintain structural plasticity in axonal remodeling. Reduced circuit asymmetry following cell type–specific Fasciclin 2 manipulation affects adult brain function. These results reveal an unexpected degree of developmental plasticity of late-born Drosophila neurons in the formation of a circuit node via the lateralized recruitment of symmetric circuit components. acknowledgement: "We thank I. Salecker (Flybow), B. Altenhein (Fas2-Gal4Mz507), A. Nose (UAS-intra- and extra-Fas2::YFP), and C. S. Goodman (UAS-Fas2PEST+/−), as well as the Bloomington Stock Center for providing materials and fly stocks. We thank S. Waddell and the lab, especially B. Senapati, for providing the opportunity to conduct memory experiments at the CNCB, University of Oxford, and for supervision and discussions during this period. We also thank W. Kallina, S. Ilgerl, D. Bartel, A. Grimm, and A. Litin for technical support and the Hummel Lab for stimulating discussions and critical comments on the manuscript. We acknowledge the early exploratory work of A. Mattia, S. Trkulja, C. Schönherr, S. Bogner, B. Simpson, L. Tomasek, H. Roth, H. Vokač, R. Gredler, F. Kapelari, T. Kolarova, C. Ignitsch, Á. Bautista-Soldevila, and M. Kassem.\r\nThis research was funded by the University of Vienna, the Vienna Doctoral School Cognition, Behaviour and Neuroscience (uni:docs fellowship) (to J.W.M.) and by the Austrian Science Fund (FWF) (Cluster of Excellence Neuronal Circuits in Health and Disease, grant DOI 10.55776/COE16; https://www.fwf.ac.at/en/research-radar/10.55776/COE16) (to T.H.). For open access purposes, the author has applied a CC BY public copyright license to any author-accepted manuscript version arising from this submission." article_number: eaea6020 article_processing_charge: Yes article_type: original author: - first_name: Johann W. full_name: Markovitsch, Johann W. last_name: Markovitsch - first_name: Daniel full_name: Mitić, Daniel last_name: Mitić - first_name: Alisa full_name: Del Pilar Jiménez García, Alisa last_name: Del Pilar Jiménez García - first_name: Alsberga full_name: Zane, Alsberga id: 60f7509a-f652-11ea-9d86-b963d6490d7c last_name: Zane orcid: 0009-0003-0415-7603 - first_name: Sarah full_name: Kainz, Sarah last_name: Kainz - first_name: Rashmit full_name: Kaur, Rashmit last_name: Kaur - first_name: Thomas full_name: Hummel, Thomas last_name: Hummel citation: ama: Markovitsch JW, Mitić D, Del Pilar Jiménez García A, et al. Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity. Science Advances. 2026;12(13). doi:10.1126/sciadv.aea6020 apa: Markovitsch, J. W., Mitić, D., Del Pilar Jiménez García, A., Zane, A., Kainz, S., Kaur, R., & Hummel, T. (2026). Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity. Science Advances. American Association for the Advancement of Science. https://doi.org/10.1126/sciadv.aea6020 chicago: Markovitsch, Johann W., Daniel Mitić, Alisa Del Pilar Jiménez García, Alsberga Zane, Sarah Kainz, Rashmit Kaur, and Thomas Hummel. “Sequential Formation of Drosophila Circuit Asymmetry via Prolonged Structural Plasticity.” Science Advances. American Association for the Advancement of Science, 2026. https://doi.org/10.1126/sciadv.aea6020. ieee: J. W. Markovitsch et al., “Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity,” Science Advances, vol. 12, no. 13. American Association for the Advancement of Science, 2026. ista: Markovitsch JW, Mitić D, Del Pilar Jiménez García A, Zane A, Kainz S, Kaur R, Hummel T. 2026. Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity. Science Advances. 12(13), eaea6020. mla: Markovitsch, Johann W., et al. “Sequential Formation of Drosophila Circuit Asymmetry via Prolonged Structural Plasticity.” Science Advances, vol. 12, no. 13, eaea6020, American Association for the Advancement of Science, 2026, doi:10.1126/sciadv.aea6020. short: J.W. Markovitsch, D. Mitić, A. Del Pilar Jiménez García, A. Zane, S. Kainz, R. Kaur, T. Hummel, Science Advances 12 (2026). date_created: 2026-04-12T22:01:48Z date_published: 2026-03-27T00:00:00Z date_updated: 2026-05-04T09:18:06Z day: '27' ddc: - '570' department: - _id: MiSi - _id: GradSch doi: 10.1126/sciadv.aea6020 file: - access_level: open_access checksum: 3eed470fe73e53d2a8d55d6fba6934e3 content_type: application/pdf creator: dernst date_created: 2026-05-04T09:16:36Z date_updated: 2026-05-04T09:16:36Z file_id: '21786' file_name: 2026_ScienceAdv_Markovitsch.pdf file_size: 11101140 relation: main_file success: 1 file_date_updated: 2026-05-04T09:16:36Z has_accepted_license: '1' intvolume: ' 12' issue: '13' language: - iso: eng license: https://creativecommons.org/licenses/by/4.0/ month: '03' oa: 1 oa_version: Published Version publication: Science Advances publication_identifier: eissn: - 2375-2548 publication_status: published publisher: American Association for the Advancement of Science quality_controlled: '1' scopus_import: '1' status: public title: Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 12 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '21708' abstract: - lang: eng text: On October 4, 2023, a proglacial lake named the South Lhonak lake was the source of a catastrophic Glacier Lake Outburst Flood (GLOF) in the Teesta river basin area, resulting in 24 fatalities and leaving over 70 persons missing. The GLOF also destroyed 13 bridges and a major hydropower plant in the Chungthang region. Over 60,000 individuals in four districts of Sikkim were impacted by this GLOF event. This study examines the factors that led to the GLOF event. Our study shows that the cause of this GLOF was initiated by a landslide, that dumped a substantial amount (~ 38.31 million m3) of debris into the South Lhonak Lake. Furthermore, the glacier that was connected to the lake, lost a big chunk of ice mass (~ 7 million m3) due to calving. The combination of these two processes led to the collapse of the left lateral moraine that consequently generated flood waves which breached the terminal moraine dam of the lake. We recommend monitoring land subsidence and calving events for large proglacial lakes to prevent the disastrous consequences of such GLOFs in the future. acknowledgement: This work was carried out independently without the support of any funding agency or sponsors. The authors thank the SARPROZ team for providing an evaluation license for the MTInSAR processing software. article_number: '9741' article_processing_charge: Yes article_type: original author: - first_name: Litan Kumar full_name: Mohanty, Litan Kumar last_name: Mohanty - first_name: Prateek full_name: Gantayat, Prateek id: 02734268-3e8d-11ef-80a1-cec4a088d004 last_name: Gantayat - first_name: Ankur full_name: Dixit, Ankur last_name: Dixit - first_name: Manik full_name: Das Adhikari, Manik last_name: Das Adhikari - first_name: Rahul full_name: Biswas, Rahul last_name: Biswas - first_name: Vivek Kumar full_name: Singh, Vivek Kumar last_name: Singh citation: ama: Mohanty LK, GANTAYAT P, Dixit A, Das Adhikari M, Biswas R, Singh VK. Sequence of events that led to the South Lhonak lake outburst flood in Sikkim, India. Scientific Reports. 2026;16. doi:10.1038/s41598-026-35895-7 apa: Mohanty, L. K., GANTAYAT, P., Dixit, A., Das Adhikari, M., Biswas, R., & Singh, V. K. (2026). Sequence of events that led to the South Lhonak lake outburst flood in Sikkim, India. Scientific Reports. Springer Nature. https://doi.org/10.1038/s41598-026-35895-7 chicago: Mohanty, Litan Kumar, PRATEEK GANTAYAT, Ankur Dixit, Manik Das Adhikari, Rahul Biswas, and Vivek Kumar Singh. “Sequence of Events That Led to the South Lhonak Lake Outburst Flood in Sikkim, India.” Scientific Reports. Springer Nature, 2026. https://doi.org/10.1038/s41598-026-35895-7. ieee: L. K. Mohanty, P. GANTAYAT, A. Dixit, M. Das Adhikari, R. Biswas, and V. K. Singh, “Sequence of events that led to the South Lhonak lake outburst flood in Sikkim, India,” Scientific Reports, vol. 16. Springer Nature, 2026. ista: Mohanty LK, GANTAYAT P, Dixit A, Das Adhikari M, Biswas R, Singh VK. 2026. Sequence of events that led to the South Lhonak lake outburst flood in Sikkim, India. Scientific Reports. 16, 9741. mla: Mohanty, Litan Kumar, et al. “Sequence of Events That Led to the South Lhonak Lake Outburst Flood in Sikkim, India.” Scientific Reports, vol. 16, 9741, Springer Nature, 2026, doi:10.1038/s41598-026-35895-7. short: L.K. Mohanty, P. GANTAYAT, A. Dixit, M. Das Adhikari, R. Biswas, V.K. Singh, Scientific Reports 16 (2026). corr_author: '1' date_created: 2026-04-12T22:01:48Z date_published: 2026-03-24T00:00:00Z date_updated: 2026-05-04T07:54:53Z day: '24' ddc: - '550' department: - _id: FrPe doi: 10.1038/s41598-026-35895-7 external_id: pmid: - '41876546' file: - access_level: open_access checksum: cf13f61c38609ce6518d74562319c35f content_type: application/pdf creator: dernst date_created: 2026-05-04T07:24:59Z date_updated: 2026-05-04T07:24:59Z file_id: '21785' file_name: 2026_ScienceAdv_Mohanty.pdf file_size: 17406006 relation: main_file success: 1 file_date_updated: 2026-05-04T07:24:59Z has_accepted_license: '1' intvolume: ' 16' language: - iso: eng license: https://creativecommons.org/licenses/by-nc-nd/4.0/ month: '03' oa: 1 oa_version: Published Version pmid: 1 publication: Scientific Reports publication_identifier: eissn: - 2045-2322 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Sequence of events that led to the South Lhonak lake outburst flood in Sikkim, India tmp: image: /images/cc_by_nc_nd.png legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) short: CC BY-NC-ND (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 16 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '21709' abstract: - lang: eng text: 'JWST’s “little red dots” (LRDs) are increasingly interpreted as active galactic nuclei (AGN) obscured by dense thermalized gas rather than dust as evidenced by their X-ray weakness, blackbody-like continua, and Balmer line profiles. Key questions are how LRDs connect to standard UV-luminous AGN, whether transitional phases exist, and whether they are observable. We present the “X-ray dot” (XRD), a compact source at z = 3.28 observed by the NIRSpec Wide Guaranteed Time Observation survey. The XRD exhibits LRD hallmarks: a blackbody-like (Teff ≃ 6400 K) red continuum, a faint but blue rest-UV excess, falling mid-IR emission, and broad Balmer lines (FWHM ∼ 2700–3200 km s−1). Unlike LRDs, however, it is remarkably X-ray luminous (L2−10 keV = 1044.18 erg s−1) and has a continuum inflection that is blueward of the Balmer limit. We find that the red rest-optical and blue mid-IR continuum cannot be reproduced by standard dust-attenuated AGN models without invoking extremely steep extinction curves, nor can the weak mid-IR emission be reconciled with well-established X-ray–torus scaling relations. We therefore consider an alternative scenario: the XRD may be an LRD in transition, where the gas envelope dominates the optical continuum but optically thin sight lines allow X-rays to escape. The XRD may thus provide a physical link between LRDs and standard AGN, offering direct evidence that LRDs are powered by supermassive black holes and providing insight into their accretion properties.' acknowledgement: "We would like to thank the anonymous reviewer for their constructive comments, which improved the final manuscript.\r\n\r\nWe thank Bernd Husemann for his critical contributions to the NIRSpec Wide GTO survey, and in particular his help in selecting high-priority X-ray-luminous targets.\r\n\r\nR.E.H. acknowledges support by the German Aerospace Center (DLR) and the Federal Ministry for Economic Affairs and Energy (BMWi) through program 50OR2403 “RUBIES.” A.d.G. acknowledges support from a Clay Fellowship awarded by the Smithsonian Astrophysical Observatory. A.J.B. acknowledges funding from the “FirstGalaxies” Advanced grant from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement No. 789056). R.P.N. thanks Neil Pappalardo and Jane Pappalardo for their generous support of the MIT Pappalardo Fellowships in Physics. Support for this work was provided by the Brinson Foundation through a Brinson Prize Fellowship grant. H.Ü. acknowledges funding by the European Union (ERC APEX, 101164796). 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. G.V. acknowledges support from European Union’s HE ERC Starting grant No. 101040227—WINGS. B.W. acknowledges support provided by NASA through Hubble Fellowship grant HST-HF2-51592.001 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, In., for NASA, under the contract NAS 5-26555.\r\n\r\nThe data products presented herein were retrieved from the Dawn JWST Archive (DJA). DJA is an initiative of the Cosmic Dawn Center (DAWN).\r\n\r\nThis work is based in part on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with programs Nos. GTO-1213. The data described here may be obtained from the MAST archive at DOI: 10.17909/qffz-b324.\r\n\r\nThis Letter employs a list of Chandra datasets, obtained by the Chandra X-ray Observatory, contained in DOI: 10.25574/cdc.540.\r\n\r\nThis work is based on observations taken by the 3D-HST Treasury Program (GO 12177 and 12328) with the NASA/ESA HST, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.\r\n\r\nThis work makes use of color palettes created by Martin Krzywinski designed for colorblindness. The color palettes and more information can be found at http://mkweb.bcgsc.ca/colorblind/.\r\n\r\nFacilities: CXO - Chandra X-ray Observatory satellite (ACIS), HST - Hubble Space Telescope satellite (ACS, WFC3) - , CFHT - Canada-France-Hawaii Telescope (WIRCam), JWST - James Webb Space Telescope (NIRSpec), Spitzer - Spitzer Space Telescope satellite (IRAC, MIPS) - , JCMT - James Clerk Maxwell Telescope (SCUBA).\r\n\r\nSoftware: Astropy (Astropy Collaboration et al. 2013, 2018, 2022), dust_attenuation, dust_extinction (K. Gordon 2024), jax (J. Bradbury et al. 2018), LaTeX (L. Lamport 1994), Matplotlib (J. D. Hunter 2007), NumPy (T. E. Oliphant 2006; S. van der Walt et al. 2011; C. R. Harris et al. 2020), NumPyro (D. Phan et al. 2019), scipy (P. Virtanen et al. 2020), sedpy (B. Johnson & J. Leja 2017), specutils (Astropy-Specutils Development Team 2019), unite (R. E. Hviding 2025)." article_number: L18 article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: Raphael E. full_name: Hviding, Raphael E. last_name: Hviding - first_name: Anna full_name: De Graaff, Anna last_name: De Graaff - first_name: Hanpu full_name: Liu, Hanpu last_name: Liu - first_name: Andy D. full_name: Goulding, Andy D. last_name: Goulding - first_name: Yilun full_name: Ma, Yilun last_name: Ma - first_name: Jenny E. full_name: Greene, Jenny E. last_name: Greene - first_name: Leindert A. full_name: Boogaard, Leindert A. last_name: Boogaard - first_name: Andrew J. full_name: Bunker, Andrew J. last_name: Bunker - first_name: Nikko J. full_name: Cleri, Nikko J. last_name: Cleri - first_name: Marijn full_name: Franx, Marijn last_name: Franx - first_name: Michaela full_name: Hirschmann, Michaela last_name: Hirschmann - first_name: Joel full_name: Leja, Joel last_name: Leja - first_name: Jorryt J full_name: Matthee, Jorryt J id: 7439a258-f3c0-11ec-9501-9df22fe06720 last_name: Matthee orcid: 0000-0003-2871-127X - first_name: Rohan P. full_name: Naidu, Rohan P. last_name: Naidu - first_name: David J. full_name: Setton, David J. last_name: Setton - first_name: Hannah full_name: Übler, Hannah last_name: Übler - first_name: Giacomo full_name: Venturi, Giacomo last_name: Venturi - first_name: Bingjie full_name: Wang, Bingjie last_name: Wang citation: ama: 'Hviding RE, De Graaff A, Liu H, et al. The X-ray dot: Exotic dust or a late-stage Little Red Dot? The Astrophysical Journal Letters. 2026;1000(1). doi:10.3847/2041-8213/ae4c88' apa: 'Hviding, R. E., De Graaff, A., Liu, H., Goulding, A. D., Ma, Y., Greene, J. E., … Wang, B. (2026). The X-ray dot: Exotic dust or a late-stage Little Red Dot? The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/ae4c88' chicago: 'Hviding, Raphael E., Anna De Graaff, Hanpu Liu, Andy D. Goulding, Yilun Ma, Jenny E. Greene, Leindert A. Boogaard, et al. “The X-Ray Dot: Exotic Dust or a Late-Stage Little Red Dot?” The Astrophysical Journal Letters. IOP Publishing, 2026. https://doi.org/10.3847/2041-8213/ae4c88.' ieee: 'R. E. Hviding et al., “The X-ray dot: Exotic dust or a late-stage Little Red Dot?,” The Astrophysical Journal Letters, vol. 1000, no. 1. IOP Publishing, 2026.' ista: 'Hviding RE, De Graaff A, Liu H, Goulding AD, Ma Y, Greene JE, Boogaard LA, Bunker AJ, Cleri NJ, Franx M, Hirschmann M, Leja J, Matthee JJ, Naidu RP, Setton DJ, Übler H, Venturi G, Wang B. 2026. The X-ray dot: Exotic dust or a late-stage Little Red Dot? The Astrophysical Journal Letters. 1000(1), L18.' mla: 'Hviding, Raphael E., et al. “The X-Ray Dot: Exotic Dust or a Late-Stage Little Red Dot?” The Astrophysical Journal Letters, vol. 1000, no. 1, L18, IOP Publishing, 2026, doi:10.3847/2041-8213/ae4c88.' short: R.E. Hviding, A. De Graaff, H. Liu, A.D. Goulding, Y. Ma, J.E. Greene, L.A. Boogaard, A.J. Bunker, N.J. Cleri, M. Franx, M. Hirschmann, J. Leja, J.J. Matthee, R.P. Naidu, D.J. Setton, H. Übler, G. Venturi, B. Wang, The Astrophysical Journal Letters 1000 (2026). date_created: 2026-04-12T22:01:48Z date_published: 2026-03-20T00:00:00Z date_updated: 2026-05-04T07:13:07Z day: '20' ddc: - '520' department: - _id: JoMa doi: 10.3847/2041-8213/ae4c88 external_id: arxiv: - '2601.09778' file: - access_level: open_access checksum: 1be4f361bf59aa08b8c98ed4f475a463 content_type: application/pdf creator: dernst date_created: 2026-05-04T07:11:37Z date_updated: 2026-05-04T07:11:37Z file_id: '21784' file_name: 2026_AstrophysicalJourLetters_Hviding.pdf file_size: 2821786 relation: main_file success: 1 file_date_updated: 2026-05-04T07:11:37Z has_accepted_license: '1' intvolume: ' 1000' issue: '1' language: - iso: eng month: '03' oa: 1 oa_version: Published Version publication: The Astrophysical Journal Letters publication_identifier: eissn: - 2041-8213 issn: - 2041-8205 publication_status: published publisher: IOP Publishing quality_controlled: '1' scopus_import: '1' status: public title: 'The X-ray dot: Exotic dust or a late-stage Little Red Dot?' tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 1000 year: '2026' ... --- OA_place: publisher OA_type: gold _id: '21710' abstract: - lang: eng text: "Early results from JWST suggest that Epoch of Reionization (EoR) galaxies produce copious ionizing photons, which, if they escape efficiently, could cause reionization to occur too early. We study this problem using JWST imaging and prism spectroscopy for 412 galaxies at 4.5 < z < 9.0. We fit these data simultaneously with stellar population and nebular emission models that include a parameter for the fraction of ionizing photons that escape the galaxy, fesc. We find that the ionization production efficiency, ξion = Q(H0)/LUV, increases with redshift and decreasing UV luminosity, but shows significant scatter, (log ion z, MUV) 0.3 dex. The inferred escape fractions averaged over the population are low, ranging from〈fesc〉 ≃ 2.6% ± 1.4% at 6 < z < 9 to 6.5% ± 2.2% at 4.5 < z < 6, with weak or no indication of evolution with redshift. This implies that in our models most of the ionizing photons need to be absorbed to account for the nebular emission. We compute the impact of our results on reionization, including the distributions for ξion and fesc, and the evolution and uncertainty of the UV luminosity function. Considering galaxies brighter than MUV < −16 mag would produce an intergalactic medium hydrogen-ionized fraction of xe = 0.5 at 5.3 < z < 5.8, possibly too late compared to constraints from from quasistellar\r\nobject (QSO) sight lines. Including fainter galaxies, MUV < −14 mag, we obtain xe = 0.5 at 6.0 < z < 8.1, fully consistent with QSO and cosmic microwave background data. This implies that EoR galaxies produce plenty of ionizing photons, but that these do not efficiently escape. This may be a result of high gas column densities combined with burstier star formation histories, which limit the time massive stars are able to clear channels through the gas for ionizing photons to escape." acknowledgement: "We wish to thank our colleagues in the CEERS collaboration for their hard work and valuable contributions on this project. We extend our sincerest thanks to the anonymous referee whose critical and constructive report improved the quality of this manuscript. We also thank the JADES team for providing an excellent dataset for science. We with to thank colleagues for valuable discussions, feedback, and suggestions, including John Chisholm, Kevin Huffenberger, Jessica\r\nMeh, Julian Muñoz, Irene Shivaei, Justin Spilker, Aaron Smith, and Romain Teyssier.\r\nPortions of this research were conducted with the advanced computing resources provided by Texas A&M High Performance Research Computing (HPRC, http://hprc.tamu.edu). This work benefited from support from the George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University. CP thanks Marsha and Ralph Schilling for generous support of this research. This work was partially support by the Future Investigators in NASA Earth and Space Science and Technology (FINESST) program grant No. 80NSSC23K1487. R.A. acknowledges support of grant PID2023-147386NB-I00 funded by MICIU/AEI/10.13039/501100011033 and by ERDF/EU, and the Severo Ochoa grant CEX2021-001131-S funded by MCIN/AEI/10.13039/50110001103. A.C.C. acknowledges support from a UKRI Frontier Research Guarantee Grant (PI Carnall; grant reference EP/Y037065/1) This work acknowledges support from the NASA/ESA/CSA James Webb Space Telescope through the\r\nSpace Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-03127. Support for program JWST-ERS-01345.009-A, JWST-GO-02079.013-A, JWST-GO-06368.011-A, and JWST-GO-01837.030-A, was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127. This work made use of v2.2 of the Binary Population\r\nand Spectral Synthesis (BPASS) models as described in E. R. Stanway & J. J. Eldridge (2018)." article_number: '111' article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: Casey full_name: Papovich, Casey last_name: Papovich - first_name: Justin W. full_name: Cole, Justin W. last_name: Cole - first_name: Weida full_name: Hu, Weida last_name: Hu - first_name: Steven L. full_name: Finkelstein, Steven L. last_name: Finkelstein - first_name: Lu full_name: Shen, Lu last_name: Shen - first_name: Pablo full_name: Arrabal Haro, Pablo last_name: Arrabal Haro - first_name: Ricardo O. full_name: Amorín, Ricardo O. last_name: Amorín - first_name: Bren E. full_name: Backhaus, Bren E. last_name: Backhaus - first_name: Micaela B. full_name: Bagley, Micaela B. last_name: Bagley - first_name: Rachana full_name: Bhatawdekar, Rachana last_name: Bhatawdekar - first_name: Antonello full_name: Calabrò, Antonello last_name: Calabrò - first_name: Adam C. full_name: Carnall, Adam C. last_name: Carnall - first_name: Nikko J. full_name: Cleri, Nikko J. last_name: Cleri - first_name: Emanuele full_name: Daddi, Emanuele last_name: Daddi - first_name: Mark full_name: Dickinson, Mark last_name: Dickinson - first_name: Norman A. full_name: Grogin, Norman A. last_name: Grogin - first_name: Benne W. full_name: Holwerda, Benne W. last_name: Holwerda - first_name: Anne E. full_name: Jaskot, Anne E. last_name: Jaskot - first_name: Anton M. full_name: Koekemoer, Anton M. last_name: Koekemoer - first_name: Mario full_name: Llerena, Mario last_name: Llerena - first_name: Ray A. full_name: Lucas, Ray A. last_name: Lucas - first_name: Sara full_name: Mascia, Sara id: edaf889c-c7cd-11ef-ab1b-bb28c431bd29 last_name: Mascia - first_name: Fabio full_name: Pacucci, Fabio last_name: Pacucci - first_name: Laura full_name: Pentericci, Laura last_name: Pentericci - first_name: Pablo G. full_name: Pérez-González, Pablo G. last_name: Pérez-González - first_name: Nor full_name: Pirzkal, Nor last_name: Pirzkal - first_name: Srinivasan full_name: Raghunathan, Srinivasan last_name: Raghunathan - first_name: Lise Marie full_name: Seillé, Lise Marie last_name: Seillé - first_name: Rachel S. full_name: Somerville, Rachel S. last_name: Somerville - first_name: L. Y.Aaron full_name: Yung, L. Y.Aaron last_name: Yung citation: ama: Papovich C, Cole JW, Hu W, et al. Galaxies in the epoch of reionization are all bark and no bite-plenty of ionizing photons, low escape fractions. The Astrophysical Journal. 2026;1000(1). doi:10.3847/1538-4357/ae3b25 apa: Papovich, C., Cole, J. W., Hu, W., Finkelstein, S. L., Shen, L., Arrabal Haro, P., … Yung, L. Y. A. (2026). Galaxies in the epoch of reionization are all bark and no bite-plenty of ionizing photons, low escape fractions. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ae3b25 chicago: Papovich, Casey, Justin W. Cole, Weida Hu, Steven L. Finkelstein, Lu Shen, Pablo Arrabal Haro, Ricardo O. Amorín, et al. “Galaxies in the Epoch of Reionization Are All Bark and No Bite-Plenty of Ionizing Photons, Low Escape Fractions.” The Astrophysical Journal. IOP Publishing, 2026. https://doi.org/10.3847/1538-4357/ae3b25. ieee: C. Papovich et al., “Galaxies in the epoch of reionization are all bark and no bite-plenty of ionizing photons, low escape fractions,” The Astrophysical Journal, vol. 1000, no. 1. IOP Publishing, 2026. ista: Papovich C, Cole JW, Hu W, Finkelstein SL, Shen L, Arrabal Haro P, Amorín RO, Backhaus BE, Bagley MB, Bhatawdekar R, Calabrò A, Carnall AC, Cleri NJ, Daddi E, Dickinson M, Grogin NA, Holwerda BW, Jaskot AE, Koekemoer AM, Llerena M, Lucas RA, Mascia S, Pacucci F, Pentericci L, Pérez-González PG, Pirzkal N, Raghunathan S, Seillé LM, Somerville RS, Yung LYA. 2026. Galaxies in the epoch of reionization are all bark and no bite-plenty of ionizing photons, low escape fractions. The Astrophysical Journal. 1000(1), 111. mla: Papovich, Casey, et al. “Galaxies in the Epoch of Reionization Are All Bark and No Bite-Plenty of Ionizing Photons, Low Escape Fractions.” The Astrophysical Journal, vol. 1000, no. 1, 111, IOP Publishing, 2026, doi:10.3847/1538-4357/ae3b25. short: C. Papovich, J.W. Cole, W. Hu, S.L. Finkelstein, L. Shen, P. Arrabal Haro, R.O. Amorín, B.E. Backhaus, M.B. Bagley, R. Bhatawdekar, A. Calabrò, A.C. Carnall, N.J. Cleri, E. Daddi, M. Dickinson, N.A. Grogin, B.W. Holwerda, A.E. Jaskot, A.M. Koekemoer, M. Llerena, R.A. Lucas, S. Mascia, F. Pacucci, L. Pentericci, P.G. Pérez-González, N. Pirzkal, S. Raghunathan, L.M. Seillé, R.S. Somerville, L.Y.A. Yung, The Astrophysical Journal 1000 (2026). date_created: 2026-04-12T22:01:49Z date_published: 2026-03-20T00:00:00Z date_updated: 2026-05-04T10:44:57Z day: '20' ddc: - '520' department: - _id: JoMa doi: 10.3847/1538-4357/ae3b25 external_id: arxiv: - '2505.08870' file: - access_level: open_access checksum: 0031a6f197a3fa8c2845de10b6bdc696 content_type: application/pdf creator: dernst date_created: 2026-05-04T10:40:07Z date_updated: 2026-05-04T10:40:07Z file_id: '21791' file_name: 2026_AstrophysicalJour_Papovich.pdf file_size: 6670398 relation: main_file success: 1 file_date_updated: 2026-05-04T10:40:07Z has_accepted_license: '1' intvolume: ' 1000' issue: '1' language: - iso: eng month: '03' oa: 1 oa_version: Published Version publication: The Astrophysical Journal publication_identifier: eissn: - 1538-4357 issn: - 0004-637X publication_status: published publisher: IOP Publishing quality_controlled: '1' scopus_import: '1' status: public title: Galaxies in the epoch of reionization are all bark and no bite-plenty of ionizing photons, low escape fractions tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 1000 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold PlanS_conform: '1' _id: '21711' abstract: - lang: eng text: 'Background: Low-volume trapping columns are essential for sample enrichment, desalting, and injection profile focusing on nano-LC–MS-based proteomics. They enable higher sample loading, improve chromatographic performance, and protect the analytical column by removing salts and contaminants. Recently, monolithic trap columns with micropillar architecture have emerged as alternatives to conventionally packed traps. This study compares the performance of a packed and a micropillar monolithic trap column for the analysis of tryptic peptides. Methods: A tryptic digest of HeLa cell lysate was analyzed under identical LC–MS conditions using both trap types. Peptides were detected at 214 nm and analyzed by nano-ESI on a Q Exactive Plus Orbitrap. Data were searched against the human UniProt database (February 2023) using FragPipe v20.0, and statistical evaluation of MaxLFQ intensities was performed in Perseus using Welch’s t-test and clustering analysis. Results: Over 2500 proteins were identified with both setups. The packed trap column yielded more total peptides, particularly those with post-translational modifications and higher hydrophilicity, whereas the monolithic column favored peptides of intermediate hydrophobicity. Chromatographic profiles confirmed a slight reduction in the trapping efficiency of hydrophilic peptides by the monolithic trap. Conclusions: Trap column design significantly influences peptide recovery and proteome coverage.' acknowledgement: 'The authors thank Gábor Tóth, Uppsala University, Sweden, and Armel Nicolas, Institute for Science and Technology Austria, for their support. This research was conducted during a student residency in Vienna under the auspices of OeAD. ZI: ICM-2016-03196.' article_number: '10' article_processing_charge: Yes article_type: original author: - first_name: Jadranka full_name: Miletić Vukajlović, Jadranka last_name: Miletić Vukajlović - first_name: Bojana full_name: Ilić, Bojana last_name: Ilić - first_name: Bella full_name: Bruszel, Bella id: 70abbbb3-88ea-11ec-8e0a-e8c939944834 last_name: Bruszel - first_name: Tanja full_name: Panić-Janković, Tanja last_name: Panić-Janković - first_name: Goran full_name: Mitulović, Goran last_name: Mitulović citation: ama: Miletić Vukajlović J, Ilić B, Bruszel B, Panić-Janković T, Mitulović G. Comparison of the trapping efficiency for tryptic peptides on particle-packed and micro-pillar trap columns for proteomics analyses. Proteomes. 2026;14(1). doi:10.3390/proteomes14010010 apa: Miletić Vukajlović, J., Ilić, B., Bruszel, B., Panić-Janković, T., & Mitulović, G. (2026). Comparison of the trapping efficiency for tryptic peptides on particle-packed and micro-pillar trap columns for proteomics analyses. Proteomes. MDPI. https://doi.org/10.3390/proteomes14010010 chicago: Miletić Vukajlović, Jadranka, Bojana Ilić, Bella Bruszel, Tanja Panić-Janković, and Goran Mitulović. “Comparison of the Trapping Efficiency for Tryptic Peptides on Particle-Packed and Micro-Pillar Trap Columns for Proteomics Analyses.” Proteomes. MDPI, 2026. https://doi.org/10.3390/proteomes14010010. ieee: J. Miletić Vukajlović, B. Ilić, B. Bruszel, T. Panić-Janković, and G. Mitulović, “Comparison of the trapping efficiency for tryptic peptides on particle-packed and micro-pillar trap columns for proteomics analyses,” Proteomes, vol. 14, no. 1. MDPI, 2026. ista: Miletić Vukajlović J, Ilić B, Bruszel B, Panić-Janković T, Mitulović G. 2026. Comparison of the trapping efficiency for tryptic peptides on particle-packed and micro-pillar trap columns for proteomics analyses. Proteomes. 14(1), 10. mla: Miletić Vukajlović, Jadranka, et al. “Comparison of the Trapping Efficiency for Tryptic Peptides on Particle-Packed and Micro-Pillar Trap Columns for Proteomics Analyses.” Proteomes, vol. 14, no. 1, 10, MDPI, 2026, doi:10.3390/proteomes14010010. short: J. Miletić Vukajlović, B. Ilić, B. Bruszel, T. Panić-Janković, G. Mitulović, Proteomes 14 (2026). date_created: 2026-04-12T22:01:49Z date_published: 2026-03-01T00:00:00Z date_updated: 2026-05-04T10:36:21Z day: '01' ddc: - '540' department: - _id: MassSpec doi: 10.3390/proteomes14010010 external_id: pmid: - '41893725' file: - access_level: open_access checksum: 1e0c66bbf4b6e0be626a8639ea664b63 content_type: application/pdf creator: dernst date_created: 2026-05-04T10:31:35Z date_updated: 2026-05-04T10:31:35Z file_id: '21790' file_name: 2026_Proteomes_Vukajlovic.pdf file_size: 1009723 relation: main_file success: 1 file_date_updated: 2026-05-04T10:31:35Z has_accepted_license: '1' intvolume: ' 14' issue: '1' language: - iso: eng month: '03' oa: 1 oa_version: Published Version pmid: 1 publication: Proteomes publication_identifier: eissn: - 2227-7382 publication_status: published publisher: MDPI quality_controlled: '1' scopus_import: '1' status: public title: Comparison of the trapping efficiency for tryptic peptides on particle-packed and micro-pillar trap columns for proteomics analyses tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 14 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '21712' 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. 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. article_number: '316' article_processing_charge: Yes article_type: original author: - first_name: Allison full_name: Lin, Allison last_name: Lin - first_name: Maria full_name: Charisi, Maria last_name: Charisi - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman orcid: 0000-0003-3633-5403 citation: ama: Lin A, Charisi M, Haiman Z. Lomb-scargle periodogram struggles with non-sinusoidal supermassive Black Hole binary signatures in quasar lightcurves. The Astrophysical Journal. 2026;997(2). doi:10.3847/1538-4357/ae29a7 apa: 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. IOP Publishing. https://doi.org/10.3847/1538-4357/ae29a7 chicago: Lin, Allison, Maria Charisi, and Zoltán Haiman. “Lomb-Scargle Periodogram Struggles with Non-Sinusoidal Supermassive Black Hole Binary Signatures in Quasar Lightcurves.” The Astrophysical Journal. IOP Publishing, 2026. https://doi.org/10.3847/1538-4357/ae29a7. ieee: A. Lin, M. Charisi, and Z. Haiman, “Lomb-scargle periodogram struggles with non-sinusoidal supermassive Black Hole binary signatures in quasar lightcurves,” The Astrophysical Journal, vol. 997, no. 2. IOP Publishing, 2026. 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. mla: Lin, Allison, et al. “Lomb-Scargle Periodogram Struggles with Non-Sinusoidal Supermassive Black Hole Binary Signatures in Quasar Lightcurves.” The Astrophysical Journal, vol. 997, no. 2, 316, IOP Publishing, 2026, doi:10.3847/1538-4357/ae29a7. short: A. Lin, M. Charisi, Z. Haiman, The Astrophysical Journal 997 (2026). date_created: 2026-04-12T22:01:49Z date_published: 2026-02-01T00:00:00Z date_updated: 2026-05-04T10:26:59Z day: '01' ddc: - '520' department: - _id: ZoHa doi: 10.3847/1538-4357/ae29a7 file: - access_level: open_access checksum: 5162d1539ef7d10927ef73d8b4500017 content_type: application/pdf creator: dernst date_created: 2026-05-04T10:24:49Z date_updated: 2026-05-04T10:24:49Z file_id: '21789' file_name: 2026_AstrophysicalJour_Lin.pdf file_size: 2619679 relation: main_file success: 1 file_date_updated: 2026-05-04T10:24:49Z has_accepted_license: '1' intvolume: ' 997' issue: '2' language: - iso: eng month: '02' oa: 1 oa_version: Published Version publication: The Astrophysical Journal publication_identifier: eissn: - 1538-4357 issn: - 0004-637X publication_status: published publisher: IOP Publishing quality_controlled: '1' scopus_import: '1' status: public title: Lomb-scargle periodogram struggles with non-sinusoidal supermassive Black Hole binary signatures in quasar lightcurves tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 997 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '21713' 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. 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. article_number: L44 article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: Imre full_name: Bartos, Imre last_name: Bartos - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman orcid: 0000-0003-3633-5403 citation: ama: 'Bartos I, Haiman Z. Accretion is all you need: Black Hole spin alignment in merger GW231123 indicates accretion pathway. The Astrophysical Journal Letters. 2026;996(2). doi:10.3847/2041-8213/ae2bff' apa: 'Bartos, I., & Haiman, Z. (2026). Accretion is all you need: Black Hole spin alignment in merger GW231123 indicates accretion pathway. The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/ae2bff' chicago: 'Bartos, Imre, and Zoltán Haiman. “Accretion Is All You Need: Black Hole Spin Alignment in Merger GW231123 Indicates Accretion Pathway.” The Astrophysical Journal Letters. IOP Publishing, 2026. https://doi.org/10.3847/2041-8213/ae2bff.' ieee: 'I. Bartos and Z. Haiman, “Accretion is all you need: Black Hole spin alignment in merger GW231123 indicates accretion pathway,” The Astrophysical Journal Letters, vol. 996, no. 2. IOP Publishing, 2026.' 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.' mla: 'Bartos, Imre, and Zoltán Haiman. “Accretion Is All You Need: Black Hole Spin Alignment in Merger GW231123 Indicates Accretion Pathway.” The Astrophysical Journal Letters, vol. 996, no. 2, L44, IOP Publishing, 2026, doi:10.3847/2041-8213/ae2bff.' short: I. Bartos, Z. Haiman, The Astrophysical Journal Letters 996 (2026). corr_author: '1' date_created: 2026-04-12T22:01:49Z date_published: 2026-01-10T00:00:00Z date_updated: 2026-05-04T09:54:18Z day: '10' ddc: - '520' department: - _id: ZoHa doi: 10.3847/2041-8213/ae2bff external_id: arxiv: - '2508.08558' file: - access_level: open_access checksum: ac46ba3d13f0150ccbc42665bed3ae47 content_type: application/pdf creator: dernst date_created: 2026-05-04T09:49:53Z date_updated: 2026-05-04T09:49:53Z file_id: '21788' file_name: 2026_AstrophysicalJourLetters_Bartos.pdf file_size: 866725 relation: main_file success: 1 file_date_updated: 2026-05-04T09:49:53Z has_accepted_license: '1' intvolume: ' 996' issue: '2' language: - iso: eng month: '01' oa: 1 oa_version: Published Version publication: The Astrophysical Journal Letters publication_identifier: eissn: - 2041-8213 issn: - 2041-8205 publication_status: published publisher: IOP Publishing quality_controlled: '1' scopus_import: '1' status: public title: 'Accretion is all you need: Black Hole spin alignment in merger GW231123 indicates accretion pathway' tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 996 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '21714' 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. 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. article_number: L42 article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: Zhenwei full_name: Li, Zhenwei last_name: Li - first_name: Shi full_name: Jia, Shi last_name: Jia - first_name: Dandan full_name: Wei, Dandan id: 5dd129bd-0601-11ef-b325-833284687b76 last_name: Wei - first_name: Hongwei full_name: Ge, Hongwei last_name: Ge - first_name: Hailiang full_name: Chen, Hailiang last_name: Chen - first_name: Yangyang full_name: Zhang, Yangyang last_name: Zhang - first_name: Xuefei full_name: Chen, Xuefei last_name: Chen - first_name: Zhanwen full_name: Han, Zhanwen last_name: Han citation: ama: 'Li Z, Jia S, Wei D, et al. Formation of Be stars via wind accretion: Case study on Black Hole + Be star binaries. The Astrophysical Journal Letters. 2026;996(2). doi:10.3847/2041-8213/ae3008' 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. The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/ae3008' 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.” The Astrophysical Journal Letters. IOP Publishing, 2026. https://doi.org/10.3847/2041-8213/ae3008.' ieee: 'Z. Li et al., “Formation of Be stars via wind accretion: Case study on Black Hole + Be star binaries,” The Astrophysical Journal Letters, vol. 996, no. 2. IOP Publishing, 2026.' 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.' mla: 'Li, Zhenwei, et al. “Formation of Be Stars via Wind Accretion: Case Study on Black Hole + Be Star Binaries.” The Astrophysical Journal Letters, vol. 996, no. 2, L42, IOP Publishing, 2026, doi:10.3847/2041-8213/ae3008.' short: Z. Li, S. Jia, D. Wei, H. Ge, H. Chen, Y. Zhang, X. Chen, Z. Han, The Astrophysical Journal Letters 996 (2026). date_created: 2026-04-12T22:01:50Z date_published: 2026-01-10T00:00:00Z date_updated: 2026-04-16T06:26:18Z day: '10' ddc: - '520' department: - _id: YlGo doi: 10.3847/2041-8213/ae3008 external_id: arxiv: - '2512.18565' file: - access_level: open_access checksum: 09200c1cf405101abdd298ce80c9a90d content_type: application/pdf creator: dernst date_created: 2026-04-16T06:24:30Z date_updated: 2026-04-16T06:24:30Z file_id: '21741' file_name: 2026_AstrophysicalJourLetters_Li.pdf file_size: 5202345 relation: main_file success: 1 file_date_updated: 2026-04-16T06:24:30Z has_accepted_license: '1' intvolume: ' 996' issue: '2' language: - iso: eng month: '01' oa: 1 oa_version: Published Version publication: The Astrophysical Journal Letters publication_identifier: eissn: - 2041-8213 issn: - 2041-8205 publication_status: published publisher: IOP Publishing quality_controlled: '1' scopus_import: '1' status: public title: 'Formation of Be stars via wind accretion: Case study on Black Hole + Be star binaries' tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 996 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold PlanS_conform: '1' _id: '21715' abstract: - lang: eng 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. 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.”" article_number: '129' article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: Jenny E. full_name: Greene, Jenny E. last_name: Greene - first_name: David J. full_name: Setton, David J. last_name: Setton - first_name: Lukas J. full_name: Furtak, Lukas J. last_name: Furtak - first_name: Rohan P. full_name: Naidu, Rohan P. last_name: Naidu - first_name: Marta full_name: Volonteri, Marta last_name: Volonteri - first_name: Pratika full_name: Dayal, Pratika last_name: Dayal - first_name: Ivo full_name: Labbe, Ivo last_name: Labbe - first_name: Pieter full_name: Van Dokkum, Pieter last_name: Van Dokkum - first_name: Rachel full_name: Bezanson, Rachel last_name: Bezanson - first_name: Gabriel full_name: Brammer, Gabriel last_name: Brammer - first_name: Sam E. full_name: Cutler, Sam E. last_name: Cutler - first_name: Karl full_name: Glazebrook, Karl last_name: Glazebrook - first_name: Anna full_name: De Graaff, Anna last_name: De Graaff - first_name: Michaela full_name: Hirschmann, Michaela last_name: Hirschmann - first_name: Raphael E. full_name: Hviding, Raphael E. last_name: Hviding - first_name: Vasily full_name: Kokorev, Vasily last_name: Kokorev - first_name: Joel full_name: Leja, Joel last_name: Leja - first_name: Hanpu full_name: Liu, Hanpu last_name: Liu - first_name: Yilun full_name: Ma, Yilun last_name: Ma - first_name: Jorryt J full_name: Matthee, Jorryt J id: 7439a258-f3c0-11ec-9501-9df22fe06720 last_name: Matthee orcid: 0000-0003-2871-127X - first_name: Themiya full_name: Nanayakkara, Themiya last_name: Nanayakkara - first_name: Pascal A. full_name: Oesch, Pascal A. last_name: Oesch - first_name: Richard full_name: Pan, 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 - first_name: Bingjie full_name: Wang, Bingjie last_name: Wang - first_name: John R. full_name: Weaver, John R. last_name: Weaver - first_name: Katherine E. full_name: Whitaker, Katherine E. last_name: Whitaker - first_name: Christina C. full_name: Williams, Christina C. last_name: Williams - first_name: Adi full_name: Zitrin, Adi last_name: Zitrin 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. The Astrophysical Journal. 2026;996(2). doi:10.3847/1538-4357/ae1836' 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. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ae1836' 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.” The Astrophysical Journal. IOP Publishing, 2026. https://doi.org/10.3847/1538-4357/ae1836.' ieee: 'J. E. Greene et al., “What you see is what you get: Empirically measured bolometric luminosities of Little Red Dots,” The Astrophysical Journal, vol. 996, no. 2. IOP Publishing, 2026.' 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.' mla: 'Greene, Jenny E., et al. “What You See Is What You Get: Empirically Measured Bolometric Luminosities of Little Red Dots.” The Astrophysical Journal, vol. 996, no. 2, 129, IOP Publishing, 2026, doi:10.3847/1538-4357/ae1836.' 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). date_created: 2026-04-12T22:01:50Z date_published: 2026-01-10T00:00:00Z date_updated: 2026-05-04T11:20:42Z day: '10' ddc: - '520' department: - _id: JoMa doi: 10.3847/1538-4357/ae1836 external_id: arxiv: - '2509.05434' file: - access_level: open_access checksum: 7b3cb025d4bcaa35c6e52bd0c8fb6cf4 content_type: application/pdf creator: dernst date_created: 2026-05-04T11:19:48Z date_updated: 2026-05-04T11:19:48Z file_id: '21792' file_name: 2026_AstrophysicalJour_Greene.pdf file_size: 684400 relation: main_file success: 1 file_date_updated: 2026-05-04T11:19:48Z has_accepted_license: '1' intvolume: ' 996' issue: '2' language: - iso: eng month: '01' oa: 1 oa_version: Published Version project: - _id: bd9b2118-d553-11ed-ba76-db24564edfea grant_number: '101076224' name: Young galaxies as tracers and agents of cosmic reionization publication: The Astrophysical Journal publication_identifier: eissn: - 1538-4357 issn: - 0004-637X publication_status: published publisher: IOP Publishing quality_controlled: '1' scopus_import: '1' status: public title: 'What you see is what you get: Empirically measured bolometric luminosities of Little Red Dots' tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 996 year: '2026' ... --- OA_place: publisher OA_type: hybrid PlanS_conform: '1' _id: '21716' abstract: - lang: eng 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. acknowledgement: This work was supported by JSPS KAKENHI (grant number JP22J01430) and the Osamu Hayaishi Memorial Scholarship for Study Abroad for H.N. article_number: '102881' article_processing_charge: Yes (via OA deal) article_type: original author: - first_name: Hiroki full_name: Nagai, Hiroki id: 608df3e6-e2ab-11ed-8890-c9318cec7da4 last_name: Nagai orcid: 0000-0003-1671-9434 - first_name: Xiaoqi full_name: Feng, Xiaoqi id: e0164712-22ee-11ed-b12a-d80fcdf35958 last_name: Feng orcid: 0000-0002-4008-1234 citation: ama: NAGAI H, Feng X. Genetic and epigenetic mechanisms underlying male reproductive thermotolerance. Current Opinion in Plant Biology. 2026;91(6). doi:10.1016/j.pbi.2026.102881 apa: NAGAI, H., & Feng, X. (2026). Genetic and epigenetic mechanisms underlying male reproductive thermotolerance. Current Opinion in Plant Biology. Elsevier. https://doi.org/10.1016/j.pbi.2026.102881 chicago: NAGAI, HIROKI, and Xiaoqi Feng. “Genetic and Epigenetic Mechanisms Underlying Male Reproductive Thermotolerance.” Current Opinion in Plant Biology. Elsevier, 2026. https://doi.org/10.1016/j.pbi.2026.102881. ieee: H. NAGAI and X. Feng, “Genetic and epigenetic mechanisms underlying male reproductive thermotolerance,” Current Opinion in Plant Biology, vol. 91, no. 6. Elsevier, 2026. ista: NAGAI H, Feng X. 2026. Genetic and epigenetic mechanisms underlying male reproductive thermotolerance. Current Opinion in Plant Biology. 91(6), 102881. mla: NAGAI, HIROKI, and Xiaoqi Feng. “Genetic and Epigenetic Mechanisms Underlying Male Reproductive Thermotolerance.” Current Opinion in Plant Biology, vol. 91, no. 6, 102881, Elsevier, 2026, doi:10.1016/j.pbi.2026.102881. short: H. NAGAI, X. Feng, Current Opinion in Plant Biology 91 (2026). corr_author: '1' date_created: 2026-04-12T22:01:50Z date_published: 2026-04-01T00:00:00Z date_updated: 2026-05-04T11:15:57Z day: '01' ddc: - '580' department: - _id: XiFe doi: 10.1016/j.pbi.2026.102881 has_accepted_license: '1' intvolume: ' 91' issue: '6' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1016/j.pbi.2026.102881 month: '04' oa: 1 oa_version: Published Version publication: Current Opinion in Plant Biology publication_identifier: eissn: - 1879-0356 issn: - 1369-5266 publication_status: epub_ahead publisher: Elsevier quality_controlled: '1' scopus_import: '1' status: public title: Genetic and epigenetic mechanisms underlying male reproductive thermotolerance tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 91 year: '2026' ... --- OA_place: repository OA_type: green _id: '21717' 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. 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. article_processing_charge: No arxiv: 1 author: - first_name: Ali full_name: Asadi, Ali id: 02d96aae-000e-11ec-b801-cadd0a5eefbb last_name: Asadi - first_name: Krishnendu full_name: Chatterjee, Krishnendu id: 2E5DCA20-F248-11E8-B48F-1D18A9856A87 last_name: Chatterjee orcid: 0000-0002-4561-241X - first_name: Ehsan full_name: Kafshdar Goharshadi, Ehsan id: 103b4fa0-896a-11ed-bdf8-87b697bef40d last_name: Kafshdar Goharshadi orcid: 0000-0002-8595-0587 - first_name: Mehrdad full_name: Karrabi, Mehrdad id: 67638922-f394-11eb-9cf6-f20423e08757 last_name: Karrabi orcid: 0009-0007-5253-9170 - first_name: Ali full_name: Shafiee, Ali id: 2783031a-7378-11f0-b2d0-f17f1db2ebad last_name: Shafiee citation: ama: 'Asadi A, Chatterjee K, Goharshady E, Karrabi M, Shafiee A. Qualitative analysis of ω-regular objectives on robust MDPs. In: Proceedings of the 40th AAAI Conference on Artificial Intelligence. Vol 40. Association for the Advancement of Artificial Intelligence; 2026:36137-36145. doi:10.1609/aaai.v40i43.40931' apa: 'Asadi, A., Chatterjee, K., Goharshady, E., Karrabi, M., & Shafiee, A. (2026). Qualitative analysis of ω-regular objectives on robust MDPs. In Proceedings of the 40th AAAI Conference on Artificial Intelligence (Vol. 40, pp. 36137–36145). Singapore, Singapore: Association for the Advancement of Artificial Intelligence. https://doi.org/10.1609/aaai.v40i43.40931' chicago: Asadi, Ali, Krishnendu Chatterjee, Ehsan Goharshady, Mehrdad Karrabi, and Ali Shafiee. “Qualitative Analysis of ω-Regular Objectives on Robust MDPs.” In Proceedings of the 40th AAAI Conference on Artificial Intelligence, 40:36137–45. Association for the Advancement of Artificial Intelligence, 2026. https://doi.org/10.1609/aaai.v40i43.40931. ieee: A. Asadi, K. Chatterjee, E. Goharshady, M. Karrabi, and A. Shafiee, “Qualitative analysis of ω-regular objectives on robust MDPs,” in Proceedings of the 40th AAAI Conference on Artificial Intelligence, Singapore, Singapore, 2026, vol. 40, no. 43, pp. 36137–36145. 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.' mla: Asadi, Ali, et al. “Qualitative Analysis of ω-Regular Objectives on Robust MDPs.” Proceedings of the 40th AAAI Conference on Artificial Intelligence, vol. 40, no. 43, Association for the Advancement of Artificial Intelligence, 2026, pp. 36137–45, doi:10.1609/aaai.v40i43.40931. 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. conference: end_date: 2026-01-27 location: Singapore, Singapore name: 'AAAI: Conference on Artificial Intelligence' start_date: 2026-01-20 date_created: 2026-04-12T22:01:50Z date_published: 2026-03-14T00:00:00Z date_updated: 2026-05-04T11:38:56Z day: '14' department: - _id: KrCh - _id: GradSch doi: 10.1609/aaai.v40i43.40931 ec_funded: 1 external_id: arxiv: - '2505.04539' intvolume: ' 40' issue: '43' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.48550/arXiv.2505.04539 month: '03' oa: 1 oa_version: Preprint page: 36137-36145 project: - _id: 0599E47C-7A3F-11EA-A408-12923DDC885E call_identifier: H2020 grant_number: '863818' name: 'Formal Methods for Stochastic Models: Algorithms and Applications' publication: Proceedings of the 40th AAAI Conference on Artificial Intelligence publication_identifier: eissn: - 2374-3468 issn: - 2159-5399 publication_status: published publisher: Association for the Advancement of Artificial Intelligence quality_controlled: '1' scopus_import: '1' status: public title: Qualitative analysis of ω-regular objectives on robust MDPs type: conference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 40 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: diamond _id: '21718' 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." 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." article_number: '024' article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Nhok T full_name: Ngo, Nhok T id: 28e53c8c-896a-11ed-bdf8-f809043ce2f0 last_name: Ngo citation: ama: 'Ngo NT. Big algebra in type A for the coordinate ring of the matrix space. Symmetry, Integrability and Geometry: Methods and Applications. 2026;22. doi:10.3842/SIGMA.2026.024' apa: 'Ngo, N. T. (2026). Big algebra in type A for the coordinate ring of the matrix space. Symmetry, Integrability and Geometry: Methods and Applications. National Academy of Science of Ukraine. https://doi.org/10.3842/SIGMA.2026.024' chicago: 'Ngo, Nhok T. “Big Algebra in Type A for the Coordinate Ring of the Matrix Space.” Symmetry, Integrability and Geometry: Methods and Applications. National Academy of Science of Ukraine, 2026. https://doi.org/10.3842/SIGMA.2026.024.' ieee: 'N. T. Ngo, “Big algebra in type A for the coordinate ring of the matrix space,” Symmetry, Integrability and Geometry: Methods and Applications, vol. 22. National Academy of Science of Ukraine, 2026.' 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.' mla: 'Ngo, Nhok T. “Big Algebra in Type A for the Coordinate Ring of the Matrix Space.” Symmetry, Integrability and Geometry: Methods and Applications, vol. 22, 024, National Academy of Science of Ukraine, 2026, doi:10.3842/SIGMA.2026.024.' short: 'N.T. Ngo, Symmetry, Integrability and Geometry: Methods and Applications 22 (2026).' corr_author: '1' date_created: 2026-04-12T22:01:51Z date_published: 2026-03-14T00:00:00Z date_updated: 2026-04-16T06:11:12Z day: '14' ddc: - '510' department: - _id: TaHa doi: 10.3842/SIGMA.2026.024 external_id: arxiv: - '2501.04605' file: - access_level: open_access checksum: 29b28b5f8717ed1a084a2b551d0fd284 content_type: application/pdf creator: dernst date_created: 2026-04-16T06:06:54Z date_updated: 2026-04-16T06:06:54Z file_id: '21740' file_name: 2026_SIGMA_Ngo.pdf file_size: 975460 relation: main_file success: 1 file_date_updated: 2026-04-16T06:06:54Z has_accepted_license: '1' intvolume: ' 22' language: - iso: eng month: '03' oa: 1 oa_version: Published Version project: - _id: 34b2c9cb-11ca-11ed-8bc3-a50ba74ca4a3 grant_number: P35847 name: Geometry of the tip of the global nilpotent cone - _id: e6c64f42-ab3c-11f0-94c7-a95658059ccc grant_number: '27483' name: Big algebras in classical types publication: 'Symmetry, Integrability and Geometry: Methods and Applications' publication_identifier: eissn: - 1815-0659 publication_status: published publisher: National Academy of Science of Ukraine quality_controlled: '1' scopus_import: '1' status: public title: Big algebra in type A for the coordinate ring of the matrix space tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 22 year: '2026' ... --- OA_place: repository OA_type: green _id: '21719' 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 \U0001D457-tree decomposition of [Madry FOCS’10], achieving a poly-logarithmic approximation factor to the graph’s cut structure and supporting edge updates in \U0001D442⁡(\U0001D45B\U0001D700) amortized update time, for any arbitrarily small constant \U0001D700 ∈(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." 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." article_processing_charge: No arxiv: 1 author: - first_name: Gramoz full_name: Goranci, Gramoz last_name: Goranci - first_name: Monika H full_name: Henzinger, Monika H id: 540c9bbd-f2de-11ec-812d-d04a5be85630 last_name: Henzinger orcid: 0000-0002-5008-6530 - first_name: Peter full_name: Kiss, Peter last_name: Kiss - first_name: Ali full_name: Momeni, Ali last_name: Momeni - first_name: Gernot full_name: Zöcklein, Gernot id: 45d5e826-47af-11f1-84e5-ba87c23fe681 last_name: Zöcklein citation: ama: 'Goranci G, Henzinger M, Kiss P, Momeni A, Zöcklein G. Dynamic hierarchical j-tree decomposition and its applications. In: Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms. Vol 2026-January. Society for Industrial and Applied Mathematics; 2026:1128-1180. doi:10.1137/1.9781611978971.45' apa: Goranci, G., Henzinger, M., Kiss, P., Momeni, A., & Zöcklein, G. (2026). Dynamic hierarchical j-tree decomposition and its applications. In Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms (Vol. 2026–January, pp. 1128–1180). Society for Industrial and Applied Mathematics. https://doi.org/10.1137/1.9781611978971.45 chicago: Goranci, Gramoz, Monika Henzinger, Peter Kiss, Ali Momeni, and Gernot Zöcklein. “Dynamic Hierarchical J-Tree Decomposition and Its Applications.” In Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms, 2026–January:1128–80. Society for Industrial and Applied Mathematics, 2026. https://doi.org/10.1137/1.9781611978971.45. ieee: G. Goranci, M. Henzinger, P. Kiss, A. Momeni, and G. Zöcklein, “Dynamic hierarchical j-tree decomposition and its applications,” in Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms, 2026, vol. 2026–January, pp. 1128–1180. 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.' mla: Goranci, Gramoz, et al. “Dynamic Hierarchical J-Tree Decomposition and Its Applications.” Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms, vol. 2026–January, Society for Industrial and Applied Mathematics, 2026, pp. 1128–80, doi:10.1137/1.9781611978971.45. 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. conference: name: 'SODA: Symposium on Discrete Algorithms' date_created: 2026-04-12T22:01:51Z date_published: 2026-01-07T00:00:00Z date_updated: 2026-05-04T11:54:09Z day: '07' department: - _id: MoHe doi: 10.1137/1.9781611978971.45 ec_funded: 1 external_id: arxiv: - '2601.09139' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.48550/arXiv.2601.09139 month: '01' oa: 1 oa_version: Preprint page: 1128-1180 project: - _id: bd9ca328-d553-11ed-ba76-dc4f890cfe62 call_identifier: H2020 grant_number: '101019564' name: The design and evaluation of modern fully dynamic data structures - _id: bda196b2-d553-11ed-ba76-8e8ee6c21103 grant_number: I05982 name: Static and Dynamic Hierarchical Graph Decompositions publication: Proceedings of the 2026 Annual ACM SIAM Symposium on Discrete Algorithms publication_identifier: eissn: - '15579468' isbn: - '9781611978971' issn: - '10719040' publication_status: published publisher: Society for Industrial and Applied Mathematics quality_controlled: '1' scopus_import: '1' status: public title: Dynamic hierarchical j-tree decomposition and its applications type: conference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 2026-January year: '2026' ... --- OA_place: repository OA_type: green _id: '21720' abstract: - lang: eng text: "We present an exact fully-dynamic minimum cut algorithm that runs in \U0001D45B\U0001D45C⁡(1) deterministic update time when the minimum cut size is at most 2Θ⁡(log3/4−\U0001D450⁡\U0001D45B) for any \U0001D450 >0, improving on the previous algorithm of Jin, Sun, and Thorup (SODA 2024) whose minimum cut size limit is (log⁡\U0001D45B)\U0001D45C⁡(1). Combined with graph sparsification, we obtain the first (1 +\U0001D716)-approximate fully-dynamic minimum cut algorithm on weighted graphs, for any \U0001D716 ≥2−Θ⁡(log3/4−\U0001D450⁡\U0001D45B), in \U0001D45B\U0001D45C⁡(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)." 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. article_processing_charge: No arxiv: 1 author: - first_name: Antoine full_name: El-Hayek, Antoine id: 888a098e-fcac-11ee-aff7-d347be57b725 last_name: El-Hayek orcid: 0000-0003-4268-7368 - first_name: Monika H full_name: Henzinger, Monika H id: 540c9bbd-f2de-11ec-812d-d04a5be85630 last_name: Henzinger orcid: 0000-0002-5008-6530 - first_name: Jason full_name: Li, Jason last_name: Li citation: ama: 'El-Hayek A, Henzinger M, Li J. Deterministic and exact fully-dynamic minimum cut of superpolylogarithmic size in subpolynomial time. In: Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms. Vol 2026. Society for Industrial and Applied Mathematics; 2026:613-663. doi:10.1137/1.9781611978971.25' apa: 'El-Hayek, A., Henzinger, M., & Li, J. (2026). Deterministic and exact fully-dynamic minimum cut of superpolylogarithmic size in subpolynomial time. In Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms (Vol. 2026, pp. 613–663). Vancouver, Canada: Society for Industrial and Applied Mathematics. https://doi.org/10.1137/1.9781611978971.25' chicago: El-Hayek, Antoine, Monika Henzinger, and Jason Li. “Deterministic and Exact Fully-Dynamic Minimum Cut of Superpolylogarithmic Size in Subpolynomial Time.” In Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms, 2026:613–63. Society for Industrial and Applied Mathematics, 2026. https://doi.org/10.1137/1.9781611978971.25. ieee: A. El-Hayek, M. Henzinger, and J. Li, “Deterministic and exact fully-dynamic minimum cut of superpolylogarithmic size in subpolynomial time,” in Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms, Vancouver, Canada, 2026, vol. 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.' mla: El-Hayek, Antoine, et al. “Deterministic and Exact Fully-Dynamic Minimum Cut of Superpolylogarithmic Size in Subpolynomial Time.” Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms, vol. 2026, Society for Industrial and Applied Mathematics, 2026, pp. 613–63, doi:10.1137/1.9781611978971.25. 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. conference: end_date: 2026-01-14 location: Vancouver, Canada name: 'SODA: Symposium on Discrete Algorithms' start_date: 2026-01-11 date_created: 2026-04-12T22:01:51Z date_published: 2026-01-07T00:00:00Z date_updated: 2026-05-04T11:36:47Z day: '07' department: - _id: MoHe - _id: GradSch doi: 10.1137/1.9781611978971.25 ec_funded: 1 external_id: arxiv: - '2512.13105' intvolume: ' 2026' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.48550/arXiv.2512.13105 month: '01' oa: 1 oa_version: Preprint page: 613-663 project: - _id: bd9ca328-d553-11ed-ba76-dc4f890cfe62 call_identifier: H2020 grant_number: '101019564' name: The design and evaluation of modern fully dynamic data structures - _id: bda196b2-d553-11ed-ba76-8e8ee6c21103 grant_number: I05982 name: Static and Dynamic Hierarchical Graph Decompositions publication: Proceedings of the Annual ACM SIAM Symposium on Discrete Algorithms publication_identifier: eisbn: - '9781611978971' eissn: - 1557-9468 issn: - 1071-9040 publication_status: published publisher: Society for Industrial and Applied Mathematics quality_controlled: '1' scopus_import: '1' status: public title: Deterministic and exact fully-dynamic minimum cut of superpolylogarithmic size in subpolynomial time type: conference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 2026 year: '2026' ... --- OA_place: publisher OA_type: hybrid PlanS_conform: '1' _id: '21721' abstract: - lang: eng 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.' acknowledged_ssus: - _id: NanoFab - _id: EM-Fac 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). article_processing_charge: Yes (via OA deal) article_type: original 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 - first_name: David full_name: Saintillan, David last_name: Saintillan - first_name: Jérémie A full_name: Palacci, Jérémie A id: 8fb92548-2b22-11eb-b7c1-a3f0d08d7c7d last_name: Palacci orcid: 0000-0002-7253-9465 citation: ama: Grober DB, Dhar T, Saintillan D, Palacci JA. The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs. Nature Physics. 2026. doi:10.1038/s41567-026-03189-4 apa: Grober, D. B., Dhar, T., Saintillan, D., & Palacci, J. A. (2026). The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs. Nature Physics. Springer Nature. https://doi.org/10.1038/s41567-026-03189-4 chicago: Grober, Daniel B, Tanumoy Dhar, David Saintillan, and Jérémie A Palacci. “The Hydrodynamic Torque Dipole from Rotary Bacterial Flagella Powers Symmetric Discs.” Nature Physics. Springer Nature, 2026. https://doi.org/10.1038/s41567-026-03189-4. ieee: D. B. Grober, T. Dhar, D. Saintillan, and J. A. Palacci, “The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs,” Nature Physics. Springer Nature, 2026. ista: Grober DB, Dhar T, Saintillan D, Palacci JA. 2026. The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs. Nature Physics. mla: Grober, Daniel B., et al. “The Hydrodynamic Torque Dipole from Rotary Bacterial Flagella Powers Symmetric Discs.” Nature Physics, Springer Nature, 2026, doi:10.1038/s41567-026-03189-4. short: D.B. Grober, T. Dhar, D. Saintillan, J.A. Palacci, Nature Physics (2026). corr_author: '1' date_created: 2026-04-12T22:01:51Z date_published: 2026-03-27T00:00:00Z date_updated: 2026-04-16T06:20:23Z day: '27' ddc: - '570' department: - _id: JePa doi: 10.1038/s41567-026-03189-4 has_accepted_license: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1038/s41567-026-03189-4 month: '03' oa: 1 oa_version: Published Version project: - _id: bdac72da-d553-11ed-ba76-eae56e802b74 grant_number: '101086998' name: 'VULCAN: matter, powered from within' publication: Nature Physics publication_identifier: eissn: - 1745-2481 issn: - 1745-2473 publication_status: epub_ahead publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: The hydrodynamic torque dipole from rotary bacterial flagella powers symmetric discs tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold PlanS_conform: '1' _id: '21725' abstract: - lang: eng 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⊙." 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)." article_number: '69' article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: David R. full_name: Miller, David R. last_name: Miller - first_name: Ilaria full_name: Caiazzo, Ilaria id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d last_name: Caiazzo orcid: 0000-0002-4770-5388 - first_name: Jeremy full_name: Heyl, Jeremy last_name: Heyl - first_name: Harvey B. full_name: Richer, Harvey B. last_name: Richer - first_name: Mark A. full_name: Hollands, Mark A. last_name: Hollands - first_name: Pier Emmanuel full_name: Tremblay, Pier Emmanuel last_name: Tremblay - first_name: Kareem full_name: El-Badry, Kareem last_name: El-Badry - first_name: Antonio C. full_name: Rodriguez, Antonio C. last_name: Rodriguez - first_name: Zachary P. full_name: Vanderbosch, Zachary P. last_name: Vanderbosch citation: ama: Miller DR, Caiazzo I, Heyl J, et al. The White Dwarf initial–final mass relation from open clusters in Gaia DR3. The Astrophysical Journal. 2026;996(1). doi:10.3847/1538-4357/ae18c8 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. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ae18c8 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.” The Astrophysical Journal. IOP Publishing, 2026. https://doi.org/10.3847/1538-4357/ae18c8. ieee: D. R. Miller et al., “The White Dwarf initial–final mass relation from open clusters in Gaia DR3,” The Astrophysical Journal, vol. 996, no. 1. IOP Publishing, 2026. 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. mla: Miller, David R., et al. “The White Dwarf Initial–Final Mass Relation from Open Clusters in Gaia DR3.” The Astrophysical Journal, vol. 996, no. 1, 69, IOP Publishing, 2026, doi:10.3847/1538-4357/ae18c8. 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). date_created: 2026-04-12T22:01:52Z date_published: 2026-01-01T00:00:00Z date_updated: 2026-04-13T08:39:39Z day: '01' ddc: - '520' department: - _id: IlCa doi: 10.3847/1538-4357/ae18c8 external_id: arxiv: - '2510.24877' file: - access_level: open_access checksum: 65a8237a519188af83b6dc4d47ad85fa content_type: application/pdf creator: dernst date_created: 2026-04-13T08:36:50Z date_updated: 2026-04-13T08:36:50Z file_id: '21733' file_name: 2026_AstrophysicalJournal_Miller.pdf file_size: 19310053 relation: main_file success: 1 file_date_updated: 2026-04-13T08:36:50Z has_accepted_license: '1' intvolume: ' 996' issue: '1' keyword: - White dwarf stars - Open star clusters - Compact objects - Stellar evolution language: - iso: eng month: '01' oa: 1 oa_version: Published Version publication: The Astrophysical Journal publication_identifier: eissn: - 1538-4357 issn: - 0004-637X publication_status: published publisher: IOP Publishing quality_controlled: '1' scopus_import: '1' status: public title: The White Dwarf initial–final mass relation from open clusters in Gaia DR3 tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 996 year: '2026' ... --- OA_place: repository OA_type: green _id: '21726' abstract: - lang: eng 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. 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. article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Denitsa Rangelova full_name: Baykusheva, Denitsa Rangelova id: 71b4d059-2a03-11ee-914d-dfa3beed6530 last_name: Baykusheva orcid: 0000-0002-7438-1139 - first_name: Deven full_name: Carmichael, Deven last_name: Carmichael - first_name: Clara S. full_name: Weber, Clara S. last_name: Weber - first_name: I. Te full_name: Lu, I. Te last_name: Lu - first_name: Filippo full_name: Glerean, Filippo last_name: Glerean - first_name: Tepie full_name: Meng, Tepie last_name: Meng - first_name: Pedro B.M. full_name: De Oliveira, Pedro B.M. last_name: De Oliveira - first_name: Christopher C. full_name: Homes, Christopher C. last_name: Homes - first_name: Igor A. full_name: Zaliznyak, Igor A. last_name: Zaliznyak - first_name: G. D. full_name: Gu, G. D. last_name: Gu - first_name: Mark P.M. full_name: Dean, Mark P.M. last_name: Dean - first_name: Angel full_name: Rubio, Angel last_name: Rubio - first_name: Dante M. full_name: Kennes, Dante M. last_name: Kennes - first_name: Martin full_name: Claassen, Martin last_name: Claassen - first_name: Matteo full_name: Mitrano, Matteo last_name: Mitrano citation: ama: Baykusheva DR, Carmichael D, Weber CS, et al. Quantum control of Hubbard excitons. Nature Materials. 2026. doi:10.1038/s41563-026-02517-6 apa: Baykusheva, D. R., Carmichael, D., Weber, C. S., Lu, I. T., Glerean, F., Meng, T., … Mitrano, M. (2026). Quantum control of Hubbard excitons. Nature Materials. Springer Nature. https://doi.org/10.1038/s41563-026-02517-6 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.” Nature Materials. Springer Nature, 2026. https://doi.org/10.1038/s41563-026-02517-6. ieee: D. R. Baykusheva et al., “Quantum control of Hubbard excitons,” Nature Materials. Springer Nature, 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. mla: Baykusheva, Denitsa Rangelova, et al. “Quantum Control of Hubbard Excitons.” Nature Materials, Springer Nature, 2026, doi:10.1038/s41563-026-02517-6. 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). corr_author: '1' date_created: 2026-04-12T22:01:53Z date_published: 2026-03-09T00:00:00Z date_updated: 2026-04-13T07:29:34Z day: '09' department: - _id: DeBa doi: 10.1038/s41563-026-02517-6 external_id: arxiv: - '2601.20695 ' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.48550/arXiv.2601.20695 month: '03' oa: 1 oa_version: Preprint publication: Nature Materials publication_identifier: eissn: - 1476-4660 issn: - 1476-1122 publication_status: epub_ahead publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Quantum control of Hubbard excitons type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 year: '2026' ... --- OA_place: repository OA_type: green _id: '21737' abstract: - lang: eng 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. 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" article_number: '2602.09958' article_processing_charge: No arxiv: 1 author: - first_name: Albert full_name: Chern, Albert last_name: Chern - first_name: Sadashige full_name: Ishida, Sadashige id: 6F7C4B96-A8E9-11E9-A7CA-09ECE5697425 last_name: Ishida orcid: 0000-0002-3121-3100 citation: ama: Chern A, Ishida S. L’Hopital rules for complex-valued functions in higher dimensions. arXiv. doi:10.48550/ARXIV.2602.09958 apa: Chern, A., & Ishida, S. (n.d.). L’Hopital rules for complex-valued functions in higher dimensions. arXiv. https://doi.org/10.48550/ARXIV.2602.09958 chicago: Chern, Albert, and Sadashige Ishida. “L’Hopital Rules for Complex-Valued Functions in Higher Dimensions.” ArXiv, n.d. https://doi.org/10.48550/ARXIV.2602.09958. ieee: A. Chern and S. Ishida, “L’Hopital rules for complex-valued functions in higher dimensions,” arXiv. . ista: Chern A, Ishida S. L’Hopital rules for complex-valued functions in higher dimensions. arXiv, 2602.09958. mla: Chern, Albert, and Sadashige Ishida. “L’Hopital Rules for Complex-Valued Functions in Higher Dimensions.” ArXiv, 2602.09958, doi:10.48550/ARXIV.2602.09958. short: A. Chern, S. Ishida, ArXiv (n.d.). corr_author: '1' date_created: 2026-04-15T16:28:24Z date_published: 2026-02-10T00:00:00Z date_updated: 2026-04-28T10:56:30Z day: '10' ddc: - '510' department: - _id: GradSch - _id: ChWo doi: 10.48550/ARXIV.2602.09958 external_id: arxiv: - '2602.09958' file: - access_level: open_access checksum: 6a76591c723d3e949ad5afa9f7dbb2ee content_type: application/pdf creator: dernst date_created: 2026-04-28T10:53:27Z date_updated: 2026-04-28T10:53:27Z file_id: '21771' file_name: 2026_arXiv_2602.09958.pdf file_size: 867109 relation: main_file success: 1 file_date_updated: 2026-04-28T10:53:27Z has_accepted_license: '1' keyword: - l’Hopital theorem - complex functions language: - iso: eng month: '02' oa: 1 oa_version: Preprint project: - _id: 34bc2376-11ca-11ed-8bc3-9a3b3961a088 grant_number: '101045083' name: Computational Discovery of Numerical Algorithms for Animation and Simulation of Natural Phenomena publication: arXiv publication_status: submitted status: public title: L'Hopital rules for complex-valued functions in higher dimensions tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: preprint user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 year: '2026' ... --- OA_place: publisher OA_type: hybrid PlanS_conform: '1' _id: '21743' abstract: - lang: eng 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. 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. article_number: '45' article_processing_charge: Yes (via OA deal) article_type: original arxiv: 1 author: - first_name: Martin full_name: Bauer, Martin last_name: Bauer - first_name: Sadashige full_name: Ishida, Sadashige id: 6F7C4B96-A8E9-11E9-A7CA-09ECE5697425 last_name: Ishida orcid: 0000-0002-3121-3100 - first_name: Peter W. full_name: Michor, Peter W. last_name: Michor citation: ama: Bauer M, Ishida S, Michor PW. Symplectic structures on the space of space curves. Journal of Nonlinear Science. 2026;36(2). doi:10.1007/s00332-026-10266-8 apa: Bauer, M., Ishida, S., & Michor, P. W. (2026). Symplectic structures on the space of space curves. Journal of Nonlinear Science. Springer Nature. https://doi.org/10.1007/s00332-026-10266-8 chicago: Bauer, Martin, Sadashige Ishida, and Peter W. Michor. “Symplectic Structures on the Space of Space Curves.” Journal of Nonlinear Science. Springer Nature, 2026. https://doi.org/10.1007/s00332-026-10266-8. ieee: M. Bauer, S. Ishida, and P. W. Michor, “Symplectic structures on the space of space curves,” Journal of Nonlinear Science, vol. 36, no. 2. Springer Nature, 2026. ista: Bauer M, Ishida S, Michor PW. 2026. Symplectic structures on the space of space curves. Journal of Nonlinear Science. 36(2), 45. mla: Bauer, Martin, et al. “Symplectic Structures on the Space of Space Curves.” Journal of Nonlinear Science, vol. 36, no. 2, 45, Springer Nature, 2026, doi:10.1007/s00332-026-10266-8. short: M. Bauer, S. Ishida, P.W. Michor, Journal of Nonlinear Science 36 (2026). date_created: 2026-04-16T07:29:17Z date_published: 2026-04-15T00:00:00Z date_updated: 2026-04-28T09:59:01Z day: '15' ddc: - '510' department: - _id: GradSch - _id: ChWo doi: 10.1007/s00332-026-10266-8 external_id: arxiv: - '2407.19908' file: - access_level: open_access checksum: 760de2631b6fd7d57bcd5115ed36c0a2 content_type: application/pdf creator: dernst date_created: 2026-04-28T09:55:32Z date_updated: 2026-04-28T09:55:32Z file_id: '21770' file_name: 2026_JourNonlinearScience_Bauer.pdf file_size: 1108518 relation: main_file success: 1 file_date_updated: 2026-04-28T09:55:32Z has_accepted_license: '1' intvolume: ' 36' issue: '2' language: - iso: eng month: '04' oa: 1 oa_version: Published Version project: - _id: 34bc2376-11ca-11ed-8bc3-9a3b3961a088 grant_number: '101045083' name: Computational Discovery of Numerical Algorithms for Animation and Simulation of Natural Phenomena publication: Journal of Nonlinear Science publication_identifier: eissn: - 1432-1467 issn: - 0938-8974 publication_status: published publisher: Springer Nature quality_controlled: '1' related_material: record: - id: '17361' relation: earlier_version status: public scopus_import: '1' status: public title: Symplectic structures on the space of space curves tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0) short: CC BY (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 36 year: '2026' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '21744' 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. 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." article_number: '116904' article_processing_charge: Yes article_type: original author: - first_name: Yuxi full_name: Li, Yuxi last_name: Li - first_name: Trevor C. full_name: Butler, Trevor C. last_name: Butler - first_name: Stefano full_name: Nardone, Stefano last_name: Nardone - first_name: Christopher L. full_name: Jacobs, Christopher L. last_name: Jacobs - first_name: Amelia May Barnett full_name: Douglass, Amelia May Barnett id: de5f6fda-80fb-11ef-996f-a8c4ecd8e289 last_name: Douglass orcid: 0000-0001-5398-6473 - first_name: Joseph C. full_name: Madara, Joseph C. last_name: Madara - first_name: Miriam C. full_name: McDonough, Miriam C. last_name: McDonough - first_name: Jenkang full_name: Tao, Jenkang last_name: Tao - first_name: Elijah D. full_name: Lowenstein, Elijah D. last_name: Lowenstein - first_name: Luhong full_name: Wang, Luhong last_name: Wang - first_name: Deepti full_name: Pant, Deepti last_name: Pant - first_name: Samuel J. full_name: Walker, Samuel J. last_name: Walker - first_name: Annette full_name: Wang, Annette last_name: Wang - first_name: Harini full_name: Srinivasan, Harini last_name: Srinivasan - first_name: Zongfang full_name: Yang, Zongfang last_name: Yang - first_name: John N. full_name: Campbell, John N. last_name: Campbell - first_name: Linus T. full_name: Tsai, Linus T. last_name: Tsai - first_name: Bradford B. full_name: Lowell, Bradford B. last_name: Lowell - first_name: Jon M. full_name: Resch, Jon M. last_name: Resch citation: ama: Li Y, Butler TC, Nardone S, et al. A spatial and projection-based transcriptomic atlas of paraventricular hypothalamic cell types. Cell Reports. 2026;45(2). doi:10.1016/j.celrep.2025.116904 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. Cell Reports. Elsevier. https://doi.org/10.1016/j.celrep.2025.116904 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.” Cell Reports. Elsevier, 2026. https://doi.org/10.1016/j.celrep.2025.116904. ieee: Y. Li et al., “A spatial and projection-based transcriptomic atlas of paraventricular hypothalamic cell types,” Cell Reports, vol. 45, no. 2. Elsevier, 2026. 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. mla: Li, Yuxi, et al. “A Spatial and Projection-Based Transcriptomic Atlas of Paraventricular Hypothalamic Cell Types.” Cell Reports, vol. 45, no. 2, 116904, Elsevier, 2026, doi:10.1016/j.celrep.2025.116904. 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). date_created: 2026-04-16T13:51:29Z date_published: 2026-02-24T00:00:00Z date_updated: 2026-05-04T12:00:31Z day: '24' ddc: - '570' department: - _id: AmDo doi: 10.1016/j.celrep.2025.116904 external_id: pmid: - '41581146' file: - access_level: open_access checksum: 82098dd9d0ca609119f9f2c6beb4fc1e content_type: application/pdf creator: dernst date_created: 2026-05-04T11:58:51Z date_updated: 2026-05-04T11:58:51Z file_id: '21793' file_name: 2026_CellReports_Li.pdf file_size: 38532865 relation: main_file success: 1 file_date_updated: 2026-05-04T11:58:51Z has_accepted_license: '1' intvolume: ' 45' issue: '2' language: - iso: eng month: '02' oa: 1 oa_version: Published Version pmid: 1 publication: Cell Reports publication_identifier: eissn: - 2211-1247 issn: - 2639-1856 publication_status: published publisher: Elsevier quality_controlled: '1' scopus_import: '1' status: public title: A spatial and projection-based transcriptomic atlas of paraventricular hypothalamic cell types tmp: image: /images/cc_by_nc_nd.png legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) short: CC BY-NC-ND (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 45 year: '2026' ...