--- DOAJ_listed: '1' OA_place: publisher OA_type: gold PlanS_conform: '1' _id: '20649' abstract: - lang: eng text: Ionized proximity zones around luminous quasars provide a unique laboratory to characterize the Lyα emission lines from z > 6 galaxies without significant attenuation from the intergalactic medium (IGM). However, Lyα line measurements for galaxies within high-redshift quasars’ proximity zones have been rare so far. Here we present deep spectroscopic observations obtained with the NIRSpec/Micro-Shutter Assembly (MSA) instrument on the James Webb Space Telescope of galaxies in two z > 6 quasar fields. We measure the Lyα line fluxes for 50 galaxies at 6 < z < 7 with UV absolute magnitude M UV < −19 (median M UV = −19.97), among which 15 are located near the luminous quasars, i.e., within Δv < 2500 km s−1. We find that galaxies near the quasars show significant flux blueward of the systemic Lyα wavelength, and have higher Lyα equivalent width compared to galaxies at similar redshifts that are not located within the quasars’ environment. Our result indicates little or no redshift evolution for the Lyα emitter fraction from z ∼ 6.4 to z ∼ 5. Leveraging the low IGM opacity in the quasars’ vicinity, we evaluate the Lyα escape fraction (f esc Ly α) of high-redshift galaxies. Our analysis suggests that galaxies at 〈z〉 ≈ 6.4 have an average f esc Ly α = 0.14 ± 0.04. This value is consistent with reionization models where the Lyman continuum escape fraction is low ( fescLyC ≲ 0.1 ) for luminous galaxies, and where the most luminous galaxies have only a minor contribution to the total ionizing photon budget. © 2025. The Author(s). Published by the American Astronomical Society. acknowledgement: "We thank the referee for valuable comments. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program ID #3117 and #4713. Support for\r\nthis work was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute, which is operated by the\r\nAssociation of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555." article_number: L12 article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: Minghao full_name: Yue, Minghao last_name: Yue - first_name: Anna Christina full_name: Eilers, Anna Christina last_name: Eilers - 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: Rongmon full_name: Bordoloi, Rongmon last_name: Bordoloi - first_name: Frederick B. full_name: Davies, Frederick B. last_name: Davies - first_name: Joseph F. full_name: Hennawi, Joseph F. last_name: Hennawi - first_name: Daichi full_name: Kashino, Daichi last_name: Kashino - first_name: Ruari full_name: Mackenzie, Ruari last_name: Mackenzie - first_name: Robert A. full_name: Simcoe, Robert A. last_name: Simcoe citation: ama: Yue M, Eilers AC, Matthee JJ, et al. Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars. The Astrophysical Journal Letters. 2025;993(1). doi:10.3847/2041-8213/ae0e0e apa: Yue, M., Eilers, A. C., Matthee, J. J., Naidu, R. P., Bordoloi, R., Davies, F. B., … Simcoe, R. A. (2025). Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars. The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/ae0e0e chicago: Yue, Minghao, Anna Christina Eilers, Jorryt J Matthee, Rohan P. Naidu, Rongmon Bordoloi, Frederick B. Davies, Joseph F. Hennawi, Daichi Kashino, Ruari Mackenzie, and Robert A. Simcoe. “Escape Fractions from Unattenuated Lyα Emitters around Luminous z > 6 Quasars.” The Astrophysical Journal Letters. IOP Publishing, 2025. https://doi.org/10.3847/2041-8213/ae0e0e. ieee: M. Yue et al., “Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars,” The Astrophysical Journal Letters, vol. 993, no. 1. IOP Publishing, 2025. ista: Yue M, Eilers AC, Matthee JJ, Naidu RP, Bordoloi R, Davies FB, Hennawi JF, Kashino D, Mackenzie R, Simcoe RA. 2025. Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars. The Astrophysical Journal Letters. 993(1), L12. mla: Yue, Minghao, et al. “Escape Fractions from Unattenuated Lyα Emitters around Luminous z > 6 Quasars.” The Astrophysical Journal Letters, vol. 993, no. 1, L12, IOP Publishing, 2025, doi:10.3847/2041-8213/ae0e0e. short: M. Yue, A.C. Eilers, J.J. Matthee, R.P. Naidu, R. Bordoloi, F.B. Davies, J.F. Hennawi, D. Kashino, R. Mackenzie, R.A. Simcoe, The Astrophysical Journal Letters 993 (2025). date_created: 2025-11-16T23:01:24Z date_published: 2025-11-01T00:00:00Z date_updated: 2026-02-16T12:45:16Z day: '01' ddc: - '520' department: - _id: JoMa doi: 10.3847/2041-8213/ae0e0e external_id: arxiv: - '2507.05381' isi: - '001600890100001' file: - access_level: open_access checksum: 11d35c1c52c000f8c14bc6de2e9f4b3f content_type: application/pdf creator: dernst date_created: 2025-11-24T13:18:34Z date_updated: 2025-11-24T13:18:34Z file_id: '20680' file_name: 2025_AstrophysicalJour_Yue.pdf file_size: 39736710 relation: main_file success: 1 file_date_updated: 2025-11-24T13:18:34Z has_accepted_license: '1' intvolume: ' 993' isi: 1 issue: '1' language: - iso: eng license: https://creativecommons.org/licenses/by/4.0/ month: '11' 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: Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars 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: 993 year: '2025' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold PlanS_conform: '1' _id: '20660' abstract: - lang: eng text: "We used observations from the JWST Emission Line Survey (JELS) to measure the half-light radii (re) of 23 Hα-emitting starforming (SF) galaxies at z = 6.1 in the PRIMER/COSMOS field. Galaxy sizes were measured in JWST near-infrared camera observations in rest-frame Hα (tracing recent star formation) with the F466N and F470N narrow-band filters from JELS, and\r\ncompared against rest-R- and V -band (tracing established stellar populations) and near-ultraviolet sizes. We find a size–stellar mass(re − M∗) relationship with a slope that is consistent with literature values at lower redshifts, though offset to lowersizes. We observe a large scatter in re at low stellar mass (M∗ < 10^8.4 Mo) which we believe is the result of bursty star formation histories (SFHs) of SF galaxies at the Epoch of Reionization (EoR). We find that the stellar and ionized gas components are similar in size at z = 6.1. The evidence of already-established stellar components in these Hα emitters (HAEs) indicates previous episodes of star formation have occurred. As such, following other JELS studies finding our HAEs are undergoing a current burst of star formation, we believe our results indicate that SF galaxies at the end of the EoR have already experienced a bursty SFH. From our re − M∗ relationship, we find re,F444W = 0.76 ± 0.46 kpc for fixed stellar mass M∗ = 10^9.25 M, which is in agreement with other observations and simulations of SF galaxies in the literature. We find a close-pair (major) merger fraction of (fmaj. merger =0.44 ± 0.22) fmerger = 0.43 ± 0.11 for galaxy separations d <~ 25 kpc, which is in agreement with other z ≈ 6 studies." acknowledgement: "This work makes use of ASTROPY, 7 a community-developed core PYTHON package for Astronomy (Astropy Collaboration 2013, 2018, 2022), as well as the NUMPY (C. R. Harris et al. 2020) and SCIPY (P.Virtanen et al. 2020) packages(see also T. E. Oliphant 2007). All plots\r\nwere created using the MATPLOTLIB 2D graphics PYTHON package (J. D. Hunter 2007). Conversions between redshift and lookback time in our selected cosmological model were done using the Javascript cosmological calculator from E. L. Wright (2006).8 The authors would like to thank the anonymous referee for their constructive comments and suggestions which have strengthened the analysis of this work and improved the paper. The authors also gratefully acknowledge Ian Smail for providing valuable feedback and helping to guide the science of this paper. This work is based on observations made with the NASA/ESA/CSA James Webb Space\r\nTelescope. The data were obtained from the Mikulski Archive for Space Telescopes9 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 GO no. 2321 (JELS) and GO no. 1837 (PRIMER). The authors acknowledge the PRIMER team for developing their observing program with a zero-exclusive-access period. HMOS acknowledges support from an STFC PhD studentship and the Faculty of Science and Technology at Lancaster University. PNB is grateful for support from the UK STFC\r\nvia grants ST/V000594/1 and ST/Y000951/1. JSD acknowledges the support of the Royal Society via a Royal Society Research Professorship. LOF acknowledges funding by ANID BECAS/DOCTORADO NACIONAL 21220499.CLH acknowledges support from the Oxford\r\nHintze Centre for Astrophysical Surveys which is funded through generous support from the Hintze family charity foundation. EI gratefully acknowledge financial support from ANID – MILENIO –NCN2024 112 and ANID FONDECYT Regular 1221846. For the purpose of open access, the authors have applied a Creative Commons attribution (CC BY) licence to any author accepted manuscript version arising." article_processing_charge: Yes article_type: original author: - first_name: H. M.O. full_name: Stephenson, H. M.O. last_name: Stephenson - first_name: J. P. full_name: Stott, J. P. last_name: Stott - first_name: C. A. full_name: Pirie, C. A. last_name: Pirie - first_name: K. J. full_name: Duncan, K. J. last_name: Duncan - first_name: D. J. full_name: Mcleod, D. J. last_name: Mcleod - first_name: P. N. full_name: Best, P. N. last_name: Best - first_name: M. full_name: Brinch, M. last_name: Brinch - first_name: M. full_name: Clausen, M. last_name: Clausen - first_name: R. K. full_name: Cochrane, R. K. last_name: Cochrane - first_name: J. S. full_name: Dunlop, J. S. last_name: Dunlop - first_name: S. R. full_name: Flury, S. R. last_name: Flury - first_name: J. E. full_name: Geach, J. E. last_name: Geach - first_name: C. L. full_name: Hale, C. L. last_name: Hale - first_name: E. full_name: Ibar, E. last_name: Ibar - first_name: Zefeng full_name: Li, Zefeng last_name: Li - 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: R. J. full_name: Mclure, R. J. last_name: Mclure - first_name: L. full_name: Ossa-Fuentes, L. last_name: Ossa-Fuentes - first_name: A. L. full_name: Patrick, A. L. last_name: Patrick - first_name: D. full_name: Sobral, D. last_name: Sobral - first_name: A. M. full_name: Swinbank, A. M. last_name: Swinbank citation: ama: 'Stephenson HMO, Stott JP, Pirie CA, et al. The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization. Monthly Notices of the Royal Astronomical Society. 2025;544(2):1412-1431. doi:10.1093/mnras/staf1725' apa: 'Stephenson, H. M. O., Stott, J. P., Pirie, C. A., Duncan, K. J., Mcleod, D. J., Best, P. N., … Swinbank, A. M. (2025). The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/staf1725' chicago: 'Stephenson, H. M.O., J. P. Stott, C. A. Pirie, K. J. Duncan, D. J. Mcleod, P. N. Best, M. Brinch, et al. “The JWST Emission Line Survey (JELS): The Sizes and Merger Fraction of Star-Forming Galaxies during the Epoch of Reionization.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2025. https://doi.org/10.1093/mnras/staf1725.' ieee: 'H. M. O. Stephenson et al., “The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization,” Monthly Notices of the Royal Astronomical Society, vol. 544, no. 2. Oxford University Press, pp. 1412–1431, 2025.' ista: 'Stephenson HMO, Stott JP, Pirie CA, Duncan KJ, Mcleod DJ, Best PN, Brinch M, Clausen M, Cochrane RK, Dunlop JS, Flury SR, Geach JE, Hale CL, Ibar E, Li Z, Matthee JJ, Mclure RJ, Ossa-Fuentes L, Patrick AL, Sobral D, Swinbank AM. 2025. The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization. Monthly Notices of the Royal Astronomical Society. 544(2), 1412–1431.' mla: 'Stephenson, H. M. O., et al. “The JWST Emission Line Survey (JELS): The Sizes and Merger Fraction of Star-Forming Galaxies during the Epoch of Reionization.” Monthly Notices of the Royal Astronomical Society, vol. 544, no. 2, Oxford University Press, 2025, pp. 1412–31, doi:10.1093/mnras/staf1725.' short: H.M.O. Stephenson, J.P. Stott, C.A. Pirie, K.J. Duncan, D.J. Mcleod, P.N. Best, M. Brinch, M. Clausen, R.K. Cochrane, J.S. Dunlop, S.R. Flury, J.E. Geach, C.L. Hale, E. Ibar, Z. Li, J.J. Matthee, R.J. Mclure, L. Ossa-Fuentes, A.L. Patrick, D. Sobral, A.M. Swinbank, Monthly Notices of the Royal Astronomical Society 544 (2025) 1412–1431. date_created: 2025-11-23T23:01:37Z date_published: 2025-12-01T00:00:00Z date_updated: 2025-12-01T15:25:11Z day: '01' ddc: - '520' department: - _id: JoMa doi: 10.1093/mnras/staf1725 external_id: isi: - '001611415800001' file: - access_level: open_access checksum: ddb3f429d2246bbf536efb4b0e52f3a8 content_type: application/pdf creator: dernst date_created: 2025-11-24T10:35:15Z date_updated: 2025-11-24T10:35:15Z file_id: '20678' file_name: 2025_MonthlyNoticesRAS_Stephenson.pdf file_size: 3625308 relation: main_file success: 1 file_date_updated: 2025-11-24T10:35:15Z has_accepted_license: '1' intvolume: ' 544' isi: 1 issue: '2' language: - iso: eng month: '12' oa: 1 oa_version: Published Version page: 1412-1431 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: eissn: - 1365-2966 issn: - 0035-8711 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: 'The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization' 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: 544 year: '2025' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold PlanS_conform: '1' _id: '20662' abstract: - lang: eng text: Task-based functional magnetic resonance imaging (fMRI) reveals individual differences in neural correlates of cognition but faces scalability challenges due to cognitive demands, protocol variability, and limited task coverage in large datasets. Here, we propose DeepTaskGen, a deep-learning approach that synthesizes non-acquired task-based contrast maps from resting-state (rs-) fMRI. We validate this approach using the Human Connectome Project lifespan data, then generate 47 contrast maps from 7 different cognitive tasks for over 20,000 individuals from UK Biobank. DeepTaskGen outperforms several benchmarks in generating synthetic task-contrast maps, achieving superior reconstruction performance while retaining inter-individual variation essential for biomarker development. We further show comparable or superior predictive performance of synthetic maps relative to actual maps and rs-connectomes across diverse demographic, cognitive, and clinical variables. This approach facilitates the study of individual differences and the generation of task-related biomarkers by enabling the generation of arbitrary functional cognitive tasks from readily available rs-fMRI data. acknowledgement: 'Funded by the European Union (Grant agreement No 101057429). Complementary funding was received by UK Research and Innovation (UKRI) under the UK government’s Horizon Europe funding guarantee (10131373 and 10038599) and the National Key R&D Program of Ministry of Science and Technology of China (MOST 2023YFE0199700). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union, the European Health and Digital Executive Agency (HADEA), UKRI or MOST. Neither the European Union nor HADEA nor UKRI nor MOST can be held responsible for them. This work has also been supported by a Grant from the German Research Foundation to the ENIGMA task-based fMRI Working Group (DFG ER 724/4–1, WA 1539/11–1). Data used in this study were provided in part by the Human Connectome Project, WU-Minn Consortium (principal investigators: D. Van Essen and K. Ugurbil; grant number 1U54MH091657), funded by the 16 National Institutes of Health (NIH) institutes and centers supporting the NIH Blueprint for Neuroscience Research, and by the McDonnell Center for Systems Neuroscience at Washington University. Additionally, this research utilized data obtained from UK Biobank, a large-scale biomedical database. Open Access funding enabled and organized by Projekt DEAL.' article_number: '1572' article_processing_charge: Yes (via OA deal) article_type: original author: - first_name: Emin full_name: Serin, Emin last_name: Serin - first_name: Kerstin full_name: Ritter, Kerstin last_name: Ritter - first_name: Gunter full_name: Schumann, Gunter last_name: Schumann - first_name: Tobias full_name: Banaschewski, Tobias last_name: Banaschewski - first_name: Andre full_name: Marquand, Andre last_name: Marquand - first_name: Henrik full_name: Walter, Henrik last_name: Walter - first_name: George full_name: Ogoh, George last_name: Ogoh - first_name: Bernd Carsten full_name: Stahl, Bernd Carsten last_name: Stahl - first_name: Ragnhild full_name: Brandlistuen, Ragnhild last_name: Brandlistuen - first_name: Tamara full_name: Schikowski, Tamara last_name: Schikowski - first_name: Allan H. full_name: Young, Allan H. last_name: Young - first_name: Yu full_name: Xinyang, Yu last_name: Xinyang - first_name: Zuo full_name: Zhang, Zuo last_name: Zhang - first_name: Kofoworola full_name: Agunbiade, Kofoworola last_name: Agunbiade - first_name: Di full_name: Chen, Di last_name: Chen - first_name: Sylvane full_name: Desrivières, Sylvane last_name: Desrivières - first_name: Nicholas full_name: Clinton, Nicholas last_name: Clinton - first_name: Paul full_name: Thompson, Paul last_name: Thompson - first_name: Venessa full_name: Köhler, Venessa last_name: Köhler - first_name: Ameli full_name: Schwalber, Ameli last_name: Schwalber - first_name: Vince D. full_name: Calhoun, Vince D. last_name: Calhoun - first_name: Xiao full_name: Chang, Xiao last_name: Chang - first_name: Yanqing full_name: Zhang, Yanqing last_name: Zhang - first_name: Yuzhu full_name: Li, Yuzhu last_name: Li - first_name: Yuxiang full_name: Dai, Yuxiang last_name: Dai - first_name: Jiacan full_name: Yuan, Jiacan last_name: Yuan - first_name: Yunman full_name: Xia, Yunman last_name: Xia - first_name: Tianye full_name: Jia, Tianye last_name: Jia - first_name: Paul full_name: Renner, Paul last_name: Renner - first_name: Sören full_name: Hese, Sören last_name: Hese - first_name: Bernhard full_name: Spanlang, Bernhard last_name: Spanlang - first_name: Charlie full_name: Pearmund, Charlie last_name: Pearmund - first_name: Anastasios Polykarpos full_name: Athanasiadis, Anastasios Polykarpos last_name: Athanasiadis - first_name: Spase full_name: Petkoski, Spase last_name: Petkoski - first_name: Viktor full_name: Jirsa, Viktor last_name: Jirsa - first_name: Karen full_name: Schmitt, Karen last_name: Schmitt - first_name: Johannes H. full_name: Wilbertz, Johannes H. last_name: Wilbertz - first_name: Myrto full_name: Patraskaki, Myrto last_name: Patraskaki - first_name: Peter full_name: Sommer, Peter last_name: Sommer - first_name: Stefanie full_name: Heilmann-Heimbach, Stefanie last_name: Heilmann-Heimbach - first_name: Carina M. full_name: Mathey, Carina M. last_name: Mathey - first_name: Abigail J. full_name: Miller, Abigail J. last_name: Miller - first_name: Isabelle full_name: Claus, Isabelle last_name: Claus - first_name: Markus M. full_name: Nöthen, Markus M. last_name: Nöthen - first_name: Per full_name: Hoffmann, Per last_name: Hoffmann - first_name: Andreas J. full_name: Forstner, Andreas J. last_name: Forstner - first_name: Alvaro full_name: Pastor, Alvaro last_name: Pastor - first_name: Jaime full_name: Gallego, Jaime last_name: Gallego - first_name: Reiya full_name: Itatani, Reiya last_name: Itatani - first_name: Francisco full_name: Eiroa-Orosa, Francisco last_name: Eiroa-Orosa - first_name: Guillem full_name: Feixas, Guillem last_name: Feixas - first_name: Mel full_name: Slater, Mel last_name: Slater - first_name: Gaia full_name: Novarino, Gaia id: 3E57A680-F248-11E8-B48F-1D18A9856A87 last_name: Novarino orcid: 0000-0002-7673-7178 - first_name: Sarah Jane full_name: Böttger, Sarah Jane last_name: Böttger - first_name: Mira full_name: Tschorn, Mira last_name: Tschorn - first_name: Michael full_name: Rapp, Michael last_name: Rapp - first_name: Helga full_name: Ask, Helga last_name: Ask - first_name: Rikka full_name: Kjelkenes, Rikka last_name: Kjelkenes - first_name: Sara full_name: Fernandez, Sara last_name: Fernandez - first_name: Dennis full_name: Van Der Meer, Dennis last_name: Van Der Meer - first_name: Lars T. full_name: Westlye, Lars T. last_name: Westlye - first_name: Ole A. full_name: Andreassen, Ole A. last_name: Andreassen - first_name: Rieke full_name: Aden, Rieke last_name: Aden - first_name: Beke full_name: Seefried, Beke last_name: Seefried - first_name: Frauke full_name: Nees, Frauke last_name: Nees - first_name: Maja full_name: Neidhart, Maja last_name: Neidhart - first_name: Argyris full_name: Stringaris, Argyris last_name: Stringaris - first_name: Emanuel full_name: Schwarz, Emanuel last_name: Schwarz - first_name: Nathalie full_name: Holz, Nathalie last_name: Holz - first_name: Heike full_name: Tost, Heike last_name: Tost - first_name: Andreas full_name: Meyer-Lindenberg, Andreas last_name: Meyer-Lindenberg - first_name: Nina full_name: Christmann, Nina last_name: Christmann - first_name: Karina full_name: Janson, Karina last_name: Janson - first_name: Kerstin full_name: Schepanski, Kerstin last_name: Schepanski - first_name: Tatjana full_name: Schütz, Tatjana last_name: Schütz - first_name: Ulrike Helene full_name: Taron, Ulrike Helene last_name: Taron - first_name: Roland full_name: Eils, Roland last_name: Eils - first_name: Jean Charles full_name: Roy, Jean Charles last_name: Roy - first_name: Tristram A. full_name: Lett, Tristram A. last_name: Lett - first_name: Hedi full_name: Kebir, Hedi last_name: Kebir - first_name: Elli full_name: Polemiti, Elli last_name: Polemiti - first_name: Esther full_name: Hitchen, Esther last_name: Hitchen - first_name: Marcel full_name: Jentsch, Marcel last_name: Jentsch - first_name: Emin full_name: Serin, Emin last_name: Serin - first_name: Antoine full_name: Bernas, Antoine last_name: Bernas - first_name: Nilakshi full_name: Vaidya, Nilakshi last_name: Vaidya - first_name: Sven full_name: Twardziok, Sven last_name: Twardziok - first_name: Markus full_name: Ralser, Markus last_name: Ralser - first_name: Andreas full_name: Heinz, Andreas last_name: Heinz - first_name: Gunter full_name: Schumann, Gunter last_name: Schumann citation: ama: Serin E, Ritter K, Schumann G, et al. Generating synthetic task-based brain fingerprints for population neuroscience using deep learning. Communications Biology. 2025;8. doi:10.1038/s42003-025-09158-6 apa: Serin, E., Ritter, K., Schumann, G., Banaschewski, T., Marquand, A., Walter, H., … Schumann, G. (2025). Generating synthetic task-based brain fingerprints for population neuroscience using deep learning. Communications Biology. Springer Nature. https://doi.org/10.1038/s42003-025-09158-6 chicago: Serin, Emin, Kerstin Ritter, Gunter Schumann, Tobias Banaschewski, Andre Marquand, Henrik Walter, George Ogoh, et al. “Generating Synthetic Task-Based Brain Fingerprints for Population Neuroscience Using Deep Learning.” Communications Biology. Springer Nature, 2025. https://doi.org/10.1038/s42003-025-09158-6. ieee: E. Serin et al., “Generating synthetic task-based brain fingerprints for population neuroscience using deep learning,” Communications Biology, vol. 8. Springer Nature, 2025. ista: Serin E, Ritter K, Schumann G, Banaschewski T, Marquand A, Walter H, Ogoh G, Stahl BC, Brandlistuen R, Schikowski T, Young AH, Xinyang Y, Zhang Z, Agunbiade K, Chen D, Desrivières S, Clinton N, Thompson P, Köhler V, Schwalber A, Calhoun VD, Chang X, Zhang Y, Li Y, Dai Y, Yuan J, Xia Y, Jia T, Renner P, Hese S, Spanlang B, Pearmund C, Athanasiadis AP, Petkoski S, Jirsa V, Schmitt K, Wilbertz JH, Patraskaki M, Sommer P, Heilmann-Heimbach S, Mathey CM, Miller AJ, Claus I, Nöthen MM, Hoffmann P, Forstner AJ, Pastor A, Gallego J, Itatani R, Eiroa-Orosa F, Feixas G, Slater M, Novarino G, Böttger SJ, Tschorn M, Rapp M, Ask H, Kjelkenes R, Fernandez S, Van Der Meer D, Westlye LT, Andreassen OA, Aden R, Seefried B, Nees F, Neidhart M, Stringaris A, Schwarz E, Holz N, Tost H, Meyer-Lindenberg A, Christmann N, Janson K, Schepanski K, Schütz T, Taron UH, Eils R, Roy JC, Lett TA, Kebir H, Polemiti E, Hitchen E, Jentsch M, Serin E, Bernas A, Vaidya N, Twardziok S, Ralser M, Heinz A, Schumann G. 2025. Generating synthetic task-based brain fingerprints for population neuroscience using deep learning. Communications Biology. 8, 1572. mla: Serin, Emin, et al. “Generating Synthetic Task-Based Brain Fingerprints for Population Neuroscience Using Deep Learning.” Communications Biology, vol. 8, 1572, Springer Nature, 2025, doi:10.1038/s42003-025-09158-6. short: E. Serin, K. Ritter, G. Schumann, T. Banaschewski, A. Marquand, H. Walter, G. Ogoh, B.C. Stahl, R. Brandlistuen, T. Schikowski, A.H. Young, Y. Xinyang, Z. Zhang, K. Agunbiade, D. Chen, S. Desrivières, N. Clinton, P. Thompson, V. Köhler, A. Schwalber, V.D. Calhoun, X. Chang, Y. Zhang, Y. Li, Y. Dai, J. Yuan, Y. Xia, T. Jia, P. Renner, S. Hese, B. Spanlang, C. Pearmund, A.P. Athanasiadis, S. Petkoski, V. Jirsa, K. Schmitt, J.H. Wilbertz, M. Patraskaki, P. Sommer, S. Heilmann-Heimbach, C.M. Mathey, A.J. Miller, I. Claus, M.M. Nöthen, P. Hoffmann, A.J. Forstner, A. Pastor, J. Gallego, R. Itatani, F. Eiroa-Orosa, G. Feixas, M. Slater, G. Novarino, S.J. Böttger, M. Tschorn, M. Rapp, H. Ask, R. Kjelkenes, S. Fernandez, D. Van Der Meer, L.T. Westlye, O.A. Andreassen, R. Aden, B. Seefried, F. Nees, M. Neidhart, A. Stringaris, E. Schwarz, N. Holz, H. Tost, A. Meyer-Lindenberg, N. Christmann, K. Janson, K. Schepanski, T. Schütz, U.H. Taron, R. Eils, J.C. Roy, T.A. Lett, H. Kebir, E. Polemiti, E. Hitchen, M. Jentsch, E. Serin, A. Bernas, N. Vaidya, S. Twardziok, M. Ralser, A. Heinz, G. Schumann, Communications Biology 8 (2025). date_created: 2025-11-23T23:01:38Z date_published: 2025-12-01T00:00:00Z date_updated: 2025-12-01T15:24:07Z day: '01' ddc: - '570' department: - _id: GaNo doi: 10.1038/s42003-025-09158-6 external_id: isi: - '001614464000001' pmid: - '41238730' file: - access_level: open_access checksum: b8b3c1abe7048a09b920082a37e786a5 content_type: application/pdf creator: dernst date_created: 2025-11-24T09:12:19Z date_updated: 2025-11-24T09:12:19Z file_id: '20675' file_name: 2025_CommunicationsBiology_Serin.pdf file_size: 1588155 relation: main_file success: 1 file_date_updated: 2025-11-24T09:12:19Z has_accepted_license: '1' intvolume: ' 8' isi: 1 language: - iso: eng month: '12' oa: 1 oa_version: Published Version pmid: 1 publication: Communications Biology publication_identifier: eissn: - 2399-3642 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Generating synthetic task-based brain fingerprints for population neuroscience using deep learning 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: 8 year: '2025' ... --- OA_place: publisher OA_type: diamond _id: '18852' abstract: - lang: eng text: 'Recent observations have found a growing number of hypervelocity stars with speeds of ≈1500 − 2500 km s−1 that could have only been produced through thermonuclear supernovae in white dwarf binaries. Most of the observed hypervelocity runaways in this class display a surprising inflated structure: their current radii are roughly an order of magnitude greater than they would have been as white dwarfs filling their Roche lobe. While many simulations exist studying the dynamical phase leading to supernova detonation in these systems, no detailed calculations of the long-term structure of the runaways have yet been performed. We used an existing AREPO hydrodynamical simulation of a supernova in a white dwarf binary as a starting point for the evolution of these stars with the one-dimensional stellar evolution code MESA. We show that the supernova shock is not energetic enough to inflate the white dwarf over timescales longer than a few thousand years, significantly shorter than the 105 − 6 year lifetimes inferred for observed hypervelocity runaways. Although they experience a shock from a supernova less than ≈0.02 R⊙ away, our models do not experience significant interior heating, and all contract back to radii of around 0.01 R⊙ within about 104 years. Explaining the observed inflated states requires either an additional source of significant heating or some other physics that is not yet accounted for in the subsequent evolution.' acknowledgement: 'This project was originally started as part of the Kavli Summer Program which took place in the Max Planck Institute for Astrophysics in Garching in July 2023, supported by the Kavli Foundation. We are grateful to Stephen Justham, Selma de Mink, and Jim Fuller for enriching discussions. We would like to thank the anonymous referee for their helpful report. A.B. was supported by the Deutsche Forschungsgemeinschaft (DFG) through grant GE2506/18-1. K.J.S. was supported by NASA through the Astrophysics Theory Program (80NSSC20K0544) and by NASA/ESA Hubble Space Telescope programs #15871 and #15918. W.E.K. was supported by NSF Grants OAC-2311323, AST-2206523, and NASA/ESA HST-AR-Theory HSTAR-16613.002-A. K.E. was supported in part by HST-GO-17441.001-A. AB and ASR would like to thank Rob Farmer for his support with PyMESA.' article_number: A114 article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Aakash full_name: Bhat, Aakash last_name: Bhat - first_name: Evan B. full_name: Bauer, Evan B. last_name: Bauer - first_name: Rüdiger full_name: Pakmor, Rüdiger last_name: Pakmor - first_name: Ken J. full_name: Shen, Ken J. last_name: Shen - first_name: Ilaria full_name: Caiazzo, Ilaria id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d last_name: Caiazzo orcid: 0000-0002-4770-5388 - first_name: Abinaya Swaruba full_name: Rajamuthukumar, Abinaya Swaruba last_name: Rajamuthukumar - first_name: Kareem full_name: El-Badry, Kareem last_name: El-Badry - first_name: Wolfgang E. full_name: Kerzendorf, Wolfgang E. last_name: Kerzendorf citation: ama: Bhat A, Bauer EB, Pakmor R, et al. Supernova shocks cannot explain the inflated state of hypervelocity runaways from white dwarf binaries. Astronomy & Astrophysics. 2025;693(1). doi:10.1051/0004-6361/202451371 apa: Bhat, A., Bauer, E. B., Pakmor, R., Shen, K. J., Caiazzo, I., Rajamuthukumar, A. S., … Kerzendorf, W. E. (2025). Supernova shocks cannot explain the inflated state of hypervelocity runaways from white dwarf binaries. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202451371 chicago: Bhat, Aakash, Evan B. Bauer, Rüdiger Pakmor, Ken J. Shen, Ilaria Caiazzo, Abinaya Swaruba Rajamuthukumar, Kareem El-Badry, and Wolfgang E. Kerzendorf. “Supernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries.” Astronomy & Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202451371. ieee: A. Bhat et al., “Supernova shocks cannot explain the inflated state of hypervelocity runaways from white dwarf binaries,” Astronomy & Astrophysics, vol. 693, no. 1. EDP Sciences, 2025. ista: Bhat A, Bauer EB, Pakmor R, Shen KJ, Caiazzo I, Rajamuthukumar AS, El-Badry K, Kerzendorf WE. 2025. Supernova shocks cannot explain the inflated state of hypervelocity runaways from white dwarf binaries. Astronomy & Astrophysics. 693(1), A114. mla: Bhat, Aakash, et al. “Supernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries.” Astronomy & Astrophysics, vol. 693, no. 1, A114, EDP Sciences, 2025, doi:10.1051/0004-6361/202451371. short: A. Bhat, E.B. Bauer, R. Pakmor, K.J. Shen, I. Caiazzo, A.S. Rajamuthukumar, K. El-Badry, W.E. Kerzendorf, Astronomy & Astrophysics 693 (2025). date_created: 2025-01-19T23:01:51Z date_published: 2025-01-07T00:00:00Z date_updated: 2026-02-16T12:08:05Z day: '07' ddc: - '520' department: - _id: IlCa doi: 10.1051/0004-6361/202451371 external_id: arxiv: - '2407.03424' isi: - '001406577300001' file: - access_level: open_access checksum: e532b9c8123c29cfb0ee758e6d00453c content_type: application/pdf creator: dernst date_created: 2025-01-20T09:57:00Z date_updated: 2025-01-20T09:57:00Z file_id: '18861' file_name: 2025_AstronomyAstrophysics_Bhat.pdf file_size: 1692527 relation: main_file success: 1 file_date_updated: 2025-01-20T09:57:00Z has_accepted_license: '1' intvolume: ' 693' isi: 1 issue: '1' language: - iso: eng month: '01' oa: 1 oa_version: Published Version publication: Astronomy & Astrophysics publication_identifier: eissn: - 1432-0746 issn: - 0004-6361 publication_status: published publisher: EDP Sciences quality_controlled: '1' scopus_import: '1' status: public title: Supernova shocks cannot explain the inflated state of hypervelocity runaways from white dwarf 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: 693 year: '2025' ... --- OA_place: publisher OA_type: diamond _id: '18854' abstract: - lang: eng text: "Context. One of the surprising early findings with JWST has been the discovery of a strong “roll-over” or a softening of the absorption edge of Lyα in a large number of galaxies at z ≳ 6, in addition to systematic offsets from photometric redshift estimates and fundamental galaxy scaling relations. This has been interpreted as strong cumulative damped Lyα absorption (DLA) wings from high column densities of neutral atomic hydrogen (H I), signifying major gas accretion events in the formation of these galaxies.\r\nAims. To explore this new phenomenon systematically, we assembled the JWST/NIRSpec PRImordial gas Mass AssembLy (PRIMAL) legacy survey of 584 galaxies at z = 5.0 − 13.4, designed to study the physical properties and gas in and around galaxies during the reionization epoch.\r\nMethods. We characterized this benchmark sample in full and spectroscopically derived the galaxy redshifts, metallicities, star formation rates, and ultraviolet (UV) slopes. We defined a new diagnostic, the Lyα damping parameter DLyα, to measure and quantify the net effect of Lyα emission strength, the H I fraction in the intergalactic medium, or the local H I column density for each source. The JWST-PRIMAL survey is based on the spectroscopic DAWN JWST Archive (DJA-Spec). We describe DJA-Spec in this paper, detailing the reduction methods, the post-processing steps, and basic analysis tools. All the software, reduced spectra, and spectroscopically derived quantities and catalogs are made publicly available in dedicated repositories.\r\nResults. We find that the fraction of galaxies showing strong integrated DLAs with NHI > 1021 cm−2 only increases slightly from ≈60% at z ≈ 6 up to ≈65 − 90% at z > 8. Similarly, the prevalence and prominence of Lyα emission is found to increase with decreasing redshift, in qualitative agreement with previous observational results. Strong Lyα emitters (LAEs) are predominantly found to be associated with low-metallicity and UV faint galaxies. By contrast, strong DLAs are observed in galaxies with a variety of intrinsic physical properties, but predominantly at high redshifts and low metallicities.\r\nConclusions. Our results indicate that strong DLAs likely reflect a particular early assembly phase of reionization-era galaxies, at which point they are largely dominated by pristine H I gas accretion. At z = 8 − 10, this gas gradually cools and forms into stars that ionize their local surroundings, forming large ionized bubbles and producing strong observed Lyα emission at z < 8." acknowledgement: 'We would like to thank the referee for a detailed and constructive report, greatly improving the presentation of the results in this work. We would like to thank Peter Jakobsen for his vision and heroic endeavor in optimally designing the JWST/NIRSpec instrument and some of its first on-sky observations and for enlightening discussions about the intricacies of the NIRSpec data. Further, we would like to thank John Chisholm for helpful clarifications and discussions related to the escape fraction of ionizing photons and Aayush Saxena for enlightening conversations on the escape and absorption of Lyman-α photons. This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI) under contract number MB22.00072. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant DNRF140. The data products presented herein were retrieved from the DAWN JWST Archive (DJA). DJA is an initiative of the Cosmic Dawn Center, which is funded by the Danish National Research Foundation under grant DNRF140. P.D. acknowledge support from the NWO grant 016.VIDI.189.162 (“ODIN") and warmly thanks the European Commission’s and University of Groningen’s CO-FUND Rosalind Franklin program. Support from the ERC Advanced Grant INTERSTELLAR H2020/740120 is kindly acknowledged (A.F.). S.G. acknowledges financial support from the Villum Young Investigator grants 37440 and 13160 and the Cosmic Dawn Center. M.K. was supported by the ANID BASAL project FB210003. G.E.M. acknowledges financial support from the Villum Young Investigator grants 37440 and 13160 and the Cosmic Dawn Center. J.W. acknowledges support from the Science and Technology Facilities Council (STFC), by the ERC through Advanced Grant 695671 “QUENCH”, by the UKRI Frontier Research grant RISEandFALL. Support for this work was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. F.C. acknowledges support from a UKRI Frontier Research Guarantee Grant (PI Cullen; grant reference EP/X021025/1). J.H.W. acknowledges support by NSF grant AST-2108020 and NASA grants 80NSSC20K0520 and 80NSSC21K1053. NRT acknowledges support through STFC consolidated grant ST/W000857/1. M.J.H. is supported by the Swedish Research Council, VetenskapsrÅdet, and is fellow of the Knut & Alice Wallenberg foundation. This 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 (MAST) 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. Software: This work made use of and acknowledge the following software: NumPy (Harris et al. 2020), Matplotlib (Hunter 2007), LMfit (Newville et al. 2014), SciPy (Virtanen et al. 2020), grizli (Brammer 2023a), Astrodrizzle (Gonzaga et al. 2012), and MsaExp (v0.3; Brammer 2023b).' article_number: A60 article_processing_charge: No article_type: original author: - first_name: K. E. full_name: Heintz, K. E. last_name: Heintz - first_name: G. B. full_name: Brammer, G. B. last_name: Brammer - first_name: D. full_name: Watson, D. last_name: Watson - first_name: P. A. full_name: Oesch, P. A. last_name: Oesch - first_name: L. C. full_name: Keating, L. C. last_name: Keating - first_name: M. J. full_name: Hayes, M. J. last_name: Hayes - first_name: Unknown full_name: Abdurro'Uf, Unknown last_name: Abdurro'Uf - first_name: K. Z. full_name: Arellano-Córdova, K. Z. last_name: Arellano-Córdova - first_name: A. C. full_name: Carnall, A. C. last_name: Carnall - first_name: C. R. full_name: Christiansen, C. R. last_name: Christiansen - first_name: F. full_name: Cullen, F. last_name: Cullen - first_name: R. full_name: Davé, R. last_name: Davé - first_name: P. full_name: Dayal, P. last_name: Dayal - first_name: A. full_name: Ferrara, A. last_name: Ferrara - first_name: K. full_name: Finlator, K. last_name: Finlator - first_name: J. P.U. full_name: Fynbo, J. P.U. last_name: Fynbo - first_name: S. R. full_name: Flury, S. R. last_name: Flury - first_name: V. full_name: Gelli, V. last_name: Gelli - first_name: S. full_name: Gillman, S. last_name: Gillman - first_name: R. full_name: Gottumukkala, R. last_name: Gottumukkala - first_name: K. full_name: Gould, K. last_name: Gould - first_name: T. R. full_name: Greve, T. R. last_name: Greve - first_name: S. E. full_name: Hardin, S. E. last_name: Hardin - first_name: T. Y.Y. full_name: Hsiao, T. Y.Y. last_name: Hsiao - first_name: A. full_name: Hutter, A. last_name: Hutter - first_name: P. full_name: Jakobsson, P. last_name: Jakobsson - first_name: M. full_name: Killi, M. last_name: Killi - first_name: N. full_name: Khosravaninezhad, N. last_name: Khosravaninezhad - first_name: P. full_name: Laursen, P. last_name: Laursen - first_name: M. M. full_name: Lee, M. M. last_name: Lee - first_name: G. E. full_name: Magdis, G. E. last_name: Magdis - 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: R. P. full_name: Naidu, R. P. last_name: Naidu - first_name: D. full_name: Narayanan, D. last_name: Narayanan - first_name: C. full_name: Pollock, C. last_name: Pollock - first_name: M. K.M. full_name: Prescott, M. K.M. last_name: Prescott - first_name: V. full_name: Rusakov, V. last_name: Rusakov - first_name: M. full_name: Shuntov, M. last_name: Shuntov - first_name: A. full_name: Sneppen, A. last_name: Sneppen - first_name: R. full_name: Smit, R. last_name: Smit - first_name: N. R. full_name: Tanvir, N. R. last_name: Tanvir - first_name: C. full_name: Terp, C. last_name: Terp - first_name: S. full_name: Toft, S. last_name: Toft - first_name: F. full_name: Valentino, F. last_name: Valentino - first_name: A. P. full_name: Vijayan, A. P. last_name: Vijayan - first_name: J. R. full_name: Weaver, J. R. last_name: Weaver - first_name: J. H. full_name: Wise, J. H. last_name: Wise - first_name: J. full_name: Witstok, J. last_name: Witstok citation: ama: 'Heintz KE, Brammer GB, Watson D, et al. The JWST-PRIMAL archival survey: A JWST/NIRSpec reference sample for the physical properties and Lyman-α absorption and emission of ∼600 galaxies at z = 5.0-13.4. Astronomy & Astrophysics. 2025;693. doi:10.1051/0004-6361/202450243' apa: 'Heintz, K. E., Brammer, G. B., Watson, D., Oesch, P. A., Keating, L. C., Hayes, M. J., … Witstok, J. (2025). The JWST-PRIMAL archival survey: A JWST/NIRSpec reference sample for the physical properties and Lyman-α absorption and emission of ∼600 galaxies at z = 5.0-13.4. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202450243' chicago: 'Heintz, K. E., G. B. Brammer, D. Watson, P. A. Oesch, L. C. Keating, M. J. Hayes, Unknown Abdurro’Uf, et al. “The JWST-PRIMAL Archival Survey: A JWST/NIRSpec Reference Sample for the Physical Properties and Lyman-α Absorption and Emission of ∼600 Galaxies at z = 5.0-13.4.” Astronomy & Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202450243.' ieee: 'K. E. Heintz et al., “The JWST-PRIMAL archival survey: A JWST/NIRSpec reference sample for the physical properties and Lyman-α absorption and emission of ∼600 galaxies at z = 5.0-13.4,” Astronomy & Astrophysics, vol. 693. EDP Sciences, 2025.' ista: 'Heintz KE, Brammer GB, Watson D, Oesch PA, Keating LC, Hayes MJ, Abdurro’Uf U, Arellano-Córdova KZ, Carnall AC, Christiansen CR, Cullen F, Davé R, Dayal P, Ferrara A, Finlator K, Fynbo JPU, Flury SR, Gelli V, Gillman S, Gottumukkala R, Gould K, Greve TR, Hardin SE, Hsiao TYY, Hutter A, Jakobsson P, Killi M, Khosravaninezhad N, Laursen P, Lee MM, Magdis GE, Matthee JJ, Naidu RP, Narayanan D, Pollock C, Prescott MKM, Rusakov V, Shuntov M, Sneppen A, Smit R, Tanvir NR, Terp C, Toft S, Valentino F, Vijayan AP, Weaver JR, Wise JH, Witstok J. 2025. The JWST-PRIMAL archival survey: A JWST/NIRSpec reference sample for the physical properties and Lyman-α absorption and emission of ∼600 galaxies at z = 5.0-13.4. Astronomy & Astrophysics. 693, A60.' mla: 'Heintz, K. E., et al. “The JWST-PRIMAL Archival Survey: A JWST/NIRSpec Reference Sample for the Physical Properties and Lyman-α Absorption and Emission of ∼600 Galaxies at z = 5.0-13.4.” Astronomy & Astrophysics, vol. 693, A60, EDP Sciences, 2025, doi:10.1051/0004-6361/202450243.' short: K.E. Heintz, G.B. Brammer, D. Watson, P.A. Oesch, L.C. Keating, M.J. Hayes, U. Abdurro’Uf, K.Z. Arellano-Córdova, A.C. Carnall, C.R. Christiansen, F. Cullen, R. Davé, P. Dayal, A. Ferrara, K. Finlator, J.P.U. Fynbo, S.R. Flury, V. Gelli, S. Gillman, R. Gottumukkala, K. Gould, T.R. Greve, S.E. Hardin, T.Y.Y. Hsiao, A. Hutter, P. Jakobsson, M. Killi, N. Khosravaninezhad, P. Laursen, M.M. Lee, G.E. Magdis, J.J. Matthee, R.P. Naidu, D. Narayanan, C. Pollock, M.K.M. Prescott, V. Rusakov, M. Shuntov, A. Sneppen, R. Smit, N.R. Tanvir, C. Terp, S. Toft, F. Valentino, A.P. Vijayan, J.R. Weaver, J.H. Wise, J. Witstok, Astronomy & Astrophysics 693 (2025). date_created: 2025-01-19T23:01:52Z date_published: 2025-01-06T00:00:00Z date_updated: 2026-02-16T12:07:37Z day: '06' ddc: - '520' department: - _id: JoMa doi: 10.1051/0004-6361/202450243 external_id: isi: - '001390856800001' file: - access_level: open_access checksum: 67a791080ade9bfb449d249de2af7456 content_type: application/pdf creator: dernst date_created: 2025-01-20T09:17:33Z date_updated: 2025-01-20T09:17:33Z file_id: '18858' file_name: 2025_AstronomyAstrophysics_Heintz.pdf file_size: 4513466 relation: main_file success: 1 file_date_updated: 2025-01-20T09:17:33Z has_accepted_license: '1' intvolume: ' 693' isi: 1 language: - iso: eng month: '01' oa: 1 oa_version: Published Version publication: Astronomy & Astrophysics publication_identifier: eissn: - 1432-0746 issn: - 0004-6361 publication_status: published publisher: EDP Sciences quality_controlled: '1' scopus_import: '1' status: public title: 'The JWST-PRIMAL archival survey: A JWST/NIRSpec reference sample for the physical properties and Lyman-α absorption and emission of ∼600 galaxies at z = 5.0-13.4' 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: 693 year: '2025' ... --- OA_place: publisher OA_type: hybrid _id: '18936' abstract: - lang: eng text: A major obstacle to predictive understanding of evolution stems from the complexity of biological systems, which prevents detailed characterization of key evolutionary properties. Here, we highlight some of the major sources of complexity that arise when relating molecular mechanisms to their evolutionary consequences and ask whether accounting for every mechanistic detail is important to accurately predict evolutionary outcomes. To do this, we developed a mechanistic model of a bacterial promoter regulated by 2 proteins, allowing us to connect any promoter genotype to 6 phenotypes that capture the dynamics of gene expression following an environmental switch. Accounting for the mechanisms that govern how this system works enabled us to provide an in-depth picture of how regulated bacterial promoters might evolve. More importantly, we used the model to explore which factors that contribute to the complexity of this system are essential for understanding its evolution, and which can be simplified without information loss. We found that several key evolutionary properties—the distribution of phenotypic and fitness effects of mutations, the evolutionary trajectories during selection for regulation—can be accurately captured without accounting for all, or even most, parameters of the system. Our findings point to the need for a mechanistic approach to studying evolution, as it enables tackling biological complexity and in doing so improves the ability to predict evolutionary outcomes. acknowledgement: "The authors thank Nick Barton, Stepan Denisov, Claudia Igler, Srdjan Sarikas, Anna Staron, and the anonymous reviewers for useful comments and discussions that helped improve our work.\r\nFunding for this work was provided by the Wellcome Trust–Royal Society Sir Henry Dale Fellowship (216779/Z/19/Z) and the Royal Society Research Grant (RG\\R2\\232522) to M.L." article_number: iyae191 article_processing_charge: Yes (in subscription journal) article_type: original author: - first_name: Rok full_name: Grah, Rok id: 483E70DE-F248-11E8-B48F-1D18A9856A87 last_name: Grah orcid: 0000-0003-2539-3560 - first_name: Calin C full_name: Guet, Calin C id: 47F8433E-F248-11E8-B48F-1D18A9856A87 last_name: Guet orcid: 0000-0001-6220-2052 - first_name: Gašper full_name: Tkačik, Gašper id: 3D494DCA-F248-11E8-B48F-1D18A9856A87 last_name: Tkačik orcid: 0000-0002-6699-1455 - first_name: Mato full_name: Lagator, Mato id: 345D25EC-F248-11E8-B48F-1D18A9856A87 last_name: Lagator citation: ama: 'Grah R, Guet CC, Tkačik G, Lagator M. Linking molecular mechanisms to their evolutionary consequences: a primer. Genetics. 2025;229(2). doi:10.1093/genetics/iyae191' apa: 'Grah, R., Guet, C. C., Tkačik, G., & Lagator, M. (2025). Linking molecular mechanisms to their evolutionary consequences: a primer. Genetics. Oxford University Press. https://doi.org/10.1093/genetics/iyae191' chicago: 'Grah, Rok, Calin C Guet, Gašper Tkačik, and Mato Lagator. “Linking Molecular Mechanisms to Their Evolutionary Consequences: A Primer.” Genetics. Oxford University Press, 2025. https://doi.org/10.1093/genetics/iyae191.' ieee: 'R. Grah, C. C. Guet, G. Tkačik, and M. Lagator, “Linking molecular mechanisms to their evolutionary consequences: a primer,” Genetics, vol. 229, no. 2. Oxford University Press, 2025.' ista: 'Grah R, Guet CC, Tkačik G, Lagator M. 2025. Linking molecular mechanisms to their evolutionary consequences: a primer. Genetics. 229(2), iyae191.' mla: 'Grah, Rok, et al. “Linking Molecular Mechanisms to Their Evolutionary Consequences: A Primer.” Genetics, vol. 229, no. 2, iyae191, Oxford University Press, 2025, doi:10.1093/genetics/iyae191.' short: R. Grah, C.C. Guet, G. Tkačik, M. Lagator, Genetics 229 (2025). corr_author: '1' date_created: 2025-01-29T08:21:35Z date_published: 2025-02-01T00:00:00Z date_updated: 2025-05-19T14:08:02Z day: '01' ddc: - '570' department: - _id: CaGu - _id: GaTk doi: 10.1093/genetics/iyae191 external_id: isi: - '001379194200001' pmid: - '39601269' file: - access_level: open_access checksum: f730e416795969449ef49d97b82ac494 content_type: application/pdf creator: dernst date_created: 2025-04-16T09:41:04Z date_updated: 2025-04-16T09:41:04Z file_id: '19580' file_name: 2025_Genetics_Grah.pdf file_size: 1511688 relation: main_file success: 1 file_date_updated: 2025-04-16T09:41:04Z has_accepted_license: '1' intvolume: ' 229' isi: 1 issue: '2' language: - iso: eng month: '02' oa: 1 oa_version: Published Version pmid: 1 publication: Genetics publication_identifier: eissn: - 1943-2631 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: 'Linking molecular mechanisms to their evolutionary consequences: a primer' 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: 229 year: '2025' ... --- OA_place: publisher _id: '19025' abstract: - lang: eng text: 'A complete understanding of the central stars of planetary nebulae (CSPNe) remains elusive. Over the past several decades, time-series photometry of CSPNe has yielded significant results including, but not limited to, discoveries of nearly 100 binary systems, insights into pulsations and winds in young white dwarfs, and studies of stars undergoing very late thermal pulses. We have undertaken a systematic study of optical photometric variability of cataloged CSPNe, using the light curves from the Zwicky Transient Facility (ZTF). By applying appropriate variability metrics, we arrive at a list of 94 highly variable CSPN candidates. Based on the timescales of the light-curve activity, we classify the variables broadly into short- and long-timescale variables. In this first paper in this series, we focus on the former, which is the majority class comprising 83 objects. We report periods for six sources for the first time, and recover several known periodic variables. Among the aperiodic sources, most exhibit a jitter around a median flux with a stable amplitude, and a few show outbursts. We draw attention to WeSb 1, which shows a different kind of variability: prominent deep and aperiodic dips, resembling transits from a dust/debris disk. We find strong evidence for a binary nature of WeSb 1 (possibly an F-type subgiant companion). The compactness of the emission lines and inferred high electron densities make WeSb 1 a candidate for either an EGB 6-type planetary nucleus, or a symbiotic system inside an evolved planetary nebula, both of which are rare objects. To demonstrate further promise with ZTF, we report three additional newly identified periodic sources that do not appear in the list of highly variable sources. Finally, we also introduce a two-dimensional metric space defined by the von Neumann statistics and Pearson Skew and demonstrate its effectiveness in identifying unique variables of astrophysical interest, like WeSb 1.' acknowledgement: "This work is based on observations obtained with the Samuel Oschin Telescope 48 inch and the 60 inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under grants No. AST-1440341 and AST-2034437 and a collaboration including current partners Caltech, IPAC, the Oskar Klein Center at Stockholm University, the University of Maryland, University of California, Berkeley, the University of Wisconsin at Milwaukee, University of Warwick, Ruhr University Bochum, Cornell University, Northwestern University, and Drexel University. Operations are conducted by COO, IPAC, and UW.\r\n\r\nThis 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.\r\n\r\nWe are grateful to the staffs of Palomar Observatory and the Hobby-Eberly Telescope for assistance with the observations and data management. The Liverpool Telescope is operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council.\r\n\r\nThe Low-Resolution Spectrograph 2 (LRS2) on HET was developed and funded by the University of Texas at Austin McDonald Observatory and Department of Astronomy, and by Pennsylvania State University. We thank the Leibniz-Institut für Astrophysik Potsdam (AIP) and the Institut für Astrophysik Göttingen (IAG) for their contributions to the construction of the integral field units. We acknowledge the Texas Advanced Computing Center (TACC) at The University of Texas at Austin for providing high performance computing, visualization, and storage resources that have contributed to the results reported within this paper.\r\n\r\nWe thank the anonymous referee for the detailed comments, which improved the clarity of the manuscript significantly. We also thank Gunter Cibis for pointing out typographical errors in the names of a few PNe in the first draft. S.B. expresses gratitude to Kishalay De for providing the Gattini-IR and WISE data. S.B. thanks Frank J. Masci and Zachary P. Vanderbosch for useful discussions and suggestions regarding solving the issues with ZTF forced photometry on extended sources. S.B. also thanks Jim Fuller, Charles C. Steidel, Lynne Hillenbrand, and Adolfo Carvalho for useful discussions on methods and science. S.B. also thanks David O. Cook for providing access to his CLU image cutout service to generate the WeSb 1 image. S.B. acknowledges the financial support from the Wallace L. W. Sargent Graduate Fellowship during the first year of his graduate studies at Caltech. N.C. was supported through the Cancer Research UK grant A24042. S.B. thanks Martina Veresvarka for drawing our attention to the TESS light curves of WeSb 1.\r\n\r\nWe have used Python packages Numpy (Harris et al. 2020), SciPy (Virtanen et al. 2020), Matplotlib (Hunter 2007), Pandas (pandas development team 2020), Astropy (Astropy Collaboration et al. 2013, 2018), and Astroquery (Ginsburg et al. 2019) at various stages of this research." article_number: '024201' article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Soumyadeep full_name: Bhattacharjee, Soumyadeep last_name: Bhattacharjee - first_name: S. R. full_name: Kulkarni, S. R. last_name: Kulkarni - first_name: Albert K.H. full_name: Kong, Albert K.H. last_name: Kong - first_name: M. S. full_name: Tam, M. S. last_name: Tam - first_name: Howard E. full_name: Bond, Howard E. last_name: Bond - first_name: Kareem full_name: El-Badry, Kareem last_name: El-Badry - first_name: Ilaria full_name: Caiazzo, Ilaria id: 8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d last_name: Caiazzo orcid: 0000-0002-4770-5388 - first_name: Nicholas full_name: Chornay, Nicholas last_name: Chornay - first_name: Matthew J. full_name: Graham, Matthew J. last_name: Graham - first_name: Antonio C. full_name: Rodriguez, Antonio C. last_name: Rodriguez - first_name: Gregory R. full_name: Zeimann, Gregory R. last_name: Zeimann - first_name: Christoffer full_name: Fremling, Christoffer last_name: Fremling - first_name: Andrew J. full_name: Drake, Andrew J. last_name: Drake - first_name: Klaus full_name: Werner, Klaus last_name: Werner - first_name: Hector full_name: Rodriguez, Hector last_name: Rodriguez - first_name: Thomas A. full_name: Prince, Thomas A. last_name: Prince - first_name: Russ R. full_name: Laher, Russ R. last_name: Laher - first_name: Tracy X. full_name: Chen, Tracy X. last_name: Chen - first_name: Reed full_name: Riddle, Reed last_name: Riddle citation: ama: Bhattacharjee S, Kulkarni SR, Kong AKH, et al. Variability of central stars of planetary nebulae with the zwicky transient facility. I. Methods, short-timescale variables, and the unusual nucleus of WeSb 1. Publications of the Astronomical Society of the Pacific. 2025;137(2). doi:10.1088/1538-3873/ada702 apa: Bhattacharjee, S., Kulkarni, S. R., Kong, A. K. H., Tam, M. S., Bond, H. E., El-Badry, K., … Riddle, R. (2025). Variability of central stars of planetary nebulae with the zwicky transient facility. I. Methods, short-timescale variables, and the unusual nucleus of WeSb 1. Publications of the Astronomical Society of the Pacific. IOP Publishing. https://doi.org/10.1088/1538-3873/ada702 chicago: Bhattacharjee, Soumyadeep, S. R. Kulkarni, Albert K.H. Kong, M. S. Tam, Howard E. Bond, Kareem El-Badry, Ilaria Caiazzo, et al. “Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. I. Methods, Short-Timescale Variables, and the Unusual Nucleus of WeSb 1.” Publications of the Astronomical Society of the Pacific. IOP Publishing, 2025. https://doi.org/10.1088/1538-3873/ada702. ieee: S. Bhattacharjee et al., “Variability of central stars of planetary nebulae with the zwicky transient facility. I. Methods, short-timescale variables, and the unusual nucleus of WeSb 1,” Publications of the Astronomical Society of the Pacific, vol. 137, no. 2. IOP Publishing, 2025. ista: Bhattacharjee S, Kulkarni SR, Kong AKH, Tam MS, Bond HE, El-Badry K, Caiazzo I, Chornay N, Graham MJ, Rodriguez AC, Zeimann GR, Fremling C, Drake AJ, Werner K, Rodriguez H, Prince TA, Laher RR, Chen TX, Riddle R. 2025. Variability of central stars of planetary nebulae with the zwicky transient facility. I. Methods, short-timescale variables, and the unusual nucleus of WeSb 1. Publications of the Astronomical Society of the Pacific. 137(2), 024201. mla: Bhattacharjee, Soumyadeep, et al. “Variability of Central Stars of Planetary Nebulae with the Zwicky Transient Facility. I. Methods, Short-Timescale Variables, and the Unusual Nucleus of WeSb 1.” Publications of the Astronomical Society of the Pacific, vol. 137, no. 2, 024201, IOP Publishing, 2025, doi:10.1088/1538-3873/ada702. short: S. Bhattacharjee, S.R. Kulkarni, A.K.H. Kong, M.S. Tam, H.E. Bond, K. El-Badry, I. Caiazzo, N. Chornay, M.J. Graham, A.C. Rodriguez, G.R. Zeimann, C. Fremling, A.J. Drake, K. Werner, H. Rodriguez, T.A. Prince, R.R. Laher, T.X. Chen, R. Riddle, Publications of the Astronomical Society of the Pacific 137 (2025). date_created: 2025-02-16T23:02:33Z date_published: 2025-02-01T00:00:00Z date_updated: 2025-09-30T10:32:17Z day: '01' ddc: - '520' department: - _id: IlCa doi: 10.1088/1538-3873/ada702 external_id: arxiv: - '2410.03589' isi: - '001416903300001' file: - access_level: open_access checksum: 42b942ee1bf32ed225024e168174be92 content_type: application/pdf creator: dernst date_created: 2025-02-17T09:13:41Z date_updated: 2025-02-17T09:13:41Z file_id: '19034' file_name: 2025_PASP_Bhattacharjee.pdf file_size: 3657568 relation: main_file success: 1 file_date_updated: 2025-02-17T09:13:41Z has_accepted_license: '1' intvolume: ' 137' isi: 1 issue: '2' language: - iso: eng license: https://creativecommons.org/licenses/by/3.0/ month: '02' oa: 1 oa_version: Published Version publication: Publications of the Astronomical Society of the Pacific publication_identifier: issn: - 0004-6280 issnl: - 0004-6280 publication_status: published publisher: IOP Publishing quality_controlled: '1' related_material: link: - relation: erratum url: https://doi.org/10.1088/1538-3873/adbcd8 scopus_import: '1' status: public title: Variability of central stars of planetary nebulae with the zwicky transient facility. I. Methods, short-timescale variables, and the unusual nucleus of WeSb 1 tmp: image: /images/cc_by.png legal_code_url: https://creativecommons.org/licenses/by/3.0/legalcode name: Creative Commons Attribution 3.0 Unported (CC BY 3.0) short: CC BY (3.0) type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 137 year: '2025' ... --- OA_type: closed access _id: '19075' abstract: - lang: eng text: Thermoelectric (TE) materials can convert the heat produced during biochemical reactions into electrical signals, enabling the self-powered detection of biomarkers. In this work, we design and fabricate a simple Ag2Se nanofilm-based TE biosensor to precisely quantify hydrogen peroxide (H2O2) levels in liquid samples. A chemical reaction involving horseradish peroxidase, ABTS and H2O2 in the specimens produces a photothermal agent—ABTS (2,2′-azino-bis(3-ethylbenzothiazoline-6-sulfonic acid)) free radical, which triggers the heat fluctuations at the TE sensor through the photo-thermal effect, eventually enabling the sensing of H2O2. Consequently, the constructed sensor can achieve a detection limit of 0.26 μM by a three-leg TE device design. Further investigations suggest that the application of our TE sensor can be extended in testing H2O2 in beverages (including milk, soda water, and lemonade) and evaluating the load of bacterial pathogens relevant to dental diseases and infections including Streptococcus sanguinis and Methicillin-resistant Staphylococcus aureus with high analytical accuracy. This strategy utilizes the combination of high thermoelectric performance with chemical reactions to realize a straightforward and accurate biomarker detection method, making it suitable for applications in medical diagnostics, personalized health monitoring, and the food industry. acknowledgement: This work was supported by the Sichuan Science and Technology Program (Grant No. 2023YFG0220, 2023ZYD0064, and 2024YFHZ0309) and the Fundamental Research Funds for the Central Universities and Research Funding from West China School/Hospital of Stomatology Sichuan University, No. QDJF2022-2. article_processing_charge: No article_type: original author: - first_name: Huangshui full_name: Ma, Huangshui last_name: Ma - first_name: Shiyu full_name: Pu, Shiyu last_name: Pu - first_name: Shiyu full_name: Jia, Shiyu last_name: Jia - first_name: Shengduo full_name: Xu, Shengduo id: 12ab8624-4c8a-11ec-9e11-e1ac2438f22f last_name: Xu - first_name: Qiwei full_name: Yu, Qiwei last_name: Yu - first_name: Lei full_name: Yang, Lei last_name: Yang - first_name: Hao full_name: Wu, Hao last_name: Wu - first_name: Qiang full_name: Sun, Qiang last_name: Sun citation: ama: Ma H, Pu S, Jia S, et al. Laser-assisted thermoelectric-enhanced hydrogen peroxide biosensors based on Ag2Se nanofilms for sensitive detection of bacterial pathogens. Nanoscale. 2025;17(10):5858-5868. doi:10.1039/d4nr04860a apa: Ma, H., Pu, S., Jia, S., Xu, S., Yu, Q., Yang, L., … Sun, Q. (2025). Laser-assisted thermoelectric-enhanced hydrogen peroxide biosensors based on Ag2Se nanofilms for sensitive detection of bacterial pathogens. Nanoscale. Royal Society of Chemistry. https://doi.org/10.1039/d4nr04860a chicago: Ma, Huangshui, Shiyu Pu, Shiyu Jia, Shengduo Xu, Qiwei Yu, Lei Yang, Hao Wu, and Qiang Sun. “Laser-Assisted Thermoelectric-Enhanced Hydrogen Peroxide Biosensors Based on Ag2Se Nanofilms for Sensitive Detection of Bacterial Pathogens.” Nanoscale. Royal Society of Chemistry, 2025. https://doi.org/10.1039/d4nr04860a. ieee: H. Ma et al., “Laser-assisted thermoelectric-enhanced hydrogen peroxide biosensors based on Ag2Se nanofilms for sensitive detection of bacterial pathogens,” Nanoscale, vol. 17, no. 10. Royal Society of Chemistry, pp. 5858–5868, 2025. ista: Ma H, Pu S, Jia S, Xu S, Yu Q, Yang L, Wu H, Sun Q. 2025. Laser-assisted thermoelectric-enhanced hydrogen peroxide biosensors based on Ag2Se nanofilms for sensitive detection of bacterial pathogens. Nanoscale. 17(10), 5858–5868. mla: Ma, Huangshui, et al. “Laser-Assisted Thermoelectric-Enhanced Hydrogen Peroxide Biosensors Based on Ag2Se Nanofilms for Sensitive Detection of Bacterial Pathogens.” Nanoscale, vol. 17, no. 10, Royal Society of Chemistry, 2025, pp. 5858–68, doi:10.1039/d4nr04860a. short: H. Ma, S. Pu, S. Jia, S. Xu, Q. Yu, L. Yang, H. Wu, Q. Sun, Nanoscale 17 (2025) 5858–5868. date_created: 2025-02-23T23:01:57Z date_published: 2025-03-14T00:00:00Z date_updated: 2025-09-30T10:38:50Z day: '14' department: - _id: MaIb doi: 10.1039/d4nr04860a external_id: isi: - '001416656400001' pmid: - '39927897' intvolume: ' 17' isi: 1 issue: '10' language: - iso: eng month: '03' oa_version: None page: 5858-5868 pmid: 1 publication: Nanoscale publication_identifier: eissn: - 2040-3372 issn: - 2040-3364 publication_status: published publisher: Royal Society of Chemistry quality_controlled: '1' scopus_import: '1' status: public title: Laser-assisted thermoelectric-enhanced hydrogen peroxide biosensors based on Ag2Se nanofilms for sensitive detection of bacterial pathogens type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 17 year: '2025' ... --- OA_place: publisher OA_type: diamond _id: '19284' abstract: - lang: eng text: The Hα nebular emission line is an optimal tracer for recent star formation in galaxies. With the advent of JWST, this line has recently become observable at z > 3 for the first time. We present a catalog of 1050 Hα emitters at 3.7 < z < 6.7 in the GOODS fields obtained from a blind search in JWST NIRCam/grism data. We made use of the FRESCO survey’s 124 arcmin2 of observations in GOODS-North and GOODS-South with the F444W filter, probing Hα at 4.9 < z < 6.7, and the CONGRESS survey’s 62 arcmin2 of observations in GOODS-North with F356W, probing Hα at 3.8 < z < 5.1. We found an overdensity with 98 sources at z ∼ 4.4 in GOODS-N, and confirmed previously reported overdensities at z ∼ 5.2 in GOODS-N and at z ∼ 5.4 and z ∼ 5.9 in GOODS-S. We computed the observed Hα luminosity functions (LFs) in three bins centered at z ∼ 4.45, 5.30, and 6.15, which are the first such measurements at z > 3 obtained based purely on spectroscopic data, robustly tracing galaxy star formation rates (SFRs) beyond the peak of the cosmic star formation history. We compared our results with theoretical predictions from three different simulations and found good agreement at z ∼ 4 − 6. The UV LFs of this spectroscopically confirmed sample are in good agreement with pre-JWST measurements obtained with photometrically selected objects. Finally, we derived SFR functions and integrated them to compute the evolution of the cosmic SFR densities across z ∼ 4 − 6, finding values in good agreement with recent UV estimates from Lyman-break galaxies, which imply a continuous decrease in SFR density by a factor of three over z ∼ 4 to z ∼ 6. Our work shows the power of NIRCam grism observations to efficiently provide new tests for early galaxy formation models based on emission line statistics. acknowledgement: 'This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program Nos. 1895 and 3577. The authors sincerely thank the CONGRESS team (PIs: Egami & Sun) for developing their observing program with a zero-exclusive-access period. We thank Aswin Vijayan and Harley Katz for their help in analyzing the simulation data from FLARES and SPHINX. This work has received funding from the Swiss State Secretariat for Education, Research, and Innovation (SERI) under contract number MB22.00072, as well as from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant DNRF140. Support for program #1895 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. 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. MS acknowledges support from the European Research Commission Consolidator Grant 101088789 (SFEER), from the CIDEGENT/2021/059 grant by Generalitat Valenciana, and from project PID2023-149420NB-I00 funded by MICIU/AEI/10.13039/501100011033 and by ERDF/EU.' article_number: A178 article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Alba full_name: Covelo-Paz, Alba last_name: Covelo-Paz - first_name: Emma full_name: Giovinazzo, Emma last_name: Giovinazzo - first_name: Pascal A. full_name: Oesch, Pascal A. last_name: Oesch - first_name: Romain A. full_name: Meyer, Romain A. last_name: Meyer - first_name: Andrea full_name: Weibel, Andrea last_name: Weibel - first_name: Gabriel full_name: Brammer, Gabriel last_name: Brammer - first_name: Yoshinobu full_name: Fudamoto, Yoshinobu last_name: Fudamoto - first_name: Josephine full_name: Kerutt, Josephine last_name: Kerutt - first_name: Jamie full_name: Lin, Jamie last_name: Lin - first_name: Jasleen full_name: Matharu, Jasleen last_name: Matharu - first_name: Rohan P. full_name: Naidu, Rohan P. last_name: Naidu - first_name: Anna full_name: Velichko, Anna last_name: Velichko - first_name: Victoria full_name: Bollo, Victoria last_name: Bollo - first_name: Rychard full_name: Bouwens, Rychard last_name: Bouwens - first_name: John full_name: Chisholm, John last_name: Chisholm - first_name: Garth D. full_name: Illingworth, Garth D. last_name: Illingworth - first_name: Ivan full_name: Kramarenko, Ivan id: 9a9394cb-3200-11ee-973b-f5ba2a8b16e4 last_name: Kramarenko orcid: 0000-0001-5346-6048 - first_name: Daniel full_name: Magee, Daniel last_name: Magee - first_name: Michael full_name: Maseda, Michael last_name: Maseda - 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: Erica full_name: Nelson, Erica last_name: Nelson - first_name: Naveen full_name: Reddy, Naveen last_name: Reddy - first_name: Daniel full_name: Schaerer, Daniel last_name: Schaerer - first_name: Mauro full_name: Stefanon, Mauro last_name: Stefanon - first_name: Mengyuan full_name: Xiao, Mengyuan last_name: Xiao citation: ama: 'Covelo-Paz A, Giovinazzo E, Oesch PA, et al. An Hα view of galaxy buildup in the first 2 Gyr: Luminosity functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy. Astronomy & Astrophysics. 2025;694. doi:10.1051/0004-6361/202452363' apa: 'Covelo-Paz, A., Giovinazzo, E., Oesch, P. A., Meyer, R. A., Weibel, A., Brammer, G., … Xiao, M. (2025). An Hα view of galaxy buildup in the first 2 Gyr: Luminosity functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202452363' chicago: 'Covelo-Paz, Alba, Emma Giovinazzo, Pascal A. Oesch, Romain A. Meyer, Andrea Weibel, Gabriel Brammer, Yoshinobu Fudamoto, et al. “An Hα View of Galaxy Buildup in the First 2 Gyr: Luminosity Functions at z ∼ 4−6.5 from NIRCam/Grism Spectroscopy.” Astronomy & Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202452363.' ieee: 'A. Covelo-Paz et al., “An Hα view of galaxy buildup in the first 2 Gyr: Luminosity functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy,” Astronomy & Astrophysics, vol. 694. EDP Sciences, 2025.' ista: 'Covelo-Paz A, Giovinazzo E, Oesch PA, Meyer RA, Weibel A, Brammer G, Fudamoto Y, Kerutt J, Lin J, Matharu J, Naidu RP, Velichko A, Bollo V, Bouwens R, Chisholm J, Illingworth GD, Kramarenko I, Magee D, Maseda M, Matthee JJ, Nelson E, Reddy N, Schaerer D, Stefanon M, Xiao M. 2025. An Hα view of galaxy buildup in the first 2 Gyr: Luminosity functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy. Astronomy & Astrophysics. 694, A178.' mla: 'Covelo-Paz, Alba, et al. “An Hα View of Galaxy Buildup in the First 2 Gyr: Luminosity Functions at z ∼ 4−6.5 from NIRCam/Grism Spectroscopy.” Astronomy & Astrophysics, vol. 694, A178, EDP Sciences, 2025, doi:10.1051/0004-6361/202452363.' short: A. Covelo-Paz, E. Giovinazzo, P.A. Oesch, R.A. Meyer, A. Weibel, G. Brammer, Y. Fudamoto, J. Kerutt, J. Lin, J. Matharu, R.P. Naidu, A. Velichko, V. Bollo, R. Bouwens, J. Chisholm, G.D. Illingworth, I. Kramarenko, D. Magee, M. Maseda, J.J. Matthee, E. Nelson, N. Reddy, D. Schaerer, M. Stefanon, M. Xiao, Astronomy & Astrophysics 694 (2025). date_created: 2025-03-02T23:01:54Z date_published: 2025-02-12T00:00:00Z date_updated: 2026-02-16T12:08:59Z day: '12' ddc: - '520' department: - _id: JoMa doi: 10.1051/0004-6361/202452363 external_id: arxiv: - '2409.17241' isi: - '001420194600001' file: - access_level: open_access checksum: b1e74644a0cd37550e9a553f8675c93f content_type: application/pdf creator: dernst date_created: 2025-03-04T09:29:01Z date_updated: 2025-03-04T09:29:01Z file_id: '19285' file_name: 2025_AstronomyAstrophysics_CoveloPaz.pdf file_size: 1865856 relation: main_file success: 1 file_date_updated: 2025-03-04T09:29:01Z has_accepted_license: '1' intvolume: ' 694' isi: 1 language: - iso: eng month: '02' oa: 1 oa_version: Published Version publication: Astronomy & Astrophysics publication_identifier: eissn: - 1432-0746 issn: - 0004-6361 publication_status: published publisher: EDP Sciences quality_controlled: '1' related_material: link: - relation: software url: ' https://github.com/astroalba/fresco' scopus_import: '1' status: public title: 'An Hα view of galaxy buildup in the first 2 Gyr: Luminosity functions at z ∼ 4−6.5 from NIRCam/grism spectroscopy' 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: 694 year: '2025' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '19366' abstract: - lang: eng text: Staphylococcus aureus (S. aureus) is one of the most common causative agents of mammary gland infection and mastitis, but the specific role of S. aureus-derived extracellular vesicles (SaEVs) in mastitis has been poorly studied to date. Here, we aimed to investigate the response of bovine monocyte-derived macrophages (boMdM) to SaEVs of the genotype B (GTB) mastitis-related strain M5512B. Specifically, we evaluated the effects on the actin cytoskeleton, gene expression, and the SaEV proteomic cargo. Furthermore, we assessed to what extent the cellular and molecular response of boMdM to SaEVs differed from peripheral mononuclear blood cells (PBMCs) used for in vitro derivation of the former. We observed that SaEVs induced morphological changes in boMdM, leading to a pro-inflammatory and pyroptosis-related increased gene expression. Additionally, our study revealed that boMdM and PBMCs exhibited stimulus-specific differing responses. The proteomic analysis of SaEVs identified clusters of proteins related to virulence and antibiotic resistance, supporting the theory that S. aureus might use EVs to evade host defences and colonize the mammary gland. Our results bring new insights into how SaEVs might impact the host during an S. aureus infection, which can be useful for future S. aureus vaccine development. acknowledgement: "The authors thank Michele Guastalla for his contributions to the boMdM analyses and Stephan Handschin from the Scientific Center for Optical and Electron Microscopy (ScopeM) of ETH Zurich for the TEM imaging. We gratefully acknowledge the Functional Genomics Center Zurich (FGCZ) for performing the mass spectrometry analysis for this study.\r\nOpen access funding provided by Swiss Federal Institute of Technology Zurich. This work was supported by basic funding from ETH Zurich." article_processing_charge: Yes article_type: original author: - first_name: Mara D. full_name: Saenz-De-Juano, Mara D. last_name: Saenz-De-Juano - first_name: Giulia full_name: Silvestrelli, Giulia id: 12632ae8-799e-11ef-94a2-e5a3b5ef49e9 last_name: Silvestrelli - first_name: Samuel full_name: Buri, Samuel last_name: Buri - first_name: Léa V. full_name: Zinsli, Léa V. last_name: Zinsli - first_name: Mathias full_name: Schmelcher, Mathias last_name: Schmelcher - first_name: Susanne E. full_name: Ulbrich, Susanne E. last_name: Ulbrich citation: ama: Saenz-De-Juano MD, Silvestrelli G, Buri S, Zinsli LV, Schmelcher M, Ulbrich SE. Mastitis-related Staphylococcus aureus-derived extracellular vesicles induce a pro-inflammatory response in bovine monocyte-derived macrophages. Scientific Reports. 2025;15:6059. doi:10.1038/s41598-025-90466-6 apa: Saenz-De-Juano, M. D., Silvestrelli, G., Buri, S., Zinsli, L. V., Schmelcher, M., & Ulbrich, S. E. (2025). Mastitis-related Staphylococcus aureus-derived extracellular vesicles induce a pro-inflammatory response in bovine monocyte-derived macrophages. Scientific Reports. Springer Nature. https://doi.org/10.1038/s41598-025-90466-6 chicago: Saenz-De-Juano, Mara D., Giulia Silvestrelli, Samuel Buri, Léa V. Zinsli, Mathias Schmelcher, and Susanne E. Ulbrich. “Mastitis-Related Staphylococcus Aureus-Derived Extracellular Vesicles Induce a pro-Inflammatory Response in Bovine Monocyte-Derived Macrophages.” Scientific Reports. Springer Nature, 2025. https://doi.org/10.1038/s41598-025-90466-6. ieee: M. D. Saenz-De-Juano, G. Silvestrelli, S. Buri, L. V. Zinsli, M. Schmelcher, and S. E. Ulbrich, “Mastitis-related Staphylococcus aureus-derived extracellular vesicles induce a pro-inflammatory response in bovine monocyte-derived macrophages,” Scientific Reports, vol. 15. Springer Nature, p. 6059, 2025. ista: Saenz-De-Juano MD, Silvestrelli G, Buri S, Zinsli LV, Schmelcher M, Ulbrich SE. 2025. Mastitis-related Staphylococcus aureus-derived extracellular vesicles induce a pro-inflammatory response in bovine monocyte-derived macrophages. Scientific Reports. 15, 6059. mla: Saenz-De-Juano, Mara D., et al. “Mastitis-Related Staphylococcus Aureus-Derived Extracellular Vesicles Induce a pro-Inflammatory Response in Bovine Monocyte-Derived Macrophages.” Scientific Reports, vol. 15, Springer Nature, 2025, p. 6059, doi:10.1038/s41598-025-90466-6. short: M.D. Saenz-De-Juano, G. Silvestrelli, S. Buri, L.V. Zinsli, M. Schmelcher, S.E. Ulbrich, Scientific Reports 15 (2025) 6059. date_created: 2025-03-09T23:01:26Z date_published: 2025-02-19T00:00:00Z date_updated: 2025-09-30T10:58:59Z day: '19' ddc: - '570' department: - _id: LoSw doi: 10.1038/s41598-025-90466-6 external_id: isi: - '001426697000031' pmid: - '39972051' file: - access_level: open_access checksum: 51b55ae299de1fa126016a11024b499a content_type: application/pdf creator: dernst date_created: 2025-03-10T12:00:34Z date_updated: 2025-03-10T12:00:34Z file_id: '19380' file_name: 2025_ScientificReports_SaenzdeJuano.pdf file_size: 2780316 relation: main_file success: 1 file_date_updated: 2025-03-10T12:00:34Z has_accepted_license: '1' intvolume: ' 15' isi: 1 language: - iso: eng month: '02' oa: 1 oa_version: Published Version page: '6059' 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: Mastitis-related Staphylococcus aureus-derived extracellular vesicles induce a pro-inflammatory response in bovine monocyte-derived macrophages 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: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 15 year: '2025' ... --- OA_type: closed access _id: '19374' abstract: - lang: eng text: In the present study, the new ternary rare earth intermetallic compound PrNi6Si6 has been investigated. This work completes the study of the RNi6Si6 series (R = rare earth). While the RNi6Si6 compounds for R = La and Ce adopt the CeNi6Si6-type (tP52, P4/nbm, No. 125), surprisingly PrNi6Si6 crystallizes in the YNi6Si6 prototype (tP52, P − 4b2, No. 117) as do all the heavier lanthanides (but Lu). The YNi6Si6-type and its homolog CeNi6Si6 are two tetragonal ordered derivative of the cubic NaZn13-type structure. Lattice parameters for PrNi6Si6 are a = 7.7846(1) Å, c = 11.2144(1) Å, with a unit cell volume, Vobs = 679.585(5) Å3. The temperature dependence of the inverse magnetic susceptibility χ−1(T) follows the Curie–Weiss law, with calculated values of the effective magnetic moment (µeff) and Weiss temperature (Θpm) of 3.55 μB and − 4.5 K, respectively. While the observed µeff is very close to the theoretical value of 3.58 µB for the free Pr3+ ions, a negative value of the Weiss temperature suggests antiferromagnetic interactions in PrNi6Si6. Magnetization measurements confirm that PrNi₆Si₆ orders antiferromagnetically (AFM) below a Néel temperature (TN) of 9 K. The Ni atoms contribute negligibly to the magnetic properties of this phase. The specific heat of PrNi₆Si₆ is approximately 0.42 J K − 1 g − 1. Measurements of electric and thermal transport reveal that PrNi₆Si₆ exhibits metallic behavior across a wide temperature range of 2–900 K, accompanied by a relatively low thermal conductivity of around 6 W K − 1 m − 1 at room temperature. Such properties, together with its high-temperature refractory behavior, make PrNi₆Si₆ worthy of consideration in technological applications where fairly good electrical conductivity should be accompanied by a limited thermal conductivity. article_number: '100051' article_processing_charge: No article_type: original author: - first_name: Saurabh full_name: Singh, Saurabh id: 12d625da-9cb3-11ed-9667-af09d37d3f0a last_name: Singh orcid: 0000-0003-2209-5269 - first_name: A. full_name: Provino, A. last_name: Provino - first_name: I. full_name: Pallecchi, I. last_name: Pallecchi - first_name: F. full_name: Caglieris, F. last_name: Caglieris - first_name: M. full_name: Mödlinger, M. last_name: Mödlinger - first_name: P. full_name: Mele, P. last_name: Mele - first_name: G. full_name: Latronico, G. last_name: Latronico - first_name: T. full_name: Takeuchi, T. last_name: Takeuchi - first_name: P. full_name: Manfrinetti, P. last_name: Manfrinetti citation: ama: 'Singh S, Provino A, Pallecchi I, et al. The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K). Journal of Materials Science. 2025;60. doi:10.1007/s10853-024-10582-y' apa: 'Singh, S., Provino, A., Pallecchi, I., Caglieris, F., Mödlinger, M., Mele, P., … Manfrinetti, P. (2025). The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K). Journal of Materials Science. Springer Nature. https://doi.org/10.1007/s10853-024-10582-y' chicago: 'Singh, Saurabh, A. Provino, I. Pallecchi, F. Caglieris, M. Mödlinger, P. Mele, G. Latronico, T. Takeuchi, and P. Manfrinetti. “The New PrNi6Si6 Intermetallic: From Crystal Structure to Thermal and Electrical Transport Properties across a Wide Temperature Range (2–900 K).” Journal of Materials Science. Springer Nature, 2025. https://doi.org/10.1007/s10853-024-10582-y.' ieee: 'S. Singh et al., “The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K),” Journal of Materials Science, vol. 60. Springer Nature, 2025.' ista: 'Singh S, Provino A, Pallecchi I, Caglieris F, Mödlinger M, Mele P, Latronico G, Takeuchi T, Manfrinetti P. 2025. The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K). Journal of Materials Science. 60, 100051.' mla: 'Singh, Saurabh, et al. “The New PrNi6Si6 Intermetallic: From Crystal Structure to Thermal and Electrical Transport Properties across a Wide Temperature Range (2–900 K).” Journal of Materials Science, vol. 60, 100051, Springer Nature, 2025, doi:10.1007/s10853-024-10582-y.' short: S. Singh, A. Provino, I. Pallecchi, F. Caglieris, M. Mödlinger, P. Mele, G. Latronico, T. Takeuchi, P. Manfrinetti, Journal of Materials Science 60 (2025). date_created: 2025-03-09T23:01:29Z date_published: 2025-02-08T00:00:00Z date_updated: 2025-03-10T06:53:16Z day: '08' department: - _id: MaIb doi: 10.1007/s10853-024-10582-y intvolume: ' 60' language: - iso: eng month: '02' oa_version: None publication: Journal of Materials Science publication_identifier: eissn: - 1573-4803 issn: - 0022-2461 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: 'The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K)' type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 60 year: '2025' ... --- OA_type: closed access _id: '19444' abstract: - lang: eng text: As the field of neural organoids and assembloids expands, there is an emergent need for guidance and advice on designing, conducting and reporting experiments to increase the reproducibility and utility of these models. In this Perspective, we present a framework for the experimental process that encompasses ensuring the quality and integrity of human pluripotent stem cells, characterizing and manipulating neural cells in vitro, transplantation techniques and considerations for modelling human development, evolution and disease. As with all scientific endeavours, we advocate for rigorous experimental designs tailored to explicit scientific questions as well as transparent methodologies and data sharing to provide useful knowledge for current research practices and for developing regulatory standards. acknowledgement: The authors thank members of their laboratories who provided feedback on earlier versions of this manuscript, including A. Jourdon, V. Mariano, T. L. Li, N. Caporale, E. Villa and M. Sutcliffe. article_processing_charge: No article_type: original author: - first_name: Sergiu P. full_name: Pașca, Sergiu P. last_name: Pașca - first_name: Paola full_name: Arlotta, Paola last_name: Arlotta - first_name: Helen S. full_name: Bateup, Helen S. last_name: Bateup - first_name: J. Gray full_name: Camp, J. Gray last_name: Camp - first_name: Silvia full_name: Cappello, Silvia last_name: Cappello - first_name: Fred H. full_name: Gage, Fred H. last_name: Gage - first_name: Jürgen A. full_name: Knoblich, Jürgen A. last_name: Knoblich - first_name: Arnold R. full_name: Kriegstein, Arnold R. last_name: Kriegstein - first_name: Madeline A. full_name: Lancaster, Madeline A. last_name: Lancaster - first_name: Guo Li full_name: Ming, Guo Li last_name: Ming - first_name: Gaia full_name: Novarino, Gaia id: 3E57A680-F248-11E8-B48F-1D18A9856A87 last_name: Novarino orcid: 0000-0002-7673-7178 - first_name: Hideyuki full_name: Okano, Hideyuki last_name: Okano - first_name: Malin full_name: Parmar, Malin last_name: Parmar - first_name: In Hyun full_name: Park, In Hyun last_name: Park - first_name: Orly full_name: Reiner, Orly last_name: Reiner - first_name: Hongjun full_name: Song, Hongjun last_name: Song - first_name: Lorenz full_name: Studer, Lorenz last_name: Studer - first_name: Jun full_name: Takahashi, Jun last_name: Takahashi - first_name: Sally full_name: Temple, Sally last_name: Temple - first_name: Giuseppe full_name: Testa, Giuseppe last_name: Testa - first_name: Barbara full_name: Treutlein, Barbara last_name: Treutlein - first_name: Flora M. full_name: Vaccarino, Flora M. last_name: Vaccarino - first_name: Pierre full_name: Vanderhaeghen, Pierre last_name: Vanderhaeghen - first_name: Tracy full_name: Young-Pearse, Tracy last_name: Young-Pearse citation: ama: Pașca SP, Arlotta P, Bateup HS, et al. A framework for neural organoids, assembloids and transplantation studies. Nature. 2025;639(8054):315-320. doi:10.1038/s41586-024-08487-6 apa: Pașca, S. P., Arlotta, P., Bateup, H. S., Camp, J. G., Cappello, S., Gage, F. H., … Young-Pearse, T. (2025). A framework for neural organoids, assembloids and transplantation studies. Nature. Springer Nature. https://doi.org/10.1038/s41586-024-08487-6 chicago: Pașca, Sergiu P., Paola Arlotta, Helen S. Bateup, J. Gray Camp, Silvia Cappello, Fred H. Gage, Jürgen A. Knoblich, et al. “A Framework for Neural Organoids, Assembloids and Transplantation Studies.” Nature. Springer Nature, 2025. https://doi.org/10.1038/s41586-024-08487-6. ieee: S. P. Pașca et al., “A framework for neural organoids, assembloids and transplantation studies,” Nature, vol. 639, no. 8054. Springer Nature, pp. 315–320, 2025. ista: Pașca SP, Arlotta P, Bateup HS, Camp JG, Cappello S, Gage FH, Knoblich JA, Kriegstein AR, Lancaster MA, Ming GL, Novarino G, Okano H, Parmar M, Park IH, Reiner O, Song H, Studer L, Takahashi J, Temple S, Testa G, Treutlein B, Vaccarino FM, Vanderhaeghen P, Young-Pearse T. 2025. A framework for neural organoids, assembloids and transplantation studies. Nature. 639(8054), 315–320. mla: Pașca, Sergiu P., et al. “A Framework for Neural Organoids, Assembloids and Transplantation Studies.” Nature, vol. 639, no. 8054, Springer Nature, 2025, pp. 315–20, doi:10.1038/s41586-024-08487-6. short: S.P. Pașca, P. Arlotta, H.S. Bateup, J.G. Camp, S. Cappello, F.H. Gage, J.A. Knoblich, A.R. Kriegstein, M.A. Lancaster, G.L. Ming, G. Novarino, H. Okano, M. Parmar, I.H. Park, O. Reiner, H. Song, L. Studer, J. Takahashi, S. Temple, G. Testa, B. Treutlein, F.M. Vaccarino, P. Vanderhaeghen, T. Young-Pearse, Nature 639 (2025) 315–320. date_created: 2025-03-23T23:01:27Z date_published: 2025-03-13T00:00:00Z date_updated: 2025-09-30T11:13:47Z day: '13' department: - _id: GaNo doi: 10.1038/s41586-024-08487-6 external_id: isi: - '001437461900001' pmid: - '39653126' intvolume: ' 639' isi: 1 issue: '8054' language: - iso: eng month: '03' oa_version: None page: 315-320 pmid: 1 publication: Nature publication_identifier: eissn: - 1476-4687 issn: - 0028-0836 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: A framework for neural organoids, assembloids and transplantation studies type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 639 year: '2025' ... --- OA_place: repository OA_type: green _id: '19483' abstract: - lang: eng text: We prove matching upper and lower bounds for the average of the6-torsionof class groups of quadratic fields. Furthermore, we count the number of integer solutions on an affine quartic threefold. article_number: '18' article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Yik Tung full_name: Chan, Yik Tung id: c4c0afc8-9262-11ed-9231-d8b0bc743af1 last_name: Chan orcid: 0000-0001-8467-4106 - first_name: Peter full_name: Koymans, Peter last_name: Koymans - first_name: Carlo full_name: Pagano, Carlo last_name: Pagano - first_name: Efthymios full_name: Sofos, Efthymios last_name: Sofos citation: ama: Chan S, Koymans P, Pagano C, Sofos E. 6-torision and integral points on quartic threefolds. Annali della Scuola Normale Superiore di Pisa, Classe di Scienze. 2025. doi:10.2422/2036-2145.202412_006 apa: Chan, S., Koymans, P., Pagano, C., & Sofos, E. (2025). 6-torision and integral points on quartic threefolds. Annali Della Scuola Normale Superiore Di Pisa, Classe Di Scienze. Scuola Normale Superiore - Edizioni della Normale. https://doi.org/10.2422/2036-2145.202412_006 chicago: Chan, Stephanie, Peter Koymans, Carlo Pagano, and Efthymios Sofos. “6-Torision and Integral Points on Quartic Threefolds.” Annali Della Scuola Normale Superiore Di Pisa, Classe Di Scienze. Scuola Normale Superiore - Edizioni della Normale, 2025. https://doi.org/10.2422/2036-2145.202412_006. ieee: S. Chan, P. Koymans, C. Pagano, and E. Sofos, “6-torision and integral points on quartic threefolds,” Annali della Scuola Normale Superiore di Pisa, Classe di Scienze. Scuola Normale Superiore - Edizioni della Normale, 2025. ista: Chan S, Koymans P, Pagano C, Sofos E. 2025. 6-torision and integral points on quartic threefolds. Annali della Scuola Normale Superiore di Pisa, Classe di Scienze., 18. mla: Chan, Stephanie, et al. “6-Torision and Integral Points on Quartic Threefolds.” Annali Della Scuola Normale Superiore Di Pisa, Classe Di Scienze, 18, Scuola Normale Superiore - Edizioni della Normale, 2025, doi:10.2422/2036-2145.202412_006. short: S. Chan, P. Koymans, C. Pagano, E. Sofos, Annali Della Scuola Normale Superiore Di Pisa, Classe Di Scienze (2025). corr_author: '1' date_created: 2025-04-05T10:49:27Z date_published: 2025-03-07T00:00:00Z date_updated: 2025-05-14T11:40:24Z day: '07' department: - _id: TiBr doi: 10.2422/2036-2145.202412_006 external_id: arxiv: - '2403.13359' language: - iso: eng main_file_link: - open_access: '1' url: ' https://doi.org/10.48550/arXiv.2403.13359' month: '03' oa: 1 oa_version: Preprint publication: Annali della Scuola Normale Superiore di Pisa, Classe di Scienze publication_identifier: eissn: - 2036-2145 issn: - 0391-173X publication_status: epub_ahead publisher: Scuola Normale Superiore - Edizioni della Normale status: public title: 6-torision and integral points on quartic threefolds type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 year: '2025' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '19596' abstract: - lang: eng text: "We report the spectroscopic discovery of a massive quiescent galaxy at zspec = 7.29 ± 0.01, just ∼700 Myr after the big bang. RUBIES-UDS-QG-z7 was selected from public JWST/NIRCam and MIRI imaging from the PRIMER survey and observed with JWST/NIRSpec as part of RUBIES. The NIRSpec/PRISM spectrum reveals one of the strongest Balmer breaks observed thus far at z > 6, with no emission lines but tentative Balmer and Ca absorption features, as well as a Lyman break. Simultaneous modeling of the NIRSpec/PRISM spectrum and NIRCam and MIRI photometry (spanning 0.9–18 μm) shows that the galaxy formed a stellar mass of\r\n(math. formular) before z ∼ 8 and ceased forming stars 50–100 Myr prior to the time of observation, resulting in log (sSFR/Gyr- 1) < -1 . We measure a small physical size of (math formular) , which implies a high stellarmass surface density within the effective radius of (math formular) comparable to the highest densities measured in quiescent galaxies at z ∼ 2–5. The 3D stellar-mass density profile of RUBIES-UDS-QG-z7 is remarkably similar to the central densities of local massive ellipticals, suggesting that at least some of their cores may have already been in place at z > 7. The discovery of RUBIES-UDS-QG-z7 has strong implications for galaxy formation models: the estimated number density of quiescent galaxies at z ∼ 7 is >100 × larger than predicted from any model to date, indicating that quiescent galaxies have formed earlier than previously expected. " acknowledgement: "We thank the PRIMER team for making their imaging data publicly available immediately. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program #4233. Support for program #4233 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 research was supported by the International Space Science Institute (ISSI) in Bern, through ISSI International Team project #562. The Cosmic Dawn Center is funded by the Danish National Research Foundation (DNRF140). This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI), under contract number MB22.00072, as well as from the Swiss National Science Foundation (SNSF), through project grant 200020_207349. Support for this work was provided by The Brinson Foundation through a Brinson Prize Fellowship grant. Support for this work for R.P.N. was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A, awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. T.B.M. was supported by a CIERA fellowship.\r\nAll software packages used in this work are publicly available on Github: grizli, msafit, msaexp, Prospector, and sedpy. We acknowledge: astropy (Astropy Collaboration et al. 2013, 2018, 2022), matplotlib (J. D. Hunter 2007), numpy (C. R. Harris et al. 2020), scipy (P. Virtanen et al. 2020), lmfit (M. Newville et al. 2024), eMPT (N. Bonaventura et al. 2023), the jwst pipeline (H. Bushouse et al. 2024), msaexp (G. Brammer 2024a), and grizli (G. Brammer 2024b),." article_number: '11' article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: Andrea full_name: Weibel, Andrea last_name: Weibel - first_name: Anna full_name: De Graaff, Anna last_name: De Graaff - first_name: David J. full_name: Setton, David J. last_name: Setton - first_name: Tim B. full_name: Miller, Tim B. last_name: Miller - first_name: Pascal A. full_name: Oesch, Pascal A. last_name: Oesch - first_name: Gabriel full_name: Brammer, Gabriel last_name: Brammer - first_name: Claudia D.P. full_name: Lagos, Claudia D.P. last_name: Lagos - 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: Josephine F.W. full_name: Baggen, Josephine F.W. last_name: Baggen - first_name: Rachel full_name: Bezanson, Rachel last_name: Bezanson - first_name: Leindert A. full_name: Boogaard, Leindert A. last_name: Boogaard - first_name: Nikko J. full_name: Cleri, Nikko J. last_name: Cleri - first_name: Jenny E. full_name: Greene, Jenny E. last_name: Greene - first_name: Michaela full_name: Hirschmann, Michaela last_name: Hirschmann - first_name: Raphael E. full_name: Hviding, Raphael E. last_name: Hviding - first_name: Adarsh full_name: Kuruvanthodi, Adarsh last_name: Kuruvanthodi - first_name: Ivo full_name: Labbé, Ivo last_name: Labbé - first_name: Joel full_name: Leja, Joel last_name: Leja - first_name: Michael V. full_name: Maseda, Michael V. last_name: Maseda - 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: Ian full_name: Mcconachie, Ian last_name: Mcconachie - first_name: Rohan P. full_name: Naidu, Rohan P. last_name: Naidu - first_name: Guido full_name: Roberts-Borsani, Guido last_name: Roberts-Borsani - first_name: Daniel full_name: Schaerer, Daniel last_name: Schaerer - first_name: Katherine A. full_name: Suess, Katherine A. last_name: Suess - first_name: Francesco full_name: Valentino, Francesco last_name: Valentino - first_name: Pieter full_name: Van Dokkum, Pieter last_name: Van Dokkum - first_name: Bingjie full_name: Wang, Bingjie last_name: Wang citation: ama: Weibel A, De Graaff A, Setton DJ, et al. RUBIES reveals a massive quiescent galaxy at z = 7.3. The Astrophysical Journal. 2025;983(1). doi:10.3847/1538-4357/adab7a apa: Weibel, A., De Graaff, A., Setton, D. J., Miller, T. B., Oesch, P. A., Brammer, G., … Wang, B. (2025). RUBIES reveals a massive quiescent galaxy at z = 7.3. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/adab7a chicago: Weibel, Andrea, Anna De Graaff, David J. Setton, Tim B. Miller, Pascal A. Oesch, Gabriel Brammer, Claudia D.P. Lagos, et al. “RUBIES Reveals a Massive Quiescent Galaxy at z = 7.3.” The Astrophysical Journal. IOP Publishing, 2025. https://doi.org/10.3847/1538-4357/adab7a. ieee: A. Weibel et al., “RUBIES reveals a massive quiescent galaxy at z = 7.3,” The Astrophysical Journal, vol. 983, no. 1. IOP Publishing, 2025. ista: Weibel A, De Graaff A, Setton DJ, Miller TB, Oesch PA, Brammer G, Lagos CDP, Whitaker KE, Williams CC, Baggen JFW, Bezanson R, Boogaard LA, Cleri NJ, Greene JE, Hirschmann M, Hviding RE, Kuruvanthodi A, Labbé I, Leja J, Maseda MV, Matthee JJ, Mcconachie I, Naidu RP, Roberts-Borsani G, Schaerer D, Suess KA, Valentino F, Van Dokkum P, Wang B. 2025. RUBIES reveals a massive quiescent galaxy at z = 7.3. The Astrophysical Journal. 983(1), 11. mla: Weibel, Andrea, et al. “RUBIES Reveals a Massive Quiescent Galaxy at z = 7.3.” The Astrophysical Journal, vol. 983, no. 1, 11, IOP Publishing, 2025, doi:10.3847/1538-4357/adab7a. short: A. Weibel, A. De Graaff, D.J. Setton, T.B. Miller, P.A. Oesch, G. Brammer, C.D.P. Lagos, K.E. Whitaker, C.C. Williams, J.F.W. Baggen, R. Bezanson, L.A. Boogaard, N.J. Cleri, J.E. Greene, M. Hirschmann, R.E. Hviding, A. Kuruvanthodi, I. Labbé, J. Leja, M.V. Maseda, J.J. Matthee, I. Mcconachie, R.P. Naidu, G. Roberts-Borsani, D. Schaerer, K.A. Suess, F. Valentino, P. Van Dokkum, B. Wang, The Astrophysical Journal 983 (2025). date_created: 2025-04-20T22:01:28Z date_published: 2025-04-10T00:00:00Z date_updated: 2026-02-16T12:42:28Z day: '10' ddc: - '520' department: - _id: JoMa doi: 10.3847/1538-4357/adab7a external_id: arxiv: - '2409.03829' isi: - '001457334900001' file: - access_level: open_access checksum: a1132e0b18bb643f9a32674c6694375a content_type: application/pdf creator: dernst date_created: 2025-04-22T09:08:17Z date_updated: 2025-04-22T09:08:17Z file_id: '19605' file_name: 2025_AstrophysicalJour_Weibel.pdf file_size: 1964589 relation: main_file success: 1 file_date_updated: 2025-04-22T09:08:17Z has_accepted_license: '1' intvolume: ' 983' isi: 1 issue: '1' language: - iso: eng month: '04' 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: RUBIES reveals a massive quiescent galaxy at z = 7.3 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: 983 year: '2025' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '19636' abstract: - lang: eng text: This summary of the second Terrestrial Very-Long-Baseline Atom Interferometry (TVLBAI) Workshop provides a comprehensive overview of our meeting held in London in April 2024 (Second Terrestrial Very-Long-Baseline Atom Interferometry Workshop, Imperial College, April 2024), building on the initial discussions during the inaugural workshop held at CERN in March 2023 (First Terrestrial Very-Long-Baseline Atom Interferometry Workshop, CERN, March 2023). Like the summary of the first workshop (Abend et al. in AVS Quantum Sci. 6:024701, 2024), this document records a critical milestone for the international atom interferometry community. It documents our concerted efforts to evaluate progress, address emerging challenges, and refine strategic directions for future large-scale atom interferometry projects. Our commitment to collaboration is manifested by the integration of diverse expertise and the coordination of international resources, all aimed at advancing the frontiers of atom interferometry physics and technology, as set out in a Memorandum of Understanding signed by over 50 institutions (Memorandum of Understanding for the Terrestrial Very Long Baseline Atom Interferometer Study). acknowledgement: "We acknowledge the support of the CERN Physics Beyond Collider activity, the CERN Quantum Technology Initiative, the Long Range Broad Agency Announcement (BAA) for the Navy and Marine Corps Science and Technology programme, Hannover Leibniz University, and the Physics Department at Imperial College London, whose contributions were instrumental in supporting the workshop that laid the foundation for this paper.\r\nThe workshop was partially funded by contributions from the Long Range Broad Agency Announcement (BAA) for the Navy and Marine Corps Science and Technology programme, Hannover Leibniz University, and the Physics Department at Imperial College London." article_number: '42' article_processing_charge: Yes article_type: review arxiv: 1 author: - first_name: Adam full_name: Abdalla, Adam last_name: Abdalla - first_name: Mahiro full_name: Abe, Mahiro last_name: Abe - first_name: Sven full_name: Abend, Sven last_name: Abend - first_name: Mouine full_name: Abidi, Mouine last_name: Abidi - first_name: Monika full_name: Aidelsburger, Monika last_name: Aidelsburger - first_name: Ashkan full_name: Alibabaei, Ashkan last_name: Alibabaei - first_name: Baptiste full_name: Allard, Baptiste last_name: Allard - first_name: John full_name: Antoniadis, John last_name: Antoniadis - first_name: Gianluigi full_name: Arduini, Gianluigi last_name: Arduini - first_name: Nadja full_name: Augst, Nadja last_name: Augst - first_name: Philippos full_name: Balamatsias, Philippos last_name: Balamatsias - first_name: Antun full_name: Balaž, Antun last_name: Balaž - first_name: Hannah full_name: Banks, Hannah last_name: Banks - first_name: Rachel L. full_name: Barcklay, Rachel L. last_name: Barcklay - first_name: Michele full_name: Barone, Michele last_name: Barone - first_name: Michele full_name: Barsanti, Michele last_name: Barsanti - first_name: Mark G. full_name: Bason, Mark G. last_name: Bason - first_name: Angelo full_name: Bassi, Angelo last_name: Bassi - first_name: Jean Baptiste full_name: Bayle, Jean Baptiste last_name: Bayle - first_name: Charles F.A. full_name: Baynham, Charles F.A. last_name: Baynham - first_name: Quentin full_name: Beaufils, Quentin last_name: Beaufils - first_name: Sélyan full_name: Beldjoudi, Sélyan last_name: Beldjoudi - first_name: Aleksandar full_name: Belić, Aleksandar last_name: Belić - first_name: Shayne full_name: Bennetts, Shayne last_name: Bennetts - first_name: Jose full_name: Bernabeu, Jose last_name: Bernabeu - first_name: Andrea full_name: Bertoldi, Andrea last_name: Bertoldi - first_name: Clara full_name: Bigard, Clara last_name: Bigard - first_name: N. P. full_name: Bigelow, N. P. last_name: Bigelow - first_name: Robert full_name: Bingham, Robert last_name: Bingham - first_name: Diego full_name: Blas, Diego last_name: Blas - first_name: Alexey full_name: Bobrick, Alexey last_name: Bobrick - first_name: Samuel full_name: Boehringer, Samuel last_name: Boehringer - first_name: Aleksandar full_name: Bogojević, Aleksandar last_name: Bogojević - first_name: Kai full_name: Bongs, Kai last_name: Bongs - first_name: Daniela full_name: Bortoletto, Daniela last_name: Bortoletto - first_name: Philippe full_name: Bouyer, Philippe last_name: Bouyer - first_name: Christian full_name: Brand, Christian last_name: Brand - first_name: Oliver full_name: Buchmueller, Oliver last_name: Buchmueller - first_name: Gabriela full_name: Buica, Gabriela last_name: Buica - first_name: Sergio full_name: Calatroni, Sergio last_name: Calatroni - first_name: Léo full_name: Calmels, Léo last_name: Calmels - first_name: Priscilla full_name: Canizares, Priscilla last_name: Canizares - first_name: Benjamin full_name: Canuel, Benjamin last_name: Canuel - first_name: Ana full_name: Caramete, Ana last_name: Caramete - first_name: Laurentiu Ioan full_name: Caramete, Laurentiu Ioan last_name: Caramete - first_name: Matteo full_name: Carlesso, Matteo last_name: Carlesso - first_name: John full_name: Carlton, John last_name: Carlton - first_name: Samuel P. full_name: Carman, Samuel P. last_name: Carman - first_name: Andrew full_name: Carroll, Andrew last_name: Carroll - first_name: Mateo full_name: Casariego, Mateo last_name: Casariego - first_name: Minoas full_name: Chairetis, Minoas last_name: Chairetis - first_name: Vassilis full_name: Charmandaris, Vassilis last_name: Charmandaris - first_name: Upasna full_name: Chauhan, Upasna last_name: Chauhan - first_name: Jiajun full_name: Chen, Jiajun last_name: Chen - first_name: Maria Luisa Maria Luisa Marilù full_name: Chiofalo, Maria Luisa Maria Luisa Marilù last_name: Chiofalo - first_name: Donatella full_name: Ciampini, Donatella last_name: Ciampini - first_name: Alessia full_name: Cimbri, Alessia last_name: Cimbri - first_name: Pierre full_name: Cladé, Pierre last_name: Cladé - first_name: Jonathon full_name: Coleman, Jonathon last_name: Coleman - first_name: Florin Lucian full_name: Constantin, Florin Lucian last_name: Constantin - first_name: Carlo R. full_name: Contaldi, Carlo R. last_name: Contaldi - first_name: Robin full_name: Corgier, Robin last_name: Corgier - first_name: Bineet full_name: Dash, Bineet last_name: Dash - first_name: G. J. full_name: Davies, G. J. last_name: Davies - first_name: Claudia full_name: De Rham, Claudia last_name: De Rham - first_name: Albert full_name: De Roeck, Albert last_name: De Roeck - first_name: Daniel full_name: Derr, Daniel last_name: Derr - first_name: Soumyodeep full_name: Dey, Soumyodeep last_name: Dey - first_name: Fabio full_name: Di Pumpo, Fabio last_name: Di Pumpo - first_name: Goran S. full_name: Djordjevic, Goran S. last_name: Djordjevic - first_name: Babette full_name: Döbrich, Babette last_name: Döbrich - first_name: Peter full_name: Dornan, Peter last_name: Dornan - first_name: Michael full_name: Doser, Michael last_name: Doser - first_name: Giannis full_name: Drougakis, Giannis last_name: Drougakis - first_name: Jacob full_name: Dunningham, Jacob last_name: Dunningham - first_name: Alisher full_name: Duspayev, Alisher last_name: Duspayev - first_name: Sajan full_name: Easo, Sajan last_name: Easo - first_name: Joshua full_name: Eby, Joshua last_name: Eby - first_name: Maxim full_name: Efremov, Maxim last_name: Efremov - first_name: Gedminas full_name: Elertas, Gedminas last_name: Elertas - first_name: John full_name: Ellis, John last_name: Ellis - first_name: Nicholas full_name: Entin, Nicholas last_name: Entin - first_name: Stephen full_name: Fairhurst, Stephen last_name: Fairhurst - first_name: Mattia full_name: Fanì, Mattia last_name: Fanì - first_name: Farida full_name: Fassi, Farida last_name: Fassi - first_name: Pierre full_name: Fayet, Pierre last_name: Fayet - first_name: Daniel full_name: Felea, Daniel last_name: Felea - first_name: Jie full_name: Feng, Jie last_name: Feng - first_name: Robert full_name: Flack, Robert last_name: Flack - first_name: Chris full_name: Foot, Chris last_name: Foot - first_name: Tim full_name: Freegarde, Tim last_name: Freegarde - first_name: Elina full_name: Fuchs, Elina last_name: Fuchs - first_name: Naceur full_name: Gaaloul, Naceur last_name: Gaaloul - first_name: Dongfeng full_name: Gao, Dongfeng last_name: Gao - first_name: Susan full_name: Gardner, Susan last_name: Gardner - first_name: Barry M. full_name: Garraway, Barry M. last_name: Garraway - first_name: Carlos L. full_name: Garrido Alzar, Carlos L. last_name: Garrido Alzar - first_name: Alexandre full_name: Gauguet, Alexandre last_name: Gauguet - first_name: Enno full_name: Giese, Enno last_name: Giese - first_name: Patrick full_name: Gill, Patrick last_name: Gill - first_name: Gian F. full_name: Giudice, Gian F. last_name: Giudice - first_name: Eric P. full_name: Glasbrenner, Eric P. last_name: Glasbrenner - first_name: Jonah full_name: Glick, Jonah last_name: Glick - first_name: Peter W. full_name: Graham, Peter W. last_name: Graham - first_name: Eduardo full_name: Granados, Eduardo last_name: Granados - first_name: Paul F. full_name: Griffin, Paul F. last_name: Griffin - first_name: Jordan full_name: Gué, Jordan last_name: Gué - first_name: Saïda full_name: Guellati-Khelifa, Saïda last_name: Guellati-Khelifa - first_name: Subhadeep full_name: Gupta, Subhadeep last_name: Gupta - first_name: Vishu full_name: Gupta, Vishu last_name: Gupta - first_name: Lucia full_name: Hackermueller, Lucia last_name: Hackermueller - first_name: Martin full_name: Haehnelt, Martin last_name: Haehnelt - first_name: Timo full_name: Hakulinen, Timo last_name: Hakulinen - first_name: Klemens full_name: Hammerer, Klemens last_name: Hammerer - first_name: Ekim T. full_name: Hanımeli, Ekim T. last_name: Hanımeli - first_name: Tiffany full_name: Harte, Tiffany last_name: Harte - first_name: Sabrina full_name: Hartmann, Sabrina last_name: Hartmann - first_name: Leonie full_name: Hawkins, Leonie last_name: Hawkins - first_name: Aurelien full_name: Hees, Aurelien last_name: Hees - first_name: Alexander full_name: Herbst, Alexander last_name: Herbst - first_name: Thomas M. full_name: Hird, Thomas M. last_name: Hird - first_name: Richard full_name: Hobson, Richard last_name: Hobson - first_name: Jason full_name: Hogan, Jason last_name: Hogan - first_name: Bodil full_name: Holst, Bodil last_name: Holst - first_name: Michael full_name: Holynski, Michael last_name: Holynski - first_name: Onur full_name: Hosten, Onur id: 4C02D85E-F248-11E8-B48F-1D18A9856A87 last_name: Hosten orcid: 0000-0002-2031-204X - first_name: Chung Chuan full_name: Hsu, Chung Chuan last_name: Hsu - first_name: Wayne Cheng Wei full_name: Huang, Wayne Cheng Wei last_name: Huang - first_name: Kenneth M. full_name: Hughes, Kenneth M. last_name: Hughes - first_name: Kamran full_name: Hussain, Kamran last_name: Hussain - first_name: Gert full_name: Hütsi, Gert last_name: Hütsi - first_name: Antonio full_name: Iovino, Antonio last_name: Iovino - first_name: Maria Catalina full_name: Isfan, Maria Catalina last_name: Isfan - first_name: Gregor full_name: Janson, Gregor last_name: Janson - first_name: Peter full_name: Jeglič, Peter last_name: Jeglič - first_name: Philippe full_name: Jetzer, Philippe last_name: Jetzer - first_name: Yijun full_name: Jiang, Yijun last_name: Jiang - first_name: Gediminas full_name: Juzeliūnas, Gediminas last_name: Juzeliūnas - first_name: Wilhelm full_name: Kaenders, Wilhelm last_name: Kaenders - 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first_name: Fiodor full_name: Sorrentino, Fiodor last_name: Sorrentino - first_name: Alessandro D.A.M. full_name: Spallicci, Alessandro D.A.M. last_name: Spallicci - first_name: Petruta full_name: Stefanescu, Petruta last_name: Stefanescu - first_name: Nikolaos full_name: Stergioulas, Nikolaos last_name: Stergioulas - first_name: Daniel full_name: Stoerk, Daniel last_name: Stoerk - first_name: Hrudya full_name: Thaivalappil Sunilkumar, Hrudya last_name: Thaivalappil Sunilkumar - first_name: Jannik full_name: Ströhle, Jannik last_name: Ströhle - first_name: Zoie full_name: Tam, Zoie last_name: Tam - first_name: Dhruv full_name: Tandon, Dhruv last_name: Tandon - first_name: Yijun full_name: Tang, Yijun last_name: Tang - first_name: Dorothee full_name: Tell, Dorothee last_name: Tell - first_name: Jacques full_name: Tempere, Jacques last_name: Tempere - first_name: Dylan J. full_name: Temples, Dylan J. last_name: Temples - first_name: Rohit P. full_name: Thampy, Rohit P. last_name: Thampy - first_name: Ingmari C. full_name: Tietje, Ingmari C. last_name: Tietje - first_name: Guglielmo M. full_name: Tino, Guglielmo M. last_name: Tino - first_name: Jonathan N. full_name: Tinsley, Jonathan N. last_name: Tinsley - first_name: Ovidiu full_name: Tintareanu Mircea, Ovidiu last_name: Tintareanu Mircea - first_name: Kimberly full_name: Tkalčec, Kimberly last_name: Tkalčec - first_name: Andrew J. full_name: Tolley, Andrew J. last_name: Tolley - first_name: Vincenza full_name: Tornatore, Vincenza last_name: Tornatore - first_name: Alejandro full_name: Torres-Orjuela, Alejandro last_name: Torres-Orjuela - first_name: Philipp full_name: Treutlein, Philipp last_name: Treutlein - first_name: Andrea full_name: Trombettoni, Andrea last_name: Trombettoni - first_name: Christian full_name: Ufrecht, Christian last_name: Ufrecht - first_name: Juan full_name: Urrutia, Juan last_name: Urrutia - first_name: Tristan full_name: Valenzuela, Tristan last_name: Valenzuela - first_name: Linda R. full_name: Valerio, Linda R. last_name: Valerio - first_name: Maurits full_name: Van Der Grinten, Maurits last_name: Van Der Grinten - first_name: Ville full_name: Vaskonen, Ville last_name: Vaskonen - first_name: Verónica full_name: Vázquez-Aceves, Verónica last_name: Vázquez-Aceves - first_name: Hardi full_name: Veermäe, Hardi last_name: Veermäe - first_name: Flavio full_name: Vetrano, Flavio last_name: Vetrano - first_name: Nikolay V. full_name: Vitanov, Nikolay V. last_name: Vitanov - first_name: Wolf full_name: Von Klitzing, Wolf last_name: Von Klitzing - first_name: Sebastian full_name: Wald, Sebastian id: 133F200A-B015-11E9-AD41-0EDAE5697425 last_name: Wald orcid: 0000-0002-5869-1604 - first_name: Thomas full_name: Walker, Thomas last_name: Walker - first_name: Reinhold full_name: Walser, Reinhold last_name: Walser - first_name: Jin full_name: Wang, Jin last_name: Wang - first_name: Yan full_name: Wang, Yan last_name: Wang - first_name: C. A. full_name: Weidner, C. A. last_name: Weidner - first_name: André full_name: Wenzlawski, André last_name: Wenzlawski - first_name: Michael full_name: Werner, Michael last_name: Werner - first_name: Lisa full_name: Wörner, Lisa last_name: Wörner - first_name: Mohamed E. full_name: Yahia, Mohamed E. last_name: Yahia - first_name: Efe full_name: Yazgan, Efe last_name: Yazgan - first_name: Emmanuel full_name: Zambrini Cruzeiro, Emmanuel last_name: Zambrini Cruzeiro - first_name: M. full_name: Zarei, M. last_name: Zarei - first_name: Mingsheng full_name: Zhan, Mingsheng last_name: Zhan - first_name: Shengnan full_name: Zhang, Shengnan last_name: Zhang - first_name: Lin full_name: Zhou, Lin last_name: Zhou - first_name: Erik full_name: Zupanič, Erik last_name: Zupanič citation: ama: 'Abdalla A, Abe M, Abend S, et al. Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop. EPJ Quantum Technology. 2025;12. doi:10.1140/epjqt/s40507-025-00344-3' apa: 'Abdalla, A., Abe, M., Abend, S., Abidi, M., Aidelsburger, M., Alibabaei, A., … Zupanič, E. (2025). Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop. EPJ Quantum Technology. Springer Nature. https://doi.org/10.1140/epjqt/s40507-025-00344-3' chicago: 'Abdalla, Adam, Mahiro Abe, Sven Abend, Mouine Abidi, Monika Aidelsburger, Ashkan Alibabaei, Baptiste Allard, et al. “Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the Second Workshop.” EPJ Quantum Technology. Springer Nature, 2025. https://doi.org/10.1140/epjqt/s40507-025-00344-3.' ieee: 'A. Abdalla et al., “Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop,” EPJ Quantum Technology, vol. 12. Springer Nature, 2025.' ista: 'Abdalla A et al. 2025. Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop. EPJ Quantum Technology. 12, 42.' mla: 'Abdalla, Adam, et al. “Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the Second Workshop.” EPJ Quantum Technology, vol. 12, 42, Springer Nature, 2025, doi:10.1140/epjqt/s40507-025-00344-3.' short: A. Abdalla, M. Abe, S. Abend, M. Abidi, M. Aidelsburger, A. Alibabaei, B. Allard, J. Antoniadis, G. Arduini, N. Augst, P. Balamatsias, A. Balaž, H. Banks, R.L. Barcklay, M. Barone, M. Barsanti, M.G. Bason, A. Bassi, J.B. Bayle, C.F.A. Baynham, Q. Beaufils, S. Beldjoudi, A. Belić, S. Bennetts, J. Bernabeu, A. Bertoldi, C. Bigard, N.P. Bigelow, R. Bingham, D. Blas, A. Bobrick, S. Boehringer, A. Bogojević, K. Bongs, D. Bortoletto, P. Bouyer, C. Brand, O. Buchmueller, G. Buica, S. Calatroni, L. Calmels, P. Canizares, B. Canuel, A. Caramete, L.I. Caramete, M. Carlesso, J. Carlton, S.P. Carman, A. Carroll, M. Casariego, M. Chairetis, V. Charmandaris, U. Chauhan, J. Chen, M.L.M.L.M. Chiofalo, D. Ciampini, A. Cimbri, P. Cladé, J. Coleman, F.L. Constantin, C.R. Contaldi, R. Corgier, B. Dash, G.J. Davies, C. De Rham, A. De Roeck, D. Derr, S. Dey, F. Di Pumpo, G.S. Djordjevic, B. Döbrich, P. Dornan, M. Doser, G. Drougakis, J. Dunningham, A. Duspayev, S. Easo, J. Eby, M. Efremov, G. Elertas, J. Ellis, N. Entin, S. Fairhurst, M. Fanì, F. Fassi, P. Fayet, D. Felea, J. Feng, R. Flack, C. Foot, T. Freegarde, E. Fuchs, N. Gaaloul, D. Gao, S. Gardner, B.M. Garraway, C.L. Garrido Alzar, A. Gauguet, E. Giese, P. Gill, G.F. Giudice, E.P. Glasbrenner, J. Glick, P.W. Graham, E. Granados, P.F. Griffin, J. Gué, S. Guellati-Khelifa, S. Gupta, V. Gupta, L. Hackermueller, M. Haehnelt, T. Hakulinen, K. Hammerer, E.T. Hanımeli, T. Harte, S. Hartmann, L. Hawkins, A. Hees, A. Herbst, T.M. Hird, R. Hobson, J. Hogan, B. Holst, M. Holynski, O. Hosten, C.C. Hsu, W.C.W. Huang, K.M. Hughes, K. Hussain, G. Hütsi, A. Iovino, M.C. Isfan, G. Janson, P. Jeglič, P. Jetzer, Y. Jiang, G. Juzeliūnas, W. Kaenders, M. Kalliokoski, A. Kehagias, E. Kilian, C. Klempt, P. Knight, S. Koley, B. Konrad, T. Kovachy, M. Krutzik, M. Kumar, P. Kumar, H. Labiad, S.Y. Lan, A. Landragin, G. Landsberg, M. Langlois, B. Lanigan, B. Leone, C. Le Poncin-Lafitte, S. Lellouch, M. Lewicki, Y.H. Lien, L. Lombriser, E.L. Asamar, J.L. Lopez-Gonzalez, C. Lu, G.G. Luciano, N. Lundblad, C. De J. López Monjaraz, A. Lowe, M. Mackoit-Sinkevičienė, M. Maggiore, A. Majumdar, K. Makris, A. Maleknejad, A.L. Marchant, A. Mariotti, C. Markou, B. Matthews, A. Mazumdar, C. Mccabe, M. Meister, G. Mentasti, J. Menu, G. Messineo, B. Meyer-Hoppe, S. Micalizio, F. Migliaccio, P. Millington, M. Milosevic, A. Mishra, J. Mitchell, G.W. Morley, N. Mouelle, J. Müller, D. Newbold, W.T. Ni, C. Niehof, J. Noller, S. Odžak, D.K.L. Oi, A. Oikonomou, Y. Omar, C. Overstreet, V. Puthiya Veettil, J. Pahl, S. Paling, Z. Pan, G. Pappas, V. Pareek, E. Pasatembou, M. Paternostro, V.K. Pathak, E. Pelucchi, F. Pereira Dos Santos, A. Peters, A. Pichery, I. Pikovski, A. Pilaftsis, F.C. Pislan, R. Plunkett, R. Poggiani, M. Prevedelli, J. Rafelski, J. Raidal, M. Raidal, E.M. Rasel, S. Renaux-Petel, A. Richaud, P. Rivero-Antunez, T. Rodzinka, A. Roura, J. Rudolph, D. Sabulsky, M.S. Safronova, M. Sakellariadou, L. Salvi, M. Sameed, S. Sarkar, P. Schach, S.A. Schäffer, J. Schelfhout, M. Schilling, V. Schkolnik, W.P. Schleich, D. Schlippert, U. Schneider, F. Schreck, A. Schwartzman, N. Schwersenz, O. Sergijenko, H.R. Sfar, L. Shao, I. Shipsey, J. Shu, Y. Singh, C.F. Sopuerta, M. Sorba, F. Sorrentino, A.D.A.M. Spallicci, P. Stefanescu, N. Stergioulas, D. Stoerk, H. Thaivalappil Sunilkumar, J. Ströhle, Z. Tam, D. Tandon, Y. Tang, D. Tell, J. Tempere, D.J. Temples, R.P. Thampy, I.C. Tietje, G.M. Tino, J.N. Tinsley, O. Tintareanu Mircea, K. Tkalčec, A.J. Tolley, V. Tornatore, A. Torres-Orjuela, P. Treutlein, A. Trombettoni, C. Ufrecht, J. Urrutia, T. Valenzuela, L.R. Valerio, M. Van Der Grinten, V. Vaskonen, V. Vázquez-Aceves, H. Veermäe, F. Vetrano, N.V. Vitanov, W. Von Klitzing, S. Wald, T. Walker, R. Walser, J. Wang, Y. Wang, C.A. Weidner, A. Wenzlawski, M. Werner, L. Wörner, M.E. Yahia, E. Yazgan, E. Zambrini Cruzeiro, M. Zarei, M. Zhan, S. Zhang, L. Zhou, E. Zupanič, EPJ Quantum Technology 12 (2025). date_created: 2025-05-04T22:02:30Z date_published: 2025-04-03T00:00:00Z date_updated: 2025-09-30T12:22:04Z day: '03' ddc: - '530' department: - _id: OnHo doi: 10.1140/epjqt/s40507-025-00344-3 external_id: arxiv: - '2412.14960' isi: - '001489653300001' file: - access_level: open_access checksum: 00c7a97d87f7a6314df5b0c2213fbb02 content_type: application/pdf creator: dernst date_created: 2025-05-05T10:52:52Z date_updated: 2025-05-05T10:52:52Z file_id: '19653' file_name: 2025_EPJQuantumTech_Abdalla.pdf file_size: 14352192 relation: main_file success: 1 file_date_updated: 2025-05-05T10:52:52Z has_accepted_license: '1' intvolume: ' 12' isi: 1 language: - iso: eng license: https://creativecommons.org/licenses/by-nc-nd/4.0/ month: '04' oa: 1 oa_version: Published Version publication: EPJ Quantum Technology publication_identifier: eissn: - 2196-0763 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: 'Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop' 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: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 12 year: '2025' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '19638' abstract: - lang: eng text: The James Webb Space Telescope has revealed low-luminosity active galactic nuclei at redshifts of z ≳ 4–7, many of which host accreting massive black holes (BHs) with BH-to-galaxy mass (MBH/M⋆) ratios exceeding the local values by more than an order of magnitude. The origin of these overmassive BHs remains unclear but requires potential contributions from heavy seeds and/or episodes of super-Eddington accretion. We present a growth model coupled with dark matter halo assembly to explore the evolution of the MBH/M⋆ ratio under different seeding and feedback scenarios. Given the gas inflow rates in protogalaxies, BHs grow episodically at moderate super-Eddington rates, and the mass ratio increases early on, despite significant mass loss through feedback. Regardless of seeding mechanisms, the mass ratio converges to a universal value ∼0.1–0.3, set by the balance between gas feeding and star formation efficiency in the nucleus. This behavior defines an attractor in the MBH–M⋆ diagram, where overmassive BHs grow more slowly than their hosts, while undermassive seeds experience rapid growth before aligning with the attractor. We derive an analytical expression for the universal mass ratio, linking it to feedback strength and halo growth. The convergence of evolutionary tracks erases seeding information from the mass ratio by z ∼ 4–6. Detecting BHs with ∼105−6 M⊙ at higher redshifts that deviate from the convergence trend would provide key diagnostics of their birth conditions. acknowledgement: We thank the anonymous referee for a careful reading of our manuscript and for comments that helped improve this Letter. This work is supported by the Japan Society for the Promotion of Science (JSPS) KAKENHI grant No. 24KF0130. We acknowledge support from the National Natural Science Foundation of China (12073003, 12003003, 11721303, 11991052, 11950410493), and the China Manned Space Project (CMS-CSST-2021-A04 and CMS-CSST-2021-A06). L.C.H. is supported by the National Science Foundation of China (12233001), the National Key R&D Program of China (2022YFF0503401). Z.H. acknowledges support by US NSF grant AST-2006176 and by NASA grant 80NSSC22K0822. Some of the numerical calculation and analysis were performed with the Cray XC50 at the Center for Computational Astrophysics (CfCA) of the National Astronomical Observatory of Japan and with the High-performance Computing Platform of Peking University. article_number: L37 article_processing_charge: Yes article_type: letter_note arxiv: 1 author: - first_name: Haojie full_name: Hu, Haojie last_name: Hu - first_name: Kohei full_name: Inayoshi, Kohei last_name: Inayoshi - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman orcid: 0000-0003-3633-5403 - first_name: Luis C. full_name: Ho, Luis C. last_name: Ho - first_name: Ken full_name: Ohsuga, Ken last_name: Ohsuga citation: ama: Hu H, Inayoshi K, Haiman Z, Ho LC, Ohsuga K. The convergence of heavy and light seeds to overmassive black holes at cosmic dawn. The Astrophysical Journal Letters. 2025;983(2). doi:10.3847/2041-8213/adc680 apa: Hu, H., Inayoshi, K., Haiman, Z., Ho, L. C., & Ohsuga, K. (2025). The convergence of heavy and light seeds to overmassive black holes at cosmic dawn. The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/adc680 chicago: Hu, Haojie, Kohei Inayoshi, Zoltán Haiman, Luis C. Ho, and Ken Ohsuga. “The Convergence of Heavy and Light Seeds to Overmassive Black Holes at Cosmic Dawn.” The Astrophysical Journal Letters. IOP Publishing, 2025. https://doi.org/10.3847/2041-8213/adc680. ieee: H. Hu, K. Inayoshi, Z. Haiman, L. C. Ho, and K. Ohsuga, “The convergence of heavy and light seeds to overmassive black holes at cosmic dawn,” The Astrophysical Journal Letters, vol. 983, no. 2. IOP Publishing, 2025. ista: Hu H, Inayoshi K, Haiman Z, Ho LC, Ohsuga K. 2025. The convergence of heavy and light seeds to overmassive black holes at cosmic dawn. The Astrophysical Journal Letters. 983(2), L37. mla: Hu, Haojie, et al. “The Convergence of Heavy and Light Seeds to Overmassive Black Holes at Cosmic Dawn.” The Astrophysical Journal Letters, vol. 983, no. 2, L37, IOP Publishing, 2025, doi:10.3847/2041-8213/adc680. short: H. Hu, K. Inayoshi, Z. Haiman, L.C. Ho, K. Ohsuga, The Astrophysical Journal Letters 983 (2025). date_created: 2025-05-04T22:02:31Z date_published: 2025-04-20T00:00:00Z date_updated: 2026-02-16T12:44:04Z day: '20' ddc: - '520' department: - _id: ZoHa doi: 10.3847/2041-8213/adc680 external_id: arxiv: - '2503.03870' isi: - '001467616800001' file: - access_level: open_access checksum: 1a4fbeeb12e9022873e86c72d230a5ec content_type: application/pdf creator: dernst date_created: 2025-05-05T11:30:34Z date_updated: 2025-05-05T11:30:34Z file_id: '19655' file_name: 2025_AstrophysicalJourLetters_Hu.pdf file_size: 3334014 relation: main_file success: 1 file_date_updated: 2025-05-05T11:30:34Z has_accepted_license: '1' intvolume: ' 983' isi: 1 issue: '2' language: - iso: eng month: '04' 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 convergence of heavy and light seeds to overmassive black holes at cosmic dawn 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: 983 year: '2025' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold PlanS_conform: '1' _id: '19662' abstract: - lang: eng text: We investigate the effect of changes in the Coriolis force caused by changes in the rotation rate on the top-of-atmosphere (TOA) radiant energy budget of an aquaplanet general circulation model with prescribed sea surface temperatures. We analyse the effective radiative forcing caused by changes from Earth-like rotation to values between 1/32 and 8 times the Earth's rotation rate. The forcing differs by about 60 W m−2 between the fastest and slowest rotation cases, with a monotonically increasing positive forcing for faster-than-Earth-like rotations and a non-monotonically increasing negative forcing for slower rotations. The largest contributions to the forcing are due to changes in, in this order, the shortwave cloud radiative effect (SWCRE) and the clear-sky outgoing longwave radiation (OLR). From the fastest to the slowest rotation, the Hadley cell expands and the troposphere becomes drier, increasing the OLR. This contributes to negative forcing at slower-than-Earth-like rotations and to positive forcing at faster-than-Earth-like rotations. The SWCRE is influenced by changes in the low-level cloudiness within the Hadley cell and the baroclinic regime. With the expansion of the Hadley cell, the area of enhanced tropospheric stability increases, resulting in more low-level clouds, a higher SWCRE, and increased negative forcing. The non-monotonicity results from an intermediate decrease in the SWCRE caused by the disappearance of baroclinic eddies as the Hadley cell reaches global extension. At rotations faster than Earth-like, the decrease in the SWCRE, mainly due to the weakening of baroclinic eddies and storm systems, leads to an increase in positive forcing. In summary, changes in the SWCRE, driven by different circulation responses at slower-than-Earth-like and faster-than-Earth-like rotations, strongly influence the TOA radiant energy budget. These effects, along with a substantial contribution from the clear-sky OLR, could impact the habitability of Earth-like rotating planets. acknowledgement: "We thank Bjorn Stevens for suggesting the study and for substantial ideas along the way. We also thank Sebastian Rast for helping with the model compilation. This work used resources of the German Climate Computing Center (DKRZ) under project ID mh0066 for our experiments and analysis. Jiawei Bao acknowledges the European Union's Horizon 2020 for funding.Jiawei Bao has been supported by the European Union's Horizon 2020 research and innovation programme under a Marie Skłodowska-Curie grant (grant agreement no. 101034413).\r\nThe article processing charges for this open-access publication were covered by the Max Planck Society." article_processing_charge: Yes (via OA deal) article_type: original author: - first_name: Abisha Mary full_name: Gnanaraj, Abisha Mary last_name: Gnanaraj - first_name: Jiawei full_name: Bao, Jiawei id: bb9a7399-fefd-11ed-be3c-ae648fd1d160 last_name: Bao - first_name: Hauke full_name: Schmidt, Hauke last_name: Schmidt citation: ama: 'Gnanaraj AM, Bao J, Schmidt H. The impact of the rotation rate on an aquaplanet’s radiant energy budget: Insights from experiments varying the Coriolis parameter. Weather and Climate Dynamics. 2025;6(2):489-503. doi:10.5194/wcd-6-489-2025' apa: 'Gnanaraj, A. M., Bao, J., & Schmidt, H. (2025). The impact of the rotation rate on an aquaplanet’s radiant energy budget: Insights from experiments varying the Coriolis parameter. Weather and Climate Dynamics. Copernicus Publications. https://doi.org/10.5194/wcd-6-489-2025' chicago: 'Gnanaraj, Abisha Mary, Jiawei Bao, and Hauke Schmidt. “The Impact of the Rotation Rate on an Aquaplanet’s Radiant Energy Budget: Insights from Experiments Varying the Coriolis Parameter.” Weather and Climate Dynamics. Copernicus Publications, 2025. https://doi.org/10.5194/wcd-6-489-2025.' ieee: 'A. M. Gnanaraj, J. Bao, and H. Schmidt, “The impact of the rotation rate on an aquaplanet’s radiant energy budget: Insights from experiments varying the Coriolis parameter,” Weather and Climate Dynamics, vol. 6, no. 2. Copernicus Publications, pp. 489–503, 2025.' ista: 'Gnanaraj AM, Bao J, Schmidt H. 2025. The impact of the rotation rate on an aquaplanet’s radiant energy budget: Insights from experiments varying the Coriolis parameter. Weather and Climate Dynamics. 6(2), 489–503.' mla: 'Gnanaraj, Abisha Mary, et al. “The Impact of the Rotation Rate on an Aquaplanet’s Radiant Energy Budget: Insights from Experiments Varying the Coriolis Parameter.” Weather and Climate Dynamics, vol. 6, no. 2, Copernicus Publications, 2025, pp. 489–503, doi:10.5194/wcd-6-489-2025.' short: A.M. Gnanaraj, J. Bao, H. Schmidt, Weather and Climate Dynamics 6 (2025) 489–503. date_created: 2025-05-11T22:02:38Z date_published: 2025-04-25T00:00:00Z date_updated: 2025-07-09T08:40:18Z day: '25' ddc: - '550' department: - _id: CaMu doi: 10.5194/wcd-6-489-2025 ec_funded: 1 file: - access_level: open_access checksum: 2ea68f7e51ee39ccb6886719a83a78ca content_type: application/pdf creator: dernst date_created: 2025-05-12T08:23:10Z date_updated: 2025-05-12T08:23:10Z file_id: '19680' file_name: 2025_WeatherClimateDynam_Gnanaraj.pdf file_size: 6500575 relation: main_file success: 1 file_date_updated: 2025-05-12T08:23:10Z has_accepted_license: '1' intvolume: ' 6' issue: '2' language: - iso: eng month: '04' oa: 1 oa_version: Published Version page: 489-503 project: - _id: fc2ed2f7-9c52-11eb-aca3-c01059dda49c call_identifier: H2020 grant_number: '101034413' name: 'IST-BRIDGE: International postdoctoral program' publication: Weather and Climate Dynamics publication_identifier: eissn: - 2698-4016 publication_status: published publisher: Copernicus Publications quality_controlled: '1' scopus_import: '1' status: public title: 'The impact of the rotation rate on an aquaplanet''s radiant energy budget: Insights from experiments varying the Coriolis parameter' 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: 6 year: '2025' ... --- OA_place: repository OA_type: green _id: '19769' abstract: - lang: eng text: "Artifact to reproduce the experimental results presented in the article \"Sound Statistical Model Checking for Probabilities and Expected Rewards\" by Carlos E. Budde, Arnd Hartmanns, Tobias Meggendorfer, Maximilian Weininger, and Patrick Wienhöft (TACAS 2025).\r\n\r\nThe contents include all data and software (formal models, software tools, Python & bash scripts) used in the experimental evaluation presented in sections 3, 4, and 6 of the article. Detailed instructions on how to reproduce the results are bundled in the artifact." article_processing_charge: No author: - first_name: Carlos full_name: Budde, Carlos last_name: Budde - first_name: Arnd full_name: Hartmanns, Arnd last_name: Hartmanns - first_name: Tobias full_name: Meggendorfer, Tobias id: b21b0c15-30a2-11eb-80dc-f13ca25802e1 last_name: Meggendorfer orcid: 0000-0002-1712-2165 - first_name: Maximilian full_name: Weininger, Maximilian id: 02ab0197-cc70-11ed-ab61-918e71f56881 last_name: Weininger - first_name: Patrick full_name: Wienhöft, Patrick last_name: Wienhöft citation: ama: Budde C, Hartmanns A, Meggendorfer T, Weininger M, Wienhöft P. Sound statistical model checking for probabilities and expected rewards (experimental reproduction package). 2025. doi:10.5281/ZENODO.14602066 apa: Budde, C., Hartmanns, A., Meggendorfer, T., Weininger, M., & Wienhöft, P. (2025). Sound statistical model checking for probabilities and expected rewards (experimental reproduction package). Zenodo. https://doi.org/10.5281/ZENODO.14602066 chicago: Budde, Carlos, Arnd Hartmanns, Tobias Meggendorfer, Maximilian Weininger, and Patrick Wienhöft. “Sound Statistical Model Checking for Probabilities and Expected Rewards (Experimental Reproduction Package).” Zenodo, 2025. https://doi.org/10.5281/ZENODO.14602066. ieee: C. Budde, A. Hartmanns, T. Meggendorfer, M. Weininger, and P. Wienhöft, “Sound statistical model checking for probabilities and expected rewards (experimental reproduction package).” Zenodo, 2025. ista: Budde C, Hartmanns A, Meggendorfer T, Weininger M, Wienhöft P. 2025. Sound statistical model checking for probabilities and expected rewards (experimental reproduction package), Zenodo, 10.5281/ZENODO.14602066. mla: Budde, Carlos, et al. Sound Statistical Model Checking for Probabilities and Expected Rewards (Experimental Reproduction Package). Zenodo, 2025, doi:10.5281/ZENODO.14602066. short: C. Budde, A. Hartmanns, T. Meggendorfer, M. Weininger, P. Wienhöft, (2025). date_created: 2025-06-02T09:37:14Z date_published: 2025-01-07T00:00:00Z date_updated: 2025-06-02T09:45:41Z day: '07' ddc: - '000' department: - _id: KrCh doi: 10.5281/ZENODO.14602066 main_file_link: - open_access: '1' url: https://doi.org/10.5281/ZENODO.14602066 month: '01' oa: 1 oa_version: Published Version publisher: Zenodo related_material: record: - id: '19742' relation: used_in_publication status: public status: public title: Sound statistical model checking for probabilities and expected rewards (experimental reproduction package) type: research_data_reference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 year: '2025' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold _id: '20977' abstract: - lang: eng text: Hippocampal sharp-wave ripples (SPW-Rs) are high-frequency oscillations critical for memory consolidation. Despite extensive characterization in rodents, their detection in humans is limited by coarse spatial sampling, interictal epileptiform discharges (IEDs), and a lack of consensus on human ripple localization and morphology. Here, we demonstrate that mouse and human hippocampal ripples share spatial, spectral and temporal features, which are clearly distinct from IEDs. In recordings from male APP/PS1 mice, SPW-Rs were distinguishable from IEDs by multiple criteria. Hippocampal ripples recorded during NREM sleep in female and male surgical epilepsy patients exhibited similar narrowband frequency peaks and multiple ripple cycles in the CA1 and subiculum regions. Conversely, IEDs showed a broad spatial extent and wide-band frequency power. We developed a semi-automated, ripple curation toolbox (ripmap) to separate event waveforms by low-dimensional embedding to reduce false-positive rate in selected ripple channels. Our approach improves ripple detection and provides a firm foundation for future human memory research. acknowledgement: We thank Karl Rössler and Sebastian Brandner for the human SEEG implantations; Katja Kobow for providing the histopathological findings of the patients; Jay Jeschke for help with human electrode localization; Esha Brahmbhatt and Deren Aykan for help with animal habituation; Mursel Karadas for the rodent treadmill design; Nicholas Paleologos, Noam Nitzan, Michael D Hadler and Samuel McKenzie for rating events in a human ripple survey included in a previous version of the manuscript; Nicholas Paleologos for sharing NYU iEEG data for validating UMAP parameters; Julio Esparza for help on the topological analysis through discussions; Thomas Hainmüller, Yiyao Zhang and Mursel Karadas for feedback on the manuscript. We would like to acknowledge Corticale SRL (Genoa, Italy) for providing the SiNAPS probes, and NeuroNexus (Ann Arbor, MI) for their contribution of the data acquisition system and Radiens software. We further acknowledge both Corticale and NeuroNexus for training and support making this research possible. This work was supported by the German Research Foundation (DFG; Walter Benjamin Fellowship MA 10301/1-1, A.M.), NYU Langone Health Finding a Cure for Epilepsy and Seizures (FACES, A.M.), the NOMIS Fellowship (A.N.-O.), the National Institutes of Health (R01NS127954, K23NS104252, A.L.; MH122391, U19NS107616, R01MH139216 G.B.,), and the NYU Department of Neurology (A.L.). article_number: '11636' article_processing_charge: Yes article_type: original author: - first_name: Anna full_name: Maslarova, Anna last_name: Maslarova - first_name: Jiyun N. full_name: Shin, Jiyun N. last_name: Shin - first_name: Andrea C full_name: Navas Olivé, Andrea C id: 739d26c9-52e8-11ee-8d72-f14d3893b4ce last_name: Navas Olivé orcid: 0000-0002-9280-8597 - first_name: Mihály full_name: Vöröslakos, Mihály last_name: Vöröslakos - first_name: Hajo full_name: Hamer, Hajo last_name: Hamer - first_name: Arnd full_name: Doerfler, Arnd last_name: Doerfler - first_name: Simon full_name: Henin, Simon last_name: Henin - first_name: György full_name: Buzsáki, György last_name: Buzsáki - first_name: Anli full_name: Liu, Anli last_name: Liu citation: ama: Maslarova A, Shin JN, Navas Olivé AC, et al. Spatiotemporal patterns differentiate hippocampal sharp-wave ripples from interictal epileptiform discharges in mice and humans. Nature Communications. 2025;16. doi:10.1038/s41467-025-66562-6 apa: Maslarova, A., Shin, J. N., Navas Olivé, A. C., Vöröslakos, M., Hamer, H., Doerfler, A., … Liu, A. (2025). Spatiotemporal patterns differentiate hippocampal sharp-wave ripples from interictal epileptiform discharges in mice and humans. Nature Communications. Springer Nature. https://doi.org/10.1038/s41467-025-66562-6 chicago: Maslarova, Anna, Jiyun N. Shin, Andrea C Navas Olivé, Mihály Vöröslakos, Hajo Hamer, Arnd Doerfler, Simon Henin, György Buzsáki, and Anli Liu. “Spatiotemporal Patterns Differentiate Hippocampal Sharp-Wave Ripples from Interictal Epileptiform Discharges in Mice and Humans.” Nature Communications. Springer Nature, 2025. https://doi.org/10.1038/s41467-025-66562-6. ieee: A. Maslarova et al., “Spatiotemporal patterns differentiate hippocampal sharp-wave ripples from interictal epileptiform discharges in mice and humans,” Nature Communications, vol. 16. Springer Nature, 2025. ista: Maslarova A, Shin JN, Navas Olivé AC, Vöröslakos M, Hamer H, Doerfler A, Henin S, Buzsáki G, Liu A. 2025. Spatiotemporal patterns differentiate hippocampal sharp-wave ripples from interictal epileptiform discharges in mice and humans. Nature Communications. 16, 11636. mla: Maslarova, Anna, et al. “Spatiotemporal Patterns Differentiate Hippocampal Sharp-Wave Ripples from Interictal Epileptiform Discharges in Mice and Humans.” Nature Communications, vol. 16, 11636, Springer Nature, 2025, doi:10.1038/s41467-025-66562-6. short: A. Maslarova, J.N. Shin, A.C. Navas Olivé, M. Vöröslakos, H. Hamer, A. Doerfler, S. Henin, G. Buzsáki, A. Liu, Nature Communications 16 (2025). date_created: 2026-01-11T23:01:35Z date_published: 2025-12-30T00:00:00Z date_updated: 2026-01-12T09:31:56Z day: '30' ddc: - '570' department: - _id: PeJo doi: 10.1038/s41467-025-66562-6 external_id: pmid: - '39975118' file: - access_level: open_access checksum: a8a1670e197484382e087be60f643945 content_type: application/pdf creator: dernst date_created: 2026-01-12T09:30:15Z date_updated: 2026-01-12T09:30:15Z file_id: '20978' file_name: 2025_NatureComm_Maslarova.pdf file_size: 7629997 relation: main_file success: 1 file_date_updated: 2026-01-12T09:30:15Z has_accepted_license: '1' intvolume: ' 16' language: - iso: eng month: '12' oa: 1 oa_version: Published Version pmid: 1 project: - _id: 9B861AAC-BA93-11EA-9121-9846C619BF3A name: NOMIS Fellowship Program publication: Nature Communications publication_identifier: eissn: - 2041-1723 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Spatiotemporal patterns differentiate hippocampal sharp-wave ripples from interictal epileptiform discharges in mice and humans 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: '2025' ... --- DOAJ_listed: '1' OA_place: publisher OA_type: gold PlanS_conform: '1' _id: '21057' abstract: - lang: eng text: Among the most puzzling early discoveries of JWST are “little red dots” (LRDs), compact red sources that host broad Balmer emission lines, and in many cases exhibit a “V-shaped” change in slope in the rest-optical. The physical properties of LRDs currently have order-of-magnitude uncertainties, because models to explain the continuum of these sources differ immensely. Here, we leverage the complete selection of red sources in the RUBIES program, supplemented with public PRISM spectra, to study the origin of this V shape. By fitting a broken power law with a flexible inflection point, we find that a large fraction of red Hα emitters at 2 < z < 6 exhibit a strong change in slope, and that all strong inflections appear associated with the Balmer limit (0.3645 μm). Using a simple model of a reddened active galactic nucleus (AGN) with an unobscured scattered-light component, we demonstrate that the observed V shape in LRDs is unlikely to occur at any specific wavelength if the entire continuum is dominated by light from a power-law AGN continuum. In contrast, models with an intrinsic feature at the Balmer limit, such as those that are dominated by an evolved stellar population, can produce the observed spectral shapes, provided that a reddened component picks up sufficiently redward of the break. While no model can comfortably explain the full LRD spectral energy distribution, the common inflection location suggests that a single component consistently dominates the rest-frame UV optical in LRDs, and that this component is associated with T ∼ 10^4 K hydrogen. acknowledgement: "This 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. The specific observations analyzed can be accessed via DOI: 10.17909/0esg-h949. All of the data products presented herein were retrieved from the Dawn JWST Archive (DJA). DJA is an initiative of the Cosmic Dawn Center, which is funded by the Danish National Research Foundation under grant No. 140. We express gratitude toward the members of the GTO, GO, and DDT teams, whose public data we utilized in this work.\r\n\r\nSupport for this work was provided by The Brinson Foundation through a Brinson Prize Fellowship grant. Support for program No. 4233 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 research was supported by the International Space Science Institute (ISSI) in Bern, through ISSI International Team project No. 562. D.S. acknowledges helpful conversations with Xiaohui Fan and Jared Siegel that contributed to the quality of this work, in addition to aesthetic sign-off from Stephanie Permut on the colors of figures. T.B.M. was supported by a CIERA fellowship. 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." article_number: '118' article_processing_charge: Yes article_type: original arxiv: 1 author: - first_name: David J. full_name: Setton, David J. last_name: Setton - first_name: Jenny E. full_name: Greene, Jenny E. last_name: Greene - first_name: Anna full_name: de Graaff, Anna last_name: de Graaff - first_name: Yilun 逸伦 full_name: Ma, Yilun 逸伦 last_name: Ma - 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: Rachel full_name: Bezanson, Rachel last_name: Bezanson - first_name: Leindert A. full_name: Boogaard, Leindert A. last_name: Boogaard - first_name: Nikko J. full_name: Cleri, Nikko J. last_name: Cleri - first_name: Harley full_name: Katz, Harley last_name: Katz - first_name: Ivo full_name: Labbe, Ivo last_name: Labbe - first_name: Michael V. full_name: Maseda, Michael V. last_name: Maseda - first_name: Ian full_name: McConachie, Ian last_name: McConachie - first_name: Tim B. full_name: Miller, Tim B. last_name: Miller - first_name: Sedona H. full_name: Price, Sedona H. last_name: Price - first_name: Katherine A. full_name: Suess, Katherine A. last_name: Suess - first_name: Pieter full_name: van Dokkum, Pieter last_name: van Dokkum - first_name: Bingjie 冰洁 full_name: Wang 王, Bingjie 冰洁 last_name: Wang 王 - first_name: Andrea full_name: Weibel, Andrea last_name: Weibel - first_name: Katherine E. full_name: Whitaker, Katherine E. last_name: Whitaker - first_name: Christina C. full_name: Williams, Christina C. last_name: Williams citation: ama: 'Setton DJ, Greene JE, de Graaff A, et al. Little Red Dots at an inflection point: Ubiquitous v-shaped turnover consistently occurs at the Balmer limit. The Astrophysical Journal. 2025;995(1). doi:10.3847/1538-4357/ae1500' apa: 'Setton, D. J., Greene, J. E., de Graaff, A., Ma, Y. 逸伦, Leja, J., Matthee, J. J., … Williams, C. C. (2025). Little Red Dots at an inflection point: Ubiquitous v-shaped turnover consistently occurs at the Balmer limit. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ae1500' chicago: 'Setton, David J., Jenny E. Greene, Anna de Graaff, Yilun 逸伦 Ma, Joel Leja, Jorryt J Matthee, Rachel Bezanson, et al. “Little Red Dots at an Inflection Point: Ubiquitous v-Shaped Turnover Consistently Occurs at the Balmer Limit.” The Astrophysical Journal. IOP Publishing, 2025. https://doi.org/10.3847/1538-4357/ae1500.' ieee: 'D. J. Setton et al., “Little Red Dots at an inflection point: Ubiquitous v-shaped turnover consistently occurs at the Balmer limit,” The Astrophysical Journal, vol. 995, no. 1. IOP Publishing, 2025.' ista: 'Setton DJ, Greene JE, de Graaff A, Ma Y逸伦, Leja J, Matthee JJ, Bezanson R, Boogaard LA, Cleri NJ, Katz H, Labbe I, Maseda MV, McConachie I, Miller TB, Price SH, Suess KA, van Dokkum P, Wang 王 B冰洁, Weibel A, Whitaker KE, Williams CC. 2025. Little Red Dots at an inflection point: Ubiquitous v-shaped turnover consistently occurs at the Balmer limit. The Astrophysical Journal. 995(1), 118.' mla: 'Setton, David J., et al. “Little Red Dots at an Inflection Point: Ubiquitous v-Shaped Turnover Consistently Occurs at the Balmer Limit.” The Astrophysical Journal, vol. 995, no. 1, 118, IOP Publishing, 2025, doi:10.3847/1538-4357/ae1500.' short: D.J. Setton, J.E. Greene, A. de Graaff, Y.逸伦 Ma, J. Leja, J.J. Matthee, R. Bezanson, L.A. Boogaard, N.J. Cleri, H. Katz, I. Labbe, M.V. Maseda, I. McConachie, T.B. Miller, S.H. Price, K.A. Suess, P. van Dokkum, B.冰洁 Wang 王, A. Weibel, K.E. Whitaker, C.C. Williams, The Astrophysical Journal 995 (2025). date_created: 2026-01-28T15:21:47Z date_published: 2025-12-09T00:00:00Z date_updated: 2026-02-09T06:41:48Z day: '09' ddc: - '520' department: - _id: JoMa doi: 10.3847/1538-4357/ae1500 external_id: arxiv: - '2411.03424' file: - access_level: open_access checksum: 2a424eb43748a6370ff058c98adb15c6 content_type: application/pdf creator: dernst date_created: 2026-02-09T06:39:23Z date_updated: 2026-02-09T06:39:23Z file_id: '21163' file_name: 2025_AstrophysicalJournal_Setton.pdf file_size: 1989640 relation: main_file success: 1 file_date_updated: 2026-02-09T06:39:23Z has_accepted_license: '1' intvolume: ' 995' issue: '1' language: - iso: eng month: '12' 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: 'Little Red Dots at an inflection point: Ubiquitous v-shaped turnover consistently occurs at the Balmer limit' 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: 995 year: '2025' ...