[{"OA_place":"publisher","status":"public","publication":"Proceedings of the National Academy of Sciences","page":"e2512274122","department":[{"_id":"JiFr"}],"publisher":"National Academy of Sciences","oa":1,"file":[{"access_level":"open_access","date_updated":"2025-11-24T13:48:09Z","content_type":"application/pdf","file_id":"20681","relation":"main_file","creator":"dernst","success":1,"file_name":"2025_PNAS_Sheng.pdf","checksum":"38b723a909bf321d7ee537c9d064aa25","file_size":2667764,"date_created":"2025-11-24T13:48:09Z"}],"isi":1,"OA_type":"hybrid","_id":"20635","article_processing_charge":"Yes (in subscription journal)","acknowledgement":"This research was funded by Biological Breeding-National Science and Technology Major Project (2023ZD0407201), China Postdoctoral Science Foundation (2024M763575), China Agricultural University Fund (2025RC042), Chinese Universities Scientific Fund (2024RC031), and Austrian Science Fund (FWF; I 6123-B).","external_id":{"pmid":["40986351"],"isi":["001589177800001"]},"quality_controlled":"1","ddc":["580"],"tmp":{"name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)","short":"CC BY-NC-ND (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","image":"/images/cc_by_nc_nd.png"},"issue":"39","day":"23","date_created":"2025-11-12T10:03:20Z","pmid":1,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_status":"published","intvolume":" 122","article_type":"original","language":[{"iso":"eng"}],"project":[{"_id":"bd76d395-d553-11ed-ba76-f678c14f9033","grant_number":"I06123","name":"Peptide receptors for auxin canalization in Arabidopsis"}],"file_date_updated":"2025-11-24T13:48:09Z","has_accepted_license":"1","PlanS_conform":"1","volume":122,"date_published":"2025-09-23T00:00:00Z","month":"09","license":"https://creativecommons.org/licenses/by-nc-nd/4.0/","doi":"10.1073/pnas.2512274122","scopus_import":"1","citation":{"ieee":"F. Sheng et al., “Antagonistic SnRK2 and PID kinases’ action on auxin transport-mediated root gravitropism,” Proceedings of the National Academy of Sciences, vol. 122, no. 39. National Academy of Sciences, p. e2512274122, 2025.","mla":"Sheng, F., et al. “Antagonistic SnRK2 and PID Kinases’ Action on Auxin Transport-Mediated Root Gravitropism.” Proceedings of the National Academy of Sciences, vol. 122, no. 39, National Academy of Sciences, 2025, p. e2512274122, doi:10.1073/pnas.2512274122.","ista":"Sheng F, Gao Y, Wang Y, Li Y, Zhang J, Zhang Z, Qin X, Zhang S, Song W, Li J, Guo Y, Friml J, Gong Z, Zhang Q, Zhang J. 2025. Antagonistic SnRK2 and PID kinases’ action on auxin transport-mediated root gravitropism. Proceedings of the National Academy of Sciences. 122(39), e2512274122.","chicago":"Sheng, F, Y Gao, Y Wang, Y Li, JA Zhang, Z Zhang, X Qin, et al. “Antagonistic SnRK2 and PID Kinases’ Action on Auxin Transport-Mediated Root Gravitropism.” Proceedings of the National Academy of Sciences. National Academy of Sciences, 2025. https://doi.org/10.1073/pnas.2512274122.","short":"F. Sheng, Y. Gao, Y. Wang, Y. Li, J. Zhang, Z. Zhang, X. Qin, S. Zhang, W. Song, J. Li, Y. Guo, J. Friml, Z. Gong, Q. Zhang, J. Zhang, Proceedings of the National Academy of Sciences 122 (2025) e2512274122.","apa":"Sheng, F., Gao, Y., Wang, Y., Li, Y., Zhang, J., Zhang, Z., … Zhang, J. (2025). Antagonistic SnRK2 and PID kinases’ action on auxin transport-mediated root gravitropism. Proceedings of the National Academy of Sciences. National Academy of Sciences. https://doi.org/10.1073/pnas.2512274122","ama":"Sheng F, Gao Y, Wang Y, et al. Antagonistic SnRK2 and PID kinases’ action on auxin transport-mediated root gravitropism. Proceedings of the National Academy of Sciences. 2025;122(39):e2512274122. doi:10.1073/pnas.2512274122"},"abstract":[{"text":"Plants have evolved sophisticated mechanisms to adapt to environmental changes, with root gravitropism playing a pivotal role in nutrient and water acquisition. Our study reveals that SnRK2 kinases (SnRK2.2 and SnRK2.3) are critical regulators of root gravitropism through their direct phosphorylation of the auxin transporter PIN2 at S259. We demonstrate that SnRK2s-mediated phosphorylation modulates both the polar localization and transport activity of PIN2. Importantly, SnRK2s function antagonistically to the AGCVIII kinase PID, which phosphorylates PIN2 at a distinct site (S258), establishing a regulatory balance essential for adaptive root growth. Structural modeling and phosphorylation assays further suggest that SnRK2s-mediated phosphorylation at S259 sterically hinders access of PID to S258, providing a mechanistic basis for their antagonistic relationship. These findings uncover a novel regulatory mechanism, by which plants fine-tune root developmental programs to adapt to environmental stimuli, highlighting the evolutionary significance of multilayered kinase-mediated regulation in plant adaptation.","lang":"eng"}],"author":[{"last_name":"Sheng","first_name":"F","full_name":"Sheng, F"},{"last_name":"Gao","first_name":"Y","full_name":"Gao, Y"},{"first_name":"Y","last_name":"Wang","full_name":"Wang, Y"},{"full_name":"Li, Y","last_name":"Li","first_name":"Y"},{"full_name":"Zhang, JA","last_name":"Zhang","first_name":"JA"},{"first_name":"Z","last_name":"Zhang","full_name":"Zhang, Z"},{"last_name":"Qin","first_name":"X","full_name":"Qin, X"},{"last_name":"Zhang","first_name":"S","full_name":"Zhang, S"},{"full_name":"Song, W","last_name":"Song","first_name":"W"},{"full_name":"Li, J","first_name":"J","last_name":"Li"},{"full_name":"Guo, Y","first_name":"Y","last_name":"Guo"},{"last_name":"Friml","orcid":"0000-0002-8302-7596","first_name":"Jiří","id":"4159519E-F248-11E8-B48F-1D18A9856A87","full_name":"Friml, Jiří"},{"full_name":"Gong, Z","first_name":"Z","last_name":"Gong"},{"full_name":"Zhang, Q","first_name":"Q","last_name":"Zhang"},{"full_name":"Zhang, J","first_name":"J","last_name":"Zhang"}],"oa_version":"Published Version","year":"2025","title":"Antagonistic SnRK2 and PID kinases' action on auxin transport-mediated root gravitropism","type":"journal_article","publication_identifier":{"eissn":["1091-6490"],"issn":["0027-8424"]},"date_updated":"2026-02-16T12:32:51Z"},{"acknowledgement":"We acknowledge useful discussions with C. Kollath, A. Green, and D. Huse. E.P., M.L., and M.S. acknowledge support by the European Research Council under the European Union’s Horizon 2020 research and innovation program (Grant Agreement No. 850899). This research was funded in whole or in part by the Austrian Science Fund (FWF) (Grant No. 10.55776/COE1). For open access purposes, the author has applied a CC BY public copyright license to any author accepted manuscript version arising from this submission. M.L. acknowledges support by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy—EXC-2111—390814868. This research was supported in part by National Science Foundation (NSF) Grant No. PHY-2309135 to the Kavli Institute for Theoretical Physics (KITP) and by the Erwin Schrödinger International Institute for Mathematics and Physics (ESI).","article_processing_charge":"Yes","_id":"20646","OA_type":"gold","isi":1,"ddc":["539"],"quality_controlled":"1","external_id":{"isi":["001616473700003"],"arxiv":["2504.12472"]},"publication":"PRX Quantum","status":"public","OA_place":"publisher","oa":1,"file":[{"date_updated":"2025-11-14T09:44:10Z","content_type":"application/pdf","access_level":"open_access","creator":"gyalniz","relation":"main_file","file_id":"20647","success":1,"date_created":"2025-11-14T09:44:10Z","file_size":2504713,"checksum":"5d6d04ac518b4118405334e1ddc7a56d","file_name":"tldp-kvkd.pdf"}],"publisher":"American Physical Society","department":[{"_id":"GradSch"},{"_id":"BjHo"},{"_id":"MaSe"}],"intvolume":" 6","DOAJ_listed":"1","publication_status":"published","day":"12","date_created":"2025-11-14T09:40:52Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"issue":"4","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"11","doi":"10.1103/tldp-kvkd","scopus_import":"1","language":[{"iso":"eng"}],"APC_amount":"3599,50 EUR","article_type":"original","volume":6,"date_published":"2025-11-12T00:00:00Z","ec_funded":1,"PlanS_conform":"1","has_accepted_license":"1","project":[{"name":"Non-Ergodic Quantum Matter: Universality, Dynamics and Control","_id":"23841C26-32DE-11EA-91FC-C7463DDC885E","grant_number":"850899","call_identifier":"H2020"},{"_id":"3AC91DDA-15DF-11EA-824D-93A3E7B544D1","name":"FWF Open Access Fund","call_identifier":"FWF"}],"file_date_updated":"2025-11-14T09:44:10Z","corr_author":"1","related_material":{"link":[{"relation":"press_release","description":"News on ISTA website","url":"https://ista.ac.at/en/news/reaching-for-the-quantum-scars/"}]},"title":"Finding periodic orbits in projected quantum many-body dynamics","year":"2025","date_updated":"2026-05-20T07:59:04Z","publication_identifier":{"eissn":["2691-3399"]},"type":"journal_article","arxiv":1,"abstract":[{"lang":"eng","text":"Describing general quantum many-body dynamics is a challenging task due to the exponential growth of the Hilbert space with system size. The time-dependent variational principle (TDVP) provides a powerful tool to tackle this task by projecting quantum evolution onto a classical dynamical system within a variational manifold. In classical systems, periodic orbits play a crucial role in understanding the structure of the phase space and the long-term behavior of the system. However, finding periodic orbits is generally difficult, and their existence and properties in generic TDVP dynamics over matrix product states have remained largely unexplored. In this work, we develop an algorithm to systematically identify and characterize periodic orbits in TDVP dynamics. Applying our method to the periodically kicked Ising model, we uncover both stable and unstable periodic orbits. We characterize the Kolmogorov-Arnold-Moser tori in the vicinity of stable periodic orbits and track the change of the periodic orbits as we modify the Hamiltonian parameters. We observe that periodic orbits exist at any value of the coupling constant of the kicked Ising model between prethermal and fully thermalizing regimes, but their relevance to quantum dynamics and imprint on quantum eigenstates diminishes as the system leaves the prethermal regime. Our results demonstrate that periodic orbits provide valuable insights into the TDVP approximation of quantum many-body evolution and establish a closer connection between quantum and classical chaos."}],"article_number":"040333","citation":{"chicago":"Petrova, Elena, Marko Ljubotina, Gökhan Yalniz, and Maksym Serbyn. “Finding Periodic Orbits in Projected Quantum Many-Body Dynamics.” PRX Quantum. American Physical Society, 2025. https://doi.org/10.1103/tldp-kvkd.","ista":"Petrova E, Ljubotina M, Yalniz G, Serbyn M. 2025. Finding periodic orbits in projected quantum many-body dynamics. PRX Quantum. 6(4), 040333.","mla":"Petrova, Elena, et al. “Finding Periodic Orbits in Projected Quantum Many-Body Dynamics.” PRX Quantum, vol. 6, no. 4, 040333, American Physical Society, 2025, doi:10.1103/tldp-kvkd.","ieee":"E. Petrova, M. Ljubotina, G. Yalniz, and M. Serbyn, “Finding periodic orbits in projected quantum many-body dynamics,” PRX Quantum, vol. 6, no. 4. American Physical Society, 2025.","short":"E. Petrova, M. Ljubotina, G. Yalniz, M. Serbyn, PRX Quantum 6 (2025).","apa":"Petrova, E., Ljubotina, M., Yalniz, G., & Serbyn, M. (2025). Finding periodic orbits in projected quantum many-body dynamics. PRX Quantum. American Physical Society. https://doi.org/10.1103/tldp-kvkd","ama":"Petrova E, Ljubotina M, Yalniz G, Serbyn M. Finding periodic orbits in projected quantum many-body dynamics. PRX Quantum. 2025;6(4). doi:10.1103/tldp-kvkd"},"oa_version":"Published Version","author":[{"id":"0ac84990-897b-11ed-a09c-f5abb56a4ede","full_name":"Petrova, Elena","last_name":"Petrova","first_name":"Elena"},{"first_name":"Marko","orcid":"0000-0003-0038-7068","last_name":"Ljubotina","full_name":"Ljubotina, Marko","id":"F75EE9BE-5C90-11EA-905D-16643DDC885E"},{"id":"66E74FA2-D8BF-11E9-8249-8DE2E5697425","full_name":"Yalniz, Gökhan","last_name":"Yalniz","first_name":"Gökhan","orcid":"0000-0002-8490-9312"},{"id":"47809E7E-F248-11E8-B48F-1D18A9856A87","full_name":"Serbyn, Maksym","last_name":"Serbyn","orcid":"0000-0002-2399-5827","first_name":"Maksym"}]},{"language":[{"iso":"eng"}],"project":[{"call_identifier":"H2020","_id":"0599E47C-7A3F-11EA-A408-12923DDC885E","grant_number":"863818","name":"Formal Methods for Stochastic Models: Algorithms and Applications"}],"corr_author":"1","date_published":"2025-10-26T00:00:00Z","volume":16145,"ec_funded":1,"doi":"10.1007/978-3-032-08707-2_19","month":"10","scopus_import":"1","abstract":[{"lang":"eng","text":"Polynomial quantified entailments with existentially and universally quantified variables arise in many problems of verification and program analysis. We present PolyQEnt which is a tool for solving polynomial quantified entailments in which variables on both sides of the implication are real valued or unbounded integers. Our tool provides a unified framework for polynomial quantified entailment problems that arise in several papers in the literature. Our experimental evaluation over a wide range of benchmarks shows the applicability of the tool as well as its benefits as opposed to simply using existing SMT solvers to solve such constraints."}],"citation":{"ama":"Chatterjee K, Goharshady AK, Goharshady E, et al. PolyQEnt: A polynomial quantified entailment solver. In: 23rd International Symposium on Automated Technology for Verification and Analysis. Vol 16145. Springer Nature; 2025:411-424. doi:10.1007/978-3-032-08707-2_19","apa":"Chatterjee, K., Goharshady, A. K., Goharshady, E., Karrabi, M., Saadat, M., Seeliger, M., & Zikelic, D. (2025). PolyQEnt: A polynomial quantified entailment solver. In 23rd International Symposium on Automated Technology for Verification and Analysis (Vol. 16145, pp. 411–424). Bengaluru, India: Springer Nature. https://doi.org/10.1007/978-3-032-08707-2_19","short":"K. Chatterjee, A.K. Goharshady, E. Goharshady, M. Karrabi, M. Saadat, M. Seeliger, D. Zikelic, in:, 23rd International Symposium on Automated Technology for Verification and Analysis, Springer Nature, 2025, pp. 411–424.","chicago":"Chatterjee, Krishnendu, Amir Kafshdar Goharshady, Ehsan Goharshady, Mehrdad Karrabi, Milad Saadat, Maximilian Seeliger, and Dorde Zikelic. “PolyQEnt: A Polynomial Quantified Entailment Solver.” In 23rd International Symposium on Automated Technology for Verification and Analysis, 16145:411–24. Springer Nature, 2025. https://doi.org/10.1007/978-3-032-08707-2_19.","ista":"Chatterjee K, Goharshady AK, Goharshady E, Karrabi M, Saadat M, Seeliger M, Zikelic D. 2025. PolyQEnt: A polynomial quantified entailment solver. 23rd International Symposium on Automated Technology for Verification and Analysis. ATVA: Automated Technology for Verification and Analysis, LNCS, vol. 16145, 411–424.","ieee":"K. Chatterjee et al., “PolyQEnt: A polynomial quantified entailment solver,” in 23rd International Symposium on Automated Technology for Verification and Analysis, Bengaluru, India, 2025, vol. 16145, pp. 411–424.","mla":"Chatterjee, Krishnendu, et al. “PolyQEnt: A Polynomial Quantified Entailment Solver.” 23rd International Symposium on Automated Technology for Verification and Analysis, vol. 16145, Springer Nature, 2025, pp. 411–24, doi:10.1007/978-3-032-08707-2_19."},"author":[{"full_name":"Chatterjee, Krishnendu","id":"2E5DCA20-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-4561-241X","first_name":"Krishnendu","last_name":"Chatterjee"},{"first_name":"Amir Kafshdar","orcid":"0000-0003-1702-6584","last_name":"Goharshady","full_name":"Goharshady, Amir Kafshdar","id":"391365CE-F248-11E8-B48F-1D18A9856A87"},{"last_name":"Kafshdar Goharshadi","orcid":"0000-0002-8595-0587","first_name":"Ehsan","id":"103b4fa0-896a-11ed-bdf8-87b697bef40d","full_name":"Kafshdar Goharshadi, Ehsan"},{"last_name":"Karrabi","orcid":"0009-0007-5253-9170","first_name":"Mehrdad","id":"67638922-f394-11eb-9cf6-f20423e08757","full_name":"Karrabi, Mehrdad"},{"full_name":"Saadat, Milad","first_name":"Milad","last_name":"Saadat"},{"first_name":"Maximilian","last_name":"Seeliger","full_name":"Seeliger, Maximilian"},{"full_name":"Zikelic, Dorde","id":"294AA7A6-F248-11E8-B48F-1D18A9856A87","first_name":"Dorde","orcid":"0000-0002-4681-1699","last_name":"Zikelic"}],"oa_version":"Preprint","conference":{"name":"ATVA: Automated Technology for Verification and Analysis","location":"Bengaluru, India","start_date":"2025-10-27","end_date":"2025-10-31"},"year":"2025","title":"PolyQEnt: A polynomial quantified entailment solver","publication_identifier":{"issn":["0302-9743"],"isbn":["9783032087065"],"eissn":["1611-3349"]},"type":"conference","arxiv":1,"date_updated":"2025-11-24T13:11:10Z","OA_place":"repository","publication":"23rd International Symposium on Automated Technology for Verification and Analysis","alternative_title":["LNCS"],"status":"public","publisher":"Springer Nature","page":"411-424","department":[{"_id":"KrCh"}],"oa":1,"OA_type":"green","_id":"20648","article_processing_charge":"No","acknowledgement":"This work was supported by the following grants: ERC CoG 863818 (ForM-SMArt), Austrian Science Fund (FWF) 10.55776/COE12, ERC StG 101222524 (SPES), the Ethereum Foundation Research Grant FY24-1793, and the Singapore Ministry of Education (MOE) Academic Research Fund (AcRF) Tier 1 grant (Project ID:22-SISSMU-100).","quality_controlled":"1","external_id":{"arxiv":["2408.03796"]},"day":"26","date_created":"2025-11-16T23:01:24Z","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2408.03796"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_status":"published","intvolume":" 16145"},{"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.","_id":"20649","OA_type":"gold","article_processing_charge":"Yes","isi":1,"ddc":["520"],"external_id":{"arxiv":["2507.05381"],"isi":["001600890100001"]},"quality_controlled":"1","publication":"The Astrophysical Journal Letters","status":"public","OA_place":"publisher","file":[{"success":1,"file_name":"2025_AstrophysicalJour_Yue.pdf","checksum":"11d35c1c52c000f8c14bc6de2e9f4b3f","date_created":"2025-11-24T13:18:34Z","file_size":39736710,"access_level":"open_access","date_updated":"2025-11-24T13:18:34Z","content_type":"application/pdf","relation":"main_file","file_id":"20680","creator":"dernst"}],"oa":1,"publisher":"IOP Publishing","department":[{"_id":"JoMa"}],"DOAJ_listed":"1","intvolume":" 993","publication_status":"published","date_created":"2025-11-16T23:01:24Z","day":"01","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"issue":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"11","doi":"10.3847/2041-8213/ae0e0e","scopus_import":"1","language":[{"iso":"eng"}],"article_type":"original","volume":993,"date_published":"2025-11-01T00:00:00Z","PlanS_conform":"1","has_accepted_license":"1","file_date_updated":"2025-11-24T13:18:34Z","title":"Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars","year":"2025","date_updated":"2026-02-16T12:45:16Z","publication_identifier":{"issn":["2041-8205"],"eissn":["2041-8213"]},"arxiv":1,"type":"journal_article","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."}],"article_number":"L12","citation":{"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.","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.","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.","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).","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","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"},"oa_version":"Published Version","author":[{"full_name":"Yue, Minghao","first_name":"Minghao","last_name":"Yue"},{"last_name":"Eilers","first_name":"Anna Christina","full_name":"Eilers, Anna Christina"},{"last_name":"Matthee","first_name":"Jorryt J","orcid":"0000-0003-2871-127X","id":"7439a258-f3c0-11ec-9501-9df22fe06720","full_name":"Matthee, Jorryt J"},{"full_name":"Naidu, Rohan P.","first_name":"Rohan P.","last_name":"Naidu"},{"first_name":"Rongmon","last_name":"Bordoloi","full_name":"Bordoloi, Rongmon"},{"first_name":"Frederick B.","last_name":"Davies","full_name":"Davies, Frederick B."},{"full_name":"Hennawi, Joseph F.","first_name":"Joseph F.","last_name":"Hennawi"},{"full_name":"Kashino, Daichi","first_name":"Daichi","last_name":"Kashino"},{"last_name":"Mackenzie","first_name":"Ruari","full_name":"Mackenzie, Ruari"},{"full_name":"Simcoe, Robert A.","last_name":"Simcoe","first_name":"Robert A."}]},{"arxiv":1,"type":"journal_article","publication_identifier":{"issn":["2470-0010"],"eissn":["2470-0029"]},"date_updated":"2025-12-01T15:29:42Z","year":"2025","title":"What determines the maximum mass of AGN-assisted black hole mergers?","author":[{"first_name":"Ling Qin","last_name":"Xue","full_name":"Xue, Ling Qin"},{"first_name":"Hiromichi","last_name":"Tagawa","full_name":"Tagawa, Hiromichi"},{"full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","orcid":"0000-0003-3633-5403","last_name":"Haiman"},{"full_name":"Bartos, Imre","last_name":"Bartos","first_name":"Imre"}],"oa_version":"Preprint","citation":{"ama":"Xue LQ, Tagawa H, Haiman Z, Bartos I. What determines the maximum mass of AGN-assisted black hole mergers? Physical Review D. 2025;112(6). doi:10.1103/5m1n-qh9v","apa":"Xue, L. Q., Tagawa, H., Haiman, Z., & Bartos, I. (2025). What determines the maximum mass of AGN-assisted black hole mergers? Physical Review D. American Physical Society. https://doi.org/10.1103/5m1n-qh9v","short":"L.Q. Xue, H. Tagawa, Z. Haiman, I. Bartos, Physical Review D 112 (2025).","ista":"Xue LQ, Tagawa H, Haiman Z, Bartos I. 2025. What determines the maximum mass of AGN-assisted black hole mergers? Physical Review D. 112(6), 063034.","chicago":"Xue, Ling Qin, Hiromichi Tagawa, Zoltán Haiman, and Imre Bartos. “What Determines the Maximum Mass of AGN-Assisted Black Hole Mergers?” Physical Review D. American Physical Society, 2025. https://doi.org/10.1103/5m1n-qh9v.","ieee":"L. Q. Xue, H. Tagawa, Z. Haiman, and I. Bartos, “What determines the maximum mass of AGN-assisted black hole mergers?,” Physical Review D, vol. 112, no. 6. American Physical Society, 2025.","mla":"Xue, Ling Qin, et al. “What Determines the Maximum Mass of AGN-Assisted Black Hole Mergers?” Physical Review D, vol. 112, no. 6, 063034, American Physical Society, 2025, doi:10.1103/5m1n-qh9v."},"article_number":"063034","abstract":[{"lang":"eng","text":"The origin of merging binary black holes detected through gravitational waves remains a fundamental question in astrophysics. While stellar evolution imposes an upper mass limit of ∼50𝑀⊙ for black holes, some observed mergers—most notably GW190521—involve significantly more massive components, suggesting alternative formation channels. Here we investigate the maximum masses attainable by black hole mergers within active galactic nucleus (AGN) disks. Using a comprehensive semianalytic model incorporating 27 binary and environmental parameters, we explore the role of AGN disk conditions in shaping the upper end of the black hole mass spectrum. We find that an AGN disk lifetime is the dominant factor, with high-mass mergers (≳200𝑀⊙) only possible if disks persist for ≳40 Myr. The joint electromagnetic observation of an AGN-assisted merger could therefore lead to a direct measurement of the age of an AGN disk."}],"scopus_import":"1","month":"09","doi":"10.1103/5m1n-qh9v","volume":112,"date_published":"2025-09-18T00:00:00Z","article_type":"original","language":[{"iso":"eng"}],"publication_status":"published","intvolume":" 112","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2504.19570"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","issue":"6","date_created":"2025-11-16T23:01:24Z","day":"18","external_id":{"arxiv":["2504.19570"],"isi":["001583255800010"]},"quality_controlled":"1","isi":1,"article_processing_charge":"No","_id":"20651","OA_type":"green","acknowledgement":"The authors are thankful for Yang Yang and Yue Yu for valuable discussions and assistance with the programming process. H. T. was supported by the National Key R&D Program of China (Grant No. 2021YFC2203002). Z. H. is grateful for support from NASA under Grants No. 80NSSC22K0822 and No. 80NSSC24K0440. I. B. acknowledges support from the National Science Foundation under Grant No. PHY-2309024.","department":[{"_id":"ZoHa"}],"publisher":"American Physical Society","oa":1,"OA_place":"repository","status":"public","publication":"Physical Review D"},{"_id":"20658","OA_type":"green","article_processing_charge":"No","quality_controlled":"1","external_id":{"arxiv":["2504.14743"]},"OA_place":"repository","publication":"4th International Joint Conference on Discrete Geometry and Mathematical Morphology","alternative_title":["LNCS"],"status":"public","publisher":"Springer Nature","page":"133-147","department":[{"_id":"HeEd"}],"oa":1,"publication_status":"published","intvolume":" 16296","date_created":"2025-11-23T23:01:37Z","day":"01","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2504.14743"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","doi":"10.1007/978-3-032-09544-2_10","month":"11","scopus_import":"1","language":[{"iso":"eng"}],"date_published":"2025-11-01T00:00:00Z","volume":16296,"year":"2025","title":"The mid-sphere cousin of the medial axis transform","publication_identifier":{"isbn":["9783032095435"],"eissn":["1611-3349"],"issn":["0302-9743"]},"type":"conference","arxiv":1,"date_updated":"2025-11-24T10:05:11Z","abstract":[{"text":"The medial axis of a smoothly embedded surface in R^3 consists of all points for which the Euclidean distance function on the surface has at least two global minima. We generalize this notion to the mid-sphere axis, which consists of all points for which the Euclidean distance function has two interchanging saddles that swap their partners in the pairing by persistent homology. It offers a discrete-algebraic multi-scale approach to computing ridge-like structures on the surface. As a proof of concept, an algorithm that computes stair-case approximations of the mid-sphere axis is provided.","lang":"eng"}],"citation":{"apa":"Edelsbrunner, H., Stephenson, E. R., & Thoresen, M. H. (2025). The mid-sphere cousin of the medial axis transform. In 4th International Joint Conference on Discrete Geometry and Mathematical Morphology (Vol. 16296, pp. 133–147). Groningen, The Netherlands: Springer Nature. https://doi.org/10.1007/978-3-032-09544-2_10","ama":"Edelsbrunner H, Stephenson ER, Thoresen MH. The mid-sphere cousin of the medial axis transform. In: 4th International Joint Conference on Discrete Geometry and Mathematical Morphology. Vol 16296. Springer Nature; 2025:133-147. doi:10.1007/978-3-032-09544-2_10","ista":"Edelsbrunner H, Stephenson ER, Thoresen MH. 2025. The mid-sphere cousin of the medial axis transform. 4th International Joint Conference on Discrete Geometry and Mathematical Morphology. DGMM: Discrete Geometry and Mathematical Morphology, LNCS, vol. 16296, 133–147.","chicago":"Edelsbrunner, Herbert, Elizabeth R Stephenson, and Martin H Thoresen. “The Mid-Sphere Cousin of the Medial Axis Transform.” In 4th International Joint Conference on Discrete Geometry and Mathematical Morphology, 16296:133–47. Springer Nature, 2025. https://doi.org/10.1007/978-3-032-09544-2_10.","ieee":"H. Edelsbrunner, E. R. Stephenson, and M. H. Thoresen, “The mid-sphere cousin of the medial axis transform,” in 4th International Joint Conference on Discrete Geometry and Mathematical Morphology, Groningen, The Netherlands, 2025, vol. 16296, pp. 133–147.","mla":"Edelsbrunner, Herbert, et al. “The Mid-Sphere Cousin of the Medial Axis Transform.” 4th International Joint Conference on Discrete Geometry and Mathematical Morphology, vol. 16296, Springer Nature, 2025, pp. 133–47, doi:10.1007/978-3-032-09544-2_10.","short":"H. Edelsbrunner, E.R. Stephenson, M.H. Thoresen, in:, 4th International Joint Conference on Discrete Geometry and Mathematical Morphology, Springer Nature, 2025, pp. 133–147."},"author":[{"last_name":"Edelsbrunner","orcid":"0000-0002-9823-6833","first_name":"Herbert","id":"3FB178DA-F248-11E8-B48F-1D18A9856A87","full_name":"Edelsbrunner, Herbert"},{"id":"2D04F932-F248-11E8-B48F-1D18A9856A87","full_name":"Stephenson, Elizabeth R","last_name":"Stephenson","first_name":"Elizabeth R","orcid":"0000-0002-6862-208X"},{"first_name":"Martin H","last_name":"Thoresen","full_name":"Thoresen, Martin H","id":"47CB1472-F248-11E8-B48F-1D18A9856A87"}],"oa_version":"Preprint","conference":{"name":"DGMM: Discrete Geometry and Mathematical Morphology","end_date":"2025-11-06","start_date":"2025-11-03","location":"Groningen, The Netherlands"}},{"acknowledgement":"We thank Ms. Diane Latawiec for the English revision of the manuscript. Funding sources were the Spanish Ministerio de Economía y Competitividad, and Junta de Comunidades de CastillaLa Mancha (Spain). Grants PID2021-125875OB-I00 funded by MCIN/AEI/ 10.13039/501100011033 and “ERDF A way of making Europe” to RL. This work was also supported by Castilla-La Mancha Regional Government and the European Regional Development Fund (SBPLY/21/180501/000064) and the Universidad de Castilla-La Mancha (2023-GRIN-34187) to RL.","OA_type":"gold","_id":"20659","article_processing_charge":"Yes","ddc":["570"],"external_id":{"pmid":["40704638"]},"quality_controlled":"1","publication":"Histology and Histopathology","status":"public","OA_place":"publisher","file":[{"creator":"dernst","relation":"main_file","file_id":"20677","access_level":"open_access","date_updated":"2025-11-24T10:23:39Z","content_type":"application/pdf","file_name":"2025_HistologyHistopathology_Aguado.pdf","date_created":"2025-11-24T10:23:39Z","file_size":18093266,"checksum":"779d67434400c0f94af42c35ba21c672","success":1}],"oa":1,"publisher":"Sercrisma International","department":[{"_id":"RySh"}],"page":"1967-1984","intvolume":" 40","publication_status":"published","pmid":1,"date_created":"2025-11-23T23:01:37Z","day":"01","issue":"12","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"12","doi":"10.14670/HH-18-970","scopus_import":"1","language":[{"iso":"eng"}],"article_type":"original","volume":40,"date_published":"2025-12-01T00:00:00Z","PlanS_conform":"1","has_accepted_license":"1","file_date_updated":"2025-11-24T10:23:39Z","title":"Developmental regulation of GABAB receptors and downstream molecules in the mouse brain","year":"2025","date_updated":"2025-11-24T10:24:35Z","publication_identifier":{"eissn":["1699-5848"]},"type":"journal_article","abstract":[{"text":"Metabotropic GABA (GABAB) receptors have modulatory functions on neuronal excitability and\r\nneurotransmitter release. To fulfil these functions, GABAB receptors form macromolecular signaling complexes with G proteins, effectors, and other associated proteins. Here we investigated the postnatal development of GABAB receptors (GABAB1 and GABAB2 subunits) in mouse brain, focusing on potential similarities in the spatial and temporal expression pattern\r\nof their associated proteins CaV2.1, Gαo, Gβ5, and RGS7, using histoblots, immunofluorescence, and immunoelectron microscopic techniques. At all ages analyzed, histoblot showed that the six proteins were widely expressed in the brain, with mostly an\r\noverlapping pattern throughout postnatal development. In the hippocampus, immunoelectron microscopy and quantitative analysis of immunoparticles for GABAB1, GABAB2, Gαo, Gβ5, and RGS7 revealed their progressive enrichment around excitatory synapses on dendritic spines of CA1 pyramidal cells toward P15. At presynaptic sites, GABAB receptors colocalize with\r\nCaV2.1, Gαo, Gβ5, and RGS7 in the active zone and extrasynaptic membranes of axon terminals, establishing synapses on dendritic spines of CA1 pyramidal cells. In the cerebellum, double immunofluorescence at P7 and P10 revealed the colocalization of GABAB1 and CaV2.1\r\nin the whole dendritic tree of developing Purkinje cells. Immunoelectron microscopy at P15 showed that GABAB1, GABAB2, CaV2.1, Gαo, Gβ5, and RGS7 are distributed along the dendritic surface of Purkinje cells, enriched close to excitatory synapses in spines.\r\nAltogether, these data suggest that macromolecular complexes composed of GABAB1 /GABAB2/CaV2.1/ Gαo/Gβ5/RGS7 are pre-assembled during key stages of postnatal development in hippocampal and cerebellar neurons.","lang":"eng"}],"citation":{"ieee":"C. Aguado et al., “Developmental regulation of GABAB receptors and downstream molecules in the mouse brain,” Histology and Histopathology, vol. 40, no. 12. Sercrisma International, pp. 1967–1984, 2025.","mla":"Aguado, Carolina, et al. “Developmental Regulation of GABAB Receptors and Downstream Molecules in the Mouse Brain.” Histology and Histopathology, vol. 40, no. 12, Sercrisma International, 2025, pp. 1967–84, doi:10.14670/HH-18-970.","ista":"Aguado C, Alfaro-Ruiz R, Martínez-Poyato ML, Moreno-Martínez AE, García-Madrona S, Roldán-Sastre A, Alonso-Gómez P, Fernández M, Puertas-Avendaño R, Shigemoto R, Martemyanov KA, Luján R. 2025. Developmental regulation of GABAB receptors and downstream molecules in the mouse brain. Histology and Histopathology. 40(12), 1967–1984.","chicago":"Aguado, Carolina, Rocío Alfaro-Ruiz, María Llanos Martínez-Poyato, Ana Esther Moreno-Martínez, Sebastián García-Madrona, Alberto Roldán-Sastre, Pablo Alonso-Gómez, et al. “Developmental Regulation of GABAB Receptors and Downstream Molecules in the Mouse Brain.” Histology and Histopathology. Sercrisma International, 2025. https://doi.org/10.14670/HH-18-970.","short":"C. Aguado, R. Alfaro-Ruiz, M.L. Martínez-Poyato, A.E. Moreno-Martínez, S. García-Madrona, A. Roldán-Sastre, P. Alonso-Gómez, M. Fernández, R. Puertas-Avendaño, R. Shigemoto, K.A. Martemyanov, R. Luján, Histology and Histopathology 40 (2025) 1967–1984.","apa":"Aguado, C., Alfaro-Ruiz, R., Martínez-Poyato, M. L., Moreno-Martínez, A. E., García-Madrona, S., Roldán-Sastre, A., … Luján, R. (2025). Developmental regulation of GABAB receptors and downstream molecules in the mouse brain. Histology and Histopathology. Sercrisma International. https://doi.org/10.14670/HH-18-970","ama":"Aguado C, Alfaro-Ruiz R, Martínez-Poyato ML, et al. Developmental regulation of GABAB receptors and downstream molecules in the mouse brain. Histology and Histopathology. 2025;40(12):1967-1984. doi:10.14670/HH-18-970"},"oa_version":"Published Version","author":[{"full_name":"Aguado, Carolina","last_name":"Aguado","first_name":"Carolina"},{"full_name":"Alfaro-Ruiz, Rocío","first_name":"Rocío","last_name":"Alfaro-Ruiz"},{"first_name":"María Llanos","last_name":"Martínez-Poyato","full_name":"Martínez-Poyato, María Llanos"},{"full_name":"Moreno-Martínez, Ana Esther","last_name":"Moreno-Martínez","first_name":"Ana Esther"},{"first_name":"Sebastián","last_name":"García-Madrona","full_name":"García-Madrona, Sebastián"},{"last_name":"Roldán-Sastre","first_name":"Alberto","full_name":"Roldán-Sastre, Alberto"},{"last_name":"Alonso-Gómez","first_name":"Pablo","full_name":"Alonso-Gómez, Pablo"},{"full_name":"Fernández, Miriam","last_name":"Fernández","first_name":"Miriam"},{"full_name":"Puertas-Avendaño, Ricardo","last_name":"Puertas-Avendaño","first_name":"Ricardo"},{"id":"499F3ABC-F248-11E8-B48F-1D18A9856A87","full_name":"Shigemoto, Ryuichi","last_name":"Shigemoto","first_name":"Ryuichi","orcid":"0000-0001-8761-9444"},{"first_name":"Kirill A.","last_name":"Martemyanov","full_name":"Martemyanov, Kirill A."},{"first_name":"Rafael","last_name":"Luján","full_name":"Luján, Rafael"}]},{"title":"The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization","year":"2025","date_updated":"2025-12-01T15:25:11Z","type":"journal_article","publication_identifier":{"issn":["0035-8711"],"eissn":["1365-2966"]},"citation":{"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.","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.","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.","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.","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","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"},"abstract":[{"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.","lang":"eng"}],"oa_version":"Published Version","author":[{"full_name":"Stephenson, H. M.O.","first_name":"H. M.O.","last_name":"Stephenson"},{"last_name":"Stott","first_name":"J. P.","full_name":"Stott, J. P."},{"first_name":"C. A.","last_name":"Pirie","full_name":"Pirie, C. A."},{"full_name":"Duncan, K. J.","last_name":"Duncan","first_name":"K. J."},{"first_name":"D. J.","last_name":"Mcleod","full_name":"Mcleod, D. J."},{"full_name":"Best, P. N.","last_name":"Best","first_name":"P. N."},{"full_name":"Brinch, M.","first_name":"M.","last_name":"Brinch"},{"last_name":"Clausen","first_name":"M.","full_name":"Clausen, M."},{"last_name":"Cochrane","first_name":"R. K.","full_name":"Cochrane, R. K."},{"full_name":"Dunlop, J. S.","first_name":"J. S.","last_name":"Dunlop"},{"last_name":"Flury","first_name":"S. R.","full_name":"Flury, S. R."},{"full_name":"Geach, J. E.","first_name":"J. E.","last_name":"Geach"},{"last_name":"Hale","first_name":"C. L.","full_name":"Hale, C. L."},{"first_name":"E.","last_name":"Ibar","full_name":"Ibar, E."},{"full_name":"Li, Zefeng","last_name":"Li","first_name":"Zefeng"},{"full_name":"Matthee, Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X","first_name":"Jorryt J","last_name":"Matthee"},{"full_name":"Mclure, R. J.","first_name":"R. J.","last_name":"Mclure"},{"full_name":"Ossa-Fuentes, L.","first_name":"L.","last_name":"Ossa-Fuentes"},{"first_name":"A. L.","last_name":"Patrick","full_name":"Patrick, A. L."},{"first_name":"D.","last_name":"Sobral","full_name":"Sobral, D."},{"full_name":"Swinbank, A. M.","first_name":"A. M.","last_name":"Swinbank"}],"month":"12","doi":"10.1093/mnras/staf1725","scopus_import":"1","language":[{"iso":"eng"}],"article_type":"original","PlanS_conform":"1","volume":544,"date_published":"2025-12-01T00:00:00Z","has_accepted_license":"1","file_date_updated":"2025-11-24T10:35:15Z","DOAJ_listed":"1","intvolume":" 544","publication_status":"published","date_created":"2025-11-23T23:01:37Z","day":"01","issue":"2","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","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.","isi":1,"_id":"20660","OA_type":"gold","article_processing_charge":"Yes","external_id":{"isi":["001611415800001"]},"quality_controlled":"1","ddc":["520"],"status":"public","publication":"Monthly Notices of the Royal Astronomical Society","OA_place":"publisher","file":[{"success":1,"file_size":3625308,"date_created":"2025-11-24T10:35:15Z","checksum":"ddb3f429d2246bbf536efb4b0e52f3a8","file_name":"2025_MonthlyNoticesRAS_Stephenson.pdf","date_updated":"2025-11-24T10:35:15Z","content_type":"application/pdf","access_level":"open_access","creator":"dernst","file_id":"20678","relation":"main_file"}],"oa":1,"department":[{"_id":"JoMa"}],"page":"1412-1431","publisher":"Oxford University Press"},{"abstract":[{"text":"We analyse James Webb Space Telescope (JWST) Near Infrared Imager and Slitless Spectrograph (NIRISS) and Near Infrared Spectrograph (NIRSpec) spectroscopic observations in the Abell 2744 galaxy cluster field. From approximately 120 candidates, we identify 12 objects with at least two prominent emission lines among [O II] λ3727, H β λ4861, [O III] λ4959, [O III] λ5007, and H α λ6563 that are spectroscopically confirmed by both instruments. Our key findings reveal systematic differences between the two spectrographs based on source morphology and shutter aperture placement. Compact objects show comparable or higher\r\nintegrated flux in NIRSpec relative to NIRISS (within 1σ uncertainties), while extended sources consistently display higher flux in NIRISS measurements. This pattern reflects NIRSpec’s optimal coverage for compact objects while potentially undersampling extended sources. Quantitative analysis demonstrates that NIRSpec recovers at least 63 per cent of NIRISS-measured flux when the slit covers >15 per cent of the source or when Re < 1 kpc. For lower coverage or larger effective radii, the recovered flux varies from 24 per cent to 63 per cent. When studying the H α λ6563/[O III] λ5007 emission line ratio, we observe that\r\nmeasurements from these different spectrographs can vary by up to ∼0.3 dex, with significant implications for metallicity and star formation rate characterizations for individual galaxies. These results highlight the importance of considering instrumental effects when combining multi-instrument spectroscopic data and demonstrate that source morphology critically influences flux\r\nrecovery between slit-based and slitless spectroscopic modes in JWST observations.","lang":"eng"}],"citation":{"mla":"Dalmasso, Nicolò, et al. “Quantifying Spectroscopic Flux Variations between JWST NIRISS and NIRSpec: Slit Losses in Emission Line Measurements of z ∼ 1-3 Galaxies.” Monthly Notices of the Royal Astronomical Society, vol. 544, no. 2, Oxford University Press, 2025, pp. 1915–25, doi:10.1093/mnras/staf1837.","ieee":"N. Dalmasso et al., “Quantifying spectroscopic flux variations between JWST NIRISS and NIRSpec: Slit losses in emission line measurements of z ∼ 1-3 galaxies,” Monthly Notices of the Royal Astronomical Society, vol. 544, no. 2. Oxford University Press, pp. 1915–1925, 2025.","ista":"Dalmasso N, Watson PJ, Treu T, Trenti M, Vulcani B, Nanayakkara T, Bradač M, Jones T, Boyett K, Wang X, Mascia S, Pentericci L. 2025. Quantifying spectroscopic flux variations between JWST NIRISS and NIRSpec: Slit losses in emission line measurements of z ∼ 1-3 galaxies. Monthly Notices of the Royal Astronomical Society. 544(2), 1915–1925.","chicago":"Dalmasso, Nicolò, Peter J. Watson, Tommaso Treu, Michele Trenti, Benedetta Vulcani, Themiya Nanayakkara, Maruša Bradač, et al. “Quantifying Spectroscopic Flux Variations between JWST NIRISS and NIRSpec: Slit Losses in Emission Line Measurements of z ∼ 1-3 Galaxies.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2025. https://doi.org/10.1093/mnras/staf1837.","short":"N. Dalmasso, P.J. Watson, T. Treu, M. Trenti, B. Vulcani, T. Nanayakkara, M. Bradač, T. Jones, K. Boyett, X. Wang, S. Mascia, L. Pentericci, Monthly Notices of the Royal Astronomical Society 544 (2025) 1915–1925.","apa":"Dalmasso, N., Watson, P. J., Treu, T., Trenti, M., Vulcani, B., Nanayakkara, T., … Pentericci, L. (2025). Quantifying spectroscopic flux variations between JWST NIRISS and NIRSpec: Slit losses in emission line measurements of z ∼ 1-3 galaxies. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/staf1837","ama":"Dalmasso N, Watson PJ, Treu T, et al. Quantifying spectroscopic flux variations between JWST NIRISS and NIRSpec: Slit losses in emission line measurements of z ∼ 1-3 galaxies. Monthly Notices of the Royal Astronomical Society. 2025;544(2):1915-1925. doi:10.1093/mnras/staf1837"},"oa_version":"Published Version","author":[{"full_name":"Dalmasso, Nicolò","first_name":"Nicolò","last_name":"Dalmasso"},{"last_name":"Watson","first_name":"Peter J.","full_name":"Watson, Peter J."},{"last_name":"Treu","first_name":"Tommaso","full_name":"Treu, Tommaso"},{"last_name":"Trenti","first_name":"Michele","full_name":"Trenti, Michele"},{"full_name":"Vulcani, Benedetta","last_name":"Vulcani","first_name":"Benedetta"},{"full_name":"Nanayakkara, Themiya","first_name":"Themiya","last_name":"Nanayakkara"},{"full_name":"Bradač, Maruša","first_name":"Maruša","last_name":"Bradač"},{"first_name":"Tucker","last_name":"Jones","full_name":"Jones, Tucker"},{"first_name":"Kristan","last_name":"Boyett","full_name":"Boyett, Kristan"},{"first_name":"Xin","last_name":"Wang","full_name":"Wang, Xin"},{"last_name":"Mascia","first_name":"Sara","id":"edaf889c-c7cd-11ef-ab1b-bb28c431bd29","full_name":"Mascia, Sara"},{"full_name":"Pentericci, Laura","last_name":"Pentericci","first_name":"Laura"}],"title":"Quantifying spectroscopic flux variations between JWST NIRISS and NIRSpec: Slit losses in emission line measurements of z ∼ 1-3 galaxies","year":"2025","date_updated":"2025-12-01T15:23:21Z","publication_identifier":{"issn":["0035-8711"],"eissn":["1365-2966"]},"arxiv":1,"type":"journal_article","language":[{"iso":"eng"}],"article_type":"original","date_published":"2025-12-01T00:00:00Z","volume":544,"PlanS_conform":"1","has_accepted_license":"1","file_date_updated":"2025-11-24T09:02:04Z","doi":"10.1093/mnras/staf1837","month":"12","scopus_import":"1","day":"01","date_created":"2025-11-23T23:01:38Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"issue":"2","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","DOAJ_listed":"1","intvolume":" 544","publication_status":"published","publication":"Monthly Notices of the Royal Astronomical Society","status":"public","OA_place":"publisher","file":[{"relation":"main_file","file_id":"20674","creator":"dernst","access_level":"open_access","content_type":"application/pdf","date_updated":"2025-11-24T09:02:04Z","file_name":"2025_MonthlyNoticesRAS_Dalmasso.pdf","checksum":"2caff0a3b81fed114408377323298b43","date_created":"2025-11-24T09:02:04Z","file_size":1952887,"success":1}],"oa":1,"publisher":"Oxford University Press","department":[{"_id":"JoMa"}],"page":"1915-1925","acknowledgement":"This research was supported in part by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. This research was supported in part by The Dr Albert Shimmins Fund through the Albert Shimmins Postgraduate Writing Up Award (University of Melbourne). 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 programmes JWST-ERS-1324, JWST-GO-2561, and JWST-DDT-2756. BV and PW acknowledge support from the INAF Large Grant 2022 ‘Extragalactic Surveys with JWST’ (PI Pentericci), the INAF Mini\r\nGrant ‘1.05.24.07.01 RSN1: Spatially-Resolved Near-IR Emission of Intermediate-Redshift Jellyfish Galaxies’ (PI Watson), and are supported by the European Union – NextGenerationEU RFF M4C2 1.1 PRIN 2022 project 2022ZSL4BL INSIGHT. MB acknowledges support from the ERC Advanced Grant FIRSTLIGHT and Slovenian national research agency ARIS through grants N1-0238 and P1-0188. ","_id":"20661","OA_type":"gold","article_processing_charge":"Yes","isi":1,"ddc":["520"],"quality_controlled":"1","external_id":{"isi":["001615620500001"],"arxiv":["2510.27036"]}},{"scopus_import":"1","doi":"10.1073/pnas.2506400122","month":"11","file_date_updated":"2025-11-24T09:48:44Z","has_accepted_license":"1","PlanS_conform":"1","date_published":"2025-11-18T00:00:00Z","volume":122,"article_type":"original","language":[{"iso":"eng"}],"type":"journal_article","publication_identifier":{"eissn":["1091-6490"]},"date_updated":"2026-02-16T12:31:31Z","year":"2025","title":"Angle dependence as a unifying feature of root graviresponse modules","author":[{"first_name":"Suruchi","last_name":"Roychoudhry","full_name":"Roychoudhry, Suruchi"},{"full_name":"Sageman-Furnas, Katelyn","last_name":"Sageman-Furnas","first_name":"Katelyn"},{"full_name":"Taylor, Harry J.","first_name":"Harry J.","last_name":"Taylor"},{"first_name":"Iftekhar","last_name":"Showpnil","full_name":"Showpnil, Iftekhar"},{"full_name":"Wolverton, Chris","last_name":"Wolverton","first_name":"Chris"},{"id":"4159519E-F248-11E8-B48F-1D18A9856A87","full_name":"Friml, Jiří","last_name":"Friml","first_name":"Jiří","orcid":"0000-0002-8302-7596"},{"first_name":"Marta Del","last_name":"Bianco","full_name":"Bianco, Marta Del"},{"full_name":"Kepinski, Stefan","last_name":"Kepinski","first_name":"Stefan"}],"oa_version":"Published Version","citation":{"ieee":"S. Roychoudhry et al., “Angle dependence as a unifying feature of root graviresponse modules,” Proceedings of the National Academy of Sciences, vol. 122, no. 46. National Academy of Sciences, p. e2506400122, 2025.","mla":"Roychoudhry, Suruchi, et al. “Angle Dependence as a Unifying Feature of Root Graviresponse Modules.” Proceedings of the National Academy of Sciences, vol. 122, no. 46, National Academy of Sciences, 2025, p. e2506400122, doi:10.1073/pnas.2506400122.","ista":"Roychoudhry S, Sageman-Furnas K, Taylor HJ, Showpnil I, Wolverton C, Friml J, Bianco MD, Kepinski S. 2025. Angle dependence as a unifying feature of root graviresponse modules. Proceedings of the National Academy of Sciences. 122(46), e2506400122.","chicago":"Roychoudhry, Suruchi, Katelyn Sageman-Furnas, Harry J. Taylor, Iftekhar Showpnil, Chris Wolverton, Jiří Friml, Marta Del Bianco, and Stefan Kepinski. “Angle Dependence as a Unifying Feature of Root Graviresponse Modules.” Proceedings of the National Academy of Sciences. National Academy of Sciences, 2025. https://doi.org/10.1073/pnas.2506400122.","short":"S. Roychoudhry, K. Sageman-Furnas, H.J. Taylor, I. Showpnil, C. Wolverton, J. Friml, M.D. Bianco, S. Kepinski, Proceedings of the National Academy of Sciences 122 (2025) e2506400122.","apa":"Roychoudhry, S., Sageman-Furnas, K., Taylor, H. J., Showpnil, I., Wolverton, C., Friml, J., … Kepinski, S. (2025). Angle dependence as a unifying feature of root graviresponse modules. Proceedings of the National Academy of Sciences. National Academy of Sciences. https://doi.org/10.1073/pnas.2506400122","ama":"Roychoudhry S, Sageman-Furnas K, Taylor HJ, et al. Angle dependence as a unifying feature of root graviresponse modules. Proceedings of the National Academy of Sciences. 2025;122(46):e2506400122. doi:10.1073/pnas.2506400122"},"abstract":[{"text":"Gravitropism, the patterning of postembryonic growth in relation to the gravity vector, allows plants to optimize the use of limited and nonhomogenous resources in their immediate environment. Since the current model of root gravitropism has not been able to integrate all aspects of the response (perception, response, and behavior), research on gravitropism has been dominated by different theories attempting to conceptualize each aspect individually. In this work, we sought to reevaluate all the main components of the root graviresponse through the lens of angle dependence. We show angle dependence in Cholodny–Went-based auxin asymmetry and growth response, which we tracked back to angle-dependent variation in PIN asymmetry and statolith sedimentation in the columella. Thanks to this approach, we were able to suggest distinct roles for PINs and columella cell tiers, and a potential function for auxin vertical flux through the columella. Our findings provide a unifying framework to further explore the mechanisms that regulate angle-dependent gravitropic response, with major implications of time-dependent features of root graviresponse.","lang":"eng"}],"external_id":{"pmid":["41218119"]},"quality_controlled":"1","ddc":["580"],"_id":"20663","OA_type":"hybrid","article_processing_charge":"Yes (in subscription journal)","acknowledgement":"This study was funded by the BBSRC (grant no. BB/N010124/1) and Leverhulme Foundation (grant no. RPG-2018-137) to M.D.B. and S.K., a Fully Funded International Research Scholarship awarded to K.S.-F., and by NASA (grant no. 80NSSC21K0585) to C.W.","page":"e2506400122","department":[{"_id":"JiFr"}],"publisher":"National Academy of Sciences","oa":1,"file":[{"checksum":"5e1c37dddc5db8fbd0128db4a54c4f6b","file_size":1394055,"date_created":"2025-11-24T09:48:44Z","file_name":"2025_PNAS_Roychoudhry.pdf","success":1,"relation":"main_file","file_id":"20676","creator":"dernst","date_updated":"2025-11-24T09:48:44Z","content_type":"application/pdf","access_level":"open_access"}],"OA_place":"publisher","status":"public","publication":"Proceedings of the National Academy of Sciences","publication_status":"published","intvolume":" 122","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"issue":"46","date_created":"2025-11-23T23:01:38Z","day":"18","pmid":1},{"date_updated":"2026-06-10T08:45:11Z","publication_identifier":{"eissn":["2699-0016"]},"type":"journal_article","related_material":{"link":[{"url":"https://ista.ac.at/en/news/carbon-footprint-of-conference-travel/","relation":"research_data","description":"News on ISTA website"}],"record":[{"relation":"research_data","status":"public","id":"20242"}]},"title":"Quantifying the carbon footprint of conference travel: The case of NMR meetings","year":"2025","oa_version":"Published Version","author":[{"last_name":"Kapoor","first_name":"Lucky","orcid":"0000-0001-8319-2148","id":"84b9700b-15b2-11ec-abd3-831089e67615","full_name":"Kapoor, Lucky"},{"first_name":"Natalia","last_name":"Ruzickova","full_name":"Ruzickova, Natalia","id":"D2761128-D73D-11E9-A1BF-BA0DE6697425"},{"full_name":"Zivadinovic, Predrag","id":"68AA0E5A-AFDA-11E9-9994-141DE6697425","first_name":"Predrag","last_name":"Zivadinovic"},{"last_name":"Leitner","first_name":"Valentin","id":"4c665ce3-0016-11ec-bea0-e44de7a4fa3d","full_name":"Leitner, Valentin"},{"id":"44A03D04-AEA4-11E9-B225-EA2DE6697425","full_name":"Sisak, Maria A","last_name":"Sisak","first_name":"Maria A"},{"full_name":"Mweka, Cecelia N","id":"2a69ab4b-896a-11ed-bdf8-cb8641cf2b21","first_name":"Cecelia N","last_name":"Mweka"},{"last_name":"Dobbelaere","first_name":"Jeroen A","id":"c15a5412-de82-11ed-b809-8dc1aa996e40","full_name":"Dobbelaere, Jeroen A"},{"id":"38DB5788-F248-11E8-B48F-1D18A9856A87","full_name":"Katsaros, Georgios","last_name":"Katsaros","first_name":"Georgios","orcid":"0000-0001-8342-202X"},{"first_name":"Paul","orcid":"0000-0002-9350-7606","last_name":"Schanda","full_name":"Schanda, Paul","id":"7B541462-FAF6-11E9-A490-E8DFE5697425"}],"abstract":[{"text":"Conference travel contributes to the climate footprint of academic research. Here, we provide a quantitative estimate of the carbon emissions associated with conference attendance by analyzing travel data from participants of 10 international conferences in the field of magnetic resonance, namely EUROMAR, ENC and ICMRBS. We find that attending a EUROMAR conference produces, on average, more than 1 t CO2 eq.. For the analyzed conferences outside Europe, the corresponding value is about 2–3 times higher, on average, with intercontinental trips amounting to up to 5 t. We compare these conference-related emissions to other activities associated with research and show that conference travel is a substantial portion of the total climate footprint of a researcher in magnetic resonance. We explore several strategies to reduce these emissions, including the impact of selecting conference venues more strategically and the possibility of decentralized conferences. Through a detailed comparison of train versus air travel – accounting for both direct and infrastructure-related emissions – we demonstrate that train travel offers considerable carbon savings. These data may provide a basis for strategic choices of future conferences in the field and for individuals deciding on their conference attendance.","lang":"eng"}],"citation":{"apa":"Kapoor, L., Ruzickova, N., Zivadinovic, P., Leitner, V., Sisak, M. A., Mweka, C. N., … Schanda, P. (2025). Quantifying the carbon footprint of conference travel: The case of NMR meetings. Magnetic Resonance. Copernicus Publications. https://doi.org/10.5194/mr-6-243-2025","ama":"Kapoor L, Ruzickova N, Zivadinovic P, et al. Quantifying the carbon footprint of conference travel: The case of NMR meetings. Magnetic Resonance. 2025;6(2):243-256. doi:10.5194/mr-6-243-2025","ista":"Kapoor L, Ruzickova N, Zivadinovic P, Leitner V, Sisak MA, Mweka CN, Dobbelaere JA, Katsaros G, Schanda P. 2025. Quantifying the carbon footprint of conference travel: The case of NMR meetings. Magnetic Resonance. 6(2), 243–256.","chicago":"Kapoor, Lucky, Natalia Ruzickova, Predrag Zivadinovic, Valentin Leitner, Maria A Sisak, Cecelia N Mweka, Jeroen A Dobbelaere, Georgios Katsaros, and Paul Schanda. “Quantifying the Carbon Footprint of Conference Travel: The Case of NMR Meetings.” Magnetic Resonance. Copernicus Publications, 2025. https://doi.org/10.5194/mr-6-243-2025.","ieee":"L. Kapoor et al., “Quantifying the carbon footprint of conference travel: The case of NMR meetings,” Magnetic Resonance, vol. 6, no. 2. Copernicus Publications, pp. 243–256, 2025.","mla":"Kapoor, Lucky, et al. “Quantifying the Carbon Footprint of Conference Travel: The Case of NMR Meetings.” Magnetic Resonance, vol. 6, no. 2, Copernicus Publications, 2025, pp. 243–56, doi:10.5194/mr-6-243-2025.","short":"L. Kapoor, N. Ruzickova, P. Zivadinovic, V. Leitner, M.A. Sisak, C.N. Mweka, J.A. Dobbelaere, G. Katsaros, P. Schanda, Magnetic Resonance 6 (2025) 243–256."},"scopus_import":"1","month":"11","doi":"10.5194/mr-6-243-2025","volume":6,"date_published":"2025-11-10T00:00:00Z","PlanS_conform":"1","file_date_updated":"2025-11-24T08:25:19Z","project":[{"name":"IST Austria Open Access Fund","_id":"B67AFEDC-15C9-11EA-A837-991A96BB2854"}],"has_accepted_license":"1","corr_author":"1","language":[{"iso":"eng"}],"APC_amount":"1260 EUR","article_type":"original","intvolume":" 6","DOAJ_listed":"1","publication_status":"published","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","day":"10","date_created":"2025-11-23T23:01:39Z","issue":"2","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"ddc":["000"],"quality_controlled":"1","acknowledgement":"First and foremost, we are grateful to the conference organizers who have provided data, either in the form of tables or by pointing us to abstract books. We thank the reviewers and the handling editor (Gottfried Otting) for the careful reading and suggestions. This project emerged from an interactive course about energy and climate, held at IST Austria by Jeroen Dobbelaere, Georgios Katsaros and Paul Schanda. We are grateful to ISTA's Graduate School for enabling this interdisciplinary course and to all participating students. We thank the following persons for discussions and/or comments about the manuscript: Helene Van Melckebeke, Mei Hong, Jeff Hoch, Gottfried Otting and Matthias Ernst. For the preparation of the manuscript, AI tools have been used, namely for finding relevant literature (ChatGPT) and for correcting the text (Writefull, within Overleaf LaTeX).","_id":"20664","article_processing_charge":"Yes","OA_type":"gold","file":[{"relation":"main_file","file_id":"20672","creator":"dernst","access_level":"open_access","content_type":"application/pdf","date_updated":"2025-11-24T08:25:19Z","file_name":"2025_MagneticResonance_Kapoor.pdf","checksum":"c63dd47b0e77f9451821436bb77d27c9","file_size":3081399,"date_created":"2025-11-24T08:25:19Z","success":1}],"oa":1,"publisher":"Copernicus Publications","department":[{"_id":"JoFi"},{"_id":"GaTk"},{"_id":"JoCs"},{"_id":"EvBe"},{"_id":"TaHa"},{"_id":"GradSch"},{"_id":"GeKa"},{"_id":"PaSc"}],"page":"243-256","publication":"Magnetic Resonance","status":"public","OA_place":"publisher"},{"publisher":"SciPost Foundation","department":[{"_id":"MiLe"}],"oa":1,"file":[{"file_id":"20673","relation":"main_file","creator":"dernst","access_level":"open_access","date_updated":"2025-11-24T08:42:42Z","content_type":"application/pdf","file_name":"2025_SciPostPhys_Koutentakis.pdf","checksum":"04d0e47ba66c63737431d7b8ed1df4bc","date_created":"2025-11-24T08:42:42Z","file_size":1725787,"success":1}],"OA_place":"publisher","publication":"Scipost Physics","status":"public","ddc":["530"],"external_id":{"isi":["001593017800002"],"arxiv":["2504.03411"]},"quality_controlled":"1","_id":"20666","OA_type":"diamond","article_processing_charge":"No","isi":1,"acknowledgement":"G.M.K. has received funding by the Austrian Science Fund (FWF)\r\n[DOI: 10.55776/F1004]. S.I.M acknowledges support from the Missouri University of Science and Technology, Department of Physics, Startup fund. F.G. acknowledges funding by the\r\nDeutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy – EXC-2111 — 390814868. H.R.S. acknowledges support for ITAMP by the\r\nNSF. P.S. acknowledges funding by the Cluster of Excellence “Advanced Imaging of Matter” of\r\nthe Deutsche Forschungsgemeinschaft (DFG) - EXC 2056 - project ID 390715994.","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","issue":"4","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"day":"01","date_created":"2025-11-23T23:01:39Z","publication_status":"published","intvolume":" 19","DOAJ_listed":"1","has_accepted_license":"1","file_date_updated":"2025-11-24T08:42:42Z","project":[{"name":"Coherent Optical Metrology Beyond Electric-Dipole-Allowed Transitions","grant_number":"F100403","_id":"7c040762-9f16-11ee-852c-dd79eeee4ab3"}],"corr_author":"1","date_published":"2025-10-01T00:00:00Z","volume":19,"PlanS_conform":"1","article_type":"original","language":[{"iso":"eng"}],"scopus_import":"1","doi":"10.21468/SciPostPhys.19.4.093","month":"10","author":[{"first_name":"Georgios","last_name":"Koutentakis","full_name":"Koutentakis, Georgios","id":"d7b23d3a-9e21-11ec-b482-f76739596b95"},{"full_name":"Mistakidis, S. I.","first_name":"S. I.","last_name":"Mistakidis"},{"last_name":"Grusdt","first_name":"F.","full_name":"Grusdt, F."},{"full_name":"Sadeghpour, H. R.","last_name":"Sadeghpour","first_name":"H. R."},{"full_name":"Schmelcher, P.","last_name":"Schmelcher","first_name":"P."}],"oa_version":"Published Version","abstract":[{"lang":"eng","text":"We theoretically investigate the stationary properties of a spin-1/2 impurity immersed in a one-dimensional confined Bose gas. In particular, we consider coherently coupled spin states with an external field, where only one spin component interacts with the bath, enabling light dressing of the impurity and spin-dependent bath-impurity interactions. Through detailed comparisons with ab-initio many-body simulations, we demonstrate that the composite system is accurately described by a simplified effective Hamiltonian. The latter builds upon previously developed effective potential approaches in the absence of light dressing. It can be used to extract the impurity energy, residue, effective mass, and anharmonicity induced by the phononic dressing. Light-dressing is shown to increase the polaron residue, undressing the impurity from phononic excitations because of strong spin coupling. For strong repulsions, previously shown to trigger dynamical Bose polaron decay (a phenomenon called temporal orthogonality catastrophe), it is explained that strong light-dressing stabilizes a repulsive polaron-dressed state. Our results establish the effective Hamiltonian framework as a powerful tool for exploring strongly interacting polaronic systems and corroborating forthcoming experimental realizations."}],"article_number":"093","citation":{"ama":"Koutentakis G, Mistakidis SI, Grusdt F, Sadeghpour HR, Schmelcher P. Competition of light-and phonon-dressing in microwave-dressed Bose polarons. Scipost Physics. 2025;19(4). doi:10.21468/SciPostPhys.19.4.093","apa":"Koutentakis, G., Mistakidis, S. I., Grusdt, F., Sadeghpour, H. R., & Schmelcher, P. (2025). Competition of light-and phonon-dressing in microwave-dressed Bose polarons. Scipost Physics. SciPost Foundation. https://doi.org/10.21468/SciPostPhys.19.4.093","short":"G. Koutentakis, S.I. Mistakidis, F. Grusdt, H.R. Sadeghpour, P. Schmelcher, Scipost Physics 19 (2025).","mla":"Koutentakis, Georgios, et al. “Competition of Light-and Phonon-Dressing in Microwave-Dressed Bose Polarons.” Scipost Physics, vol. 19, no. 4, 093, SciPost Foundation, 2025, doi:10.21468/SciPostPhys.19.4.093.","ieee":"G. Koutentakis, S. I. Mistakidis, F. Grusdt, H. R. Sadeghpour, and P. Schmelcher, “Competition of light-and phonon-dressing in microwave-dressed Bose polarons,” Scipost Physics, vol. 19, no. 4. SciPost Foundation, 2025.","ista":"Koutentakis G, Mistakidis SI, Grusdt F, Sadeghpour HR, Schmelcher P. 2025. Competition of light-and phonon-dressing in microwave-dressed Bose polarons. Scipost Physics. 19(4), 093.","chicago":"Koutentakis, Georgios, S. I. Mistakidis, F. Grusdt, H. R. Sadeghpour, and P. Schmelcher. “Competition of Light-and Phonon-Dressing in Microwave-Dressed Bose Polarons.” Scipost Physics. SciPost Foundation, 2025. https://doi.org/10.21468/SciPostPhys.19.4.093."},"publication_identifier":{"eissn":["2542-4653"]},"arxiv":1,"type":"journal_article","date_updated":"2025-12-01T15:22:01Z","year":"2025","title":"Competition of light-and phonon-dressing in microwave-dressed Bose polarons"},{"day":"20","date_created":"2025-11-23T23:01:39Z","citation":{"short":"A. El Latif Kadry, Y. Zhang, N. Weinberger, in:, 2025 IEEE International Symposium on Information Theory Proceedings, IEEE, 2025.","mla":"El Latif Kadry, Abd, et al. “Mean Estimation in High-Dimensional Binary Timeinhomogeneous Markov Gaussian Mixture Models.” 2025 IEEE International Symposium on Information Theory Proceedings, IEEE, 2025, doi:10.1109/ISIT63088.2025.11195426.","ieee":"A. El Latif Kadry, Y. Zhang, and N. Weinberger, “Mean estimation in high-dimensional binary timeinhomogeneous Markov Gaussian mixture models,” in 2025 IEEE International Symposium on Information Theory Proceedings, Ann Arbor, MI, United States, 2025.","chicago":"El Latif Kadry, Abd, Yihan Zhang, and Nir Weinberger. “Mean Estimation in High-Dimensional Binary Timeinhomogeneous Markov Gaussian Mixture Models.” In 2025 IEEE International Symposium on Information Theory Proceedings. IEEE, 2025. https://doi.org/10.1109/ISIT63088.2025.11195426.","ista":"El Latif Kadry A, Zhang Y, Weinberger N. 2025. Mean estimation in high-dimensional binary timeinhomogeneous Markov Gaussian mixture models. 2025 IEEE International Symposium on Information Theory Proceedings. ISIT: International Symposium on Information Theory.","ama":"El Latif Kadry A, Zhang Y, Weinberger N. Mean estimation in high-dimensional binary timeinhomogeneous Markov Gaussian mixture models. In: 2025 IEEE International Symposium on Information Theory Proceedings. IEEE; 2025. doi:10.1109/ISIT63088.2025.11195426","apa":"El Latif Kadry, A., Zhang, Y., & Weinberger, N. (2025). Mean estimation in high-dimensional binary timeinhomogeneous Markov Gaussian mixture models. In 2025 IEEE International Symposium on Information Theory Proceedings. Ann Arbor, MI, United States: IEEE. https://doi.org/10.1109/ISIT63088.2025.11195426"},"abstract":[{"text":"We explore the problem of mean estimation for a high-dimensional binary symmetric Gaussian mixture model, where the label (sign) follows a time-inhomogeneous Markov chain. We propose a spectral estimator based on a partition of a subset of the samples to blocks. We develop a computationally efficient algorithm to find the optimal blocks, and derive minimax lower bounds on the estimation loss of any estimator, which establish the effectiveness of our proposed estimator. The resulting minimax rate illuminates the interplay between the sample size, dimension, signal strength, and the memory on the loss.","lang":"eng"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"None","conference":{"end_date":"2025-06-27","location":"Ann Arbor, MI, United States","start_date":"2025-06-22","name":"ISIT: International Symposium on Information Theory"},"author":[{"first_name":"Abd","last_name":"El Latif Kadry","full_name":"El Latif Kadry, Abd"},{"last_name":"Zhang","first_name":"Yihan","orcid":"0000-0002-6465-6258","id":"2ce5da42-b2ea-11eb-bba5-9f264e9d002c","full_name":"Zhang, Yihan"},{"full_name":"Weinberger, Nir","first_name":"Nir","last_name":"Weinberger"}],"title":"Mean estimation in high-dimensional binary timeinhomogeneous Markov Gaussian mixture models","year":"2025","publication_status":"published","date_updated":"2025-11-24T08:53:34Z","type":"conference","publication_identifier":{"isbn":["9798331543990"],"issn":["2157-8095"]},"status":"public","language":[{"iso":"eng"}],"publication":"2025 IEEE International Symposium on Information Theory Proceedings","date_published":"2025-10-20T00:00:00Z","department":[{"_id":"MaMo"}],"publisher":"IEEE","acknowledgement":"The research of A.K. and N.W. was supported by the Israel Science Foundation (ISF), grant no. 1782/22.","month":"10","_id":"20667","OA_type":"closed access","article_processing_charge":"No","doi":"10.1109/ISIT63088.2025.11195426","scopus_import":"1","quality_controlled":"1"},{"oa_version":"Published Version","conference":{"name":"ACL: Meeting of the Association for Computational Linguistics","end_date":"2025-08-01","location":"Vienna, Austria","start_date":"2025-07-27"},"author":[{"id":"47beb3a5-07b5-11eb-9b87-b108ec578218","full_name":"Kurtic, Eldar","last_name":"Kurtic","first_name":"Eldar"},{"full_name":"Marques, Alexandre","last_name":"Marques","first_name":"Alexandre"},{"last_name":"Pandit","first_name":"Shubhra","full_name":"Pandit, Shubhra"},{"first_name":"Mark","last_name":"Kurtz","full_name":"Kurtz, Mark"},{"orcid":"0000-0003-3650-940X","first_name":"Dan-Adrian","last_name":"Alistarh","full_name":"Alistarh, Dan-Adrian","id":"4A899BFC-F248-11E8-B48F-1D18A9856A87"}],"abstract":[{"lang":"eng","text":"Quantization is a powerful tool for accelerating large language model (LLM) inference, but the accuracy-performance trade-offs across different formats remain unclear. In this paper, we conduct the most comprehensive empirical study to date, evaluating FP8, INT8, and INT4\r\nquantization across academic benchmarks and real-world tasks on the entire Llama-3.1 model\r\nfamily. Through over 500,000 evaluations, our investigation yields several key findings: (1) FP8 (W8A8-FP) is effectively lossless across all model scales, (2) well-tuned INT8 (W8A8-INT) achieves surprisingly low (1-3%) accuracy degradation, and (3) INT4 weightonly (W4A16-INT) is more competitive than expected, rivaling 8-bit quantization. Further, we investigate the optimal quantization format for different deployments by analyzing inference performance through the popular vLLM framework. Our analysis provides clear deployment recommendations: W4A16 is the most cost-efficient for synchronous setups, while W8A8 dominates in asynchronous\r\ncontinuous batching. For mixed workloads, the optimal choice depends on the specific use\r\ncase. Our findings offer practical, data-driven guidelines for deploying quantized LLMs at scale—ensuring the best balance between speed, efficiency, and accuracy. "}],"citation":{"mla":"Kurtic, Eldar, et al. “‘Give Me BF16 or Give Me Death’? Accuracy-Performance Trade-Offs in LLM Quantization.” Proceedings of the 63rd Annual Meeting of the Association for Computational Linguistics, Association for Computational Linguistics, 2025, pp. 26872–86.","ieee":"E. Kurtic, A. Marques, S. Pandit, M. Kurtz, and D.-A. Alistarh, “‘Give me BF16 or give me death’? Accuracy-performance trade-offs in LLM quantization,” in Proceedings of the 63rd Annual Meeting of the Association for Computational Linguistics, Vienna, Austria, 2025, pp. 26872–26886.","ista":"Kurtic E, Marques A, Pandit S, Kurtz M, Alistarh D-A. 2025. “Give me BF16 or give me death”? Accuracy-performance trade-offs in LLM quantization. Proceedings of the 63rd Annual Meeting of the Association for Computational Linguistics. ACL: Meeting of the Association for Computational Linguistics, 26872–26886.","chicago":"Kurtic, Eldar, Alexandre Marques, Shubhra Pandit, Mark Kurtz, and Dan-Adrian Alistarh. “‘Give Me BF16 or Give Me Death’? Accuracy-Performance Trade-Offs in LLM Quantization.” In Proceedings of the 63rd Annual Meeting of the Association for Computational Linguistics, 26872–86. Association for Computational Linguistics, 2025.","short":"E. Kurtic, A. Marques, S. Pandit, M. Kurtz, D.-A. Alistarh, in:, Proceedings of the 63rd Annual Meeting of the Association for Computational Linguistics, Association for Computational Linguistics, 2025, pp. 26872–26886.","apa":"Kurtic, E., Marques, A., Pandit, S., Kurtz, M., & Alistarh, D.-A. (2025). “Give me BF16 or give me death”? Accuracy-performance trade-offs in LLM quantization. In Proceedings of the 63rd Annual Meeting of the Association for Computational Linguistics (pp. 26872–26886). Vienna, Austria: Association for Computational Linguistics.","ama":"Kurtic E, Marques A, Pandit S, Kurtz M, Alistarh D-A. “Give me BF16 or give me death”? Accuracy-performance trade-offs in LLM quantization. In: Proceedings of the 63rd Annual Meeting of the Association for Computational Linguistics. Association for Computational Linguistics; 2025:26872-26886."},"date_updated":"2025-11-26T11:15:11Z","publication_identifier":{"isbn":["9798891762510"],"issn":["0736-587X"]},"type":"conference","arxiv":1,"title":"“Give me BF16 or give me death”? Accuracy-performance trade-offs in LLM quantization","year":"2025","date_published":"2025-08-01T00:00:00Z","has_accepted_license":"1","file_date_updated":"2025-11-26T11:06:57Z","corr_author":"1","language":[{"iso":"eng"}],"scopus_import":"1","month":"08","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_created":"2025-11-24T14:20:46Z","day":"01","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"publication_status":"published","oa":1,"file":[{"date_created":"2025-11-26T11:06:57Z","file_size":417450,"checksum":"4c066ee20f9ab17619c95652c0eb75f1","file_name":"2025_ACL_Kurtic.pdf","success":1,"creator":"dernst","file_id":"20698","relation":"main_file","content_type":"application/pdf","date_updated":"2025-11-26T11:06:57Z","access_level":"open_access"}],"publisher":"Association for Computational Linguistics","page":"26872-26886","department":[{"_id":"DaAl"}],"publication":"Proceedings of the 63rd Annual Meeting of the Association for Computational Linguistics","status":"public","OA_place":"publisher","ddc":["000"],"external_id":{"arxiv":["2411.02355"]},"quality_controlled":"1","_id":"20684","article_processing_charge":"No","OA_type":"gold"},{"file":[{"success":1,"file_name":"2025_GeosciModelDev_Segura.pdf","file_size":8618996,"date_created":"2025-11-25T12:02:30Z","checksum":"0f6a4af94e3a6be773d0051256bcecf5","access_level":"open_access","content_type":"application/pdf","date_updated":"2025-11-25T12:02:30Z","creator":"dernst","file_id":"20692","relation":"main_file"}],"oa":1,"publisher":"Copernicus Publications","department":[{"_id":"CaMu"}],"page":"7735-7761","publication":"Geoscientific Model Development","status":"public","OA_place":"publisher","ddc":["550"],"quality_controlled":"1","acknowledgement":"This research was supported by the Horizon 2020 project nextGEMS under grant agreement no. 101003470. Most simulations were performed and analyzed on facilities of the DKRZ (HLRE-4 Levante, 2024) with resources granted under project bm1235. We would like to thank DKRZ staff for their continued support in running the simulations and hosting and handling the data, in particular Jan Frederik Engels, Hendryk Bockelmann, Fabian Wachsmann, Irina Fast, and Carsten Beyer. We also want to thank the two anonymous reviewers for their insightful comments.This research has been supported by the EU Horizon 2020 (grant no. 101003470).\r\nThe article processing charges for this open-access publication were covered by the Max Planck Society.","OA_type":"gold","_id":"20685","article_processing_charge":"Yes (via OA deal)","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","day":"23","date_created":"2025-11-24T14:23:07Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"issue":"20","DOAJ_listed":"1","intvolume":" 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Imme"},{"last_name":"Aengenheyster","first_name":"Matthias","full_name":"Aengenheyster, Matthias"},{"last_name":"Aguridan","first_name":"Razvan","full_name":"Aguridan, Razvan"},{"full_name":"Arduini, Gabriele","first_name":"Gabriele","last_name":"Arduini"},{"full_name":"Baker, Alexander J.","last_name":"Baker","first_name":"Alexander J."},{"id":"bb9a7399-fefd-11ed-be3c-ae648fd1d160","full_name":"Bao, Jiawei","last_name":"Bao","first_name":"Jiawei"},{"last_name":"Bastin","first_name":"Swantje","full_name":"Bastin, Swantje"},{"full_name":"Baulenas, Eulàlia","last_name":"Baulenas","first_name":"Eulàlia"},{"full_name":"Becker, Tobias","first_name":"Tobias","last_name":"Becker"},{"full_name":"Beyer, Sebastian","last_name":"Beyer","first_name":"Sebastian"},{"full_name":"Bockelmann, Hendryk","last_name":"Bockelmann","first_name":"Hendryk"},{"full_name":"Brüggemann, Nils","first_name":"Nils","last_name":"Brüggemann"},{"first_name":"Lukas","last_name":"Brunner","full_name":"Brunner, 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Saliou","first_name":"Saliou","last_name":"Faye"},{"first_name":"Erich","last_name":"Fischer","full_name":"Fischer, Erich"},{"full_name":"van Heerwaarden, Chiel","first_name":"Chiel","last_name":"van Heerwaarden"},{"first_name":"Cathy","last_name":"Hohenegger","full_name":"Hohenegger, Cathy"},{"first_name":"Heikki","last_name":"Järvinen","full_name":"Järvinen, Heikki"},{"last_name":"Jochum","first_name":"Markus","full_name":"Jochum, Markus"},{"full_name":"Jung, Thomas","first_name":"Thomas","last_name":"Jung"},{"full_name":"Jungclaus, Johann H.","first_name":"Johann H.","last_name":"Jungclaus"},{"full_name":"Keenlyside, Noel S.","first_name":"Noel S.","last_name":"Keenlyside"},{"first_name":"Daniel","last_name":"Klocke","full_name":"Klocke, Daniel"},{"last_name":"Konow","first_name":"Heike","full_name":"Konow, Heike"},{"full_name":"Klose, Martina","first_name":"Martina","last_name":"Klose"},{"first_name":"Szymon","last_name":"Malinowski","full_name":"Malinowski, Szymon"},{"first_name":"Olivia","last_name":"Martius","full_name":"Martius, Olivia"},{"first_name":"Thorsten","last_name":"Mauritsen","full_name":"Mauritsen, Thorsten"},{"full_name":"Mellado, Juan Pedro","last_name":"Mellado","first_name":"Juan Pedro"},{"full_name":"Mieslinger, Theresa","first_name":"Theresa","last_name":"Mieslinger"},{"first_name":"Elsa","last_name":"Mohino","full_name":"Mohino, Elsa"},{"first_name":"Hanna","last_name":"Pawłowska","full_name":"Pawłowska, Hanna"},{"first_name":"Karsten","last_name":"Peters-von Gehlen","full_name":"Peters-von Gehlen, Karsten"},{"full_name":"Sarré, Abdoulaye","last_name":"Sarré","first_name":"Abdoulaye"},{"first_name":"Pajam","last_name":"Sobhani","full_name":"Sobhani, Pajam"},{"full_name":"Stier, Philip","last_name":"Stier","first_name":"Philip"},{"full_name":"Tuppi, Lauri","last_name":"Tuppi","first_name":"Lauri"},{"first_name":"Pier Luigi","last_name":"Vidale","full_name":"Vidale, Pier Luigi"},{"first_name":"Irina","last_name":"Sandu","full_name":"Sandu, Irina"},{"first_name":"Bjorn","last_name":"Stevens","full_name":"Stevens, Bjorn"}],"abstract":[{"lang":"eng","text":"The Next Generation of Earth Modeling Systems (nextGEMS) project aimed to produce multidecadal climate simulations, for the first time, with resolved kilometer-scale (km-scale) processes in the ocean, land, and atmosphere. In only 3 years, nextGEMS achieved this milestone with the two km-scale Earth system models, ICOsahedral Non-hydrostatic model (ICON) and Integrated Forecasting System coupled to the Finite-volumE Sea ice-Ocean Model (IFS-FESOM). nextGEMS was based on three cornerstones: (1) developing km-scale Earth system models with small errors in the energy and water balance, (2) performing km-scale climate simulations with a throughput greater than 1 simulated year per day, and (3) facilitating new workflows for an efficient analysis of the large simulations with common data structures and output variables. These cornerstones shaped the timeline of nextGEMS, divided into four cycles. Each cycle marked the release of a new configuration of ICON and IFS-FESOM, which were evaluated at hackathons. The hackathon participants included experts from climate science, software engineering, and high-performance computing as well as users from the energy and agricultural sectors. The continuous efforts over the four cycles allowed us to produce 30-year simulations with ICON and IFS-FESOM, spanning the period 2020–2049 under the SSP3-7.0 scenario. The throughput was about 500 simulated days per day on the Levante supercomputer of the German Climate Computing Center (DKRZ). The simulations employed a horizontal grid of about 5 km resolution in the ocean and 10 km resolution in the atmosphere and land. Aside from this technical achievement, the simulations allowed us to gain new insights into the realism of ICON and IFS-FESOM. Beyond its time frame, nextGEMS builds the foundation of the Climate Change Adaptation Digital Twin developed in the Destination Earth initiative and paves the way for future European research on climate change."}],"citation":{"apa":"Segura, H., Pedruzo-Bagazgoitia, X., Weiss, P., Müller, S. K., Rackow, T., Lee, J., … Stevens, B. (2025). nextGEMS: Entering the era of kilometer-scale Earth system modeling. Geoscientific Model Development. Copernicus Publications. https://doi.org/10.5194/gmd-18-7735-2025","ama":"Segura H, Pedruzo-Bagazgoitia X, Weiss P, et al. nextGEMS: Entering the era of kilometer-scale Earth system modeling. Geoscientific Model Development. 2025;18(20):7735-7761. doi:10.5194/gmd-18-7735-2025","chicago":"Segura, Hans, Xabier Pedruzo-Bagazgoitia, Philipp Weiss, Sebastian K. Müller, Thomas Rackow, Junhong Lee, Edgar Dolores-Tesillos, et al. “NextGEMS: Entering the Era of Kilometer-Scale Earth System Modeling.” Geoscientific Model Development. Copernicus Publications, 2025. https://doi.org/10.5194/gmd-18-7735-2025.","ista":"Segura H et al. 2025. nextGEMS: Entering the era of kilometer-scale Earth system modeling. Geoscientific Model Development. 18(20), 7735–7761.","ieee":"H. Segura et al., “nextGEMS: Entering the era of kilometer-scale Earth system modeling,” Geoscientific Model Development, vol. 18, no. 20. Copernicus Publications, pp. 7735–7761, 2025.","mla":"Segura, Hans, et al. “NextGEMS: Entering the Era of Kilometer-Scale Earth System Modeling.” Geoscientific Model Development, vol. 18, no. 20, Copernicus Publications, 2025, pp. 7735–61, doi:10.5194/gmd-18-7735-2025.","short":"H. Segura, X. Pedruzo-Bagazgoitia, P. Weiss, S.K. Müller, T. Rackow, J. Lee, E. Dolores-Tesillos, I. Benedict, M. Aengenheyster, R. Aguridan, G. Arduini, A.J. Baker, J. Bao, S. Bastin, E. Baulenas, T. Becker, S. Beyer, H. Bockelmann, N. Brüggemann, L. Brunner, S.K. Cheedela, S. Das, J. Denissen, I. Dragaud, P. Dziekan, M. Ekblom, J.F. Engels, M. Esch, R. Forbes, C. Frauen, L. Freischem, D. García-Maroto, P. Geier, P. Gierz, Á. González-Cervera, K. Grayson, M. Griffith, O. Gutjahr, H. Haak, I. Hadade, K. Haslehner, S. ul Hasson, J. Hegewald, L. Kluft, A. Koldunov, N. Koldunov, T. Kölling, S. Koseki, S. Kosukhin, J. Kousal, P. Kuma, A.U. Kumar, R. Li, N. Maury, M. Meindl, S. Milinski, K. Mogensen, B. Niraula, J. Nowak, D.S. Praturi, U. Proske, D. Putrasahan, R. Redler, D. Santuy, D. Sármány, R. Schnur, P. Scholz, D. Sidorenko, D. Spät, B. Sützl, D. Takasuka, A. Tompkins, A. Uribe, M. Valentini, M. Veerman, A. Voigt, S. Warnau, F. Wachsmann, M. Wacławczyk, N. Wedi, K.-H. Wieners, J. Wille, M. Winkler, Y. Wu, F. Ziemen, J. Zimmermann, F.A.-M. Bender, D. Bojovic, S. Bony, S. Bordoni, P. Brehmer, M. Dengler, E. Dutra, S. Faye, E. Fischer, C. van Heerwaarden, C. Hohenegger, H. Järvinen, M. Jochum, T. Jung, J.H. Jungclaus, N.S. Keenlyside, D. Klocke, H. Konow, M. Klose, S. Malinowski, O. Martius, T. Mauritsen, J.P. Mellado, T. Mieslinger, E. Mohino, H. Pawłowska, K. Peters-von Gehlen, A. Sarré, P. Sobhani, P. Stier, L. Tuppi, P.L. Vidale, I. Sandu, B. Stevens, Geoscientific Model Development 18 (2025) 7735–7761."},"date_updated":"2025-11-25T12:33:05Z","publication_identifier":{"eissn":["1991-9603"]},"type":"journal_article","title":"nextGEMS: Entering the era of kilometer-scale Earth system modeling","year":"2025"},{"date_published":"2025-10-20T00:00:00Z","volume":702,"PlanS_conform":"1","has_accepted_license":"1","file_date_updated":"2025-11-25T12:56:18Z","language":[{"iso":"eng"}],"article_type":"original","scopus_import":"1","month":"10","doi":"10.1051/0004-6361/202554574","oa_version":"Published Version","author":[{"full_name":"Bertassi, Lorenzo","first_name":"Lorenzo","last_name":"Bertassi"},{"full_name":"Sottocorno, Erika","last_name":"Sottocorno","first_name":"Erika"},{"full_name":"Rigamonti, Fabio","first_name":"Fabio","last_name":"Rigamonti"},{"last_name":"D’Orazio","first_name":"Daniel","full_name":"D’Orazio, Daniel"},{"full_name":"Eracleous, Michael","first_name":"Michael","last_name":"Eracleous"},{"full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","orcid":"0000-0003-3633-5403","last_name":"Haiman"},{"full_name":"Dotti, Massimo","last_name":"Dotti","first_name":"Massimo"}],"abstract":[{"text":"Emission from two massive black holes (MBHs) bound in a close binary is expected to be modulated by different processes, such as the Doppler boost due to the orbital motion, accretion rate variability generated by the interaction with a circumbinary disc, and binary gravitational self-lensing. When the binary is compact enough, the two black holes are thought to be surrounded by a common broad-line region that reprocesses the impinging periodically varying ionising flux, creating broad emission lines with variable line shapes. Therefore, the study of broad emission line variability through multi-epoch spectroscopic campaigns is of paramount importance for the unambiguous identification of a binary. In this work, we study the response of a disc-like broad-line region to the Doppler-boosted ionising flux emitted by sub-milliparsec MBH binaries on a circular orbit and compare it with the response of a broad-line region illuminated by a single MBH with a periodically but isotropically varying intrinsic luminosity. We show that in the binary case, the time lags of the blue and red wings of the broad emission lines, arising from diametrically opposite sides of the circumbinary disc, are out of phase by half of the binary’s orbital period, as they each respond to the periodic ‘lighthouse’ modulation from the binary’s continuum emission. This asymmetric time lag represents a new binary signature that cannot be mimicked by a single MBH.","lang":"eng"}],"citation":{"chicago":"Bertassi, Lorenzo, Erika Sottocorno, Fabio Rigamonti, Daniel D’Orazio, Michael Eracleous, Zoltán Haiman, and Massimo Dotti. “Testing Compact Massive Black Hole Binary Candidates through Multi-Epoch Spectroscopy.” Astronomy & Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202554574.","ista":"Bertassi L, Sottocorno E, Rigamonti F, D’Orazio D, Eracleous M, Haiman Z, Dotti M. 2025. Testing compact massive black hole binary candidates through multi-epoch spectroscopy. Astronomy & Astrophysics. 702, A165.","ieee":"L. Bertassi et al., “Testing compact massive black hole binary candidates through multi-epoch spectroscopy,” Astronomy & Astrophysics, vol. 702. EDP Sciences, 2025.","mla":"Bertassi, Lorenzo, et al. “Testing Compact Massive Black Hole Binary Candidates through Multi-Epoch Spectroscopy.” Astronomy & Astrophysics, vol. 702, A165, EDP Sciences, 2025, doi:10.1051/0004-6361/202554574.","short":"L. Bertassi, E. Sottocorno, F. Rigamonti, D. D’Orazio, M. Eracleous, Z. Haiman, M. Dotti, Astronomy & Astrophysics 702 (2025).","apa":"Bertassi, L., Sottocorno, E., Rigamonti, F., D’Orazio, D., Eracleous, M., Haiman, Z., & Dotti, M. (2025). Testing compact massive black hole binary candidates through multi-epoch spectroscopy. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202554574","ama":"Bertassi L, Sottocorno E, Rigamonti F, et al. Testing compact massive black hole binary candidates through multi-epoch spectroscopy. Astronomy & Astrophysics. 2025;702. doi:10.1051/0004-6361/202554574"},"article_number":"A165","date_updated":"2025-12-01T15:31:55Z","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"type":"journal_article","arxiv":1,"title":"Testing compact massive black hole binary candidates through multi-epoch spectroscopy","year":"2025","file":[{"file_id":"20693","relation":"main_file","creator":"dernst","access_level":"open_access","date_updated":"2025-11-25T12:56:18Z","content_type":"application/pdf","file_name":"2025_AstronomyAstrophysics_Bertassi.pdf","checksum":"dbaf156cb6684bf5c3f5fb76fc890d5a","date_created":"2025-11-25T12:56:18Z","file_size":2035081,"success":1}],"oa":1,"publisher":"EDP Sciences","department":[{"_id":"ZoHa"}],"publication":"Astronomy & Astrophysics","status":"public","OA_place":"publisher","ddc":["520"],"external_id":{"arxiv":["2504.06349"],"isi":["001597841900015"]},"quality_controlled":"1","acknowledgement":"MD acknowledge funding from MIUR under the grant PRIN 2017-MB8AEZ, and financial support from ICSC – Centro Nazionale di Ricerca in High Performance Computing, Big Data and Quantum Computing, funded by European Union – NextGenerationEU. This study is supported by the Italian Ministry for Research and University (MUR) under Grant ‘Progetto Dipartimenti di Eccellenza 2023-2027’ (BiCoQ). FR acknowledges the support from the Next Generation EU funds within the National Recovery and Resilience Plan (PNRR), Mission 4 – Education and Research, Component 2 – From Research to Business (M4C2), Investment Line 3.1 – Strengthening and creation of Research Infrastructures, Project IR0000012 – CTA+ – Cherenkov Telescope Array Plus. DJD acknowledges support from the Danish Independent Research Fund through Sapere Aude Starting Grant No. 121587 ZH acknowledges support from NSF grant AST-2006176 and NASA grants 80NSSC22K0822 and 80NSSC24K0440.","_id":"20686","OA_type":"diamond","article_processing_charge":"No","isi":1,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_created":"2025-11-24T14:23:22Z","day":"20","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"intvolume":" 702","publication_status":"published"},{"abstract":[{"text":"Subgiants and early red giants are crucial for studying the first dredge-up, a key evolutionary phase in which the convective envelope deepens, mixing previously interior-processed material and bringing it to the surface. Yet, very few have been seismically characterized with Kepler because their oscillation frequencies are close to the 30 minute sampling frequency of the mission. We developed a new method as part of the new PyA2Z code of identifying super-Nyquist oscillators and inferring their global seismic parameters, νmax and large separation, Δν.\r\n\r\nApplying PyA2Z to 2065 Kepler targets, we seismically characterize 285 super-Nyquist and 168 close-to-Nyquist stars with masses from 0.8 to 1.6 M⊙. In combination with APOGEE spectroscopy, Gaia spectrophotometry, and stellar models, we derive stellar ages for the sample. There is good agreement between the predicted and actual positions of stars on the HR diagram (luminosity vs. effective temperature) as a function of mass and composition. While the timing of dredge-up is consistent with predictions, the magnitude and mass dependence show discrepancies with models, possibly due to uncertainties in model physics or calibration issues in observed abundance scales.","lang":"eng"}],"article_number":"A144","citation":{"ama":"Liagre BRB, García RA, Mathur S, et al. Beyond the Nyquist frequency. Astronomy & Astrophysics. 2025;702. doi:10.1051/0004-6361/202555167","apa":"Liagre, B. R. B., García, R. A., Mathur, S., Pinsonneault, M. H., Serenelli, A., Zinn, J. C., … Palakkatharappil, D. B. (2025). Beyond the Nyquist frequency. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202555167","short":"B.R.B. Liagre, R.A. García, S. Mathur, M.H. Pinsonneault, A. Serenelli, J.C. Zinn, K. Cao, D. Godoy-Rivera, J. Tayar, P.G. Beck, D.H. Grossmann, D.B. Palakkatharappil, Astronomy & Astrophysics 702 (2025).","ista":"Liagre BRB, García RA, Mathur S, Pinsonneault MH, Serenelli A, Zinn JC, Cao K, Godoy-Rivera D, Tayar J, Beck PG, Grossmann DH, Palakkatharappil DB. 2025. Beyond the Nyquist frequency. Astronomy & Astrophysics. 702, A144.","chicago":"Liagre, Bastien Raymond Bernard, R. A. García, S. Mathur, M. H. Pinsonneault, A. Serenelli, J. C. Zinn, K. Cao, et al. “Beyond the Nyquist Frequency.” Astronomy & Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202555167.","ieee":"B. R. B. Liagre et al., “Beyond the Nyquist frequency,” Astronomy & Astrophysics, vol. 702. EDP Sciences, 2025.","mla":"Liagre, Bastien Raymond Bernard, et al. “Beyond the Nyquist Frequency.” Astronomy & Astrophysics, vol. 702, A144, EDP Sciences, 2025, doi:10.1051/0004-6361/202555167."},"oa_version":"Published Version","author":[{"full_name":"Liagre, Bastien Raymond Bernard","id":"662f1873-cab4-11f0-a719-8087d302868d","first_name":"Bastien Raymond Bernard","last_name":"Liagre"},{"full_name":"García, R. A.","first_name":"R. A.","last_name":"García"},{"full_name":"Mathur, S.","first_name":"S.","last_name":"Mathur"},{"full_name":"Pinsonneault, M. H.","first_name":"M. H.","last_name":"Pinsonneault"},{"full_name":"Serenelli, A.","first_name":"A.","last_name":"Serenelli"},{"first_name":"J. C.","last_name":"Zinn","full_name":"Zinn, J. C."},{"full_name":"Cao, K.","last_name":"Cao","first_name":"K."},{"full_name":"Godoy-Rivera, D.","last_name":"Godoy-Rivera","first_name":"D."},{"full_name":"Tayar, J.","first_name":"J.","last_name":"Tayar"},{"last_name":"Beck","first_name":"P. G.","full_name":"Beck, P. G."},{"full_name":"Grossmann, D. H.","last_name":"Grossmann","first_name":"D. H."},{"last_name":"Palakkatharappil","first_name":"D. B.","full_name":"Palakkatharappil, D. B."}],"title":"Beyond the Nyquist frequency","year":"2025","date_updated":"2025-12-01T15:32:48Z","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"type":"journal_article","arxiv":1,"language":[{"iso":"eng"}],"article_type":"original","volume":702,"date_published":"2025-10-01T00:00:00Z","PlanS_conform":"1","has_accepted_license":"1","file_date_updated":"2025-11-26T10:46:24Z","corr_author":"1","month":"10","doi":"10.1051/0004-6361/202555167","scopus_import":"1","day":"01","date_created":"2025-11-24T14:23:36Z","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","intvolume":" 702","publication_status":"published","publication":"Astronomy & Astrophysics","status":"public","OA_place":"publisher","file":[{"success":1,"file_name":"2025_AstronomyAstrophysics_Liagre.pdf","checksum":"38fd0aa23b6945dc22be90caf55bfb6c","date_created":"2025-11-26T10:46:24Z","file_size":3081589,"access_level":"open_access","content_type":"application/pdf","date_updated":"2025-11-26T10:46:24Z","relation":"main_file","file_id":"20697","creator":"dernst"}],"oa":1,"publisher":"EDP Sciences","acknowledgement":"This paper includes data collected by the Kepler mission and obtained from the MAST data archive at the Space Telescope Science Institute (STScI). Funding for the Kepler mission is provided by the NASA Science Mission Directorate. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. R.A.G. acknowledges the support from the GOLF and PLATO Centre National D’Études Spatiales grants. S.M. acknowledges support by the Spanish Ministry of Science and Innovation with the grant number PID2019-107061GB-C66, and through AEI under the Severo Ochoa Centres of Excellence Programme 2020–2023 (CEX2019-000920-S). B.L. thanks École Normale Supérieure Paris-Saclay (France) for its stipend that made possible to fund a long stay abroad. SM, DHG, DGR, and RAG acknowledge support from the Spanish Ministry of Science and Innovation with the grant no. PID2023-149439NB-C41. PGB acknowledges support by the Spanish Ministry of Science and Innovation with the Ramón y Cajal fellowship number RYC-2021-033137-I and the number MRR4032204. PGB, DHG, DGR, and RAG acknowledge support from the Spanish Ministry of Science and Innovation with the grant no. PID2023-146453NB-100 (PLAtoSOnG). AS acknowledges support by the Spanish Ministry of Science, Innovation and Universities through the grant PID2023-149918NB-I00 and the program Unidad de Excelencia María de Maeztu CEX2020-001058-M, and Generalitat de Catalunya through grant 2021-SGR-1526. MHP acknowledges support from NASA grant 80NSSC24K0637. MHP acknowledges support from the Fundación Occident and the Instituto de Astrofísica de Canarias under the Visiting Researcher Programme 2022-2025 agreed between both institutions. DGR acknowledges support from the Juan de la Cierva program under contract JDC2022-049054-I. DHG acknowledges the support of a fellowship from “la Caixa” Foundation (ID 100010434). The fellowship code is LCF/BQ/DI23/11990068. Software: AstroPy (Astropy Collaboration 2013, 2018), Matplotlib (Hunter 2007), NumPy (Harris et al. 2020), SciPy (Virtanen et al. 2020)","article_processing_charge":"No","_id":"20687","OA_type":"diamond","isi":1,"ddc":["520"],"external_id":{"arxiv":["2508.15654"],"isi":["001597841900002"]},"quality_controlled":"1"},{"project":[{"grant_number":"101034413","_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c","name":"IST-BRIDGE: International postdoctoral program","call_identifier":"H2020"}],"corr_author":"1","date_published":"2025-10-09T00:00:00Z","ec_funded":1,"language":[{"iso":"eng"}],"scopus_import":"1","doi":"10.1109/lics65433.2025.00049","month":"10","author":[{"full_name":"Grobelna, Marta","last_name":"Grobelna","first_name":"Marta"},{"last_name":"Kretinsky","orcid":"0000-0002-8122-2881","first_name":"Jan","id":"44CEF464-F248-11E8-B48F-1D18A9856A87","full_name":"Kretinsky, Jan"},{"id":"02ab0197-cc70-11ed-ab61-918e71f56881","full_name":"Weininger, Maximilian","last_name":"Weininger","first_name":"Maximilian","orcid":"0000-0002-0163-2152"}],"conference":{"end_date":"2025-06-26","location":"Singapore, Singapore","start_date":"2025-06-23","name":"LICS: Logic in Computer Science"},"oa_version":"Preprint","abstract":[{"text":"We consider two-player zero-sum concurrent stochastic games (CSGs) played on graphs with reachability and safety objectives. These include degenerate classes such as Markov decision processes or turn-based stochastic games, which can be solved by linear or quadratic programming; however, in practice, value iteration (VI) outperforms the other approaches and is the most implemented method. Similarly, for CSGs, this practical performance makes VI an attractive alternative to the standard theoretical solution via the existential theory of reals.VI starts with an under-approximation of the sought values for each state and iteratively updates them, traditionally terminating once two consecutive approximations are ϵ-close. However, this stopping criterion lacks guarantees on the precision of the approximation, which is the goal of this work. We provide bounded (a.k.a. interval) VI for CSGs: it complements standard VI with a converging sequence of over-approximations and terminates once the over- and under-approximations are ϵ-close.","lang":"eng"}],"citation":{"apa":"Grobelna, M., Kretinsky, J., & Weininger, M. (2025). Stopping criteria for value iteration on concurrent stochastic reachability and safety games. In 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science (pp. 568–580). Singapore, Singapore: IEEE. https://doi.org/10.1109/lics65433.2025.00049","ama":"Grobelna M, Kretinsky J, Weininger M. Stopping criteria for value iteration on concurrent stochastic reachability and safety games. In: 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science. IEEE; 2025:568-580. doi:10.1109/lics65433.2025.00049","mla":"Grobelna, Marta, et al. “Stopping Criteria for Value Iteration on Concurrent Stochastic Reachability and Safety Games.” 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, IEEE, 2025, pp. 568–80, doi:10.1109/lics65433.2025.00049.","ieee":"M. Grobelna, J. Kretinsky, and M. Weininger, “Stopping criteria for value iteration on concurrent stochastic reachability and safety games,” in 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, Singapore, Singapore, 2025, pp. 568–580.","chicago":"Grobelna, Marta, Jan Kretinsky, and Maximilian Weininger. “Stopping Criteria for Value Iteration on Concurrent Stochastic Reachability and Safety Games.” In 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, 568–80. IEEE, 2025. https://doi.org/10.1109/lics65433.2025.00049.","ista":"Grobelna M, Kretinsky J, Weininger M. 2025. Stopping criteria for value iteration on concurrent stochastic reachability and safety games. 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science. LICS: Logic in Computer Science, 568–580.","short":"M. Grobelna, J. Kretinsky, M. Weininger, in:, 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, IEEE, 2025, pp. 568–580."},"publication_identifier":{"eisbn":["9798331579005"]},"type":"conference","arxiv":1,"date_updated":"2025-11-26T07:34:19Z","year":"2025","title":"Stopping criteria for value iteration on concurrent stochastic reachability and safety games","publisher":"IEEE","department":[{"_id":"KrCh"}],"page":"568-580","oa":1,"OA_place":"repository","publication":"2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science","status":"public","external_id":{"arxiv":["2505.21087"]},"quality_controlled":"1","article_processing_charge":"No","_id":"20688","OA_type":"green","acknowledgement":"This research was funded in part by the German Research Foundation (DFG) project 427755713 GOPro, the MUNI Award in Science and Humanities (MUNI/I/1757/2021) of the Grant Agency of Masaryk University, the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No 101034413, and the ERC Starting Grant DEUCE (101077178).","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2505.21087","open_access":"1"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_created":"2025-11-24T14:23:49Z","day":"09","publication_status":"published"},{"publication_identifier":{"eisbn":["9798331579005"]},"type":"conference","arxiv":1,"date_updated":"2025-11-25T07:59:25Z","year":"2025","title":"Multiplicative rewards in Markovian models","author":[{"full_name":"Baier, Christel","first_name":"Christel","last_name":"Baier"},{"orcid":"0000-0002-4561-241X","first_name":"Krishnendu","last_name":"Chatterjee","full_name":"Chatterjee, Krishnendu","id":"2E5DCA20-F248-11E8-B48F-1D18A9856A87"},{"first_name":"Tobias","orcid":"0000-0002-1712-2165","last_name":"Meggendorfer","full_name":"Meggendorfer, Tobias","id":"b21b0c15-30a2-11eb-80dc-f13ca25802e1"},{"first_name":"Jakob","last_name":"Piribauer","full_name":"Piribauer, Jakob"}],"oa_version":"Preprint","conference":{"name":"LICS: Logic in Computer Science","location":"Singapore, Singapore","start_date":"2025-06-23","end_date":"2025-06-26"},"abstract":[{"lang":"eng","text":"This paper studies the expected value of multiplicative rewards, where rewards obtained in each step are multiplied (instead of the usual addition), in Markov chains (MCs) and Markov decision processes (MDPs). One of the key differences to additive rewards is that the expected value may diverge to ∞ not only due to recurrent, but also due to transient states.For MCs, computing the value is shown to be possible in polynomial time given an oracle for the comparison of succinctly represented integers (CSRI), which is only known to be solvable in polynomial time subject to number-theoretic conjectures. Interestingly, distinguishing whether the value is ∞ or 0 is at least as hard as CSRI, while determining if it is one of these two can be done in polynomial time. In MDPs, the optimal value can be computed in polynomial space. Further refined complexity results and results on the complexity of optimal schedulers are presented. The techniques developed for MDPs additionally allow to solve the multiplicative variant of the stochastic shortest path problem. Finally, for MCs and MDPs where an absorbing state is reached almost surely, all considered problems are solvable in polynomial time."}],"citation":{"short":"C. Baier, K. Chatterjee, T. Meggendorfer, J. Piribauer, in:, 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, IEEE, 2025, pp. 499–512.","ista":"Baier C, Chatterjee K, Meggendorfer T, Piribauer J. 2025. Multiplicative rewards in Markovian models. 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science. LICS: Logic in Computer Science, 499–512.","chicago":"Baier, Christel, Krishnendu Chatterjee, Tobias Meggendorfer, and Jakob Piribauer. “Multiplicative Rewards in Markovian Models.” In 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, 499–512. IEEE, 2025. https://doi.org/10.1109/lics65433.2025.00044.","ieee":"C. Baier, K. Chatterjee, T. Meggendorfer, and J. Piribauer, “Multiplicative rewards in Markovian models,” in 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, Singapore, Singapore, 2025, pp. 499–512.","mla":"Baier, Christel, et al. “Multiplicative Rewards in Markovian Models.” 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, IEEE, 2025, pp. 499–512, doi:10.1109/lics65433.2025.00044.","ama":"Baier C, Chatterjee K, Meggendorfer T, Piribauer J. Multiplicative rewards in Markovian models. In: 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science. IEEE; 2025:499-512. doi:10.1109/lics65433.2025.00044","apa":"Baier, C., Chatterjee, K., Meggendorfer, T., & Piribauer, J. (2025). Multiplicative rewards in Markovian models. In 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science (pp. 499–512). Singapore, Singapore: IEEE. https://doi.org/10.1109/lics65433.2025.00044"},"scopus_import":"1","doi":"10.1109/lics65433.2025.00044","month":"10","project":[{"grant_number":"863818","_id":"0599E47C-7A3F-11EA-A408-12923DDC885E","name":"Formal Methods for Stochastic Models: Algorithms and Applications","call_identifier":"H2020"}],"corr_author":"1","date_published":"2025-10-09T00:00:00Z","ec_funded":1,"language":[{"iso":"eng"}],"publication_status":"published","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2504.18277","open_access":"1"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","day":"09","date_created":"2025-11-24T14:24:00Z","quality_controlled":"1","external_id":{"arxiv":["2504.18277"]},"_id":"20689","OA_type":"green","article_processing_charge":"No","acknowledgement":"This work was partly funded by the ERC CoG 863818 (ForM-SMArt), the Austrian Science Fund (FWF) 10.55776/COE12, the DFG Grant 389792660 as part of TRR 248 (Foundations of Perspicuous Software Systems), the Cluster of Excellence EXC 2050/1 (CeTI, project ID\r\n390696704, as part of Germany’s Excellence Strategy), and by the BMBF (Federal Ministry of Education and Research) in DAAD project 57616814 (SECAI, School of Embedded and\r\nComposite AI) as part of the program Konrad Zuse Schools of Excellence in Artificial Intelligence.","publisher":"IEEE","department":[{"_id":"KrCh"}],"page":"499-512","oa":1,"OA_place":"repository","publication":"2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science","status":"public"},{"author":[{"full_name":"Brihaye, Thomas","first_name":"Thomas","last_name":"Brihaye"},{"full_name":"Chatterjee, Krishnendu","id":"2E5DCA20-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-4561-241X","first_name":"Krishnendu","last_name":"Chatterjee"},{"full_name":"Mohr, Stefanie","last_name":"Mohr","first_name":"Stefanie"},{"full_name":"Weininger, Maximilian","id":"02ab0197-cc70-11ed-ab61-918e71f56881","orcid":"0000-0002-0163-2152","first_name":"Maximilian","last_name":"Weininger"}],"conference":{"name":"LICS: Logic in Computer Science","end_date":"2025-06-26","start_date":"2025-06-23","location":"Singapore, Singapore"},"oa_version":"Preprint","abstract":[{"text":"Cumulative prospect theory (CPT) is the first theory for decision-making under uncertainty that combines full theoretical soundness and empirically realistic features [1], [Page 2]. While CPT was originally considered in one-shot settings for risk-aware decision-making, we consider CPT in sequential decision-making. The most fundamental and well-studied models for sequential decision-making are Markov chains (MCs), and their generalization Markov decision processes (MDPs). The complexity theoretic study of MCs and MDPs with CPT is a fundamental problem that has not been addressed in the literature.Our contributions are as follows: First, we present an alternative viewpoint for the CPT-value of MCs and MDPs. This allows us to establish a connection with multi-objective reachability analysis and conclude the strategy complexity result that memoryless randomized strategies are necessary and sufficient for optimality. Second, based on this connection, we provide an algorithm for computing the CPT-value in MDPs with infinite-horizon objectives. We show that the problem is in EXPTIME and fixed-parameter tractable. Moreover, we provide a polynomial-time algorithm for the special case of MCs.","lang":"eng"}],"citation":{"ieee":"T. Brihaye, K. Chatterjee, S. Mohr, and M. Weininger, “Risk-aware Markov decision processes using cumulative prospect theory,” in 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, Singapore, Singapore, 2025, pp. 458–471.","mla":"Brihaye, Thomas, et al. “Risk-Aware Markov Decision Processes Using Cumulative Prospect Theory.” 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, IEEE, 2025, pp. 458–71, doi:10.1109/lics65433.2025.00041.","chicago":"Brihaye, Thomas, Krishnendu Chatterjee, Stefanie Mohr, and Maximilian Weininger. “Risk-Aware Markov Decision Processes Using Cumulative Prospect Theory.” In 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, 458–71. IEEE, 2025. https://doi.org/10.1109/lics65433.2025.00041.","ista":"Brihaye T, Chatterjee K, Mohr S, Weininger M. 2025. Risk-aware Markov decision processes using cumulative prospect theory. 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science. LICS: Logic in Computer Science, 458–471.","short":"T. Brihaye, K. Chatterjee, S. Mohr, M. Weininger, in:, 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science, IEEE, 2025, pp. 458–471.","apa":"Brihaye, T., Chatterjee, K., Mohr, S., & Weininger, M. (2025). Risk-aware Markov decision processes using cumulative prospect theory. In 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science (pp. 458–471). Singapore, Singapore: IEEE. https://doi.org/10.1109/lics65433.2025.00041","ama":"Brihaye T, Chatterjee K, Mohr S, Weininger M. Risk-aware Markov decision processes using cumulative prospect theory. In: 2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science. IEEE; 2025:458-471. doi:10.1109/lics65433.2025.00041"},"publication_identifier":{"eisbn":["9798331579005"]},"arxiv":1,"type":"conference","date_updated":"2025-11-25T07:59:49Z","year":"2025","title":"Risk-aware Markov decision processes using cumulative prospect theory","project":[{"_id":"0599E47C-7A3F-11EA-A408-12923DDC885E","grant_number":"863818","name":"Formal Methods for Stochastic Models: Algorithms and Applications","call_identifier":"H2020"},{"_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c","grant_number":"101034413","name":"IST-BRIDGE: International postdoctoral program","call_identifier":"H2020"}],"corr_author":"1","date_published":"2025-10-09T00:00:00Z","ec_funded":1,"language":[{"iso":"eng"}],"scopus_import":"1","doi":"10.1109/lics65433.2025.00041","month":"10","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2505.09514"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","day":"09","date_created":"2025-11-24T14:43:47Z","publication_status":"published","publisher":"IEEE","department":[{"_id":"KrCh"}],"page":"458-471","oa":1,"OA_place":"repository","publication":"2025 40th Annual ACM/IEEE Symposium on Logic in Computer Science","status":"public","external_id":{"arxiv":["2505.09514"]},"quality_controlled":"1","OA_type":"green","_id":"20690","article_processing_charge":"No","acknowledgement":"This project has received funding from the Fonds de la Recherche Scientifique - FNRS under grant No. T.0027.21, the Belgian National Lottery; the ERC CoG 863818 (ForM-SMArt), the Austrian Science Fund (FWF) 10.55776/COE12; the DFG project 427755713, GOPro, and the DFG research training group GRK 2428 Continuous Verification of Cyber-Physical Systems\r\n(ConVeY); the EU’s Horizon 2020 research and innovation programmes under the Marie Sklodowska-Curie grant agreement No. 101034413 (IST-BRIDGE) and the ERC Starting Grant DEUCE (101077178)."}]