[{"_id":"22998","external_id":{"pmid":["42722132"],"biorxivid":["10.1101/2025.04.09.647826"]},"year":"2026","researchdata_availability":"no","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"publisher","article_type":"original","author":[{"first_name":"Kseniia","last_name":"Khudiakova","full_name":"Khudiakova, Kseniia","orcid":"0000-0002-6246-1465","id":"4E6DC800-AE37-11E9-AC72-31CAE5697425"},{"last_name":"Barton","full_name":"Barton, Nicholas H","first_name":"Nicholas H","id":"4880FE40-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8548-5240"},{"last_name":"Arnqvist","full_name":"Arnqvist, Göran","first_name":"Göran"}],"related_material":{"record":[{"relation":"earlier_version","id":"21968","status":"public"}]},"abstract":[{"text":"Balancing selection, a form of selection that maintains genetic diversity, is difficult to detect, and the importance of balancing selection for the maintenance of genetic variation may be larger than often assumed. We model the possibility that the diversity-promoting effects of balancing selection extend to other loci that show sign epistasis with a locus under balancing selection. Rather than focusing on overdominance, as was done in previous efforts, we explore the effects of negative frequency dependence and show that this has important effects on the conditions under which the diversity-promoting effect of epistasis can occur in diploids. Our results show that not only recombination rate but also the dominance of sign epistasis are key parameters that determine the maintenance of polymorphism beyond the locus under direct balancing selection. We suggest that the effect we explore may play a significant role, especially when balancing selection acts on major effect loci.","lang":"eng"}],"publication":"Theoretical Population Biology","quality_controlled":"1","pmid":1,"publication_status":"epub_ahead","das_tickbox":"1","date_published":"2026-09-17T00:00:00Z","dataavailabilitystatement":"The Python code used for the numerical analyses is available online at https://github.com/khudyakovaks/Sign-epistasis-extends-the-effects-of-balancing-selection-on-genetic-diversity.","date_updated":"2026-10-07T06:38:02Z","OA_type":"hybrid","project":[{"grant_number":"26293","_id":"34d33d68-11ca-11ed-8bc3-ec13763c0ca8","name":"The impact of deleterious mutations on small populations"}],"tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"fulldoi":"https://doi.org/10.1016/j.tpb.2026.09.001","volume":172,"main_file_link":[{"url":"https://doi.org/10.1016/j.tpb.2026.09.001","open_access":"1"}],"oa":1,"article_processing_charge":"Yes (via OA deal)","acknowledgement":"This work was funded by grants from the Swedish Research Council (2023-03730 to G.A.) and the DOC fellowship from the Austrian Academy of Science (26293 to K.K.). We thank L. Rowe for valuable discussions.","publication_identifier":{"issn":["0040-5809"],"eissn":["1096-0325"]},"biorxivid":1,"day":"17","page":"48-55","title":"Sign epistasis extends the effects of balancing selection on genetic diversity","oa_version":"Published Version","date_created":"2026-09-27T22:01:51Z","supplementarymaterial":"yes","has_accepted_license":"1","type":"journal_article","language":[{"iso":"eng"}],"doi":"10.1016/j.tpb.2026.09.001","department":[{"_id":"JaMa"},{"_id":"GradSch"},{"_id":"NiBa"}],"ddc":["500","570"],"status":"public","keyword":["Sign epistasis","Balancing selection","Within-population genetic variation"],"PlanS_conform":"1","citation":{"chicago":"Khudiakova, Kseniia, Nicholas H Barton, and Göran Arnqvist. “Sign Epistasis Extends the Effects of Balancing Selection on Genetic Diversity.” Theoretical Population Biology, 2026. https://doi.org/10.1016/j.tpb.2026.09.001.","ama":"Khudiakova K, Barton NH, Arnqvist G. Sign epistasis extends the effects of balancing selection on genetic diversity. Theoretical Population Biology. 2026;172:48-55. doi:10.1016/j.tpb.2026.09.001","apa":"Khudiakova, K., Barton, N. H., & Arnqvist, G. (2026). Sign epistasis extends the effects of balancing selection on genetic diversity. Theoretical Population Biology. https://doi.org/10.1016/j.tpb.2026.09.001","ista":"Khudiakova K, Barton NH, Arnqvist G. 2026. Sign epistasis extends the effects of balancing selection on genetic diversity. Theoretical Population Biology. 172, 48–55.","mla":"Khudiakova, Kseniia, et al. “Sign Epistasis Extends the Effects of Balancing Selection on Genetic Diversity.” Theoretical Population Biology, vol. 172, 2026, pp. 48–55, doi:10.1016/j.tpb.2026.09.001.","ieee":"K. Khudiakova, N. H. Barton, and G. Arnqvist, “Sign epistasis extends the effects of balancing selection on genetic diversity,” Theoretical Population Biology, vol. 172. pp. 48–55, 2026.","short":"K. Khudiakova, N.H. Barton, G. Arnqvist, Theoretical Population Biology 172 (2026) 48–55."},"scopus_import":"1","intvolume":" 172","corr_author":"1","month":"09"},{"project":[{"name":"The impact of deleterious mutations on small populations","_id":"34d33d68-11ca-11ed-8bc3-ec13763c0ca8","grant_number":"26293"}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1101/2025.04.09.647826"}],"oa":1,"article_processing_charge":"No","tmp":{"short":"CC BY-NC (4.0)","image":"/images/cc_by_nc.png","legal_code_url":"https://creativecommons.org/licenses/by-nc/4.0/legalcode","name":"Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)"},"fulldoi":"https://doi.org/10.1101/2025.04.09.647826","author":[{"orcid":"0000-0002-6246-1465","id":"4E6DC800-AE37-11E9-AC72-31CAE5697425","first_name":"Kseniia","last_name":"Khudiakova","full_name":"Khudiakova, Kseniia"},{"id":"4880FE40-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8548-5240","full_name":"Barton, Nicholas H","last_name":"Barton","first_name":"Nicholas H"},{"first_name":"Goran","last_name":"Arnqvist","full_name":"Arnqvist, Goran"}],"related_material":{"record":[{"status":"public","id":"21918","relation":"dissertation_contains"},{"id":"22998","status":"public","relation":"later_version"}]},"abstract":[{"text":"Balancing selection, a form of selection that maintains genetic diversity, is difficult to detect, and the importance of balancing selection for the maintenance of genetic variation may be larger than often assumed. We model the possibility that the diversity-promoting effects of balancing selection extend to other loci that show sign epistasis with a locus under balancing selection. Rather than focusing on overdominance, as was done in previous efforts, we explore the effects of negative frequency dependence and show that this has important effects on the conditions under which the diversity-promoting effect of epistasis can occur in diploids. Our results show that not only recombination rate but also the dominance of sign epistasis are key parameters that determine the maintenance of polymorphism beyond the locus under direct balancing selection. We suggest that the effect we explore may play a significant role, especially when balancing selection acts on major effect loci.","lang":"eng"}],"publication":"bioRxiv","_id":"21968","year":"2026","OA_place":"repository","user_id":"8b945eb4-e2f2-11eb-945a-df72226e66a9","date_published":"2026-04-23T00:00:00Z","OA_type":"green","date_updated":"2026-10-07T06:38:01Z","publication_status":"draft","status":"public","corr_author":"1","month":"04","citation":{"apa":"Khudiakova, K., Barton, N. H., & Arnqvist, G. (n.d.). Sign epistasis extends the effects of balancing selection on genetic diversity. bioRxiv. https://doi.org/10.1101/2025.04.09.647826","ama":"Khudiakova K, Barton NH, Arnqvist G. Sign epistasis extends the effects of balancing selection on genetic diversity. bioRxiv. doi:10.1101/2025.04.09.647826","chicago":"Khudiakova, Kseniia, Nicholas H Barton, and Goran Arnqvist. “Sign Epistasis Extends the Effects of Balancing Selection on Genetic Diversity.” BioRxiv, n.d. https://doi.org/10.1101/2025.04.09.647826.","ista":"Khudiakova K, Barton NH, Arnqvist G. Sign epistasis extends the effects of balancing selection on genetic diversity. bioRxiv, 10.1101/2025.04.09.647826.","mla":"Khudiakova, Kseniia, et al. “Sign Epistasis Extends the Effects of Balancing Selection on Genetic Diversity.” BioRxiv, doi:10.1101/2025.04.09.647826.","short":"K. Khudiakova, N.H. Barton, G. Arnqvist, BioRxiv (n.d.).","ieee":"K. Khudiakova, N. H. Barton, and G. Arnqvist, “Sign epistasis extends the effects of balancing selection on genetic diversity,” bioRxiv. ."},"oa_version":"Preprint","acknowledgement":"This work was funded by grants from the Swedish Research Council (2023-03730 to G.A.) and the DOC fellowship from the Austrian Academy of Science (26293 to K.K.).","day":"23","title":"Sign epistasis extends the effects of balancing selection on genetic diversity","department":[{"_id":"NiBa"},{"_id":"JaMa"}],"doi":"10.1101/2025.04.09.647826","date_created":"2026-06-09T12:26:11Z","type":"preprint","language":[{"iso":"eng"}]},{"title":"Core-hole excitation dynamics of one-dimensional ultracold trapped fermions","day":"22","publication_identifier":{"eissn":["2643-1564"]},"acknowledgement":"This work has been funded by the Cluster of Excellence “Advanced Imaging of Matter” of the Deutsche Forschungsgemeinschaft (DFG)—EXC 2056—Project No. 390715994. G.M.K. has received funding by the Austrian Science Fund (FWF) [Grant DOI: 10.55776/F1004]. For this work, the HPC-cluster Hummel-2 at University of Hamburg was used. The cluster was funded by Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)—498394658.","oa_version":"Published Version","language":[{"iso":"eng"}],"has_accepted_license":"1","type":"journal_article","supplementarymaterial":"yes","date_created":"2026-09-27T22:01:52Z","file":[{"file_id":"23067","file_name":"2026_PhysicalReviewResearch_BeckerA.pdf","relation":"main_file","file_size":2520954,"date_updated":"2026-10-07T06:55:14Z","access_level":"open_access","date_created":"2026-10-07T06:55:14Z","creator":"dernst","success":1,"content_type":"application/pdf","checksum":"7c886e062b11058f00c2049ba47fe3df"}],"department":[{"_id":"MiLe"}],"doi":"10.1103/njcx-z6np","arxiv":1,"file_date_updated":"2026-10-07T06:55:14Z","article_number":"033346","status":"public","ddc":["530"],"issue":"3","publisher":"American Physical Society","intvolume":" 8","scopus_import":"1","citation":{"chicago":"Becker, A., Georgios Koutentakis, and P Schmelcher. “Core-Hole Excitation Dynamics of One-Dimensional Ultracold Trapped Fermions.” Physical Review Research. American Physical Society, 2026. https://doi.org/10.1103/njcx-z6np.","apa":"Becker, A., Koutentakis, G., & Schmelcher, P. (2026). Core-hole excitation dynamics of one-dimensional ultracold trapped fermions. Physical Review Research. American Physical Society. https://doi.org/10.1103/njcx-z6np","ama":"Becker A, Koutentakis G, Schmelcher P. Core-hole excitation dynamics of one-dimensional ultracold trapped fermions. Physical Review Research. 2026;8(3). doi:10.1103/njcx-z6np","ista":"Becker A, Koutentakis G, Schmelcher P. 2026. Core-hole excitation dynamics of one-dimensional ultracold trapped fermions. Physical Review Research. 8(3), 033346.","mla":"Becker, A., et al. “Core-Hole Excitation Dynamics of One-Dimensional Ultracold Trapped Fermions.” Physical Review Research, vol. 8, no. 3, 033346, American Physical Society, 2026, doi:10.1103/njcx-z6np.","short":"A. Becker, G. Koutentakis, P. Schmelcher, Physical Review Research 8 (2026).","ieee":"A. Becker, G. Koutentakis, and P. Schmelcher, “Core-hole excitation dynamics of one-dimensional ultracold trapped fermions,” Physical Review Research, vol. 8, no. 3. American Physical Society, 2026."},"PlanS_conform":"1","month":"09","corr_author":"1","OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","researchdata_availability":"upon request","year":"2026","external_id":{"arxiv":["2604.23785"]},"_id":"23002","DOAJ_listed":"1","publication":"Physical Review Research","quality_controlled":"1","abstract":[{"text":"We investigate the nonequilibrium dynamics of core-hole excitations in a one-dimensional fermionic few-body system consisting of a spin-polarized Fermi bath coupled to a single heavy mobile impurity. The bath is initially prepared in a particle-hole configuration by emptying a selected bath single-particle orbital, while the impurity is displaced with respect to the center of the bath confinement potential. The quench dynamics are initialized by suddenly switching on the impurity-bath interaction. To resolve the resulting dynamics, we combine two complementary ab initio approaches, namely, the MultiLayer MultiConfiguration Time-Dependent Hartree method for mixtures and a multichannel Born-Oppenheimer framework. We show that the postquench response is governed by the interaction strength, impurity confinement, mass imbalance, and the location of the initially prepared hole within the Fermi sea. The density evolution and impurity center-of-mass motion reveal a competition between mixing and demixing of impurity and bath, while the von Neumann entropy demonstrates the buildup of pronounced many-body correlations. Most importantly, the occupation dynamics of the initially emptied orbital identifies deep core holes as substantially more robust against refilling than bulk or edge vacancies. Our results establish core-hole excitations as robust dynamical many-body features in trapped ultracold fermions and provide a controlled route toward probing orthogonality response, correlation buildup, and hole refilling in real time.","lang":"eng"}],"article_type":"original","author":[{"first_name":"A.","full_name":"Becker, A.","last_name":"Becker"},{"first_name":"Georgios","full_name":"Koutentakis, Georgios","last_name":"Koutentakis","id":"d7b23d3a-9e21-11ec-b482-f76739596b95"},{"last_name":"Schmelcher","full_name":"Schmelcher, P","first_name":"P"}],"publication_status":"published","date_updated":"2026-10-07T06:57:07Z","dataavailabilitystatement":"The data that support the findings of this article are not publicly available upon publication because it is not technically feasible and/or the cost of preparing, depositing, and hosting the data would be prohibitive within the terms of this research project. The data are available from the authors upon reasonable request.","OA_type":"gold","das_tickbox":"1","date_published":"2026-09-22T00:00:00Z","project":[{"name":"Coherent Optical Metrology Beyond Electric-Dipole-Allowed Transitions","_id":"7c040762-9f16-11ee-852c-dd79eeee4ab3","grant_number":"F100403"}],"volume":8,"fulldoi":"https://doi.org/10.1103/njcx-z6np","tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"article_processing_charge":"Yes","oa":1},{"OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","year":"2026","researchdata_availability":"yes","external_id":{"arxiv":["2603.06371"]},"_id":"23029","publication":"Physical Review B","quality_controlled":"1","abstract":[{"lang":"eng","text":"Josephson junction (JJ) chains combine the coherence of superconductivity with the controllability of microwave-frequency circuits, making them a powerful platform for circuit quantum electrodynamics. In this work, we consider a long JJ chain that effectively realizes a multimode cavity with nonlinear dispersion and additional multimode interactions. Individual modes appearing due to the finite size of the chain can be experimentally probed via microwave spectroscopy, both in equilibrium and in driven far-from-equilibrium settings. We study the role of multimode interactions in degrading internal coherence—observable as excess linewidth—in both equilibrium and driven regimes. Focusing on two-into-two mode scattering as the leading relaxation process, we classify the relevant scattering processes and derive their expected temperature- and frequency-scaling under equilibrium conditions. For experimentally relevant parameters, we show that the equilibrium decay rate is dominated by nonresonant processes, however, weakly driving a particular set of modes out of equilibrium enhances resonant scattering, leading to observable signatures in the distribution function and linewidth. Finally, in the strong nonequilibrium regime, we report a crossover to a qualitatively different nonequilibrium steady state."}],"article_type":"original","author":[{"id":"539e1e1a-e604-11ee-a1df-f02b018e5c8c","first_name":"Lucia","last_name":"Vigliotti","full_name":"Vigliotti, Lucia"},{"first_name":"Andrew P","full_name":"Higginbotham, Andrew P","last_name":"Higginbotham","orcid":"0000-0003-2607-2363","id":"4AD6785A-F248-11E8-B48F-1D18A9856A87"},{"id":"47809E7E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-2399-5827","last_name":"Serbyn","full_name":"Serbyn, Maksym","first_name":"Maksym"}],"publication_status":"published","date_updated":"2026-10-07T09:42:41Z","OA_type":"hybrid","dataavailabilitystatement":"The data and the source code that support the findings of this paper are openly available at: https://doi.org/10.5281/zenodo.19456426.","date_published":"2026-10-01T00:00:00Z","das_tickbox":"1","project":[{"_id":"34a7f947-11ca-11ed-8bc3-c5dc2bbaae25","grant_number":"F8609","name":"Center for Correlated Quantum Materials and Solid State Quantum Systems: Probing topology in circuits and quantum materials"}],"volume":114,"fulldoi":"https://doi.org/10.1103/cw3m-thsw","tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"article_processing_charge":"Yes (via OA deal)","oa":1,"title":"Plasmon decay and nonequilibrium steady states in Josephson junction chains","day":"01","publication_identifier":{"issn":["2469-9950"],"eissn":["2469-9969"]},"acknowledgement":"We acknowledge useful discussions with Anton Bubis, Vladimir Manucharyan, Alexander Mirlin, and Thomas Scaffidi. We are grateful to Eli Levenson-Falk and Alexander Mirlin for their feedback on the manuscript. This research was supported in part by Grant NSF PHY-2309135 to the Kavli Institute for Theoretical Physics (KITP), and by the Austrian Science Fund (FWF) SFB F86.","oa_version":"Published Version","language":[{"iso":"eng"}],"has_accepted_license":"1","type":"journal_article","supplementarymaterial":"yes","date_created":"2026-10-02T08:33:31Z","file":[{"file_id":"23069","file_name":"2026_PhysicalReviewB_Vigliotti.pdf","file_size":2531016,"relation":"main_file","date_updated":"2026-10-07T09:39:01Z","access_level":"open_access","date_created":"2026-10-07T09:39:01Z","creator":"dernst","success":1,"checksum":"95db327e1005564d09334763789ad7ae","content_type":"application/pdf"}],"department":[{"_id":"MaSe"},{"_id":"AnHi"}],"doi":"10.1103/cw3m-thsw","article_number":"194501","arxiv":1,"file_date_updated":"2026-10-07T09:39:01Z","status":"public","ddc":["530"],"issue":"19","publisher":"American Physical Society","intvolume":" 114","scopus_import":"1","citation":{"ista":"Vigliotti L, Higginbotham AP, Serbyn M. 2026. Plasmon decay and nonequilibrium steady states in Josephson junction chains. Physical Review B. 114(19), 194501.","apa":"Vigliotti, L., Higginbotham, A. P., & Serbyn, M. (2026). Plasmon decay and nonequilibrium steady states in Josephson junction chains. Physical Review B. American Physical Society. https://doi.org/10.1103/cw3m-thsw","chicago":"Vigliotti, Lucia, Andrew P Higginbotham, and Maksym Serbyn. “Plasmon Decay and Nonequilibrium Steady States in Josephson Junction Chains.” Physical Review B. American Physical Society, 2026. https://doi.org/10.1103/cw3m-thsw.","ama":"Vigliotti L, Higginbotham AP, Serbyn M. Plasmon decay and nonequilibrium steady states in Josephson junction chains. Physical Review B. 2026;114(19). doi:10.1103/cw3m-thsw","ieee":"L. Vigliotti, A. P. Higginbotham, and M. Serbyn, “Plasmon decay and nonequilibrium steady states in Josephson junction chains,” Physical Review B, vol. 114, no. 19. American Physical Society, 2026.","short":"L. Vigliotti, A.P. Higginbotham, M. Serbyn, Physical Review B 114 (2026).","mla":"Vigliotti, Lucia, et al. “Plasmon Decay and Nonequilibrium Steady States in Josephson Junction Chains.” Physical Review B, vol. 114, no. 19, 194501, American Physical Society, 2026, doi:10.1103/cw3m-thsw."},"PlanS_conform":"1","month":"10","corr_author":"1"},{"oa":1,"article_processing_charge":"Yes (via OA deal)","volume":69,"fulldoi":"https://doi.org/10.1002/rsa.70095","tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"project":[{"grant_number":"101076777","_id":"bd95085b-d553-11ed-ba76-e55d3349be45","name":"Randomness and structure in combinatorics"}],"das_tickbox":"0","date_published":"2026-09-01T00:00:00Z","date_updated":"2026-10-07T07:13:30Z","OA_type":"hybrid","publication_status":"published","abstract":[{"lang":"eng","text":"A famous conjecture by Itai and Zehavi states that, for every 𝑑\r\n-vertex-connected graph 𝐺\r\n and every vertex 𝑟\r\n in 𝐺\r\n, there are 𝑑\r\n spanning trees of 𝐺\r\n such that, for every vertex 𝑣\r\n in 𝐺 ∖{𝑟}\r\n, the paths between 𝑟\r\n and 𝑣\r\n in different trees are internally vertex-disjoint. We show that with high probability the Itai–Zehavi conjecture holds asymptotically for the Erdős–Rényi random graph 𝐺(𝑛,𝑝)\r\n when 𝑛𝑝 =𝜔(log𝑛)\r\n and for random regular graphs 𝐺(𝑛,𝑑)\r\n when 𝑑 =𝜔(log𝑛)\r\n. Moreover, we essentially confirm the conjecture up to a constant factor for sparser random regular graphs. This answers a question of Draganić and Krivelevich positively. Our proof makes use of recent developments on sprinkling techniques in random regular graphs."}],"quality_controlled":"1","publication":"Random Structures and Algorithms","author":[{"first_name":"Lawrence","full_name":"Hollom, Lawrence","last_name":"Hollom"},{"id":"9aa8388e-d003-11ee-8458-c4c1d7447977","first_name":"Lyuben","full_name":"Lichev, Lyuben","last_name":"Lichev"},{"full_name":"Mond, Adva","last_name":"Mond","first_name":"Adva"},{"first_name":"Julien","full_name":"Portier, Julien","last_name":"Portier"},{"first_name":"Yiting","last_name":"Wang","full_name":"Wang, Yiting","id":"1917d194-076e-11ed-97cd-837255f88785"}],"article_type":"original","year":"2026","researchdata_availability":"no","OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"23001","external_id":{"arxiv":["2506.23970"]},"month":"09","intvolume":" 69","PlanS_conform":"1","citation":{"mla":"Hollom, Lawrence, et al. “Approximate Itai–Zehavi Conjecture for Random Graphs.” Random Structures and Algorithms, vol. 69, no. 2, e70095, Wiley, 2026, doi:10.1002/rsa.70095.","ieee":"L. Hollom, L. Lichev, A. Mond, J. Portier, and Y. Wang, “Approximate Itai–Zehavi conjecture for random graphs,” Random Structures and Algorithms, vol. 69, no. 2. Wiley, 2026.","short":"L. Hollom, L. Lichev, A. Mond, J. Portier, Y. Wang, Random Structures and Algorithms 69 (2026).","chicago":"Hollom, Lawrence, Lyuben Lichev, Adva Mond, Julien Portier, and Yiting Wang. “Approximate Itai–Zehavi Conjecture for Random Graphs.” Random Structures and Algorithms. Wiley, 2026. https://doi.org/10.1002/rsa.70095.","ama":"Hollom L, Lichev L, Mond A, Portier J, Wang Y. Approximate Itai–Zehavi conjecture for random graphs. Random Structures and Algorithms. 2026;69(2). doi:10.1002/rsa.70095","apa":"Hollom, L., Lichev, L., Mond, A., Portier, J., & Wang, Y. (2026). Approximate Itai–Zehavi conjecture for random graphs. Random Structures and Algorithms. Wiley. https://doi.org/10.1002/rsa.70095","ista":"Hollom L, Lichev L, Mond A, Portier J, Wang Y. 2026. Approximate Itai–Zehavi conjecture for random graphs. Random Structures and Algorithms. 69(2), e70095."},"scopus_import":"1","publisher":"Wiley","status":"public","arxiv":1,"article_number":"e70095","file_date_updated":"2026-10-07T07:10:43Z","issue":"2","ddc":["500"],"department":[{"_id":"MaKw"},{"_id":"GradSch"}],"doi":"10.1002/rsa.70095","file":[{"access_level":"open_access","date_created":"2026-10-07T07:10:43Z","file_id":"23068","date_updated":"2026-10-07T07:10:43Z","file_size":457581,"relation":"main_file","file_name":"2026_RandomStructAlgorithms_Hollom.pdf","success":1,"creator":"dernst","checksum":"9a786460a47542f24576e947987e558a","content_type":"application/pdf"}],"has_accepted_license":"1","type":"journal_article","language":[{"iso":"eng"}],"date_created":"2026-09-27T22:01:52Z","supplementarymaterial":"yes","oa_version":"Published Version","day":"01","title":"Approximate Itai–Zehavi conjecture for random graphs","acknowledgement":"Hollom was supported by the Internal Graduate Studentship of Trinity College, Cambridge. Mond was supported by UK Research and Innovation grant MR/W007320/2. Wang was supported by the ERC Starting Grant “RANDSTRUCT” No. 101076777. Lichev was supported by the Austrian Science Fund (FWF) [10.55776/ESP624]. For open access purposes, the authors have applied a CC BY public copyright license to any author-accepted manuscript version arising from this submission. Open Access funding provided by Technische Universitat Wien.\r\n\r\nPart of this research was done during a visit of the fourth author to IST Austria. We thank IST Austria for its hospitality. We also thank the anonymous referees for their comments and suggestions. Open Access funding provided by Technische Universitat Wien. This work was supported by the European Research Council, UK Research and Innovation, the Austrian Science Fund, and Trinity College.","publication_identifier":{"eissn":["1098-2418"],"issn":["1042-9832"]}},{"date_updated":"2026-10-07T08:33:58Z","dataavailabilitystatement":"The data that support the findings of this study are available from thecorresponding author upon reasonable request.","das_tickbox":"1","date_published":"2026-09-15T00:00:00Z","publication_status":"epub_ahead","pmid":1,"article_type":"original","author":[{"first_name":"Qian","full_name":"Xue, Qian","last_name":"Xue"},{"first_name":"Jing","full_name":"Yu, Jing","last_name":"Yu"},{"first_name":"Juguo","last_name":"Dai","full_name":"Dai, Juguo"},{"full_name":"Yang, Linlin","last_name":"Yang","first_name":"Linlin"},{"first_name":"Xiaoyu","last_name":"Bi","full_name":"Bi, Xiaoyu"},{"last_name":"Ren","full_name":"Ren, Yuchuan","first_name":"Yuchuan"},{"last_name":"Zhang","full_name":"Zhang, Jia","first_name":"Jia"},{"full_name":"Qi, Xuede","last_name":"Qi","first_name":"Xuede"},{"first_name":"Yudi","last_name":"Wang","full_name":"Wang, Yudi"},{"last_name":"Xu","full_name":"Xu, Ying","first_name":"Ying"},{"first_name":"Jordi","full_name":"Arbiol, Jordi","last_name":"Arbiol"},{"last_name":"He","full_name":"He, Ren","first_name":"Ren","id":"366c4efa-f61c-11f0-808b-d12a4547ac69"},{"first_name":"Xueqiang","full_name":"Qi, Xueqiang","last_name":"Qi"},{"first_name":"Andreu","last_name":"Cabot","full_name":"Cabot, Andreu"}],"publication":"Angewandte Chemie International Edition","quality_controlled":"1","abstract":[{"lang":"eng","text":"Lattice strain engineering can regulate the electronic structure of electrocatalysts, but stabilizing distorted metastable phases remains challenging. Here, we report an N,N-dimethylformamide-assisted strategy for synthesizing metastable hexagonal close-packed (HCP) Ni nanoparticles with local lattice-spacing deviations reaching approximately 5.2%. Structural and spectroscopic analyses support a dilute interstitial-carbon-stabilized HCP Ni framework dominated by expanded metallic Ni─Ni coordination rather than ordered Ni3C. Carbon-associated perturbations inhibit structural relaxation and retain the distorted HCP framework. Operando x-ray absorption and infrared spectroscopies indicate the formation of a NiOOH-like working surface coupled to an HCP-derived subsurface framework, accompanied by potential-dependent changes in the interfacial hydrogen-bonding environment and urea-derived species. Calculations using idealized metallic models show that HCP lattice strain induces a Ni d-band upshift, anisotropic Ni─Ni bonding, and localized charge redistribution, modifying adsorption-energy trends for the urea oxidation reaction. The optimized HCP-Ni delivers an apparent steady-state Tafel slope of 26.95 mV dec−1, over twice the electrochemically active surface area-normalized activity of the face-centered cubic-containing controls, and approximately 98% apparent urea conversion after 22 h. It sustains current for over 120 h in three-electrode testing and enables over 400 h of urea-assisted zinc–air battery cycling. This work demonstrates dilute interstitial-carbon stabilization as a route to strained metastable electrocatalysts."}],"external_id":{"pmid":["42745541"]},"_id":"23004","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","researchdata_availability":"upon request","year":"2026","article_processing_charge":"No","fulldoi":"https://doi.org/10.1002/anie.2874510","department":[{"_id":"MaIb"}],"doi":"10.1002/anie.2874510","supplementarymaterial":"yes","date_created":"2026-09-27T22:01:53Z","language":[{"iso":"eng"}],"type":"journal_article","oa_version":"None","publication_identifier":{"issn":["1433-7851"],"eissn":["1521-3773"]},"acknowledgement":"Q. X., J. Y., X. B., Y. R., J. Z. and X. Q. thank the China Scholarship Council (CSC) for the scholarship support. These experiments were performed at BL22 CLAESS (proposal 20250340148) and BL01 MIRAS(proposal 20250340424, 20250370488) beamlines at ALBA Synchrotron with the collaboration of ALBA staff. The authors acknowledge the use of instrumentation as well as the technical advice provided by JEMCA. This research was financially supported by the Science and Technology Research Program of Chongqing Municipal Education Com-mission (No. KJZD-K202401110) and the Natural Science Foundation of Chongqing (No. CSTB2023NSCQ-MSX0378). ICN2 is supported by the Severo Ochoa program from Spanish MCIN / AEI (Grant No.: CEX2021-001214-S) and is funded by the CERCA Programme / Generalitat de Catalunya. ICN2 acknowledges funding from Generalitat de Catalunya2021SGR00457. The authors thank support from the project AMaDE(PID2023-149158OB-C43), funded by MCIN/ AEI/10.13039/501100011033/and by “ERDF A way of making Europe”, by the “European Union”.ICN2 acknowledges funding from Grant IU16-014206 (METCAM-FIB)funded by the European Union through the European Regional Devel-opment Fund (ERDF), with the support of the Ministry of Research and Universities, Generalitat de Catalunya. ICN2 is founding member ofe-DREAM.","title":"Dilute interstitial carbon stabilization of highly strained metastable HCP Nickel for enhanced electrocatalysis","day":"15","month":"09","corr_author":"1","scopus_import":"1","citation":{"ama":"Xue Q, Yu J, Dai J, et al. Dilute interstitial carbon stabilization of highly strained metastable HCP Nickel for enhanced electrocatalysis. Angewandte Chemie International Edition. 2026. doi:10.1002/anie.2874510","apa":"Xue, Q., Yu, J., Dai, J., Yang, L., Bi, X., Ren, Y., … Cabot, A. (2026). Dilute interstitial carbon stabilization of highly strained metastable HCP Nickel for enhanced electrocatalysis. Angewandte Chemie International Edition. Wiley. https://doi.org/10.1002/anie.2874510","chicago":"Xue, Qian, Jing Yu, Juguo Dai, Linlin Yang, Xiaoyu Bi, Yuchuan Ren, Jia Zhang, et al. “Dilute Interstitial Carbon Stabilization of Highly Strained Metastable HCP Nickel for Enhanced Electrocatalysis.” Angewandte Chemie International Edition. Wiley, 2026. https://doi.org/10.1002/anie.2874510.","ista":"Xue Q, Yu J, Dai J, Yang L, Bi X, Ren Y, Zhang J, Qi X, Wang Y, Xu Y, Arbiol J, He R, Qi X, Cabot A. 2026. Dilute interstitial carbon stabilization of highly strained metastable HCP Nickel for enhanced electrocatalysis. Angewandte Chemie International Edition., e2874510.","mla":"Xue, Qian, et al. “Dilute Interstitial Carbon Stabilization of Highly Strained Metastable HCP Nickel for Enhanced Electrocatalysis.” Angewandte Chemie International Edition, e2874510, Wiley, 2026, doi:10.1002/anie.2874510.","short":"Q. Xue, J. Yu, J. Dai, L. Yang, X. Bi, Y. Ren, J. Zhang, X. Qi, Y. Wang, Y. Xu, J. Arbiol, R. He, X. Qi, A. Cabot, Angewandte Chemie International Edition (2026).","ieee":"Q. Xue et al., “Dilute interstitial carbon stabilization of highly strained metastable HCP Nickel for enhanced electrocatalysis,” Angewandte Chemie International Edition. Wiley, 2026."},"keyword":["electrocatalysis","HCP nickel","interstitial carbon","kinetic trapping","lattice strain engineering","urea oxidation reaction"],"publisher":"Wiley","article_number":"e2874510","status":"public"},{"publisher":"American Physical Society","article_number":"L140103","arxiv":1,"status":"public","issue":"14","month":"09","intvolume":" 114","scopus_import":"1","citation":{"ama":"Bhakuni DS, Verdel R, Desaules J-YM, Serbyn M, Ljubotina M, Dalmonte M. Anomalously fast transport in nonintegrable lattice gauge theories. Physical Review B. 2026;114(14). doi:10.1103/3371-88bl","chicago":"Bhakuni, Devendra Singh, Roberto Verdel, Jean-Yves Marc Desaules, Maksym Serbyn, Marko Ljubotina, and Marcello Dalmonte. “Anomalously Fast Transport in Nonintegrable Lattice Gauge Theories.” Physical Review B. American Physical Society, 2026. https://doi.org/10.1103/3371-88bl.","apa":"Bhakuni, D. S., Verdel, R., Desaules, J.-Y. M., Serbyn, M., Ljubotina, M., & Dalmonte, M. (2026). Anomalously fast transport in nonintegrable lattice gauge theories. Physical Review B. American Physical Society. https://doi.org/10.1103/3371-88bl","ista":"Bhakuni DS, Verdel R, Desaules J-YM, Serbyn M, Ljubotina M, Dalmonte M. 2026. Anomalously fast transport in nonintegrable lattice gauge theories. Physical Review B. 114(14), L140103.","mla":"Bhakuni, Devendra Singh, et al. “Anomalously Fast Transport in Nonintegrable Lattice Gauge Theories.” Physical Review B, vol. 114, no. 14, L140103, American Physical Society, 2026, doi:10.1103/3371-88bl.","ieee":"D. S. Bhakuni, R. Verdel, J.-Y. M. Desaules, M. Serbyn, M. Ljubotina, and M. Dalmonte, “Anomalously fast transport in nonintegrable lattice gauge theories,” Physical Review B, vol. 114, no. 14. American Physical Society, 2026.","short":"D.S. Bhakuni, R. Verdel, J.-Y.M. Desaules, M. Serbyn, M. Ljubotina, M. Dalmonte, Physical Review B 114 (2026)."},"oa_version":"Preprint","title":"Anomalously fast transport in nonintegrable lattice gauge theories","day":"09","publication_identifier":{"issn":["2469-9950"],"eissn":["2469-9969"]},"acknowledgement":"We thank Riccardo Andreoni, Wouter\r\nBuijsman, Mario Collura, John Goold, Zala Lenarciˇ c,ˇ\r\nCristiano Muzzi, Romain Vasseur, and Marko Žnidaric for ˇ\r\ndiscussions. M.L. acknowledges support by the Deutsche\r\nForschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy – EXC-2111–\r\n390814868. M.L. and M.S. acknowledge support by the\r\nEuropean Research Council under the European Union’s\r\nHorizon 2020 research and innovation program (Grant Agreement No. 850899). J.-Y.D. acknowledges funding from the\r\nEuropean Union’s Horizon 2020 research and innovation\r\nprogramme under the Marie Skłodowska-Curie Grant Agreement No. 101034413. M.L., J.-Y.D., and M.S. acknowledge\r\nsupport by the Erwin Schrödinger International Institute\r\nfor Mathematics and Physics (ESI). M.D. was partly supported by the QUANTERA DYNAMITE PCI2022-132919,\r\nby the EU-Flagship programme Pasquans2, by the PNRR\r\nMUR Project PE0000023-NQSTI, and the PRIN programme\r\n(Project CoQuS). M.D. and R.V. were supported by the\r\nERC Consolidator Grant WaveNets. D.S.B. acknowledges\r\nthe CINECA Grant under the ISCRA-C (HP10C66VX2)\r\nprogram. The tensor network numerical simulations were performed with the ITensor library [94]. M.D. is also supported\r\nby the INFN Iniziativa specifica Quantum.","department":[{"_id":"MaSe"}],"doi":"10.1103/3371-88bl","language":[{"iso":"eng"}],"type":"journal_article","supplementarymaterial":"no","date_created":"2026-10-01T15:48:35Z","project":[{"_id":"23841C26-32DE-11EA-91FC-C7463DDC885E","grant_number":"850899","call_identifier":"H2020","name":"Non-Ergodic Quantum Matter: Universality, Dynamics and Control"},{"call_identifier":"H2020","name":"IST-BRIDGE: International postdoctoral program","grant_number":"101034413","_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c"}],"article_processing_charge":"No","oa":1,"main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2509.08889"}],"volume":114,"fulldoi":"https://doi.org/10.1103/3371-88bl","publication":"Physical Review B","quality_controlled":"1","abstract":[{"lang":"eng","text":"Kinetic constraints are generally expected to slow down dynamics in many-body systems, obstructing or even\r\ncompletely suppressing transport of conserved charges. Here, we show how gauge theories can defy this wisdom\r\nby yielding constrained models with faster-than-diffusive dynamics. We first show how, upon integrating out\r\nthe gauge fields, one-dimensional U(1) lattice gauge theories are exactly mapped onto XX models with nonlocal\r\nconstraints. This class of kinetically constrained models interpolates between free theories and highly constrained\r\nlocal fermionic models. We find that energy transport is superdiffusive over a broad parameter regime. Even\r\nmore drastically, spin transport exhibits ballistic behavior, albeit with anomalous finite-volume properties as a\r\nconsequence of gauge invariance. Our findings are relevant to current efforts in quantum simulations of gauge theory dynamics and anomalous hydrodynamics in closed quantum many-body systems."}],"author":[{"first_name":"Devendra Singh","last_name":"Bhakuni","full_name":"Bhakuni, Devendra Singh"},{"full_name":"Verdel, Roberto","last_name":"Verdel","first_name":"Roberto"},{"orcid":"0000-0002-3749-6375","id":"6c292945-a610-11ed-9eec-c3be1ad62a80","first_name":"Jean-Yves Marc","last_name":"Desaules","full_name":"Desaules, Jean-Yves Marc"},{"full_name":"Serbyn, Maksym","last_name":"Serbyn","first_name":"Maksym","id":"47809E7E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-2399-5827"},{"last_name":"Ljubotina","full_name":"Ljubotina, Marko","first_name":"Marko","id":"F75EE9BE-5C90-11EA-905D-16643DDC885E","orcid":"0000-0003-0038-7068"},{"first_name":"Marcello","full_name":"Dalmonte, Marcello","last_name":"Dalmonte"}],"article_type":"letter_note","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"repository","year":"2026","researchdata_availability":"no","external_id":{"arxiv":["2509.08889"]},"_id":"23027","ec_funded":1,"OA_type":"green","date_updated":"2026-10-07T09:29:50Z","dataavailabilitystatement":"There are no publicly available research\r\ndata or software supporting this manuscript. Requests for further information or data should be sent to the authors.","date_published":"2026-09-09T00:00:00Z","das_tickbox":"1","publication_status":"published"},{"date_updated":"2026-10-07T08:50:37Z","OA_type":"green","dataavailabilitystatement":"Bulk and single cell RNA-sequencing data generated in this study have been uploaded to the\r\nGene expression omnibus (GEO) with accessions GSE346330 and GSE346338 respectively. \r\nBulk RNA-seq data used to identify htCONDELs are publicly available with the following GEO\r\naccessions: GSE146481, GSE144825, and GSE232949. Splicing data from additional species\r\nwas downloaded from https://apps.kaessmannlab.org/alternative-splicing/ and GTEx v10 sQTL\r\ndata was downloaded from https://gtexportal.org/api/v2/association/dynsqtl.\r\nCode for this study is available at: https://github.com/astarr97/Splicing. Code to perform the\r\nalignment of RNA-seq data from hybrid cells is available at: https://github.com/banwang27/multi1216 celltypes. ","date_published":"2026-09-18T00:00:00Z","das_tickbox":"1","publication_status":"submitted","author":[{"first_name":"Alexander L.","full_name":"Starr, Alexander L.","last_name":"Starr"},{"orcid":"0000-0002-5615-5277","id":"68cb85a0-39f7-11eb-9559-9aaab4f6a247","first_name":"Ana","last_name":"Villalba Requena","full_name":"Villalba Requena, Ana"},{"full_name":"Rever, Jenna","last_name":"Rever","first_name":"Jenna"},{"id":"7f9e985d-7380-11f0-bf20-b4121a7bdcbc","full_name":"Chen, Yuwei","last_name":"Chen","first_name":"Yuwei"},{"last_name":"Pauler","full_name":"Pauler, Florian","first_name":"Florian","id":"48EA0138-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-7462-0048"},{"first_name":"Leslie","last_name":"Magtanong","full_name":"Magtanong, Leslie"},{"full_name":"Maxwell, Christopher A.","last_name":"Maxwell","first_name":"Christopher A."},{"id":"37B36620-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0003-2279-1061","last_name":"Hippenmeyer","full_name":"Hippenmeyer, Simon","first_name":"Simon"},{"last_name":"Fraser","full_name":"Fraser, Hunter B.","first_name":"Hunter B."}],"publication":"bioRxiv","abstract":[{"text":"Alternative splicing represents a major source of potential evolutionary novelty in protein sequence. Despite this, relatively few studies have investigated the functional impacts of human-specific alternative splicing. Here, we analyze RNA-sequencing data from nine iPSC-derived cell types and identify dozens of human transcriptomic conserved deletions (htCONDELs): evolutionary divergence in splicing that leads to the partial or full removal of conserved protein-coding sequence from the human transcriptome. We investigated one example in detail: an htCONDEL in the gene\r\nHMMR\r\n , which encodes a centrosomal protein that binds microtubules and regulates mitosis. We found that this htCONDEL, which produces a human-specific isoform lacking a conserved microtubule-binding domain, enables cells to flexibly divide with a broader range of mitotic spindle orientations\r\n in vitro\r\n . Introducing the human\r\n HMMR\r\n isoform into mice similarly alters the orientation of cell division in the developing neocortex and increases the production of outer radial glia-like cells, the expansion of which played an essential role in increasing human brain size. Combined with previous work implicating the same\r\n HMMR\r\n isoform in carcinoma progression, our results suggest that evolution of\r\nHMMR\r\n splicing in humans increased plasticity in cell division, potentially leading to tradeoffs between advantageous effects on brain development and deleterious effects on cancer risk later in life.","lang":"eng"}],"external_id":{"biorxivid":["10.64898/2026.09.16.752114"]},"_id":"23011","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"repository","researchdata_availability":"yes","year":"2026","main_file_link":[{"url":"https://doi.org/10.64898/2026.09.16.752114","open_access":"1"}],"article_processing_charge":"No","oa":1,"fulldoi":"https://doi.org/10.64898/2026.09.16.752114","project":[{"grant_number":"COE16","_id":"9e227eae-b037-11f1-b1e2-fb7da760c1dd","name":"Neuronal circuits in health and disease (Hippenmeyer)"}],"acknowledged_ssus":[{"_id":"Bio"},{"_id":"LifeSc"},{"_id":"PreCl"}],"department":[{"_id":"SiHi"}],"doi":"10.64898/2026.09.16.752114","supplementarymaterial":"yes","date_created":"2026-10-01T07:21:25Z","language":[{"iso":"eng"}],"type":"preprint","oa_version":"Preprint","acknowledgement":"We would like to acknowledge the MSKCC transgenic mouse core facility for generating\r\nhumanized mice, as well as Nancy Du, Xiang Chen, and other Du lab members for mouse\r\nbreeding and genotyping. This research was supported by the Scientific Service Units (SSU) of\r\nIST Austria through resources provided by the Imaging and Optics- (IOF), Lab Support- (LSF)\r\nand Preclinical Facilities (PCF). We would also like to thank Fee Wielath and Kerstin Feistel for\r\nhelpful discussions. Some figures were made with biorender. Work in the Fraser laboratory is supported by NIH grants R01HG012285 and R35GM156526.\r\nWork in the Hippenmeyer laboratory is supported by ISTA institutional funds and FWF Cluster of\r\nExcellence COE16 (10.55776/COE16) to S.H. Work in the Maxwell laboratory is supported by\r\nthe National Sciences and Engineering Research Council of Canada (NSERC, RGPIN-2019-\r\n06215 and 2025-05766) and the Canadian Institutes of Health Research (F24-00975). J.R. is\r\nsupported by a Canada Graduate Research Scholarship-Doctoral (612468 - 2026) from\r\nNSERC. A.L.S. is supported by the FutureHouse postdoctoral fellowship program and the Kavli\r\nFoundation. ","title":"A human transcriptomic deletion links cortical expansion and cancer","day":"18","biorxivid":1,"month":"09","corr_author":"1","citation":{"ista":"Starr AL, Villalba Requena A, Rever J, Chen Y, Pauler F, Magtanong L, Maxwell CA, Hippenmeyer S, Fraser HB. A human transcriptomic deletion links cortical expansion and cancer. bioRxiv, 10.64898/2026.09.16.752114.","ama":"Starr AL, Villalba Requena A, Rever J, et al. A human transcriptomic deletion links cortical expansion and cancer. bioRxiv. doi:10.64898/2026.09.16.752114","apa":"Starr, A. L., Villalba Requena, A., Rever, J., Chen, Y., Pauler, F., Magtanong, L., … Fraser, H. B. (n.d.). A human transcriptomic deletion links cortical expansion and cancer. bioRxiv. https://doi.org/10.64898/2026.09.16.752114","chicago":"Starr, Alexander L., Ana Villalba Requena, Jenna Rever, Yuwei Chen, Florian Pauler, Leslie Magtanong, Christopher A. Maxwell, Simon Hippenmeyer, and Hunter B. Fraser. “A Human Transcriptomic Deletion Links Cortical Expansion and Cancer.” BioRxiv, n.d. https://doi.org/10.64898/2026.09.16.752114.","short":"A.L. Starr, A. Villalba Requena, J. Rever, Y. Chen, F. Pauler, L. Magtanong, C.A. Maxwell, S. Hippenmeyer, H.B. Fraser, BioRxiv (n.d.).","ieee":"A. L. Starr et al., “A human transcriptomic deletion links cortical expansion and cancer,” bioRxiv. .","mla":"Starr, Alexander L., et al. “A Human Transcriptomic Deletion Links Cortical Expansion and Cancer.” BioRxiv, doi:10.64898/2026.09.16.752114."},"status":"public"},{"main_file_link":[{"url":"https://doi.org/10.1101/2025.04.28.651046","open_access":"1"}],"oa":1,"article_processing_charge":"No","fulldoi":"https://doi.org/10.1016/j.neuron.2026.08.015","article_type":"original","author":[{"first_name":"Rachel A.","last_name":"Essner","full_name":"Essner, Rachel A."},{"full_name":"Ruda, Kiersten","last_name":"Ruda","first_name":"Kiersten"},{"last_name":"Choh","full_name":"Choh, Hannah J.","first_name":"Hannah J."},{"first_name":"Hakan","last_name":"Kücükdereli","full_name":"Kücükdereli, Hakan","id":"5d5f6ea4-ef9e-11f0-a10a-85e12a3552af"},{"first_name":"Oren","last_name":"Amsalem","full_name":"Amsalem, Oren"},{"full_name":"Edelhaus, Julia","last_name":"Edelhaus","first_name":"Julia"},{"first_name":"Gracesenia","full_name":"Chahyadinata, Gracesenia","last_name":"Chahyadinata"},{"last_name":"Grødem","full_name":"Grødem, Sverre","first_name":"Sverre"},{"last_name":"Lensjø","full_name":"Lensjø, Kristian K.","first_name":"Kristian K."},{"first_name":"Teresa E.","full_name":"Lever, Teresa E.","last_name":"Lever"},{"first_name":"Mark L.","last_name":"Andermann","full_name":"Andermann, Mark L."}],"abstract":[{"text":"The peripheral neural pathways that relay oral and post-ingestive chemo- and mechanosensory signals to the brain during food consumption are increasingly well understood. Far less is known about how these and other body signals are integrated and organized in the brainstem lateral parabrachial nucleus (LPBN), a key interoceptive sensory hub. We established methods for dense calcium imaging of 100s of neurons from mouse LPBN. Food consumption drove a seconds-long wave of activity across LPBN, with dynamics mirroring the movement of food through the upper gastrointestinal tract as observed using X-ray videofluoroscopy. By imaging the same neurons across days, we found that spatially clustered subsets of neurons encoded oral signals, stomach filling, visceral malaise, arousal, and/or body movement. Moreover, only certain subsets were modulated by cortical input. Together, these experiments establish a platform for understanding how peripheral and central interoceptive signals are integrated in the brainstem to guide behavior.","lang":"eng"}],"publication":"Neuron","quality_controlled":"1","_id":"23003","external_id":{"biorxivid":["10.1101/2025.04.28.651046"],"pmid":["42753729"]},"year":"2026","researchdata_availability":"yes","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"repository","das_tickbox":"1","date_published":"2026-09-17T00:00:00Z","dataavailabilitystatement":"This study did not generate any new, unique reagents.Single-neuron calcium imaging traces from all experiments have been deposited at Mendeley Data at 10.17632/wh6f8xt64y.1 and are publicly available as of the date of publication. Raw two-photon calcium imaging and fiber photometry datasets are available from the lead contact upon request.\r\nAll original code is deposited on GitHub (https://github.com/kmruda/PBN_sensing_body_signals) as well as Zenodo at 10.5281/zenodo.21926666 and is publicly available as of the date of publication.\r\nAny additional information required to reanalyze the data is available upon request from the lead contact, Mark L. Andermann (manderma@bidmc.harvard.edu).","date_updated":"2026-10-07T08:40:54Z","OA_type":"green","pmid":1,"publication_status":"epub_ahead","publisher":"Cell Press","status":"public","month":"09","citation":{"ista":"Essner RA, Ruda K, Choh HJ, Kücükdereli H, Amsalem O, Edelhaus J, Chahyadinata G, Grødem S, Lensjø KK, Lever TE, Andermann ML. 2026. Brainstem sensing of multiple body signals during food consumption. Neuron.","apa":"Essner, R. A., Ruda, K., Choh, H. J., Kücükdereli, H., Amsalem, O., Edelhaus, J., … Andermann, M. L. (2026). Brainstem sensing of multiple body signals during food consumption. Neuron. Cell Press. https://doi.org/10.1016/j.neuron.2026.08.015","chicago":"Essner, Rachel A., Kiersten Ruda, Hannah J. Choh, Hakan Kücükdereli, Oren Amsalem, Julia Edelhaus, Gracesenia Chahyadinata, et al. “Brainstem Sensing of Multiple Body Signals during Food Consumption.” Neuron. Cell Press, 2026. https://doi.org/10.1016/j.neuron.2026.08.015.","ama":"Essner RA, Ruda K, Choh HJ, et al. Brainstem sensing of multiple body signals during food consumption. Neuron. 2026. doi:10.1016/j.neuron.2026.08.015","ieee":"R. A. Essner et al., “Brainstem sensing of multiple body signals during food consumption,” Neuron. Cell Press, 2026.","short":"R.A. Essner, K. Ruda, H.J. Choh, H. Kücükdereli, O. Amsalem, J. Edelhaus, G. Chahyadinata, S. Grødem, K.K. Lensjø, T.E. Lever, M.L. Andermann, Neuron (2026).","mla":"Essner, Rachel A., et al. “Brainstem Sensing of Multiple Body Signals during Food Consumption.” Neuron, Cell Press, 2026, doi:10.1016/j.neuron.2026.08.015."},"scopus_import":"1","oa_version":"Preprint","acknowledgement":"We thank S. Zhang, K. Evans, C. Massengill, J.S. Alvarado, and members of the Andermann lab for helpful discussion and feedback. We thank J. Mathai for the use of the LabScope for fluoroscopy experiments. We thank J. Fernando, P. Prasad, D. Guarino, J. DeBolt, Z. Stolberg, and A. Pinilla for animal husbandry and other technical assistance. Authors were supported by NSF GRFP DGE1745303, NIH F31DC020631, and NIH T32DK007516 (R.A.E.); NIH F32DK135247 and NIH T32DK007516 (K.R.); the BBRF Young Investigator Grant (H.K.); the Research Council of Norway Grant 250259 (S.G. and K.K.L.); and the Pew Innovation Fund, the McKnight Foundation, the Klarman Family Foundation, the Harvard Brain Science Initiative Bipolar Disorder Seed Grant supported by Kent and Liz Dauten, the NIH (DP1AT010971, DP1DK139958, and P01HL149630), a gift from Paul Weisman, and the K. Lisa Yang Brain-Body Center (M.L.A.).","publication_identifier":{"issn":["0896-6273"],"eissn":["1097-4199"]},"day":"17","biorxivid":1,"title":"Brainstem sensing of multiple body signals during food consumption","doi":"10.1016/j.neuron.2026.08.015","department":[{"_id":"MaJö"}],"date_created":"2026-09-27T22:01:53Z","supplementarymaterial":"yes","type":"journal_article","language":[{"iso":"eng"}]},{"volume":393,"fulldoi":"https://doi.org/10.1126/science.ael0758","article_processing_charge":"No","pmid":1,"publication_status":"published","date_published":"2026-09-17T00:00:00Z","das_tickbox":"0","OA_type":"closed access","date_updated":"2026-10-07T08:10:18Z","_id":"23000","external_id":{"pmid":["42752153"]},"researchdata_availability":"no","year":"2026","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","author":[{"id":"96aecfa5-8931-11ee-af30-aa6a5d6eee0e","orcid":"0000-0003-0456-0753","full_name":"Bravo, Jack Peter Kelly","last_name":"Bravo","first_name":"Jack Peter Kelly"}],"article_type":"comment","abstract":[{"lang":"eng","text":"Ancient viral warfare could be at the root of modern class 1 CRISPR bacterial defense systems"}],"publication":"Science","quality_controlled":"1","citation":{"ista":"Bravo JPK. 2026. A viral origin for RNA-guided immunity. Science. 393(6817), 1187–1188.","apa":"Bravo, J. P. K. (2026). A viral origin for RNA-guided immunity. Science. AAAS. https://doi.org/10.1126/science.ael0758","ama":"Bravo JPK. A viral origin for RNA-guided immunity. Science. 2026;393(6817):1187-1188. doi:10.1126/science.ael0758","chicago":"Bravo, Jack Peter Kelly. “A Viral Origin for RNA-Guided Immunity.” Science. AAAS, 2026. https://doi.org/10.1126/science.ael0758.","short":"J.P.K. Bravo, Science 393 (2026) 1187–1188.","ieee":"J. P. K. Bravo, “A viral origin for RNA-guided immunity,” Science, vol. 393, no. 6817. AAAS, pp. 1187–1188, 2026.","mla":"Bravo, Jack Peter Kelly. “A Viral Origin for RNA-Guided Immunity.” Science, vol. 393, no. 6817, AAAS, 2026, pp. 1187–88, doi:10.1126/science.ael0758."},"scopus_import":"1","intvolume":" 393","corr_author":"1","month":"09","issue":"6817","status":"public","publisher":"AAAS","date_created":"2026-09-27T22:01:52Z","supplementarymaterial":"no","type":"journal_article","language":[{"iso":"eng"}],"department":[{"_id":"JaBr"}],"doi":"10.1126/science.ael0758","publication_identifier":{"eissn":["1095-9203"],"issn":["0036-8075"]},"day":"17","page":"1187-1188","title":"A viral origin for RNA-guided immunity","oa_version":"None"},{"OA_type":"gold","date_updated":"2026-10-07T10:33:29Z","das_tickbox":"0","date_published":"2026-09-10T00:00:00Z","publication_status":"published","author":[{"first_name":"Yilun","full_name":"Ma, Yilun","last_name":"Ma"},{"first_name":"Jenny E.","last_name":"Greene","full_name":"Greene, Jenny E."},{"full_name":"Volonteri, Marta","last_name":"Volonteri","first_name":"Marta"},{"last_name":"Goulding","full_name":"Goulding, Andy D.","first_name":"Andy D."},{"first_name":"David J.","full_name":"Setton, David J.","last_name":"Setton"},{"last_name":"Annunziatella","full_name":"Annunziatella, Marianna","first_name":"Marianna"},{"first_name":"Eiichi","last_name":"Egami","full_name":"Egami, Eiichi"},{"last_name":"Fan","full_name":"Fan, Xiaohui","first_name":"Xiaohui"},{"last_name":"Kokorev","full_name":"Kokorev, Vasily","first_name":"Vasily"},{"first_name":"Ivo","last_name":"Labbe","full_name":"Labbe, Ivo"},{"last_name":"Lin","full_name":"Lin, Xiaojing","first_name":"Xiaojing"},{"first_name":"Danilo","full_name":"Marchesini, Danilo","last_name":"Marchesini"},{"last_name":"Matthee","full_name":"Matthee, Jorryt J","first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X"},{"first_name":"Themiya","last_name":"Nanayakkara","full_name":"Nanayakkara, Themiya"},{"first_name":"Luke","last_name":"Robbins","full_name":"Robbins, Luke"},{"full_name":"Sajina, Anna","last_name":"Sajina","first_name":"Anna"},{"first_name":"Marcin","last_name":"Sawicki","full_name":"Sawicki, Marcin"}],"article_type":"original","publication":"The Astrophysical Journal Letters","quality_controlled":"1","abstract":[{"lang":"eng","text":"One of the most surprising results of early James Webb Space Telescope (JWST) observations is the discovery of an abundance of red, compact, broad-line objects dubbed “little red dots” (LRDs) at z > 4. Their spatial density (∼10−4–10−5 cMpc−3) is 100 times more abundant than UV-selected quasars at that redshift if one extrapolates the quasar luminosity function (QLF) down to the LRD regime. However, whether LRDs dominate black hole accretion at quasar-like luminosities (Lbol ≳ 1045−46 erg s−1) remains unanswered, as probing the bright end of the LRD luminosity function requires a much larger area than that which is able to be surveyed by JWST. In this work, we present our search for the brightest LRDs (K < 23.7) at 4.5 < z < 4.9 using wide-area multiwavelength imaging surveys from the near-UV to the infrared bands. With over 15 deg2 of sky coverage, we only identify one single LRD candidate at zphot ≈ 4.6, which translates into a spatial density of n(M5100 < −23.5) ≈ 10−8 cMpc−3—this is nearly 10 times less abundant than the UV-selected quasars at similar optical luminosity. When combined with the LRD sample identified by JWST at the same redshift range, we find a sharp cutoff in the optical luminosity function at λL5100 ≈ 2.2 × 1044 erg s−1, while the quasar luminosity function (QLF) turnover occurs at ≳20 times higher luminosity. We therefore confirm the exclusively low-luminosity nature of LRDs, ruling out that LRDs are the counterparts of quasars. Furthermore, we speculate that, if the shape of the luminosity function holds up, it points to LRDs being powered by low-mass black holes with a narrow range of Eddington-level accretion rates."}],"external_id":{"arxiv":["2509.02662"]},"DOAJ_listed":"1","_id":"23042","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"publisher","researchdata_availability":"no","year":"2026","oa":1,"article_processing_charge":"Yes","tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"volume":1008,"fulldoi":"https://doi.org/10.3847/2041-8213/aea071","file":[{"date_created":"2026-10-07T10:30:30Z","access_level":"open_access","file_id":"23071","file_name":"2026_AstrophysicalJourLetters_Ma.pdf","date_updated":"2026-10-07T10:30:30Z","relation":"main_file","file_size":2895298,"creator":"dernst","success":1,"checksum":"1d17f212c0ef64b99b5947591d61216f","content_type":"application/pdf"}],"department":[{"_id":"JoMa"}],"doi":"10.3847/2041-8213/aea071","supplementarymaterial":"yes","date_created":"2026-10-04T22:01:53Z","language":[{"iso":"eng"}],"type":"journal_article","has_accepted_license":"1","oa_version":"Published Version","publication_identifier":{"eissn":["2041-8213"],"issn":["2041-8205"]},"acknowledgement":"Y.M. thanks Hanpu Liu and Minghao Guo for useful discussion. Y.M. is also grateful for the suggestions from Xiaowei Ou and Jiaxuan Li on figure improvement. M.A. acknowledges support by the National Aeronautics and Space Administration (NASA) through an award (RSA 1628138) issued by JPL/Caltech. D.M., L.R., and A.S. acknowledge support by NASA under award No. 80NSSC21K0630, issued through the Astrophysics Data Analysis Program (ADAP).\r\n\r\nThe Hyper Suprime-Cam (HSC) collaboration includes the astronomical communities of Japan, Taiwan, and Princeton University. The HSC instrumentation and software were developed by the National Astronomical Observatory of Japan (NAOJ), the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), the University of Tokyo, the High Energy Accelerator Research Organization (KEK), the Academia Sinica Institute for Astronomy and Astrophysics in Taiwan (ASIAA), and Princeton University. Funding was contributed by the FIRST program from the Japanese Cabinet Office, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), the Japan Society for the Promotion of Science (JSPS), Japan Science and Technology Agency (JST), the Toray Science Foundation, NAOJ, Kavli IPMU, KEK, ASIAA, and Princeton University.\r\n\r\nThis Letter is based in part on data collected at the Subaru Telescope and retrieved from the HSC data archive system, which is operated by Subaru Telescope and Astronomy Data Center (ADC) at NAOJ. Data analysis was in part carried out with the cooperation of Center for Computational Astrophysics (CfCA) at NAOJ. We are honored and grateful for the opportunity of observing the Universe from Maunakea, which has the cultural, historical, and natural significance in Hawai‘i.\r\n\r\nThis Letter makes use of software developed for Vera C. Rubin Observatory (M. Juric et al. 2017; J. Bosch et al. 2019; Ž. Ivezić et al. 2019). We thank the Rubin Observatory for making their code available as free software at http://pipelines.lsst.io/.\r\n\r\nThis Letter also partially makes use of the CLAUDS data (M. Sawicki et al. 2019), whose data products can be accessed from https://www.clauds.net.","title":"No luminous Little Red Dots: A sharp cutoff in their luminosity function","day":"10","month":"09","scopus_import":"1","citation":{"ieee":"Y. Ma et al., “No luminous Little Red Dots: A sharp cutoff in their luminosity function,” The Astrophysical Journal Letters, vol. 1008, no. 2. IOP Publishing, 2026.","short":"Y. Ma, J.E. Greene, M. Volonteri, A.D. Goulding, D.J. Setton, M. Annunziatella, E. Egami, X. Fan, V. Kokorev, I. Labbe, X. Lin, D. Marchesini, J.J. Matthee, T. Nanayakkara, L. Robbins, A. Sajina, M. Sawicki, The Astrophysical Journal Letters 1008 (2026).","mla":"Ma, Yilun, et al. “No Luminous Little Red Dots: A Sharp Cutoff in Their Luminosity Function.” The Astrophysical Journal Letters, vol. 1008, no. 2, L64, IOP Publishing, 2026, doi:10.3847/2041-8213/aea071.","ista":"Ma Y, Greene JE, Volonteri M, Goulding AD, Setton DJ, Annunziatella M, Egami E, Fan X, Kokorev V, Labbe I, Lin X, Marchesini D, Matthee JJ, Nanayakkara T, Robbins L, Sajina A, Sawicki M. 2026. No luminous Little Red Dots: A sharp cutoff in their luminosity function. The Astrophysical Journal Letters. 1008(2), L64.","ama":"Ma Y, Greene JE, Volonteri M, et al. No luminous Little Red Dots: A sharp cutoff in their luminosity function. The Astrophysical Journal Letters. 2026;1008(2). doi:10.3847/2041-8213/aea071","apa":"Ma, Y., Greene, J. E., Volonteri, M., Goulding, A. D., Setton, D. J., Annunziatella, M., … Sawicki, M. (2026). No luminous Little Red Dots: A sharp cutoff in their luminosity function. The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/aea071","chicago":"Ma, Yilun, Jenny E. Greene, Marta Volonteri, Andy D. Goulding, David J. Setton, Marianna Annunziatella, Eiichi Egami, et al. “No Luminous Little Red Dots: A Sharp Cutoff in Their Luminosity Function.” The Astrophysical Journal Letters. IOP Publishing, 2026. https://doi.org/10.3847/2041-8213/aea071."},"PlanS_conform":"1","intvolume":" 1008","publisher":"IOP Publishing","ddc":["520"],"issue":"2","article_number":"L64","file_date_updated":"2026-10-07T10:30:30Z","arxiv":1,"status":"public"},{"oa_version":"Preprint","title":"Probing cosmology through higher-order CMB lensing statistics","day":"16","publication_identifier":{"eissn":["2470-0029"],"issn":["2470-0010"]},"acknowledgement":"We thank Will Coulton, Adrian Bayer, and Max Lee for useful discussions. S. F. C., J. C. H., and Z. H. acknowledge support from NASA Grant No. 80NSSC24K1093 [ATP]. J. C. H. also acknowledges support from NASA Grant No. 80NSSC23K0463 [ADAP]. J. C. H. thanks the Kavli Institute for Theoretical Physics (KITP) for hospitality during the completion of this work; this research was supported in part by Grant No. NSF PHY-2309135 to the KITP. The authors also acknowledge the Texas Advanced Computing Center (TACC) at The University of Texas at Austin for providing computational resources that have contributed to the research results reported within this paper. We acknowledge computing resources from Columbia University’s Shared Research Computing Facility project, which is supported by NIH Research Facility Improvement Grant No. 1G20RR030893-01, and associated funds from the New York State Empire State Development, Division of Science Technology and Innovation (NYSTAR) Contract No. C090171, both awarded April 15, 2010. This is not an official Simons Observatory collaboration paper.","doi":"10.1103/CLVJ-GL8P","department":[{"_id":"ZoHa"}],"language":[{"iso":"eng"}],"type":"journal_article","supplementarymaterial":"no","date_created":"2026-10-04T22:01:56Z","publisher":"American Physical Society","arxiv":1,"article_number":"023535","status":"public","issue":"2","month":"07","intvolume":" 114","scopus_import":"1","citation":{"mla":"Chen, Shu Fan, et al. “Probing Cosmology through Higher-Order CMB Lensing Statistics.” Physical Review D, vol. 114, no. 2, 023535, American Physical Society, 2026, doi:10.1103/CLVJ-GL8P.","short":"S.F. Chen, J.C. Hill, Z. Haiman, Physical Review D 114 (2026).","ieee":"S. F. Chen, J. C. Hill, and Z. Haiman, “Probing cosmology through higher-order CMB lensing statistics,” Physical Review D, vol. 114, no. 2. American Physical Society, 2026.","ama":"Chen SF, Hill JC, Haiman Z. Probing cosmology through higher-order CMB lensing statistics. Physical Review D. 2026;114(2). doi:10.1103/CLVJ-GL8P","apa":"Chen, S. F., Hill, J. C., & Haiman, Z. (2026). Probing cosmology through higher-order CMB lensing statistics. Physical Review D. American Physical Society. https://doi.org/10.1103/CLVJ-GL8P","chicago":"Chen, Shu Fan, J. Colin Hill, and Zoltán Haiman. “Probing Cosmology through Higher-Order CMB Lensing Statistics.” Physical Review D. American Physical Society, 2026. https://doi.org/10.1103/CLVJ-GL8P.","ista":"Chen SF, Hill JC, Haiman Z. 2026. Probing cosmology through higher-order CMB lensing statistics. Physical Review D. 114(2), 023535."},"publication":"Physical Review D","quality_controlled":"1","abstract":[{"text":"We investigate the cosmological information in higher-order statistics of the cosmic microwave background (CMB) lensing convergence field for a near-term experiment with noise properties similar to the Simons Observatory (SO). Using a fully field-level forward-modeling pipeline based on ray-traced simulations from the massivenus suite and realistic SO-like CMB lensing reconstruction, we naturally include nonlinear structure formation, post-Born effects, and higher-order reconstruction noise. We measure several non-Gaussian statistics, including Minkowski functionals, peak and minima counts, moments, and wavelet-scattering coefficients. We train Gaussian-process emulators to model each statistic’s dependence on the matter density fraction Ω𝑚, the scalar power spectrum amplitude 𝐴𝑠, and the neutrino mass sum 𝑀𝜈. We quantify the relative information gain these statistics provide beyond the lensing power spectrum and identify which are most robust to reconstruction noise. We find that morphology-based statistics, particularly Minkowski functionals and peak/minima counts, offer significant complementary constraining power: combining all non-Gaussian statistics with the power spectrum yields reductions of 40% and 38% in the marginalized uncertainties on Ω𝑚 and 𝐴𝑠, respectively, and a 70% reduction in the one-sided uncertainty on 𝑀𝜈. These gains remain non-negligible even when the power spectrum is extended to larger scales and combined with primary CMB and BAO data, with Minkowski functionals providing an additional 11% improvement in 𝜎(𝑀𝜈) and 35% in 𝜎(Ω𝑚) beyond the extended power spectrum. By contrast, moments and wavelet-scattering coefficients provide more limited gains at SO noise levels. Our results highlight the potential of non-Gaussian statistics to enhance cosmological constraints from SO and future CMB surveys.","lang":"eng"}],"author":[{"first_name":"Shu Fan","last_name":"Chen","full_name":"Chen, Shu Fan"},{"last_name":"Hill","full_name":"Hill, J. Colin","first_name":"J. Colin"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","orcid":"0000-0003-3633-5403","full_name":"Haiman, Zoltán","last_name":"Haiman","first_name":"Zoltán"}],"article_type":"original","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"repository","year":"2026","researchdata_availability":"yes","external_id":{"arxiv":["2603.12335"]},"_id":"23054","date_updated":"2026-10-07T13:02:05Z","dataavailabilitystatement":"The data that support the findings of this article are openly available [https://doi.org/10.1103/PhysRevD.98.023535].","OA_type":"green","date_published":"2026-07-16T00:00:00Z","das_tickbox":"1","publication_status":"published","oa":1,"article_processing_charge":"No","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2603.12335","open_access":"1"}],"fulldoi":"https://doi.org/10.1103/CLVJ-GL8P","volume":114},{"oa_version":"Published Version","acknowledgement":"This project has received funding from the European Research Council (ERC) under \r\nthe European Union’s Horizon 2020 research and innovation programme (Grant \r\nagreements No. 949120 and No. 805041). This research was supported by the \r\nScientific Service Units of The Institute of Science and Technology Austria (ISTA) \r\nthrough resources provided by the Miba Machine Shop and the Imaging & Optics \r\nFacility. ","publication_identifier":{"issn":["2663-337X"]},"day":"02","title":"Microscale electrical behavior of highly charged individual aerosol particles using optical tweezers","page":"88","doi":"10.15479/AT-ISTA-23033","department":[{"_id":"GradSch"},{"_id":"ScWa"},{"_id":"CaMu"}],"file":[{"content_type":"application/vnd.openxmlformats-officedocument.wordprocessingml.document","checksum":"4c294f690c2eabdbb0f9215fb6e75fa0","creator":"astoelln","file_name":"2026_Stoellner_Andrea_Thesis.docx","date_updated":"2026-10-02T13:31:50Z","file_size":8706369,"relation":"source_file","file_id":"23040","date_created":"2026-10-02T13:31:50Z","access_level":"closed"},{"date_created":"2026-10-05T12:02:57Z","access_level":"closed","relation":"main_file","file_size":4131543,"date_updated":"2026-10-05T12:06:04Z","file_name":"2026_Stoellner_Andrea_Thesis.pdf","file_id":"23059","embargo_to":"open_access","content_type":"application/pdf","checksum":"410066c4b83297091699d5c324676d9e","embargo":"2027-04-05","creator":"cchlebak"}],"date_created":"2026-10-02T10:03:57Z","alternative_title":["ISTA Thesis"],"type":"dissertation","has_accepted_license":"1","language":[{"iso":"eng"}],"publisher":"Institute of Science and Technology Austria","keyword":["aerosol physics","electrostatics","optics","optical tweezers","atmospheric electricity"],"ddc":["530"],"status":"public","file_date_updated":"2026-10-05T12:06:04Z","corr_author":"1","month":"10","degree_awarded":"PhD","citation":{"ama":"Stöllner A. Microscale electrical behavior of highly charged individual aerosol particles using optical tweezers. 2026. doi:10.15479/AT-ISTA-23033","apa":"Stöllner, A. (2026). Microscale electrical behavior of highly charged individual aerosol particles using optical tweezers. Institute of Science and Technology Austria. https://doi.org/10.15479/AT-ISTA-23033","chicago":"Stöllner, Andrea. “Microscale Electrical Behavior of Highly Charged Individual Aerosol Particles Using Optical Tweezers.” Institute of Science and Technology Austria, 2026. https://doi.org/10.15479/AT-ISTA-23033.","ista":"Stöllner A. 2026. Microscale electrical behavior of highly charged individual aerosol particles using optical tweezers. Institute of Science and Technology Austria.","mla":"Stöllner, Andrea. Microscale Electrical Behavior of Highly Charged Individual Aerosol Particles Using Optical Tweezers. Institute of Science and Technology Austria, 2026, doi:10.15479/AT-ISTA-23033.","ieee":"A. Stöllner, “Microscale electrical behavior of highly charged individual aerosol particles using optical tweezers,” Institute of Science and Technology Austria, 2026.","short":"A. Stöllner, Microscale Electrical Behavior of Highly Charged Individual Aerosol Particles Using Optical Tweezers, Institute of Science and Technology Austria, 2026."},"doi_confirm":"1","author":[{"id":"4bdcf7f6-eb97-11eb-a6c2-9981bbdc3bed","orcid":"0000-0002-0464-8440","full_name":"Stöllner, Andrea","last_name":"Stöllner","first_name":"Andrea"}],"related_material":{"record":[{"relation":"part_of_dissertation","status":"public","id":"20705"},{"relation":"part_of_dissertation","status":"public","id":"23038"}]},"_id":"23033","year":"2026","OA_place":"publisher","user_id":"8b945eb4-e2f2-11eb-945a-df72226e66a9","date_published":"2026-10-02T00:00:00Z","ec_funded":1,"date_updated":"2026-10-09T11:09:10Z","publication_status":"published","OA_embargo":"6","acknowledged_ssus":[{"_id":"M-Shop"},{"_id":"Bio"}],"project":[{"grant_number":"949120","_id":"0aa60e99-070f-11eb-9043-a6de6bdc3afa","name":"Tribocharge: a multi-scale approach to an enduring problem in physics","call_identifier":"H2020"},{"call_identifier":"H2020","name":"Organization of CLoUdS, and implications of Tropical cyclones and for the Energetics of the tropics, in current and waRming climate","grant_number":"805041","_id":"629205d8-2b32-11ec-9570-e1356ff73576"}],"article_processing_charge":"No","tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"fulldoi":"https://doi.org/10.15479/AT-ISTA-23033","supervisor":[{"first_name":"Scott R","full_name":"Waitukaitis, Scott R","last_name":"Waitukaitis","orcid":"0000-0002-2299-3176","id":"3A1FFC16-F248-11E8-B48F-1D18A9856A87"},{"first_name":"Caroline J","last_name":"Muller","full_name":"Muller, Caroline J","orcid":"0000-0001-5836-5350","id":"f978ccb0-3f7f-11eb-b193-b0e2bd13182b"}]},{"project":[{"name":"Tribocharge: a multi-scale approach to an enduring problem in physics","call_identifier":"H2020","grant_number":"949120","_id":"0aa60e99-070f-11eb-9043-a6de6bdc3afa"},{"call_identifier":"H2020","name":"Organization of CLoUdS, and implications of Tropical cyclones and for the Energetics of the tropics, in current and waRming climate","grant_number":"805041","_id":"629205d8-2b32-11ec-9570-e1356ff73576"}],"acknowledged_ssus":[{"_id":"M-Shop"}],"fulldoi":"https://doi.org/10.48550/arXiv.2604.16040","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2604.16040"}],"article_processing_charge":"No","oa":1,"external_id":{"arxiv":["2604.16040"]},"_id":"23038","OA_place":"repository","user_id":"8b945eb4-e2f2-11eb-945a-df72226e66a9","year":"2026","related_material":{"record":[{"relation":"dissertation_contains","id":"23033","status":"public"}]},"author":[{"full_name":"Stöllner, Andrea","last_name":"Stöllner","first_name":"Andrea","id":"4bdcf7f6-eb97-11eb-a6c2-9981bbdc3bed","orcid":"0000-0002-0464-8440"},{"first_name":"Isaac C. D.","full_name":"Lenton, Isaac C. D.","last_name":"Lenton"},{"id":"f978ccb0-3f7f-11eb-b193-b0e2bd13182b","orcid":"0000-0001-5836-5350","last_name":"Muller","full_name":"Muller, Caroline J","first_name":"Caroline J"},{"full_name":"Waitukaitis, Scott R","last_name":"Waitukaitis","first_name":"Scott R","id":"3A1FFC16-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-2299-3176"}],"publication":"arXiv","abstract":[{"lang":"eng","text":"Electrical discharge at the smallest possible length and charge scales is not well understood. Using optical tweezers, we investigate spontaneous discharges of a single micron-scale particle levitated in air. These ``microdischarges'' have a typical size of $\\sim$40 $|e|$, but can be as small as a few $|e|$ and as large as several hundred. The absence of a well-defined trigger charge and the weak dependence on particle size suggest events are not classical gaseous breakdown. Instead, we show that microdischarge events arise from the rapid capture of ions left in the tracks of nearby passing ionizing radiation. Our results highlight the role of natural ionizing radiation in initiating micron-scale discharges and provide a platform for studying discharge physics in electrode-free environments and at the smallest scales."}],"publication_status":"draft","ec_funded":1,"date_updated":"2026-10-09T11:09:09Z","OA_type":"green","date_published":"2026-04-17T00:00:00Z","arxiv":1,"status":"public","citation":{"mla":"Stöllner, Andrea, et al. “Discharge at the Microscale: Using Optical Tweezers to Observe Muon-Induced Discharges of a Levitated Microparticle in Air.” ArXiv, doi:10.48550/arXiv.2604.16040.","ieee":"A. Stöllner, I. C. D. Lenton, C. J. Muller, and S. R. Waitukaitis, “Discharge at the microscale: Using optical tweezers to observe Muon-induced discharges of a levitated microparticle in air,” arXiv. .","short":"A. Stöllner, I.C.D. Lenton, C.J. Muller, S.R. Waitukaitis, ArXiv (n.d.).","apa":"Stöllner, A., Lenton, I. C. D., Muller, C. J., & Waitukaitis, S. R. (n.d.). Discharge at the microscale: Using optical tweezers to observe Muon-induced discharges of a levitated microparticle in air. arXiv. https://doi.org/10.48550/arXiv.2604.16040","ama":"Stöllner A, Lenton ICD, Muller CJ, Waitukaitis SR. Discharge at the microscale: Using optical tweezers to observe Muon-induced discharges of a levitated microparticle in air. arXiv. doi:10.48550/arXiv.2604.16040","chicago":"Stöllner, Andrea, Isaac C. D. Lenton, Caroline J Muller, and Scott R Waitukaitis. “Discharge at the Microscale: Using Optical Tweezers to Observe Muon-Induced Discharges of a Levitated Microparticle in Air.” ArXiv, n.d. https://doi.org/10.48550/arXiv.2604.16040.","ista":"Stöllner A, Lenton ICD, Muller CJ, Waitukaitis SR. Discharge at the microscale: Using optical tweezers to observe Muon-induced discharges of a levitated microparticle in air. arXiv, 10.48550/arXiv.2604.16040."},"month":"04","corr_author":"1","acknowledgement":"We thank Todor Asenov and Abdulhamid Baghdadi\r\nfor their outstanding technical support. This project\r\nhas received funding from the European Research Council\r\n(ERC) under the European Union’s Horizon 2020 research\r\nand innovation programme (Grant agreements No. 949120\r\nand No. 805041). This research was supported by the\r\nScientific Service Units of The Institute of Science and\r\nTechnology Austria (ISTA) through resources provided\r\nby the Miba Machine Shop.","title":"Discharge at the microscale: Using optical tweezers to observe Muon-induced discharges of a levitated microparticle in air","day":"17","oa_version":"Preprint","date_created":"2026-10-02T11:35:14Z","language":[{"iso":"eng"}],"type":"preprint","doi":"10.48550/arXiv.2604.16040","department":[{"_id":"CaMu"},{"_id":"ScWa"}]},{"publisher":"IOP Publishing","status":"public","arxiv":1,"file_date_updated":"2026-10-12T06:31:40Z","article_number":"73","issue":"1","ddc":["520"],"month":"03","intvolume":" 999","PlanS_conform":"1","citation":{"short":"B. Ludwig, M.R. Drout, Y.L.L. Götberg, D. Lang, A. Laroche, The Astrophysical Journal 999 (2026).","ieee":"B. Ludwig, M. R. Drout, Y. L. L. Götberg, D. Lang, and A. Laroche, “The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The ultraviolet photometric catalog and stripped-star candidate selection,” The Astrophysical Journal, vol. 999, no. 1. IOP Publishing, 2026.","mla":"Ludwig, B., et al. “The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The Ultraviolet Photometric Catalog and Stripped-Star Candidate Selection.” The Astrophysical Journal, vol. 999, no. 1, 73, IOP Publishing, 2026, doi:10.3847/1538-4357/ae2d13.","ista":"Ludwig B, Drout MR, Götberg YLL, Lang D, Laroche A. 2026. The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The ultraviolet photometric catalog and stripped-star candidate selection. The Astrophysical Journal. 999(1), 73.","apa":"Ludwig, B., Drout, M. R., Götberg, Y. L. L., Lang, D., & Laroche, A. (2026). The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The ultraviolet photometric catalog and stripped-star candidate selection. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ae2d13","chicago":"Ludwig, B., M. R. Drout, Ylva Louise Linsdotter Götberg, D. Lang, and A. Laroche. “The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The Ultraviolet Photometric Catalog and Stripped-Star Candidate Selection.” The Astrophysical Journal. IOP Publishing, 2026. https://doi.org/10.3847/1538-4357/ae2d13.","ama":"Ludwig B, Drout MR, Götberg YLL, Lang D, Laroche A. The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The ultraviolet photometric catalog and stripped-star candidate selection. The Astrophysical Journal. 2026;999(1). doi:10.3847/1538-4357/ae2d13"},"scopus_import":"1","oa_version":"Published Version","day":"01","title":"The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The ultraviolet photometric catalog and stripped-star candidate selection","acknowledgement":"We thank Anna O’Grady, Christopher D. Matzner, Joshua S. Speagle, Carles Badenes, Marten van Kerkwijk, Selma de Mink, Hugues Sana, Kareem El-Badry, and Lisa Blomberg for helpful conversations. We would also like to thank the anonymous referee for their thoughtful and constructive comments, which helped to improve the clarity and depth of this work.\r\n\r\nB.L. has received financial support from the Flemish Government under the long-term structural Methusalem funding program by means of the project SOUL: Stellar evolution in full glory, grant METH/24/012 at KU Leuven. M.R.D. acknowledges support from the NSERC through grant RGPIN-2019-06186, the Canada Research Chairs Program, and the Dunlap Institute at the University of Toronto. A.L. acknowledges support from the NSERC and is funded through a NSERC Canada Graduate Scholarship—Doctoral. A.L. is also supported by the Data Sciences Institute at the University of Toronto through grant number DSI- DSFY3R1P02.\r\n\r\nFacility: Swift (NASA Neil Gehrels Swift Observatory Mission) - .\r\n\r\nSoftware: astropy (Astropy Collaboration et al. 2013, 2018, 2022), astroquery (A. Ginsburg et al. 2019), matplotlib (J. D. Hunter 2007), numpy (C. R. Harris et al. 2020), pandas (W. McKinney 2010; pandas development team 2020), Photutils (L. Bradley et al. 2022, 2024), SciPy (P. Virtanen et al. 2020), the Tractor (D. Lang et al. 2016a), TOPCAT(M. B. Taylor 2005, 2006).","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"doi":"10.3847/1538-4357/ae2d13","department":[{"_id":"YlGo"}],"file":[{"file_size":25748518,"relation":"main_file","date_updated":"2026-10-12T06:31:40Z","file_name":"2026_AstrophysicalJour_Ludwig.pdf","file_id":"23098","date_created":"2026-10-12T06:31:40Z","access_level":"open_access","content_type":"application/pdf","checksum":"0d78d1da920aa065861ba98b50811058","success":1,"creator":"dernst"}],"type":"journal_article","has_accepted_license":"1","language":[{"iso":"eng"}],"date_created":"2026-10-04T22:01:55Z","supplementarymaterial":"yes","oa":1,"article_processing_charge":"Yes","fulldoi":"https://doi.org/10.3847/1538-4357/ae2d13","volume":999,"tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"abstract":[{"lang":"eng","text":"Most massive stars (∼8–25M⊙) interact with a binary companion during their lifetimes. These interactions can remove the hydrogen-rich envelope, producing intermediate-mass (∼2–8M⊙) and helium-rich stars. These “stripped stars” are predicted to emit predominantly in the ultraviolet (UV) and can therefore be identified via a UV excess—provided they are not outshone by their companion. However, despite their importance to binary evolution, supernovae, and ionizing feedback, few stripped stars have been confirmed. This is likely due to the scarcity of wide-field, high angular-resolution, UV surveys of stellar populations with reliable distances and extinction estimates. To address this, we present the Stripped-Star Ultraviolet Magellanic Clouds Survey catalog. We use the Tractor forward modeling software to perform point-spread function photometry on 2420 Swift UVOT images of the LMC and SMC. The resulting catalog contains 734,862 sources in three UV filters to a depth of ∼20 Vega mag. We perform validation tests on the photometry pipeline and highlight the catalog’s broad applicability. We then identify sources with excess UV light compared to main-sequence stars and apply a series of quality cuts. From this, we identify 522 candidate stripped stars in the LMC and 298 in the SMC. We assess the potential contamination from other UV excess systems and argue the dominant uncertainty to be dust: early main-sequence stars can mimic the colors of stripped-star binaries when extinction is overcorrected. This survey lays the groundwork for the first systematic census of stripped stars and opens new windows into binary evolution and massive star populations."}],"quality_controlled":"1","publication":"The Astrophysical Journal","article_type":"original","author":[{"first_name":"B.","full_name":"Ludwig, B.","last_name":"Ludwig"},{"last_name":"Drout","full_name":"Drout, M. R.","first_name":"M. R."},{"orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","first_name":"Ylva Louise Linsdotter","last_name":"Götberg","full_name":"Götberg, Ylva Louise Linsdotter"},{"first_name":"D.","last_name":"Lang","full_name":"Lang, D."},{"last_name":"Laroche","full_name":"Laroche, A.","first_name":"A."}],"year":"2026","researchdata_availability":"no","OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"23051","external_id":{"arxiv":["2505.18632"]},"das_tickbox":"0","date_published":"2026-03-01T00:00:00Z","date_updated":"2026-10-12T06:54:27Z","OA_type":"gold","publication_status":"published"},{"publication_status":"published","OA_type":"gold","date_updated":"2026-10-12T08:21:05Z","date_published":"2026-02-20T00:00:00Z","das_tickbox":"1","external_id":{"arxiv":["2506.16510"]},"DOAJ_listed":"1","_id":"23052","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"publisher","researchdata_availability":"no","year":"2026","author":[{"first_name":"Abby","last_name":"Mintz","full_name":"Mintz, Abby"},{"first_name":"David J.","last_name":"Setton","full_name":"Setton, David J."},{"last_name":"Greene","full_name":"Greene, Jenny E.","first_name":"Jenny E."},{"first_name":"Joel","full_name":"Leja, Joel","last_name":"Leja"},{"last_name":"Wang","full_name":"Wang, Bingjie","first_name":"Bingjie"},{"full_name":"Burnham, Emilie","last_name":"Burnham","first_name":"Emilie"},{"last_name":"Suess","full_name":"Suess, Katherine A.","first_name":"Katherine A."},{"first_name":"Hakim","last_name":"Atek","full_name":"Atek, Hakim"},{"first_name":"Rachel","full_name":"Bezanson, Rachel","last_name":"Bezanson"},{"last_name":"Brammer","full_name":"Brammer, Gabriel","first_name":"Gabriel"},{"first_name":"Sam E.","last_name":"Cutler","full_name":"Cutler, Sam E."},{"first_name":"Pratika","last_name":"Dayal","full_name":"Dayal, Pratika"},{"first_name":"Robert","full_name":"Feldmann, Robert","last_name":"Feldmann"},{"first_name":"Lukas J.","full_name":"Furtak, Lukas J.","last_name":"Furtak"},{"full_name":"Glazebrook, Karl","last_name":"Glazebrook","first_name":"Karl"},{"last_name":"Khullar","full_name":"Khullar, Gourav","first_name":"Gourav"},{"last_name":"Kokorev","full_name":"Kokorev, Vasily","first_name":"Vasily"},{"first_name":"Ivo","last_name":"Labbé","full_name":"Labbé, Ivo"},{"first_name":"Jorryt J","full_name":"Matthee, Jorryt J","last_name":"Matthee","orcid":"0000-0003-2871-127X","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"first_name":"Michael V.","last_name":"Maseda","full_name":"Maseda, Michael V."},{"first_name":"Tim B.","full_name":"Miller, Tim B.","last_name":"Miller"},{"first_name":"Ikki","last_name":"Mitsuhashi","full_name":"Mitsuhashi, Ikki"},{"first_name":"Themiya","full_name":"Nanayakkara, Themiya","last_name":"Nanayakkara"},{"first_name":"Richard","last_name":"Pan","full_name":"Pan, Richard"},{"last_name":"Price","full_name":"Price, Sedona H.","first_name":"Sedona H."},{"last_name":"Weaver","full_name":"Weaver, John R.","first_name":"John R."},{"full_name":"Whitaker, Katherine E.","last_name":"Whitaker","first_name":"Katherine E."},{"full_name":"Wu, Belinda","last_name":"Wu","first_name":"Belinda"}],"article_type":"original","quality_controlled":"1","publication":"The Astrophysical Journal","abstract":[{"text":"While bursty star formation in low-mass galaxies has been observed in local populations and reproduced in simulations, the dormant phase of the burst cycle has not been well studied beyond the local Universe due to observational limitations. We present a unique sample of 43 JWST PRISM spectra of low-mass galaxies (M⋆ < 10^9.5 M⊙) at cosmic noon (1 < z < 3), uniformly selected on F200W magnitude and precise photometric redshifts enabled by 20-band JWST photometry from the UNCOVER and MegaScience surveys. The spectra reveal numerous strong Balmer breaks, which are negatively correlated with the galaxies’ Hα equivalent width. By comparing these observations to synthetic samples of spectra generated using a simple parameterization of bursty star formation histories, we show that star formation in low-mass galaxies at cosmic noon is likely dominated by burst cycles with long timescales (≳100 Myr) and large deviations below the star-forming main sequence (≳0.8 dex). Our results suggest that galaxies in this population—at least those within our detection limits—should not be classified solely by their current star formation rates, but instead viewed as a unified population undergoing dynamic movement above and below the star-forming main sequence. The derived constraints demonstrate that long-timescale fluctuations are important for this class of galaxies, indicating that galaxy-scale gas cycles—rather than molecular-cloud-scale stochasticity—are the primary regulators of star formation variability in low-mass galaxies at cosmic noon.","lang":"eng"}],"tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"fulldoi":"https://doi.org/10.3847/1538-4357/ae328c","volume":998,"article_processing_charge":"Yes","oa":1,"supplementarymaterial":"yes","date_created":"2026-10-04T22:01:56Z","language":[{"iso":"eng"}],"type":"journal_article","has_accepted_license":"1","file":[{"access_level":"open_access","date_created":"2026-10-12T08:18:07Z","file_name":"2026_AstrophysicalJour_Mintz.pdf","relation":"main_file","file_size":3955341,"date_updated":"2026-10-12T08:18:07Z","file_id":"23103","content_type":"application/pdf","checksum":"07b1a08dec5787883b195b73a2c4f2e5","creator":"dernst","success":1}],"department":[{"_id":"JoMa"}],"doi":"10.3847/1538-4357/ae328c","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"acknowledgement":"A.M. acknowledges support from the National Science Foundation Graduate Research Fellowship under grant No. DGE-2444107. A.M. thanks Helena Treiber for helpful discussions. Support for this work was provided by The Brinson Foundation through a Brinson Prize Fellowship grant.\r\n\r\nThis work is based in part on observations made with the NASA/ESA/CSA James Webb Space Telescope obtained from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. Financial support for programs JWST-GO-1837, JWST-GO-2561, JWST-GO-4111, and JWST-GO-6405 is gratefully acknowledged and is provided by NASA through grants from the Space Telescope Science Institute, which is operated by the Associations of Universities for Research in Astronomy, Incorporated, under NASA contract NAS 5-03127. These observations are associated with programs JWST-GO-2561, JWST-ERS-1324, JWST-DD-2756, JWST-GO-4111, HST-GO-11689, HST-GO-13386, HST-GO/DD-13495, HST-GO-13389, HST-GO-15117, and HST-GO/DD-17231. Some of the data presented in this article were obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute. The specific observations analyzed can be accessed via doi:10.17909/grtw-hr67. Some of the data products presented herein were retrieved from the Dawn JWST Archive (DJA). DJA is an initiative of the Cosmic Dawn Center, which is funded by the Danish National Research Foundation under grant No. 140.\r\n\r\nFacilities: JWST - James Webb Space Telescope (NIRCam and NIRSpec), HST - Hubble Space Telescope satellite (WFC3 and ACS).\r\n\r\nSoftware: NumPy (https://numpy.org, C. R. Harris et al. 2020), Astropy (https://astropy.org, Astropy Collaboration et al. 2013, 2018, 2022), Matplotlib (https://matplotlib.org, J. D. Hunter 2007), SciPy (https://scipy.org, P. Virtanen et al. 2020).","title":"Taking a break at cosmic noon: Continuum-selected low-mass galaxies require long burst cycles","day":"20","oa_version":"Published Version","scopus_import":"1","PlanS_conform":"1","citation":{"mla":"Mintz, Abby, et al. “Taking a Break at Cosmic Noon: Continuum-Selected Low-Mass Galaxies Require Long Burst Cycles.” The Astrophysical Journal, vol. 998, no. 2, 257, IOP Publishing, 2026, doi:10.3847/1538-4357/ae328c.","ieee":"A. Mintz et al., “Taking a break at cosmic noon: Continuum-selected low-mass galaxies require long burst cycles,” The Astrophysical Journal, vol. 998, no. 2. IOP Publishing, 2026.","short":"A. Mintz, D.J. Setton, J.E. Greene, J. Leja, B. Wang, E. Burnham, K.A. Suess, H. Atek, R. Bezanson, G. Brammer, S.E. Cutler, P. Dayal, R. Feldmann, L.J. Furtak, K. Glazebrook, G. Khullar, V. Kokorev, I. Labbé, J.J. Matthee, M.V. Maseda, T.B. Miller, I. Mitsuhashi, T. Nanayakkara, R. Pan, S.H. Price, J.R. Weaver, K.E. Whitaker, B. Wu, The Astrophysical Journal 998 (2026).","apa":"Mintz, A., Setton, D. J., Greene, J. E., Leja, J., Wang, B., Burnham, E., … Wu, B. (2026). Taking a break at cosmic noon: Continuum-selected low-mass galaxies require long burst cycles. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ae328c","ama":"Mintz A, Setton DJ, Greene JE, et al. Taking a break at cosmic noon: Continuum-selected low-mass galaxies require long burst cycles. The Astrophysical Journal. 2026;998(2). doi:10.3847/1538-4357/ae328c","chicago":"Mintz, Abby, David J. Setton, Jenny E. Greene, Joel Leja, Bingjie Wang, Emilie Burnham, Katherine A. Suess, et al. “Taking a Break at Cosmic Noon: Continuum-Selected Low-Mass Galaxies Require Long Burst Cycles.” The Astrophysical Journal. IOP Publishing, 2026. https://doi.org/10.3847/1538-4357/ae328c.","ista":"Mintz A, Setton DJ, Greene JE, Leja J, Wang B, Burnham E, Suess KA, Atek H, Bezanson R, Brammer G, Cutler SE, Dayal P, Feldmann R, Furtak LJ, Glazebrook K, Khullar G, Kokorev V, Labbé I, Matthee JJ, Maseda MV, Miller TB, Mitsuhashi I, Nanayakkara T, Pan R, Price SH, Weaver JR, Whitaker KE, Wu B. 2026. Taking a break at cosmic noon: Continuum-selected low-mass galaxies require long burst cycles. The Astrophysical Journal. 998(2), 257."},"intvolume":" 998","month":"02","ddc":["520"],"issue":"2","article_number":"257","file_date_updated":"2026-10-12T08:18:07Z","arxiv":1,"status":"public","publisher":"IOP Publishing"},{"article_processing_charge":"Yes (in subscription journal)","oa":1,"fulldoi":"https://doi.org/10.1088/1538-3873/ae3a19","volume":138,"tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"date_updated":"2026-10-12T08:13:30Z","OA_type":"hybrid","dataavailabilitystatement":"This research has made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC. This research has made use of the SVO Filter Profile Service “Carlos Rodrigo,” funded by MCIN/AEI/10.13039/501100011033/ through grant PID2023-146210NB-I00.\r\n\r\nSoftware: The Tractor (Lang et al. 2016), HEASARC (NASA High Energy Astrophysics Science Archive Research Center 2024), Astropy (Astropy Collaboration et al. 2013, 2018, 2022).","date_published":"2026-02-01T00:00:00Z","das_tickbox":"1","publication_status":"published","quality_controlled":"1","publication":"Publications of the Astronomical Society of the Pacific","abstract":[{"lang":"eng","text":"Stripped stars are hot, helium-rich stars formed when binary interactions remove a star’s hydrogen envelope. While low-mass (≲1 M⊙) and high-mass (≳8 M⊙) stripped stars are well studied as hot subdwarfs and Wolf–Rayet stars, their intermediate-mass counterparts (1–8 M⊙) have only recently been discovered. The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS) identified UV-excess sources (i.e., sources lying blueward of the main sequence) in the Magellanic Clouds using Swift-UVOT photometry and selected 820 photometric stripped-star candidates. However, the completeness and purity of this sample remain poorly understood. We forward model the population of stripped stars in the Magellanic Clouds using a binary population synthesis model combined with spatially resolved star formation histories and simulated UV photometry. To assess survey sensitivity, we inject simulated sources into real Swift-UVOT images and reproduce the SUMS selection process, including crowding, extinction, and photometric quality cuts. For the SMC and LMC, we respectively recover 31% and 15% of sources with intrinsic UV excess, and 11% and 7% of all stripped stars. The rest are missed due to dilution by luminous companions, crowding, high extinction, and limited survey coverage. The observed population is biased toward systems with low-mass companions formed by common envelope evolution and systems with compact object companions. We predict contamination of the observed stripped-star candidates by main-sequence stars with spurious UV excess due to crowding and provide guidelines for selecting higher-purity subsamples. Our population synthesis model matches the number and properties of observed stripped star candidates with masses of (2–5) M⊙ well. It underpredicts the number of lower- and higher-mass candidates, perhaps due to contamination."}],"author":[{"first_name":"Lisa","full_name":"Blomberg, Lisa","last_name":"Blomberg"},{"last_name":"El-Badry","full_name":"El-Badry, Kareem","first_name":"Kareem"},{"last_name":"Ludwig","full_name":"Ludwig, Bethany","first_name":"Bethany"},{"first_name":"Maria R.","full_name":"Drout, Maria R.","last_name":"Drout"},{"id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","orcid":"0000-0002-6960-6911","full_name":"Götberg, Ylva Louise Linsdotter","last_name":"Götberg","first_name":"Ylva Louise Linsdotter"}],"article_type":"original","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","OA_place":"publisher","year":"2026","researchdata_availability":"no","external_id":{"arxiv":["2510.18965"]},"_id":"23053","month":"02","intvolume":" 138","scopus_import":"1","PlanS_conform":"1","citation":{"ama":"Blomberg L, El-Badry K, Ludwig B, Drout MR, Götberg YLL. Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess. Publications of the Astronomical Society of the Pacific. 2026;138(2). doi:10.1088/1538-3873/ae3a19","apa":"Blomberg, L., El-Badry, K., Ludwig, B., Drout, M. R., & Götberg, Y. L. L. (2026). Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess. Publications of the Astronomical Society of the Pacific. IOP Publishing. https://doi.org/10.1088/1538-3873/ae3a19","chicago":"Blomberg, Lisa, Kareem El-Badry, Bethany Ludwig, Maria R. Drout, and Ylva Louise Linsdotter Götberg. “Intermediate-Mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered via UV Excess.” Publications of the Astronomical Society of the Pacific. IOP Publishing, 2026. https://doi.org/10.1088/1538-3873/ae3a19.","ista":"Blomberg L, El-Badry K, Ludwig B, Drout MR, Götberg YLL. 2026. Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess. Publications of the Astronomical Society of the Pacific. 138(2), 024202.","mla":"Blomberg, Lisa, et al. “Intermediate-Mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered via UV Excess.” Publications of the Astronomical Society of the Pacific, vol. 138, no. 2, 024202, IOP Publishing, 2026, doi:10.1088/1538-3873/ae3a19.","short":"L. Blomberg, K. El-Badry, B. Ludwig, M.R. Drout, Y.L.L. Götberg, Publications of the Astronomical Society of the Pacific 138 (2026).","ieee":"L. Blomberg, K. El-Badry, B. Ludwig, M. R. Drout, and Y. L. L. Götberg, “Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess,” Publications of the Astronomical Society of the Pacific, vol. 138, no. 2. IOP Publishing, 2026."},"publisher":"IOP Publishing","arxiv":1,"article_number":"024202","file_date_updated":"2026-10-12T08:12:05Z","status":"public","ddc":["520"],"issue":"2","file":[{"checksum":"ca48567fc6bf68b73872bd551bd6b069","content_type":"application/pdf","creator":"dernst","success":1,"access_level":"open_access","date_created":"2026-10-12T08:12:05Z","file_name":"2026_PubAstronomicalSocietyPacific_Blomberg.pdf","file_size":4294927,"date_updated":"2026-10-12T08:12:05Z","relation":"main_file","file_id":"23102"}],"doi":"10.1088/1538-3873/ae3a19","department":[{"_id":"YlGo"}],"language":[{"iso":"eng"}],"type":"journal_article","has_accepted_license":"1","supplementarymaterial":"yes","date_created":"2026-10-04T22:01:56Z","oa_version":"Published Version","title":"Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess","day":"01","publication_identifier":{"issn":["0004-6280"],"eissn":["1538-3873"]},"acknowledgement":"We thank the referee for their constructive comments. We thank Hugues Sana’s group at KU Lueven and Greg Green for useful discussions. This research was supported by NSF grants AST-2508988 and AST-2307232. B.L. has received financial support from the Flemish Government under the long-term structural Methusalem funding program by means of the project SOUL: Stellar evolution in full glory, grant METH/24/012 at KU Leuven. M.R.D. acknowledges support from the NSERC through grant RGPIN-2019-06186, the Canada Research Chairs Program, the Ontario Early Researchers Award ER22-17-164, and the Dunlap Institute at the University of Toronto.\r\n\r\nThis project was developed in part at the Lorentz Center workshop “From discovery to a population: benchmarking stripped stars and companions” held in 2024 July in Leiden, Netherlands.\r\n\r\nThis research has made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC. This research has made use of the SVO Filter Profile Service “Carlos Rodrigo,” funded by MCIN/AEI/10.13039/501100011033/ through grant PID2023-146210NB-I00.\r\n\r\nSoftware: The Tractor (Lang et al. 2016), HEASARC (NASA High Energy Astrophysics Science Archive Research Center 2024), Astropy (Astropy Collaboration et al. 2013, 2018, 2022)."},{"publisher":"Wiley","ddc":["540","570"],"article_number":"e75903","status":"public","month":"09","scopus_import":"1","citation":{"ista":"Kiem DH, Nauman M, Choi J, Graf D, Kim J, Yang H, Park JG, Jo Y, Han MJ. 2026. Crucial role of magnetic dipole and anomalous field dependence in NiPS3. Small., e75903.","ama":"Kiem DH, Nauman M, Choi J, et al. Crucial role of magnetic dipole and anomalous field dependence in NiPS3. Small. 2026. doi:10.1002/smll.75903","apa":"Kiem, D. H., Nauman, M., Choi, J., Graf, D., Kim, J., Yang, H., … Han, M. J. (2026). Crucial role of magnetic dipole and anomalous field dependence in NiPS3. Small. Wiley. https://doi.org/10.1002/smll.75903","chicago":"Kiem, Do Hoon, Muhammad Nauman, Joonyoung Choi, David Graf, Junghyun Kim, Heejun Yang, Je Geun Park, Younjung Jo, and Myung Joon Han. “Crucial Role of Magnetic Dipole and Anomalous Field Dependence in NiPS3.” Small. Wiley, 2026. https://doi.org/10.1002/smll.75903.","short":"D.H. Kiem, M. Nauman, J. Choi, D. Graf, J. Kim, H. Yang, J.G. Park, Y. Jo, M.J. Han, Small (2026).","ieee":"D. H. Kiem et al., “Crucial role of magnetic dipole and anomalous field dependence in NiPS3,” Small. Wiley, 2026.","mla":"Kiem, Do Hoon, et al. “Crucial Role of Magnetic Dipole and Anomalous Field Dependence in NiPS3.” Small, e75903, Wiley, 2026, doi:10.1002/smll.75903."},"oa_version":"Published Version","publication_identifier":{"issn":["1613-6810"],"eissn":["1613-6829"]},"acknowledgement":"M. J. H. was supported by a National Research Foundation of Korea (NRF) grant funded by the Korean government (MSIT) (Grant No. RS-2025-00559042). This work was supported by the Samsung Science & Technology Foundation (Grant No. SSTF-BA2101-05). Y. J. was supported by a National Research Foundation of Korea (NRF) grant (RS-2024-00337640, RS-2023-00301914). A portion of this work was performed at the National High Magnetic Field Laboratory, which is supported by National Science Foundation Cooperative Agreement No. DMR-2128556 and the State of Florida. This work was also supported by the Leading Researcher Program of the National Research Foundation of Korea (Grant No. RS-2020-NR049405).","title":"Crucial role of magnetic dipole and anomalous field dependence in NiPS3","day":"26","doi":"10.1002/smll.75903","department":[{"_id":"KiMo"}],"supplementarymaterial":"yes","date_created":"2026-10-04T22:01:57Z","language":[{"iso":"eng"}],"type":"journal_article","has_accepted_license":"1","main_file_link":[{"url":"https://doi.org/10.1002/smll.75903","open_access":"1"}],"oa":1,"article_processing_charge":"No","tmp":{"image":"/images/cc_by_nc_nd.png","short":"CC BY-NC-ND (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)"},"fulldoi":"https://doi.org/10.1002/smll.75903","author":[{"first_name":"Do Hoon","full_name":"Kiem, Do Hoon","last_name":"Kiem"},{"full_name":"Nauman, Muhammad","last_name":"Nauman","first_name":"Muhammad","id":"32c21954-2022-11eb-9d5f-af9f93c24e71","orcid":"0000-0002-2111-4846"},{"first_name":"Joonyoung","full_name":"Choi, Joonyoung","last_name":"Choi"},{"full_name":"Graf, David","last_name":"Graf","first_name":"David"},{"first_name":"Junghyun","full_name":"Kim, Junghyun","last_name":"Kim"},{"first_name":"Heejun","last_name":"Yang","full_name":"Yang, Heejun"},{"last_name":"Park","full_name":"Park, Je Geun","first_name":"Je Geun"},{"first_name":"Younjung","full_name":"Jo, Younjung","last_name":"Jo"},{"first_name":"Myung Joon","full_name":"Han, Myung Joon","last_name":"Han"}],"article_type":"original","quality_controlled":"1","publication":"Small","abstract":[{"lang":"eng","text":"NiPS3 has attracted considerable attention, yet the origin of its intriguing magnetic behaviors remains elusive due to limited insight into its low-energy anisotropy. Here, high-field torque magnetometry measurements are performed, revealing a previously unrecognized anisotropic spin response that reflects interaction terms beyond the standard XY or XXZ models. In combination with relativistic density functional theory calculations and magnetic force response theory, an effective low-energy spin Hamiltonian is constructed, elucidating not only the observed anomalous magnetic behavior but also other recent experiments. Remarkably, the magnetic dipole interaction and the associated spin-flop transition play a crucial role in driving the deviation from two-dimensional spin alignment, providing direct insight into the underlying anisotropic energy hierarchy. The generalized Hamiltonian can serve as the important fundamental ground for future study, and our approach adopted here will hopefully be relevant to many other related material systems."}],"external_id":{"pmid":["42799549"]},"_id":"23058","OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","researchdata_availability":"upon request","year":"2026","date_updated":"2026-10-12T08:31:21Z","dataavailabilitystatement":"The data that support the findings of this study are available from the corresponding author upon reasonable request.","OA_type":"hybrid","date_published":"2026-09-26T00:00:00Z","das_tickbox":"1","publication_status":"epub_ahead","pmid":1},{"article_processing_charge":"No","month":"09","conference":{"end_date":"2026-06-18","start_date":"2026-06-15","location":"Glasgow, United Kingdom","name":"Quantum 2.0"},"citation":{"ama":"De Zordo N, Borja Espinosa CN, Al Hyder R, et al. Detecting polar molecules with superconducting microwave resonators. In: Quantum 2.0 Conference and Exhibition. Optica Publishing Group; 2026.","apa":"De Zordo, N., Borja Espinosa, C. N., Al Hyder, R., Li, J., Kersten, W., Kanagin, A., … Redchenko, E. (2026). Detecting polar molecules with superconducting microwave resonators. In Quantum 2.0 Conference and Exhibition. Glasgow, United Kingdom: Optica Publishing Group.","chicago":"De Zordo, Nikolaus, Carla N Borja Espinosa, Ragheed Al Hyder, Jinglun Li, Wenzel Kersten, Andrew Kanagin, Georgios Koutentakis, et al. “Detecting Polar Molecules with Superconducting Microwave Resonators.” In Quantum 2.0 Conference and Exhibition. Optica Publishing Group, 2026.","ista":"De Zordo N, Borja Espinosa CN, Al Hyder R, Li J, Kersten W, Kanagin A, Koutentakis G, Kluibenschedl F, Lemeshko M, Fink JM, Schmiedmayer J, Redchenko E. 2026. Detecting polar molecules with superconducting microwave resonators. Quantum 2.0 Conference and Exhibition. Quantum 2.0, Technical Digest Series, , QM4D.3.","mla":"De Zordo, Nikolaus, et al. “Detecting Polar Molecules with Superconducting Microwave Resonators.” Quantum 2.0 Conference and Exhibition, QM4D.3, Optica Publishing Group, 2026.","ieee":"N. De Zordo et al., “Detecting polar molecules with superconducting microwave resonators,” in Quantum 2.0 Conference and Exhibition, Glasgow, United Kingdom, 2026.","short":"N. De Zordo, C.N. Borja Espinosa, R. Al Hyder, J. Li, W. Kersten, A. Kanagin, G. Koutentakis, F. Kluibenschedl, M. Lemeshko, J.M. Fink, J. Schmiedmayer, E. Redchenko, in:, Quantum 2.0 Conference and Exhibition, Optica Publishing Group, 2026."},"scopus_import":"1","publisher":"Optica Publishing Group","status":"public","article_number":"QM4D.3","department":[{"_id":"JoFi"},{"_id":"GradSch"},{"_id":"MiLe"}],"date_published":"2026-09-01T00:00:00Z","das_tickbox":"0","date_updated":"2026-10-12T07:52:45Z","OA_type":"closed access","type":"conference","language":[{"iso":"eng"}],"publication_status":"published","date_created":"2026-10-04T22:01:56Z","alternative_title":["Technical Digest Series"],"abstract":[{"lang":"eng","text":"We report progress toward strong electric-dipole coupling of polar molecules in cryogenic crystals to superconducting microwave resonators for hybrid quantum computing. We detect crystal-shifted inversion transitions of ammonia in neon using a multimode resonator."}],"publication":"Quantum 2.0 Conference and Exhibition","quality_controlled":"1","author":[{"last_name":"De Zordo","full_name":"De Zordo, Nikolaus","first_name":"Nikolaus"},{"first_name":"Carla N","last_name":"Borja Espinosa","full_name":"Borja Espinosa, Carla N","id":"18777c01-896a-11ed-bdf8-e4851dc07d16"},{"id":"d1c405be-ae15-11ed-8510-ccf53278162e","full_name":"Al Hyder, Ragheed","last_name":"Al Hyder","first_name":"Ragheed"},{"first_name":"Jinglun","last_name":"Li","full_name":"Li, Jinglun","id":"ff19510a-0d2c-11ef-b018-c338ad2f4325"},{"last_name":"Kersten","full_name":"Kersten, Wenzel","first_name":"Wenzel"},{"first_name":"Andrew","full_name":"Kanagin, Andrew","last_name":"Kanagin"},{"first_name":"Georgios","full_name":"Koutentakis, Georgios","last_name":"Koutentakis","id":"d7b23d3a-9e21-11ec-b482-f76739596b95"},{"last_name":"Kluibenschedl","full_name":"Kluibenschedl, Florian","first_name":"Florian","id":"7499e70e-eb2c-11ec-b98b-f925648bc9d9","orcid":"0000-0003-4695-5526"},{"orcid":"0000-0002-6990-7802","id":"37CB05FA-F248-11E8-B48F-1D18A9856A87","first_name":"Mikhail","last_name":"Lemeshko","full_name":"Lemeshko, Mikhail"},{"full_name":"Fink, Johannes M","last_name":"Fink","first_name":"Johannes M","id":"4B591CBA-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8112-028X"},{"full_name":"Schmiedmayer, Jörg","last_name":"Schmiedmayer","first_name":"Jörg"},{"id":"2C21D6E8-F248-11E8-B48F-1D18A9856A87","first_name":"Elena","last_name":"Redchenko","full_name":"Redchenko, Elena"}],"oa_version":"None","year":"2026","day":"01","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"Detecting polar molecules with superconducting microwave resonators","_id":"23055","publication_identifier":{"isbn":["9781957171616"]}},{"day":"30","title":"Predicting ionic conductivity of sulfide glass solid-state electrolytes using max-flow methodology","acknowledgement":"We thank the Danish e-Infrastructure Cooperation (DeiC) for access to computational resources at Sophia and LUMI-C (DeiC-AAU-N5-202200005). This work was supported by the Independent Research Fund Denmark (1026-00037), European Union (ERC, NewGLASS, 101044664), and Danish Data Science Academy, which in turn is funded by the Novo Nordisk Foundation (NNF21SA0069429) and VILLUM FONDEN (40516). Y.B.B. acknowledges support from the Austrian Science Fund (FWF) 10.55776/ESP9584724.","publication_identifier":{"eissn":["2041-1723"]},"oa_version":"Published Version","type":"journal_article","has_accepted_license":"1","language":[{"iso":"eng"}],"date_created":"2026-10-11T22:02:03Z","supplementarymaterial":"yes","doi":"10.1038/s41467-026-77363-w","department":[{"_id":"HeEd"}],"file":[{"date_created":"2026-10-12T09:00:06Z","access_level":"open_access","file_id":"23104","relation":"main_file","file_size":1889857,"date_updated":"2026-10-12T09:00:06Z","file_name":"2026_NatureComm_Pegoraro.pdf","success":1,"creator":"dernst","content_type":"application/pdf","checksum":"eba760f5982a89f59664957e00c5d2d6"}],"status":"public","article_number":"10343","file_date_updated":"2026-10-12T09:00:06Z","ddc":["500"],"publisher":"Springer Nature","intvolume":" 17","citation":{"ista":"Pegoraro M, Christensen R, Sørensen SS, Lindbjerg AR, Du T, Bokor Bleile Y, Svane AM, Biscio CAN, Fajstrup L, Smedskjaer MM. 2026. Predicting ionic conductivity of sulfide glass solid-state electrolytes using max-flow methodology. Nature Communications. 17, 10343.","ama":"Pegoraro M, Christensen R, Sørensen SS, et al. Predicting ionic conductivity of sulfide glass solid-state electrolytes using max-flow methodology. Nature Communications. 2026;17. doi:10.1038/s41467-026-77363-w","chicago":"Pegoraro, Matteo, Rasmus Christensen, Søren S. Sørensen, Anders R. Lindbjerg, Tao Du, Yossi Bokor Bleile, Anne Marie Svane, Christophe A.N. Biscio, Lisbeth Fajstrup, and Morten M. Smedskjaer. “Predicting Ionic Conductivity of Sulfide Glass Solid-State Electrolytes Using Max-Flow Methodology.” Nature Communications. Springer Nature, 2026. https://doi.org/10.1038/s41467-026-77363-w.","apa":"Pegoraro, M., Christensen, R., Sørensen, S. S., Lindbjerg, A. R., Du, T., Bokor Bleile, Y., … Smedskjaer, M. M. (2026). Predicting ionic conductivity of sulfide glass solid-state electrolytes using max-flow methodology. Nature Communications. Springer Nature. https://doi.org/10.1038/s41467-026-77363-w","short":"M. Pegoraro, R. Christensen, S.S. Sørensen, A.R. Lindbjerg, T. Du, Y. Bokor Bleile, A.M. Svane, C.A.N. Biscio, L. Fajstrup, M.M. Smedskjaer, Nature Communications 17 (2026).","ieee":"M. Pegoraro et al., “Predicting ionic conductivity of sulfide glass solid-state electrolytes using max-flow methodology,” Nature Communications, vol. 17. Springer Nature, 2026.","mla":"Pegoraro, Matteo, et al. “Predicting Ionic Conductivity of Sulfide Glass Solid-State Electrolytes Using Max-Flow Methodology.” Nature Communications, vol. 17, 10343, Springer Nature, 2026, doi:10.1038/s41467-026-77363-w."},"PlanS_conform":"1","scopus_import":"1","month":"09","year":"2026","researchdata_availability":"yes","OA_place":"publisher","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"23087","DOAJ_listed":"1","external_id":{"pmid":["42811056"]},"abstract":[{"text":"Disordered materials such as glasses are promising candidates as solid-state electrolytes for batteries, but they tend to exhibit low ionic conductivity and current methods for investigating and predicting the ionic conductivity of electrolyte materials are inefficient. Here, we propose a framework that summarizes the topological properties of the electrolyte material’s atomic structure with a weighted graph based on periodic boundary conditions. We then compute a variation of the max-flow algorithm, a commonly used model in continuum models of transportation and liquid flow, on this summary and show that it is compatible with the simulated periodic atomic structures. Using molecular dynamics simulations of various glassy solid-state electrolyte families including both mobile lithium and sodium ions, we validate the approach by showing a positive correlation between the area-normalized maximum flow predicted from the static glass structures and the ionic conductivity as obtained from the simulations, especially in the case of high-conductivity sulfide glass electrolytes. We envision that the developed methodology, which only relies on static atomic structure, will accelerate the discovery of highly conductive sulfide glassy electrolytes for high-performance all-solid-state batteries.","lang":"eng"}],"publication":"Nature Communications","quality_controlled":"1","author":[{"last_name":"Pegoraro","full_name":"Pegoraro, Matteo","first_name":"Matteo"},{"full_name":"Christensen, Rasmus","last_name":"Christensen","first_name":"Rasmus"},{"full_name":"Sørensen, Søren S.","last_name":"Sørensen","first_name":"Søren S."},{"first_name":"Anders R.","full_name":"Lindbjerg, Anders R.","last_name":"Lindbjerg"},{"first_name":"Tao","full_name":"Du, Tao","last_name":"Du"},{"id":"920a7385-7995-11ef-9bfd-8c434cd8f3c2","orcid":"0000-0002-4861-9174","last_name":"Bleile","full_name":"Bleile, Yossi","first_name":"Yossi"},{"full_name":"Svane, Anne Marie","last_name":"Svane","first_name":"Anne Marie"},{"first_name":"Christophe A.N.","full_name":"Biscio, Christophe A.N.","last_name":"Biscio"},{"first_name":"Lisbeth","last_name":"Fajstrup","full_name":"Fajstrup, Lisbeth"},{"first_name":"Morten M.","full_name":"Smedskjaer, Morten M.","last_name":"Smedskjaer"}],"article_type":"original","pmid":1,"publication_status":"published","das_tickbox":"1","date_published":"2026-09-30T00:00:00Z","date_updated":"2026-10-12T09:03:58Z","OA_type":"gold","dataavailabilitystatement":"All data supporting the findings of this study are available within the article and Supplementary Information files. Source data are provided with this paper. The developed code to perform the max-flow calculations is available as part of the Topological Materials Analysis (ToMA) library, which is available at Zenodo (https://doi.org/10.5281/zenodo.10781424) and Github (https://github.com/yossibokorbleile/TopologicalMaterialAnalysis), with documentation available at https://yossi.eu/toma/. To enhance usability, we have included a brief documentation on how to compile ToMA as well as a minimal working example of the code together with an example trajectory directly in the ToMA repository. LAMMPS is an open-source code available at https://lammps.sandia.gov.","project":[{"_id":"9106a876-16d5-11f0-9cad-bbf11c9952f9","grant_number":"ESP 9584724","name":"Quantitative Unbiased Shape Analysis with Geometry & Topology"}],"fulldoi":"https://doi.org/10.1038/s41467-026-77363-w","volume":17,"tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"article_processing_charge":"Yes","oa":1}]