[{"abstract":[{"lang":"eng","text":"The Vera C. Rubin Observatory has now seen first light, and over a 10 year duration, Legacy Survey of Space and Time (LSST) is projected to catalog tens of millions of quasars, many of which are expected to be associated with subparsec supermassive black hole binaries (SMBHBs). Out of these SMBHBs, up to thousands of relatively massive binary-quasars are expected to exhibit gravitational self-lensing flares (SLFs) that last for at least 20–30 days. We assess the effectiveness of the Lomb-Scargle (LS) periodogram and matched filters (MFs) as methods for systematic searches for these binaries, using toy-models of hydrodynamical, Doppler, and self-lensing variability from equal-mass, eccentric SMBHBs. We inject SLFs into random realizations of damped random walk (DRW) lightcurves, representing stochastic quasar variability, and compute the LS periodogram with and without the SLF. We find that periodograms of SLF+DRW light-curves do not have maximum peak heights that could not arise from DRW-only periodograms. On the other hand, the matched filter signal-to-noise ratio (SNR) can distinguish SLFs from noise even with LSST-like cadences and DRW noise. Furthermore, we develop a three-step procedure with matched filters, which can also recover injected binary parameters from these light-curves. We expect this method to be computationally efficient enough to be applicable to millions of quasar light-curves in LSST."}],"type":"journal_article","oa_version":"Published Version","article_type":"original","date_created":"2026-10-18T22:01:53Z","author":[{"last_name":"Park","first_name":"Kevin S","id":"c0a7603b-66e5-11f0-aaf9-b02edf8b2969","full_name":"Park, Kevin S"},{"full_name":"Haiman, Zoltán","orcid":"0000-0003-3633-5403","last_name":"Haiman","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"},{"first_name":"Chengcheng","last_name":"Xin","full_name":"Xin, Chengcheng"},{"first_name":"Tzuken","last_name":"Shen","full_name":"Shen, Tzuken"},{"last_name":"Villar","first_name":"Ashley","full_name":"Villar, Ashley"},{"full_name":"Davelaar, Jordy","last_name":"Davelaar","first_name":"Jordy"}],"status":"public","title":"Self-lensing flares from black hole binaries. V. Systematic searches in LSST","_id":"23159","PlanS_conform":"1","supplementarymaterial":"yes","date_updated":"2026-10-19T08:08:21Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"apa":"Park, K. S., Haiman, Z., Xin, C., Shen, T., Villar, A., &#38; Davelaar, J. (2026). Self-lensing flares from black hole binaries. V. Systematic searches in LSST. <i>Physical Review D</i>. American Physical Society. <a href=\"https://doi.org/10.1103/p328-62sl\">https://doi.org/10.1103/p328-62sl</a>","chicago":"Park, Kevin S, Zoltán Haiman, Chengcheng Xin, Tzuken Shen, Ashley Villar, and Jordy Davelaar. “Self-Lensing Flares from Black Hole Binaries. V. Systematic Searches in LSST.” <i>Physical Review D</i>. American Physical Society, 2026. <a href=\"https://doi.org/10.1103/p328-62sl\">https://doi.org/10.1103/p328-62sl</a>.","ista":"Park KS, Haiman Z, Xin C, Shen T, Villar A, Davelaar J. 2026. Self-lensing flares from black hole binaries. V. Systematic searches in LSST. Physical Review D. 113(4), 043055.","short":"K.S. Park, Z. Haiman, C. Xin, T. Shen, A. Villar, J. Davelaar, Physical Review D 113 (2026).","ieee":"K. S. Park, Z. Haiman, C. Xin, T. Shen, A. Villar, and J. Davelaar, “Self-lensing flares from black hole binaries. V. Systematic searches in LSST,” <i>Physical Review D</i>, vol. 113, no. 4. American Physical Society, 2026.","mla":"Park, Kevin S., et al. “Self-Lensing Flares from Black Hole Binaries. V. Systematic Searches in LSST.” <i>Physical Review D</i>, vol. 113, no. 4, 043055, American Physical Society, 2026, doi:<a href=\"https://doi.org/10.1103/p328-62sl\">10.1103/p328-62sl</a>.","ama":"Park KS, Haiman Z, Xin C, Shen T, Villar A, Davelaar J. Self-lensing flares from black hole binaries. V. Systematic searches in LSST. <i>Physical Review D</i>. 2026;113(4). doi:<a href=\"https://doi.org/10.1103/p328-62sl\">10.1103/p328-62sl</a>"},"publication_identifier":{"issn":["2470-0010"],"eissn":["2470-0029"]},"acknowledgement":"We acknowledge support by NASA Grants No. 80NSSC22K0822 and No. 80NSSC24K0440 (Z. H). V. A. V. acknowledges support through the David and Lucile Packard Foundation, National Science Foundation under No. PHY-2019786 (The NSF AI Institute for Artificial Intelligence and Fundamental Interactions, [63]), No. AST-2433718, No. AST-2407922 and No. AST-2406110, as well as an Aramont Fellowship for Emerging Science Research. J. D. acknowledges support by a joint Columbia/Flatiron Postdoctoral Fellowship. Research at the Flatiron Institute is supported by the Simons Foundation. This research was supported in part by the National Science Foundation under Grant No. NSF PHY-1748958 to the Kavli Institute for Theoretical Physics (KITP). This research has made use of NASA’s Astrophysics Data System. The authors acknowledge the Texas Advanced Computing Center (TACC) at The University of Texas at Austin for providing computational resources. V. A. V. acknowledges support through the David and Lucile Packard Foundation, National Science Foundation under No. AST-2433718, No. AST-2407922 and No. AST-2406110, as well as an Aramont Fellowship for Emerging Science Research. This work is supported by the National Science Foundation under Cooperative Agreement No. PHY-2019786 (The NSF AI Institute for Artificial Intelligence and Fundamental Interactions, [63]).","scopus_import":"1","issue":"4","publication":"Physical Review D","language":[{"iso":"eng"}],"OA_place":"publisher","OA_type":"hybrid","intvolume":"       113","publication_status":"published","year":"2026","quality_controlled":"1","tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"ddc":["520"],"arxiv":1,"das_tickbox":"1","fulldoi":"https://doi.org/10.1103/p328-62sl","article_processing_charge":"Yes (in subscription journal)","has_accepted_license":"1","file_date_updated":"2026-10-19T08:06:17Z","date_published":"2026-02-25T00:00:00Z","publisher":"American Physical Society","month":"02","department":[{"_id":"GradSch"},{"_id":"ZoHa"}],"external_id":{"arxiv":["2512.08427"]},"oa":1,"day":"25","dataavailabilitystatement":"The data are not publicly available. The data are available from the authors upon reasonable request.","doi":"10.1103/p328-62sl","researchdata_availability":"no","file":[{"success":1,"date_created":"2026-10-19T08:06:17Z","checksum":"764bd6512975216dd63655da64ceeb95","access_level":"open_access","creator":"dernst","relation":"main_file","file_id":"23167","file_name":"2026_PhysicalReviewD_Park.pdf","content_type":"application/pdf","date_updated":"2026-10-19T08:06:17Z","file_size":3535182}],"volume":113,"article_number":"043055"},{"publisher":"Institute of Mathematical Statistics","mathsc":["05C80"],"month":"10","department":[{"_id":"MaKw"},{"_id":"GradSch"}],"external_id":{"arxiv":["2505.22875"]},"oa":1,"day":"01","doi":"10.1214/26-AAP2345","researchdata_availability":"no","file":[{"access_level":"open_access","relation":"main_file","creator":"dernst","success":1,"date_created":"2026-10-19T07:33:58Z","checksum":"46101e61d29cf40f0a204801d15a848f","content_type":"application/pdf","date_updated":"2026-10-19T07:33:58Z","file_name":"2026_AnnalsAppliedProbability_Hollom.pdf","file_size":320593,"file_id":"23165"}],"volume":36,"intvolume":"        36","publication_status":"published","quality_controlled":"1","year":"2026","ddc":["500"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"arxiv":1,"das_tickbox":"0","fulldoi":"https://doi.org/10.1214/26-AAP2345","article_processing_charge":"Yes (in subscription journal)","keyword":["Random regular graphs","coupling","contiguity","total variation distance","decomposition"],"has_accepted_license":"1","file_date_updated":"2026-10-19T07:33:58Z","date_published":"2026-10-01T00:00:00Z","publication_identifier":{"eissn":["2168-8737"],"issn":["1050-5164"]},"acknowledgement":"We are grateful to Béla Bollobás, to Matthew Kwan and to Fabio\r\nToninelli for their helpful comments and suggestions, and to Nicholas Wormald for useful\r\nremarks on a preliminary version of this work and pointing us towards the reference [29].\r\nThe authors would also like to thank several anonymous referees for many useful suggestions,\r\nincluding pointing out that Lemma 2.10 already appeared in [11].\r\nPart of this research was done during a visit of the fourth author to IST Austria. We thank\r\nIST Austria for its hospitality.\r\nFor open access purposes, the authors have applied a CC BY public copyright license to\r\nany author accepted manuscript version arising from this submission. L. Hollom was supported by the Internal Graduate Studentship of Trinity College, Cambridge.\r\nL. Lichev was supported by the Austrian Science Fund (FWF) grant No. 10.55776/ESP624.\r\nA. Mond was supported by UK Research and Innovation grant MR/W007320/2. Wang was\r\nsupported by the ERC Starting Grant “RANDSTRUCT” No. 101076777.","scopus_import":"1","issue":"5","publication":"Annals of Applied Probability","language":[{"iso":"eng"}],"OA_type":"hybrid","OA_place":"publisher","abstract":[{"text":"In this work we establish several monotonicity and decomposition results in the framework of random regular graphs. Among other results, we\r\nshow that, for a wide range of parameters d1 ≤ d2, there exists a coupling of\r\nG(n,d1) and G(n,d2) satisfying that G(n,d1) ⊆ G(n,d2) with high probability, confirming a conjecture of Gao, Isaev and McKay in a new regime.\r\nOur contributions include new tools for analysing contiguity and total variation distance between random regular graph models, a novel procedure for\r\ngenerating unions of random edge-disjoint perfect matchings, and refined estimates of Gao’s bounds on the number of perfect matchings in random regular graphs. In addition, we make progress towards another conjecture of Isaev,\r\nMcKay, Southwell and Zhukovskii.","lang":"eng"}],"type":"journal_article","oa_version":"Published Version","article_type":"original","status":"public","date_created":"2026-10-18T22:01:52Z","author":[{"full_name":"Hollom, Lawrence","first_name":"Lawrence","last_name":"Hollom"},{"id":"9aa8388e-d003-11ee-8458-c4c1d7447977","last_name":"Lichev","first_name":"Lyuben","full_name":"Lichev, Lyuben"},{"full_name":"Mond, Adva","first_name":"Adva","last_name":"Mond"},{"last_name":"Portier","first_name":"Julien","full_name":"Portier, Julien"},{"id":"1917d194-076e-11ed-97cd-837255f88785","last_name":"Wang","first_name":"Yiting","full_name":"Wang, Yiting"}],"title":"Monotonicity and decompositions of random regular graphs","_id":"23155","PlanS_conform":"1","date_updated":"2026-10-19T07:39:17Z","supplementarymaterial":"no","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"mla":"Hollom, Lawrence, et al. “Monotonicity and Decompositions of Random Regular Graphs.” <i>Annals of Applied Probability</i>, vol. 36, no. 5, Institute of Mathematical Statistics, 2026, pp. 4716–38, doi:<a href=\"https://doi.org/10.1214/26-AAP2345\">10.1214/26-AAP2345</a>.","ama":"Hollom L, Lichev L, Mond A, Portier J, Wang Y. Monotonicity and decompositions of random regular graphs. <i>Annals of Applied Probability</i>. 2026;36(5):4716-4738. doi:<a href=\"https://doi.org/10.1214/26-AAP2345\">10.1214/26-AAP2345</a>","ieee":"L. Hollom, L. Lichev, A. Mond, J. Portier, and Y. Wang, “Monotonicity and decompositions of random regular graphs,” <i>Annals of Applied Probability</i>, vol. 36, no. 5. Institute of Mathematical Statistics, pp. 4716–4738, 2026.","ista":"Hollom L, Lichev L, Mond A, Portier J, Wang Y. 2026. Monotonicity and decompositions of random regular graphs. Annals of Applied Probability. 36(5), 4716–4738.","short":"L. Hollom, L. Lichev, A. Mond, J. Portier, Y. Wang, Annals of Applied Probability 36 (2026) 4716–4738.","chicago":"Hollom, Lawrence, Lyuben Lichev, Adva Mond, Julien Portier, and Yiting Wang. “Monotonicity and Decompositions of Random Regular Graphs.” <i>Annals of Applied Probability</i>. Institute of Mathematical Statistics, 2026. <a href=\"https://doi.org/10.1214/26-AAP2345\">https://doi.org/10.1214/26-AAP2345</a>.","apa":"Hollom, L., Lichev, L., Mond, A., Portier, J., &#38; Wang, Y. (2026). Monotonicity and decompositions of random regular graphs. <i>Annals of Applied Probability</i>. Institute of Mathematical Statistics. <a href=\"https://doi.org/10.1214/26-AAP2345\">https://doi.org/10.1214/26-AAP2345</a>"},"page":"4716-4738","project":[{"_id":"bd95085b-d553-11ed-ba76-e55d3349be45","name":"Randomness and structure in combinatorics","grant_number":"101076777"},{"name":"THRESHOLDS IN SEMI-RANDOM PROCESSES AND GRAPH EMBEDDINGS","_id":"e19fef4c-1f3d-11f0-ac04-b8b1af6886d8","grant_number":"E624"}]},{"volume":17,"file":[{"date_created":"2026-10-19T08:32:00Z","checksum":"fee032060eb71cba73afa8e301b9ee94","success":1,"creator":"dernst","relation":"main_file","access_level":"open_access","file_id":"23169","file_size":1361818,"file_name":"2026_ChemicalScience_Wu.pdf","date_updated":"2026-10-19T08:32:00Z","content_type":"application/pdf"}],"doi":"10.1039/d6sc00798h","researchdata_availability":"yes","external_id":{"pmid":["42388815"]},"department":[{"_id":"LifeSc"}],"month":"08","publisher":"Royal Society of Chemistry","dataavailabilitystatement":"CCDC 2514117, 2514118, 2286782 and 2478322 (compound 1, compound 1d, oligomer 5, and oligomer 6, respectively) contain the supplementary crystallographic data for this paper.54a–d \r\n\r\nThe supporting data have been provided as part of the supplementary information (SI). Supplementary information: SI figures, detailed experimental protocols, crystallographic studies, and characterisation of new compounds. See DOI: https://doi.org/10.1039/d6sc00798h.","day":"19","oa":1,"fulldoi":"https://doi.org/10.1039/d6sc00798h","das_tickbox":"1","file_date_updated":"2026-10-19T08:32:00Z","date_published":"2026-08-19T00:00:00Z","has_accepted_license":"1","article_processing_charge":"Yes","year":"2026","pmid":1,"quality_controlled":"1","publication_status":"published","intvolume":"        17","tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"ddc":["540"],"language":[{"iso":"eng"}],"OA_type":"gold","OA_place":"publisher","acknowledgement":"We acknowledge financial support from the European Research Council (ERC) under the European Union's Horizon Europe Framework Programme (grant agreement no. ERC-2021-ADG-320892) and from the China Scholarship Council (CSC, predoctoral fellowship to J. W.). We thank L. Allmendinger for assistance with NMR measurements, P. Mayer for his assistance in solving the crystal structures of 1 and 1d, L. Bodero for assistance with automated solid-phase synthesis, M. Rogovoi for providing monomer precursors, and M. Loos for the purification and analysis of compounds 15a–19a. We thank M. Soler-Lopez (ID23-1, ESRF, Grenoble) and I. Bento (EMBL P13, Petra III, DESY, Hamburg) for assistance during data collection at the synchrotron beamlines.","publication_identifier":{"eissn":["2041-6539"],"issn":["2041-6520"]},"publication":"Chemical Science","issue":"32","scopus_import":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2026-10-19T08:35:08Z","supplementarymaterial":"yes","PlanS_conform":"1","DOAJ_listed":"1","page":"15479–15489","citation":{"apa":"Wu, J., Corvaglia, V., Chakrabortty, T., Mandal, P. K., &#38; Huc, I. (2026). Tailoring the major groove of DNA mimic foldamers. <i>Chemical Science</i>. Royal Society of Chemistry. <a href=\"https://doi.org/10.1039/d6sc00798h\">https://doi.org/10.1039/d6sc00798h</a>","chicago":"Wu, Jiaojiao, Valentina Corvaglia, Tulika Chakrabortty, Pradeep K Mandal, and Ivan Huc. “Tailoring the Major Groove of DNA Mimic Foldamers.” <i>Chemical Science</i>. Royal Society of Chemistry, 2026. <a href=\"https://doi.org/10.1039/d6sc00798h\">https://doi.org/10.1039/d6sc00798h</a>.","ista":"Wu J, Corvaglia V, Chakrabortty T, Mandal PK, Huc I. 2026. Tailoring the major groove of DNA mimic foldamers. Chemical Science. 17(32), 15479–15489.","short":"J. Wu, V. Corvaglia, T. Chakrabortty, P.K. Mandal, I. Huc, Chemical Science 17 (2026) 15479–15489.","ieee":"J. Wu, V. Corvaglia, T. Chakrabortty, P. K. Mandal, and I. Huc, “Tailoring the major groove of DNA mimic foldamers,” <i>Chemical Science</i>, vol. 17, no. 32. Royal Society of Chemistry, pp. 15479–15489, 2026.","ama":"Wu J, Corvaglia V, Chakrabortty T, Mandal PK, Huc I. Tailoring the major groove of DNA mimic foldamers. <i>Chemical Science</i>. 2026;17(32):15479–15489. doi:<a href=\"https://doi.org/10.1039/d6sc00798h\">10.1039/d6sc00798h</a>","mla":"Wu, Jiaojiao, et al. “Tailoring the Major Groove of DNA Mimic Foldamers.” <i>Chemical Science</i>, vol. 17, no. 32, Royal Society of Chemistry, 2026, pp. 15479–15489, doi:<a href=\"https://doi.org/10.1039/d6sc00798h\">10.1039/d6sc00798h</a>."},"article_type":"original","oa_version":"Published Version","type":"journal_article","abstract":[{"lang":"eng","text":"Single stranded helically folded aromatic oligoamides bearing anionic phosphonate side chains have been shown to bind to some DNA-binding proteins better than DNA itself. However, these DNA mimic foldamers have until now mainly consisted of a single repeat motif, like a poly(dA:dT) DNA duplex, and contained limited sequence information. Here, we introduce new monomers designed to display different chemical functionalities in the major groove of the DNA mimics. Four new Fmoc-protected amino acid monomers have been synthesized and incorporated into oligomers. Sixteen foldamer sequences were prepared on solid phase. Their conformation in solution and in the solid state and their conformational dynamics were investigated using NMR, circular dichroism, molecular modeling, and X-ray crystallography. The results show that three of four new monomers behaved as designed, and that their introduction enhances the conformational dynamics of the DNA mimic foldamers. In a fourth case, conformational behavior proved to be more complex than expected. The modified sequences retained an ability to bind to bacterial histone-like protein HU. These results showcase design strategies to manipulate large molecular biomimetics where not only side chains but also main chain components are varied. The new monomers pave the way to complex DNA mimic foldamer sequences targeting proteins that recognize sequence-selective DNA-binding proteins such as transcription factors or restriction enzymes."}],"_id":"22012","title":"Tailoring the major groove of DNA mimic foldamers","author":[{"full_name":"Wu, Jiaojiao","last_name":"Wu","first_name":"Jiaojiao"},{"full_name":"Corvaglia, Valentina","first_name":"Valentina","last_name":"Corvaglia"},{"first_name":"Tulika","last_name":"Chakrabortty","full_name":"Chakrabortty, Tulika"},{"orcid":"0000-0001-5996-956X","full_name":"Mandal, Pradeep K","last_name":"Mandal","first_name":"Pradeep K","id":"6a3def15-d4b4-11ef-9fa9-a24c1f545ec3"},{"full_name":"Huc, Ivan","first_name":"Ivan","last_name":"Huc"}],"date_created":"2026-06-16T08:04:15Z","status":"public"},{"publication_identifier":{"eissn":["1432-0835"],"issn":["0944-2669"]},"acknowledgement":"Morris Brooks gratefully acknowledges support from the ERC Advanced Grant CLaQS, grant agreement No. 834782. Open access funding provided by University of Zurich.","publication":"Calculus of Variations and Partial Differential Equations","scopus_import":"1","issue":"10","language":[{"iso":"eng"}],"OA_place":"publisher","OA_type":"hybrid","type":"journal_article","oa_version":"Published Version","article_type":"original","abstract":[{"lang":"eng","text":"We study the renormalized Nelson model in a semiclassical regime where the field becomes\r\nclassical while the particle remains quantum. The degree of classicality is measured by a\r\nsmall parameter ε << 1. In this scaling the particle evolves on microscopic times, whereas\r\nthe field exhibits nontrivial dynamics only on the macroscopic scale t = O(ε^−2). The natural\r\nsemiclassical model is the coupled Schrödinger–Klein–Gordon (SKG) system, which\r\nencodes the time-scale separation through an explicit ε-dependence. Based on this scale separation\r\nin SKG, we apply the adiabatic principle to derive a new PDE for the classical field,\r\nthe ε-free adiabatic Klein–Gordon (aKG) equation, where the field is driven by the instantaneous\r\nground state of the particle. Our main result is a norm approximation of the Nelson\r\ndynamics by the aKGsolution corrected by a quasi-free fluctuation dynamics around the classical\r\nfield, generated by a renormalized Bogoliubov–Nelson Hamiltonian. As a corollary, we\r\nobtain convergence of the reduced one-body densities for both subsystems, where the fluctuation\r\ncorrection vanishes, thereby justifying aKG as a semiclassical Born–Oppenheimer\r\ntype approximation of the renormalized Nelson model."}],"title":"Adiabatic Klein–Gordon dynamics for the renormalized Nelson model","_id":"23153","date_created":"2026-10-18T22:01:52Z","author":[{"id":"B7ECF9FC-AA38-11E9-AC9A-0930E6697425","last_name":"Brooks","first_name":"Morris","orcid":"0000-0002-6249-0928","full_name":"Brooks, Morris"},{"id":"cbddacee-2b11-11eb-a02e-a2e14d04e52d","first_name":"David Johannes","last_name":"Mitrouskas","full_name":"Mitrouskas, David Johannes"}],"status":"public","supplementarymaterial":"yes","date_updated":"2026-10-19T07:55:13Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","PlanS_conform":"1","citation":{"chicago":"Brooks, Morris, and David Johannes Mitrouskas. “Adiabatic Klein–Gordon Dynamics for the Renormalized Nelson Model.” <i>Calculus of Variations and Partial Differential Equations</i>. Springer, 2026. <a href=\"https://doi.org/10.1007/s00526-026-03436-9\">https://doi.org/10.1007/s00526-026-03436-9</a>.","apa":"Brooks, M., &#38; Mitrouskas, D. J. (2026). Adiabatic Klein–Gordon dynamics for the renormalized Nelson model. <i>Calculus of Variations and Partial Differential Equations</i>. Springer. <a href=\"https://doi.org/10.1007/s00526-026-03436-9\">https://doi.org/10.1007/s00526-026-03436-9</a>","mla":"Brooks, Morris, and David Johannes Mitrouskas. “Adiabatic Klein–Gordon Dynamics for the Renormalized Nelson Model.” <i>Calculus of Variations and Partial Differential Equations</i>, vol. 65, no. 10, 270, Springer, 2026, doi:<a href=\"https://doi.org/10.1007/s00526-026-03436-9\">10.1007/s00526-026-03436-9</a>.","ama":"Brooks M, Mitrouskas DJ. Adiabatic Klein–Gordon dynamics for the renormalized Nelson model. <i>Calculus of Variations and Partial Differential Equations</i>. 2026;65(10). doi:<a href=\"https://doi.org/10.1007/s00526-026-03436-9\">10.1007/s00526-026-03436-9</a>","ista":"Brooks M, Mitrouskas DJ. 2026. Adiabatic Klein–Gordon dynamics for the renormalized Nelson model. Calculus of Variations and Partial Differential Equations. 65(10), 270.","ieee":"M. Brooks and D. J. Mitrouskas, “Adiabatic Klein–Gordon dynamics for the renormalized Nelson model,” <i>Calculus of Variations and Partial Differential Equations</i>, vol. 65, no. 10. Springer, 2026.","short":"M. Brooks, D.J. Mitrouskas, Calculus of Variations and Partial Differential Equations 65 (2026)."},"external_id":{"arxiv":["2509.14226"],"pmid":["42865432"]},"publisher":"Springer","mathsc":["81Q05"],"department":[{"_id":"RoSe"}],"month":"10","dataavailabilitystatement":"No data are associated with this article.","day":"01","oa":1,"volume":65,"doi":"10.1007/s00526-026-03436-9","researchdata_availability":"no","file":[{"file_name":"2026_CalculusVariations_Brooks.pdf","content_type":"application/pdf","date_updated":"2026-10-19T07:53:14Z","file_size":905142,"file_id":"23166","access_level":"open_access","creator":"dernst","relation":"main_file","success":1,"date_created":"2026-10-19T07:53:14Z","checksum":"406bc9d144c35c9485d277c842d38c36"}],"article_number":"270","publication_status":"published","quality_controlled":"1","pmid":1,"year":"2026","intvolume":"        65","ddc":["500"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"das_tickbox":"1","fulldoi":"https://doi.org/10.1007/s00526-026-03436-9","arxiv":1,"has_accepted_license":"1","file_date_updated":"2026-10-19T07:53:14Z","date_published":"2026-10-01T00:00:00Z","article_processing_charge":"Yes (via OA deal)"},{"acknowledgement":"This publication is based upon work from the Ethics Crossover Group within the cost Action improve (“3Rs concepts to improve the quality of biomedical science”), ca21139, supported by cost (European Cooperation in Science and Technology).\r\nWe sincerely thank Nuno Franco for critical reviewing the manuscript.\r\nWe acknowledge support by Open Access Publishing Fund of Karl Landsteiner University, Krems, Austria.","publication_identifier":{"issn":["2588-9559"],"eissn":["2588-9567"]},"publication":"Journal of Applied Animal Ethics Research","scopus_import":"1","issue":"1","language":[{"iso":"eng"}],"OA_place":"publisher","OA_type":"hybrid","type":"journal_article","oa_version":"Published Version","article_type":"original","abstract":[{"text":"The concept of Culture of Care fosters a research environment where lab animals and humans are cared for and respected. Several aspects, such as perception of suffering, time, perceived value of an animal, potential benefits of the research, and public opinion, might influence care for animals. The European Directive 2010/63/EU on the protection of animals used for scientific purposes has represented an advance in animal welfare standards and care. However, the question of how we care about animals in practice, and of why this debate is important to reflect on still exist. Therefore, we draw upon the case study of laboratory non-human primates, to illustrate how these tensions go from theory to practice. It illustrates the conflicts and emotions, by exposing the limitations of the standards and norms in the field. Debating care requires a more comprehensive notion of care, one that goes beyond normative decisions to enable care in practice.","lang":"eng"}],"title":"How we care about laboratory animals: Acknowledging differences towards a more comprehensive concept of caring","_id":"23157","status":"public","author":[{"full_name":"Schober, Sophie","id":"80b0a0ef-4b9f-11ec-b119-8d9d94c4a1d8","first_name":"Sophie","last_name":"Schober"},{"full_name":"Vitale, Augusto","last_name":"Vitale","first_name":"Augusto"},{"full_name":"Riso, Brigida","first_name":"Brigida","last_name":"Riso"}],"date_created":"2026-10-18T22:01:53Z","date_updated":"2026-10-19T08:28:37Z","supplementarymaterial":"no","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","PlanS_conform":"1","citation":{"mla":"Schober, Sophie, et al. “How We Care about Laboratory Animals: Acknowledging Differences towards a More Comprehensive Concept of Caring.” <i>Journal of Applied Animal Ethics Research</i>, vol. 8, no. 1, Brill Academic Publishers, 2026, pp. 88–104, doi:<a href=\"https://doi.org/10.1163/25889567-bja10078\">10.1163/25889567-bja10078</a>.","ama":"Schober S, Vitale A, Riso B. How we care about laboratory animals: Acknowledging differences towards a more comprehensive concept of caring. <i>Journal of Applied Animal Ethics Research</i>. 2026;8(1):88-104. doi:<a href=\"https://doi.org/10.1163/25889567-bja10078\">10.1163/25889567-bja10078</a>","ieee":"S. Schober, A. Vitale, and B. Riso, “How we care about laboratory animals: Acknowledging differences towards a more comprehensive concept of caring,” <i>Journal of Applied Animal Ethics Research</i>, vol. 8, no. 1. Brill Academic Publishers, pp. 88–104, 2026.","short":"S. Schober, A. Vitale, B. Riso, Journal of Applied Animal Ethics Research 8 (2026) 88–104.","ista":"Schober S, Vitale A, Riso B. 2026. How we care about laboratory animals: Acknowledging differences towards a more comprehensive concept of caring. Journal of Applied Animal Ethics Research. 8(1), 88–104.","chicago":"Schober, Sophie, Augusto Vitale, and Brigida Riso. “How We Care about Laboratory Animals: Acknowledging Differences towards a More Comprehensive Concept of Caring.” <i>Journal of Applied Animal Ethics Research</i>. Brill Academic Publishers, 2026. <a href=\"https://doi.org/10.1163/25889567-bja10078\">https://doi.org/10.1163/25889567-bja10078</a>.","apa":"Schober, S., Vitale, A., &#38; Riso, B. (2026). How we care about laboratory animals: Acknowledging differences towards a more comprehensive concept of caring. <i>Journal of Applied Animal Ethics Research</i>. Brill Academic Publishers. <a href=\"https://doi.org/10.1163/25889567-bja10078\">https://doi.org/10.1163/25889567-bja10078</a>"},"page":"88-104","publisher":"Brill Academic Publishers","department":[{"_id":"PreCl"}],"month":"09","day":"01","oa":1,"volume":8,"researchdata_availability":"no","doi":"10.1163/25889567-bja10078","file":[{"file_size":464277,"file_name":"2026_JourAppliedAnimalEthicsResearch_Schober.pdf","content_type":"application/pdf","date_updated":"2026-10-19T08:25:17Z","file_id":"23168","creator":"dernst","relation":"main_file","access_level":"open_access","checksum":"a148db5e47af7cbfccaecf8cec0beff6","date_created":"2026-10-19T08:25:17Z","success":1}],"publication_status":"published","quality_controlled":"1","year":"2026","intvolume":"         8","tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"ddc":["570"],"das_tickbox":"0","fulldoi":"https://doi.org/10.1163/25889567-bja10078","has_accepted_license":"1","file_date_updated":"2026-10-19T08:25:17Z","date_published":"2026-09-01T00:00:00Z","article_processing_charge":"Yes (via OA deal)","keyword":["culture of care","culture of care in practice","lab animals","interspecies relationships"]},{"OA_place":"repository","OA_type":"green","language":[{"iso":"eng"}],"publication":"Discrete and Computational Geometry","scopus_import":"1","acknowledgement":"The authors would like to thank both Béla Bollobás and the anonymous reviewer for their careful readings of the manuscript and for their valuable comments. The first author was funded by Trinity College, Cambridge. The second author was funded in whole or in part by the Austrian Science Fund (FWF) 10.55776/ESP624. The third author was supported by UK Research and Innovation grant MR/W007320/2. The fourth author was funded by EPSRC (Engineering and Physical Sciences Research Council) and by the Cambridge Commonwealth, European and International Trust.","publication_identifier":{"eissn":["1432-0444"],"issn":["0179-5376"]},"citation":{"apa":"Hollom, L., Lichev, L., Mond, A., &#38; Portier, J. (2026). A note on high-dimensional discrepancy of subtrees. <i>Discrete and Computational Geometry</i>. Springer. <a href=\"https://doi.org/10.1007/s00454-025-00790-x\">https://doi.org/10.1007/s00454-025-00790-x</a>","chicago":"Hollom, Lawrence, Lyuben Lichev, Adva Mond, and Julien Portier. “A Note on High-Dimensional Discrepancy of Subtrees.” <i>Discrete and Computational Geometry</i>. Springer, 2026. <a href=\"https://doi.org/10.1007/s00454-025-00790-x\">https://doi.org/10.1007/s00454-025-00790-x</a>.","ista":"Hollom L, Lichev L, Mond A, Portier J. 2026. A note on high-dimensional discrepancy of subtrees. Discrete and Computational Geometry.","short":"L. Hollom, L. Lichev, A. Mond, J. Portier, Discrete and Computational Geometry (2026).","ieee":"L. Hollom, L. Lichev, A. Mond, and J. Portier, “A note on high-dimensional discrepancy of subtrees,” <i>Discrete and Computational Geometry</i>. Springer, 2026.","ama":"Hollom L, Lichev L, Mond A, Portier J. A note on high-dimensional discrepancy of subtrees. <i>Discrete and Computational Geometry</i>. 2026. doi:<a href=\"https://doi.org/10.1007/s00454-025-00790-x\">10.1007/s00454-025-00790-x</a>","mla":"Hollom, Lawrence, et al. “A Note on High-Dimensional Discrepancy of Subtrees.” <i>Discrete and Computational Geometry</i>, Springer, 2026, doi:<a href=\"https://doi.org/10.1007/s00454-025-00790-x\">10.1007/s00454-025-00790-x</a>."},"project":[{"_id":"e19fef4c-1f3d-11f0-ac04-b8b1af6886d8","name":"THRESHOLDS IN SEMI-RANDOM PROCESSES AND GRAPH EMBEDDINGS","grant_number":"E624"}],"date_updated":"2026-10-19T08:20:42Z","supplementarymaterial":"no","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"A note on high-dimensional discrepancy of subtrees","_id":"23158","author":[{"last_name":"Hollom","first_name":"Lawrence","full_name":"Hollom, Lawrence"},{"last_name":"Lichev","first_name":"Lyuben","id":"9aa8388e-d003-11ee-8458-c4c1d7447977","full_name":"Lichev, Lyuben"},{"first_name":"Adva","last_name":"Mond","full_name":"Mond, Adva"},{"last_name":"Portier","first_name":"Julien","full_name":"Portier, Julien"}],"status":"public","date_created":"2026-10-18T22:01:53Z","type":"journal_article","oa_version":"Preprint","article_type":"original","abstract":[{"text":"For a tree T and a function f:E(T)→Sd, the imbalance of a subtree T′⊆T is given by |∑e∈E(T′)f(e)|. The d-dimensional discrepancy of the tree T is the minimum, over all functions f as above, of the maximum imbalance of a subtree of T. We prove tight asymptotic bounds for the discrepancy of a tree T, confirming a conjecture of Krishna, Michaeli, Sarantis, Wang and Wang. We also settle a related conjecture on oriented discrepancy of subtrees by the same authors.","lang":"eng"}],"researchdata_availability":"no","doi":"10.1007/s00454-025-00790-x","day":"09","dataavailabilitystatement":"Data sharing not applicable to this article as no datasets were generated or analysed during the current study.","oa":1,"external_id":{"arxiv":["2412.04170"]},"publisher":"Springer","month":"10","mathsc":["05C05","05C35","11K38"],"department":[{"_id":"MaKw"}],"date_published":"2026-10-09T00:00:00Z","article_processing_charge":"No","keyword":["Trees","High-dimensional discrepancy","Oriented discrepancy"],"das_tickbox":"1","fulldoi":"https://doi.org/10.1007/s00454-025-00790-x","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2412.04170","open_access":"1"}],"arxiv":1,"publication_status":"epub_ahead","year":"2026","quality_controlled":"1"},{"publication":"Nature","scopus_import":"1","publication_identifier":{"issn":["0028-0836"],"eissn":["1476-4687"]},"acknowledgement":"This work would not have been possible without the technical support in cultivation from K. Hager, F. Baraket, A. Malits and S. Harrer. We thank the Imaging and Optics Facility (IOF) at ISTA for their help in setting up the anaerobic environment during imaging and the Cell Imaging & Ultrastructure Research (CIUS) facility at the University of Vienna for their support. Proteomics analyses were performed by the Mass Spectrometry Facility at Max Perutz Labs using the VBCF instrument pool. We also thank P. Klahn (University of Gothenburg, Sweden), M. Stadler and members of his department (HZI Braunschweig) as well as R. Cox (LUH Hannover) for providing different cytochalasans and P. Bieling (King’s College London) for discussion. Most of this work was funded by the Austrian Science Fund (FWF) with grant DOI 10.55776/Z437 (available at https://doi.org/10.55776/Z437) and further supported by an emerging field grant with grant DOI 10.55776/EFP25 (available at https://doi.org/10.55776/EFP25) to C.S. For open access purposes, the author has applied a CC BY public copyright license to any author accepted manuscript version arising from this submission. This work was further supported by a European Research Council grant ERC-SyG (101071793) to M.S., by the German Research Council through the CytoLabs consortium (Research Unit 5170 to K.R. and T.E.B.S.), by the Japan Society for the Promotion of Science Grant-in-Aid for Scientific Research 22H04985 to H.I. and M.N. Furthermore, R.H. was supported by CZI grant DAF2020-225401 and a grant (https://doi.org/10.37921/120055ratwvi) from the Chan Zuckerberg Initiative DAF. Open access funding provided by University of Vienna.","OA_place":"publisher","OA_type":"hybrid","language":[{"iso":"eng"}],"title":"Dynamic protrusions mediate crawling motility in Asgard archaea","_id":"23171","author":[{"last_name":"Radler","first_name":"Philipp","id":"40136C2A-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-9198-2182 ","full_name":"Radler, Philipp"},{"first_name":"Tobias","last_name":"Viehboeck","full_name":"Viehboeck, Tobias"},{"first_name":"Zhen-Hao","last_name":"Luo","full_name":"Luo, Zhen-Hao"},{"full_name":"Maslać, Nevena","last_name":"Maslać","first_name":"Nevena"},{"full_name":"Schmidt, Katharina","last_name":"Schmidt","first_name":"Katharina"},{"full_name":"Hauschild, Robert","orcid":"0000-0001-9843-3522","id":"4E01D6B4-F248-11E8-B48F-1D18A9856A87","first_name":"Robert","last_name":"Hauschild"},{"first_name":"Masaru K.","last_name":"Nobu","full_name":"Nobu, Masaru K."},{"full_name":"Bulgheresi, Silvia","first_name":"Silvia","last_name":"Bulgheresi"},{"full_name":"Stradal, Theresia E. B.","last_name":"Stradal","first_name":"Theresia E. B."},{"full_name":"Rottner, Klemens","first_name":"Klemens","last_name":"Rottner"},{"full_name":"Imachi, Hiroyuki","first_name":"Hiroyuki","last_name":"Imachi"},{"id":"41E9FBEA-F248-11E8-B48F-1D18A9856A87","last_name":"Sixt","first_name":"Michael K","orcid":"0000-0002-6620-9179","full_name":"Sixt, Michael K"},{"full_name":"Schleper, Christa","last_name":"Schleper","first_name":"Christa"}],"date_created":"2026-10-19T09:26:53Z","status":"public","oa_version":"Published Version","type":"journal_article","article_type":"original","abstract":[{"lang":"eng","text":"Crawling motility is a hallmark of eukaryotic cells and requires a dynamic actin cytoskeleton, regulated adhesion and spatially organized signalling pathways1,2. Asgard archaea, which are considered the closest known prokaryotic relatives of eukaryotes, potentially encode these functions within their large set of ‘eukaryotic signature proteins’3,4,5,6. The few cultivated members show a complex cell morphology, consisting of a central cell body from which several protrusions extend, filled with an actin-based cytoskeleton7,8. Here, live-cell microscopy of two organisms of the Lokiarchaea and Hodarchaea lineages7,9 showed that they dynamically and greatly change their cell shape on a minute time scale and grow and retract their extensive protrusions with a speed of 1.5–4.8 µm min−1, respectively. After adhering to a glass surface, cells use their protrusions to undergo active crawling motion. In the presence of selected actin inhibitors, however, the observed dynamics were arrested, suggesting a central role of actin in these processes. The observed cellular plasticity and motility are unique features among prokaryotes and might have been crucial for the emergence of the first eukaryotic cells that are thought to have formed through the association of a member of the Asgard archaea and an α-proteobacterium, the ancestor of mitochondria."}],"citation":{"ieee":"P. Radler <i>et al.</i>, “Dynamic protrusions mediate crawling motility in Asgard archaea,” <i>Nature</i>. Springer Nature, 2026.","short":"P. Radler, T. Viehboeck, Z.-H. Luo, N. Maslać, K. Schmidt, R. Hauschild, M.K. Nobu, S. Bulgheresi, T.E.B. Stradal, K. Rottner, H. Imachi, M.K. Sixt, C. Schleper, Nature (2026).","ista":"Radler P, Viehboeck T, Luo Z-H, Maslać N, Schmidt K, Hauschild R, Nobu MK, Bulgheresi S, Stradal TEB, Rottner K, Imachi H, Sixt MK, Schleper C. 2026. Dynamic protrusions mediate crawling motility in Asgard archaea. Nature.","mla":"Radler, Philipp, et al. “Dynamic Protrusions Mediate Crawling Motility in Asgard Archaea.” <i>Nature</i>, Springer Nature, 2026, doi:<a href=\"https://doi.org/10.1038/s41586-026-11063-9\">10.1038/s41586-026-11063-9</a>.","ama":"Radler P, Viehboeck T, Luo Z-H, et al. Dynamic protrusions mediate crawling motility in Asgard archaea. <i>Nature</i>. 2026. doi:<a href=\"https://doi.org/10.1038/s41586-026-11063-9\">10.1038/s41586-026-11063-9</a>","apa":"Radler, P., Viehboeck, T., Luo, Z.-H., Maslać, N., Schmidt, K., Hauschild, R., … Schleper, C. (2026). Dynamic protrusions mediate crawling motility in Asgard archaea. <i>Nature</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41586-026-11063-9\">https://doi.org/10.1038/s41586-026-11063-9</a>","chicago":"Radler, Philipp, Tobias Viehboeck, Zhen-Hao Luo, Nevena Maslać, Katharina Schmidt, Robert Hauschild, Masaru K. Nobu, et al. “Dynamic Protrusions Mediate Crawling Motility in Asgard Archaea.” <i>Nature</i>. Springer Nature, 2026. <a href=\"https://doi.org/10.1038/s41586-026-11063-9\">https://doi.org/10.1038/s41586-026-11063-9</a>."},"project":[{"grant_number":"101071793","name":"Pushing from within: Control of cell shape, integrity and motility by cytoskeletal pushing forces","_id":"bd91e723-d553-11ed-ba76-fe7eeb2185fd"},{"grant_number":"CZI01","name":"Tools for automation and feedback microscopy","_id":"c08e9ad1-5a5b-11eb-8a69-9d1cf3b07473"}],"date_updated":"2026-10-19T09:40:50Z","supplementarymaterial":"yes","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","PlanS_conform":"1","dataavailabilitystatement":"The plots in this manuscript were created using Jupyter Notebook; the source data for all figures have been provided in data source tables. Microscopy raw data for supplementary videos, the Jupyter notebooks to generate the plots and the raw files for the structural phylogenetic analysis are available at https://doi.org/10.6084/m9.figshare.30676367. The remaining raw microscopy data generated for this manuscript are available from https://www.ebi.ac.uk/biostudies/bioimages/studies/S-BIAD3928. The mass spectrometry proteomics data from the Co-IP experiments have been deposited to the ProteomeXchange Consortium via the PRIDE partner repository79 and are available at https://www.ebi.ac.uk/pride/archive/projects/PXD068820. The mass spectrometry proteomics data of the proteome analysis is available at https://www.ebi.ac.uk/pride/archive/projects/PXD074767. Source data are provided with this paper.","day":"30","oa":1,"external_id":{"pmid":["42816618"]},"publisher":"Springer Nature","month":"09","department":[{"_id":"MiSi"},{"_id":"Bio"}],"doi":"10.1038/s41586-026-11063-9","researchdata_availability":"yes","ddc":["570"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"publication_status":"epub_ahead","pmid":1,"year":"2026","quality_controlled":"1","has_accepted_license":"1","date_published":"2026-09-30T00:00:00Z","article_processing_charge":"Yes (via OA deal)","das_tickbox":"1","fulldoi":"https://doi.org/10.1038/s41586-026-11063-9","acknowledged_ssus":[{"_id":"Bio"}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1038/s41586-026-11063-9"}]},{"oa":1,"day":"01","dataavailabilitystatement":"All our implementations and data are archived and available at Zenodo5\r\nand are evaluated as an artifact in the ICSE 2025 artifact evaluation. Furthermore, our\r\napproach is integrated into the software verifier Bubaak [CR25] which we submitted as\r\npart of our contribution to SV-COMP 2025.","publisher":"Gesellschaft für Informatik","month":"03","department":[{"_id":"ToHe"}],"researchdata_availability":"yes","doi":"10.18420/se2026_45","file":[{"success":1,"date_created":"2026-10-19T08:39:37Z","checksum":"3371c63711ed26efa41744834d337d28","access_level":"open_access","creator":"dernst","relation":"main_file","file_id":"23170","file_name":"2026_LNI_Richter.pdf","date_updated":"2026-10-19T08:39:37Z","content_type":"application/pdf","file_size":147208}],"volume":"P-377","tmp":{"image":"/images/cc_by_sa.png","short":"CC BY-SA (4.0)","name":"Creative Commons Attribution-ShareAlike 4.0 International Public License (CC BY-SA 4.0)","legal_code_url":"https://creativecommons.org/licenses/by-sa/4.0/legalcode"},"ddc":["000"],"publication_status":"published","quality_controlled":"1","year":"2026","article_processing_charge":"No","keyword":["Software Verification","Cooperation","Program Decomposition"],"has_accepted_license":"1","conference":{"location":"Bonn, Switzerland","name":"SE: Software Engineering","end_date":"2026-02-27","start_date":"2026-02-23"},"file_date_updated":"2026-10-19T08:39:37Z","alternative_title":["Lecture Notes in Informatics"],"date_published":"2026-03-01T00:00:00Z","das_tickbox":"1","fulldoi":"https://doi.org/10.18420/se2026_45","scopus_import":"1","publication":"Software Engineering 2026","publication_identifier":{"eissn":["1617-5468"]},"OA_type":"hybrid","OA_place":"publisher","language":[{"iso":"eng"}],"date_created":"2026-08-02T22:01:54Z","author":[{"full_name":"Richter, Cedric","first_name":"Cedric","last_name":"Richter"},{"full_name":"Chalupa, Marek","last_name":"Chalupa","first_name":"Marek","id":"87e34708-d6c6-11ec-9f5b-9391e7be2463"},{"full_name":"Jakobs, Marie Christine","first_name":"Marie Christine","last_name":"Jakobs"},{"full_name":"Wehrheim, Heike","last_name":"Wehrheim","first_name":"Heike"}],"status":"public","title":"Off-the-Shelf cooperative software verification by splitting programs dynamically","_id":"22622","abstract":[{"text":"Cooperative software verification aims at improving the effectiveness and efficiency of software verification by enabling multiple verification tools to work together. Existing cooperative verification schemes, however, typically require specialized interfaces or tight integration, limiting their practical applicability. In our International Conference on Software Engineering (ICSE) 2025 publication, we introduce dynamic program splitting – a novel approach that enables cooperation between off-the-shelf verification tools without requiring any modifications. The key idea is to probe verification tools on a given verification task under a time limit and split tasks dynamically that cannot be verified under the given time constraints. The process continues recursively, incrementally identifying program parts that are particularly hard for the given verifier. The remaining unverified parts are provided to a second verifier, allowing to leverage the complementary strengths of different tools. Our evaluation on SV-COMP benchmarks demonstrates that cooperation through dynamic program splitting enables the verification of tasks that none of the individual verifiers can solve on their own.","lang":"eng"}],"oa_version":"Published Version","type":"conference","page":"41-42","citation":{"mla":"Richter, Cedric, et al. “Off-the-Shelf Cooperative Software Verification by Splitting Programs Dynamically.” <i>Software Engineering 2026</i>, vol. P-377, Gesellschaft für Informatik, 2026, pp. 41–42, doi:<a href=\"https://doi.org/10.18420/se2026_45\">10.18420/se2026_45</a>.","ama":"Richter C, Chalupa M, Jakobs MC, Wehrheim H. Off-the-Shelf cooperative software verification by splitting programs dynamically. In: <i>Software Engineering 2026</i>. Vol P-377. Gesellschaft für Informatik; 2026:41-42. doi:<a href=\"https://doi.org/10.18420/se2026_45\">10.18420/se2026_45</a>","ista":"Richter C, Chalupa M, Jakobs MC, Wehrheim H. 2026. Off-the-Shelf cooperative software verification by splitting programs dynamically. Software Engineering 2026. SE: Software Engineering, Lecture Notes in Informatics, vol. P-377, 41–42.","ieee":"C. Richter, M. Chalupa, M. C. Jakobs, and H. Wehrheim, “Off-the-Shelf cooperative software verification by splitting programs dynamically,” in <i>Software Engineering 2026</i>, Bonn, Switzerland, 2026, vol. P-377, pp. 41–42.","short":"C. Richter, M. Chalupa, M.C. Jakobs, H. Wehrheim, in:, Software Engineering 2026, Gesellschaft für Informatik, 2026, pp. 41–42.","chicago":"Richter, Cedric, Marek Chalupa, Marie Christine Jakobs, and Heike Wehrheim. “Off-the-Shelf Cooperative Software Verification by Splitting Programs Dynamically.” In <i>Software Engineering 2026</i>, P-377:41–42. Gesellschaft für Informatik, 2026. <a href=\"https://doi.org/10.18420/se2026_45\">https://doi.org/10.18420/se2026_45</a>.","apa":"Richter, C., Chalupa, M., Jakobs, M. C., &#38; Wehrheim, H. (2026). Off-the-Shelf cooperative software verification by splitting programs dynamically. In <i>Software Engineering 2026</i> (Vol. P-377, pp. 41–42). Bonn, Switzerland: Gesellschaft für Informatik. <a href=\"https://doi.org/10.18420/se2026_45\">https://doi.org/10.18420/se2026_45</a>"},"license":"https://creativecommons.org/licenses/by-sa/4.0/","supplementarymaterial":"no","date_updated":"2026-10-19T08:49:32Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87"},{"ddc":["540"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"publication_status":"epub_ahead","pmid":1,"quality_controlled":"1","year":"2026","has_accepted_license":"1","date_published":"2026-10-13T00:00:00Z","article_processing_charge":"Yes (via OA deal)","das_tickbox":"1","fulldoi":"https://doi.org/10.1021/acschembio.6c00587","acknowledged_ssus":[{"_id":"NMR"},{"_id":"LifeSc"}],"main_file_link":[{"url":"https://doi.org/10.1021/acschembio.6c00587","open_access":"1"}],"day":"13","dataavailabilitystatement":"Supporting Information is available free of charge at https://pubs.acs.org/10.1021/acschembio.6c00587.\r\n\r\nDetailed description of experimental methods; spectra supporting the residue assignment for IiMDH; relaxation analysis of IiMDH proline-Cδ sites; NMR spectra of isolated [13Cδ,15N,2Hβγ4]-Pro (PDF)","corr_author":"1","oa":1,"external_id":{"pmid":["42863127"]},"publisher":"American Chemical Society","department":[{"_id":"PaSc"},{"_id":"GradSch"}],"month":"10","doi":"10.1021/acschembio.6c00587","title":"Chemoenzymatic proline isotope labeling for solution and magic-angle spinning protein nuclear magnetic resonance","_id":"23173","author":[{"full_name":"Rohden, Darja","first_name":"Darja","last_name":"Rohden","id":"81dc668a-19fa-11f0-bf31-d56534059ef3"},{"orcid":"0000-0002-9043-136X","full_name":"Napoli, Federico","id":"d42e08e7-f4fc-11eb-af0a-d71e26138f1b","last_name":"Napoli","first_name":"Federico"},{"full_name":"Lichtenecker, Roman J.","last_name":"Lichtenecker","first_name":"Roman J."},{"full_name":"Schanda, Paul","orcid":"0000-0002-9350-7606","last_name":"Schanda","first_name":"Paul","id":"7B541462-FAF6-11E9-A490-E8DFE5697425"}],"status":"public","date_created":"2026-10-19T11:12:28Z","oa_version":"Published Version","type":"journal_article","article_type":"original","abstract":[{"lang":"eng","text":"The prevalence of proline residues in intrinsically disordered proteins, functional hinges of enzymes, and protein interaction sites highlights the importance of studying their local dynamics and interactions at atomic resolution. While nuclear magnetic resonance (NMR) spectroscopy is, in principle, ideally suited for such investigations, the absence of an amide proton precludes the use of conventional 1H–15N amide-detected experiments. 1H–13C-based approaches, though possible, remain challenging in large proteins. In this work, we present a selective labeling strategy that introduces an isolated 1H2δ–13Cδ–15N spin system in proline residues in otherwise deuterated proteins. Our method leverages the enzymatic conversion of ornithine, synthesized from cost-effective isotopic precursors. We demonstrate the utility of this approach by applying it to a 134 kDa enzyme using magic-angle spinning NMR, highlighting its potential to efficiently probe functionally relevant sites in proteins."}],"citation":{"apa":"Rohden, D., Napoli, F., Lichtenecker, R. J., &#38; Schanda, P. (2026). Chemoenzymatic proline isotope labeling for solution and magic-angle spinning protein nuclear magnetic resonance. <i>ACS Chemical Biology</i>. American Chemical Society. <a href=\"https://doi.org/10.1021/acschembio.6c00587\">https://doi.org/10.1021/acschembio.6c00587</a>","chicago":"Rohden, Darja, Federico Napoli, Roman J. Lichtenecker, and Paul Schanda. “Chemoenzymatic Proline Isotope Labeling for Solution and Magic-Angle Spinning Protein Nuclear Magnetic Resonance.” <i>ACS Chemical Biology</i>. American Chemical Society, 2026. <a href=\"https://doi.org/10.1021/acschembio.6c00587\">https://doi.org/10.1021/acschembio.6c00587</a>.","ieee":"D. Rohden, F. Napoli, R. J. Lichtenecker, and P. Schanda, “Chemoenzymatic proline isotope labeling for solution and magic-angle spinning protein nuclear magnetic resonance,” <i>ACS Chemical Biology</i>. American Chemical Society, 2026.","short":"D. Rohden, F. Napoli, R.J. Lichtenecker, P. Schanda, ACS Chemical Biology (2026).","ista":"Rohden D, Napoli F, Lichtenecker RJ, Schanda P. 2026. Chemoenzymatic proline isotope labeling for solution and magic-angle spinning protein nuclear magnetic resonance. ACS Chemical Biology.","mla":"Rohden, Darja, et al. “Chemoenzymatic Proline Isotope Labeling for Solution and Magic-Angle Spinning Protein Nuclear Magnetic Resonance.” <i>ACS Chemical Biology</i>, American Chemical Society, 2026, doi:<a href=\"https://doi.org/10.1021/acschembio.6c00587\">10.1021/acschembio.6c00587</a>.","ama":"Rohden D, Napoli F, Lichtenecker RJ, Schanda P. Chemoenzymatic proline isotope labeling for solution and magic-angle spinning protein nuclear magnetic resonance. <i>ACS Chemical Biology</i>. 2026. doi:<a href=\"https://doi.org/10.1021/acschembio.6c00587\">10.1021/acschembio.6c00587</a>"},"project":[{"grant_number":"I05812","_id":"eb9c82eb-77a9-11ec-83b8-aadd536561cf","name":"AlloSpace. The emergence and mechanisms of allostery"}],"date_updated":"2026-10-19T11:20:33Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication":"ACS Chemical Biology","scopus_import":"1","publication_identifier":{"issn":["1554-8929"],"eissn":["1554-8937"]},"acknowledgement":"We thank Undina Guillerm, Rajkumar Singh and Anna Kapitonova for help with protein production. We are grateful to Dominique Madern for discussions and for providing the plasmid of IiMDH. We acknowledge the Scientific Service Units (SSU) of the Institute of Science and Technology Austria (ISTA) through resources provided by the NMR Facility and the Lab Support Facility, as well as the NMR centre and MS centre of the University of Vienna. This work was supported by the Austrian Science Fund (FWF; project number I5812-B) through a French-Austrian binational research project, as well as by the L’Oréal-UNESCO For Women in Science Fellowship, awarded in cooperation with the Austrian Academy of Sciences (ÖAW) and the Austrian Commission for UNESCO.","OA_place":"publisher","OA_type":"hybrid","language":[{"iso":"eng"}]},{"citation":{"mla":"Torres Rodriguez, Santiago. “Implications for the Formation of Oort Cloud-like Structures and Interstellar Comets in Dense Environments.” <i>Astronomy &#38; Astrophysics</i>, vol. 708, A301, EDP Sciences, 2026, doi:<a href=\"https://doi.org/10.1051/0004-6361/202554978\">10.1051/0004-6361/202554978</a>.","ama":"Torres Rodriguez S. Implications for the formation of Oort cloud-like structures and interstellar comets in dense environments. <i>Astronomy &#38; Astrophysics</i>. 2026;708. doi:<a href=\"https://doi.org/10.1051/0004-6361/202554978\">10.1051/0004-6361/202554978</a>","ista":"Torres Rodriguez S. 2026. Implications for the formation of Oort cloud-like structures and interstellar comets in dense environments. Astronomy &#38; Astrophysics. 708, A301.","short":"S. Torres Rodriguez, Astronomy &#38; Astrophysics 708 (2026).","ieee":"S. Torres Rodriguez, “Implications for the formation of Oort cloud-like structures and interstellar comets in dense environments,” <i>Astronomy &#38; Astrophysics</i>, vol. 708. EDP Sciences, 2026.","chicago":"Torres Rodriguez, Santiago. “Implications for the Formation of Oort Cloud-like Structures and Interstellar Comets in Dense Environments.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2026. <a href=\"https://doi.org/10.1051/0004-6361/202554978\">https://doi.org/10.1051/0004-6361/202554978</a>.","apa":"Torres Rodriguez, S. (2026). Implications for the formation of Oort cloud-like structures and interstellar comets in dense environments. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202554978\">https://doi.org/10.1051/0004-6361/202554978</a>"},"DOAJ_listed":"1","project":[{"_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c","call_identifier":"H2020","name":"IST-BRIDGE: International postdoctoral program","grant_number":"101034413"}],"PlanS_conform":"1","date_updated":"2026-10-20T08:14:04Z","supplementarymaterial":"no","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","status":"public","author":[{"first_name":"Santiago","last_name":"Torres Rodriguez","id":"a8df4360-4328-11ee-8f1a-e502d0c83fc2","full_name":"Torres Rodriguez, Santiago","orcid":"0000-0002-3150-8988"}],"date_created":"2026-10-04T22:01:54Z","title":"Implications for the formation of Oort cloud-like structures and interstellar comets in dense environments","_id":"23046","abstract":[{"lang":"eng","text":"Most stars form in dense stellar environments, where frequent close encounters can strongly perturb and reshape the early architecture of planetary systems. The Solar System, with its rich population of distant comets, provides a natural laboratory to study these processes. We performed detailed numerical simulations using the LonelyPlanets framework that combines NBODY6++GPU and REBOUND to explore the evolution of debris disks around Solar System analogues embedded in stellar clusters. Two initial configurations are considered, the Extended model and the Compact model, each containing four giant planets and either an extended or compact debris disk. We find that compact disks primarily form Kuiper belt and scattered disk-like populations through planet–disk interactions, while extended disks are more strongly shaped by stellar encounters, producing Oort cloud-like structures and interstellar comets with ejection velocities of 1–3 km s−1. Stellar perturbations are most effective for encounter inclinations between 0° and 30°, giving rise to distinct dynamical populations, like Sednoids, and inner Oort cloud analogues, and a characteristic tail in semimajor axis-eccentricity space. In coplanar encounters, the disk remains largely flattened, whereas polar flybys redistribute angular momentum vertically, producing nearly isotropic outer populations that resemble an emerging Oort cloud. Our results suggest that cometary reservoirs and interstellar objects are natural byproducts of planet–disk interactions and stellar flybys in dense clusters, linking the architecture of outer planetary systems to their birth environments."}],"type":"journal_article","oa_version":"Published Version","article_type":"original","OA_place":"publisher","OA_type":"diamond","language":[{"iso":"eng"}],"scopus_import":"1","publication":"Astronomy & Astrophysics","acknowledgement":"We thank the referee for their suggestions and comments,\r\nwhich helped us improve the quality and clarity of the paper. S.T. thanks\r\nYlva Götberg, Maxwell Cai, Diptajyoti Mukherjee, Simon Portegies Zwart, and\r\nAnthony Brown for their valuable feedback and comments. S.T. acknowledges\r\nthe funding from the European Union’s Horizon 2020 research and innovation\r\nprogram under the Marie Skłodowska-Curie grant agreement No 101034413.","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"ec_funded":1,"article_processing_charge":"No","has_accepted_license":"1","file_date_updated":"2026-10-07T12:22:19Z","date_published":"2026-04-01T00:00:00Z","arxiv":1,"das_tickbox":"1","fulldoi":"https://doi.org/10.1051/0004-6361/202554978","tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"ddc":["520"],"intvolume":"       708","publication_status":"published","quality_controlled":"1","year":"2026","article_number":"A301","researchdata_availability":"no","doi":"10.1051/0004-6361/202554978","file":[{"file_id":"23076","file_size":9478404,"file_name":"2026_AstronomyAstrophysics_Torres.pdf","date_updated":"2026-10-07T12:22:19Z","content_type":"application/pdf","checksum":"3ea1c5f0fabaa005a4aac7e46f4b6d9c","date_created":"2026-10-07T12:22:19Z","success":1,"creator":"dernst","relation":"main_file","access_level":"open_access"}],"volume":708,"oa":1,"corr_author":"1","dataavailabilitystatement":"Movies associated with Figs. 3 and 9 are available at https://www.aanda.org","day":"01","publisher":"EDP Sciences","month":"04","department":[{"_id":"LiBu"}],"external_id":{"arxiv":["2510.23653"]}},{"language":[{"iso":"eng"}],"OA_place":"publisher","OA_type":"gold","acknowledgement":"We thank P. Luzio, N. Bright, and M. S. Robinson for helpful discussions;\r\nJ. Stacey and Y. Fujiharu for technical discussions and assistance; F. Beck for assistance with\r\ncomputing infrastructure; and M. Riggi for discussion of data presentation and figure design.\r\nCryo-E\r\nM data was collected at the Department of Cell and Virus Structure, Max Planck Institute\r\nof Biochemistry. Funding: This work was funded by: the Wellcome Trust, Wellcome Discovery\r\nAward 227915/Z/23/Z (to D.J.O., J.A.G.B., and D.G.S.) and Wellcome PRF 207455/Z/17/Z (to\r\nD.J.O.); the Max Planck Society (to J.A.G.B.); the Medical Research Council (UKRI) MC_\r\nUP_1201/16 (to J.A.G.B.) and MRC DT P MR/N013433/1 (to J.G.G.K.); EMBO Long-term\r\nPostdoctoral Fellowship ALT F-383-\r\n2022\r\n(to G.T.); and the Wellcome Trust/Royal Society, Sir\r\nHenry Dale Fellowship 210481 (to D.C.G) and the Biotechnology and Biological Sciences\r\nResearch Council (UKRI) responsive mode grants BB/W005905/1 and UKRI715 (to D.C.G.).","publication_identifier":{"eissn":["2375-2548"]},"publication":"Science Advances","scopus_import":"1","issue":"20","date_updated":"2026-10-20T08:11:46Z","supplementarymaterial":"yes","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","PlanS_conform":"1","citation":{"mla":"Kaufman, Jonathan G. G., et al. “Architecture of Clathrin-Independent AP3:ARF1-Coated Carriers.” <i>Science Advances</i>, vol. 12, no. 20, eaed1529, AAAS, 2026, doi:<a href=\"https://doi.org/10.1126/sciadv.aed1529\">10.1126/sciadv.aed1529</a>.","ama":"Kaufman JGG, Tagiltsev G, Stalder DS, et al. Architecture of clathrin-independent AP3:ARF1-coated carriers. <i>Science Advances</i>. 2026;12(20). doi:<a href=\"https://doi.org/10.1126/sciadv.aed1529\">10.1126/sciadv.aed1529</a>","ieee":"J. G. G. Kaufman <i>et al.</i>, “Architecture of clathrin-independent AP3:ARF1-coated carriers,” <i>Science Advances</i>, vol. 12, no. 20. AAAS, 2026.","short":"J.G.G. Kaufman, G. Tagiltsev, D.S. Stalder, R.J. Taylor, I. Sava, H. Guo, K.A. Ciazynska, N.R. Zaccai, S.R. Gray, Y. Vallis, S. Höning, B.T. Kelly, D.C. Gershlick, J.A.G. Briggs, D.J. Owen, Science Advances 12 (2026).","ista":"Kaufman JGG, Tagiltsev G, Stalder DS, Taylor RJ, Sava I, Guo H, Ciazynska KA, Zaccai NR, Gray SR, Vallis Y, Höning S, Kelly BT, Gershlick DC, Briggs JAG, Owen DJ. 2026. Architecture of clathrin-independent AP3:ARF1-coated carriers. Science Advances. 12(20), eaed1529.","chicago":"Kaufman, Jonathan G.G., Grigory Tagiltsev, Danièle S. Stalder, Rebecca J. Taylor, Ioana Sava, Hui Guo, Katarzyna A. Ciazynska, et al. “Architecture of Clathrin-Independent AP3:ARF1-Coated Carriers.” <i>Science Advances</i>. AAAS, 2026. <a href=\"https://doi.org/10.1126/sciadv.aed1529\">https://doi.org/10.1126/sciadv.aed1529</a>.","apa":"Kaufman, J. G. G., Tagiltsev, G., Stalder, D. S., Taylor, R. J., Sava, I., Guo, H., … Owen, D. J. (2026). Architecture of clathrin-independent AP3:ARF1-coated carriers. <i>Science Advances</i>. AAAS. <a href=\"https://doi.org/10.1126/sciadv.aed1529\">https://doi.org/10.1126/sciadv.aed1529</a>"},"DOAJ_listed":"1","oa_version":"Published Version","type":"journal_article","article_type":"original","abstract":[{"lang":"eng","text":"The AP3 complex mediates cargo sorting and carrier assembly for the trafficking of transmembrane proteins from endosomes to lysosomes. AP3 is generally believed to localize to clathrin-free, ARF1-positive, elongated carriers in cells, but the architecture of AP3-based coats was unknown. Using in vitro reconstitution and cryo–electron tomography, we demonstrate that AP3:ARF1 spontaneously remodels membranes containing cargo and the phosphoinositide PI(3,5)P\r\n                    <jats:sub>2</jats:sub>\r\n                    into tubular structures coated in spiraling rows of AP3 arches and ARF1 dimers. Targeted point mutations disrupting critical AP3:ARF1 and AP3:AP3 lattice interfaces disrupt AP3 recruitment, carrier formation, and lysosomal cargo trafficking in cells. We propose that AP3 generates tubular carriers on endosomes by organizing ARF1 dimers into elongated membrane-deforming arrays while simultaneously selecting cargo. By demonstrating that AP3:ARF1 can generate carriers without using a clathrin lattice, we explain the clathrin independence of AP3-mediated trafficking."}],"title":"Architecture of clathrin-independent AP3:ARF1-coated carriers","_id":"22306","date_created":"2026-07-13T10:52:15Z","author":[{"first_name":"Jonathan G.G.","last_name":"Kaufman","full_name":"Kaufman, Jonathan G.G."},{"first_name":"Grigory","last_name":"Tagiltsev","full_name":"Tagiltsev, Grigory"},{"first_name":"Danièle S.","last_name":"Stalder","full_name":"Stalder, Danièle S."},{"full_name":"Taylor, Rebecca J.","first_name":"Rebecca J.","last_name":"Taylor"},{"last_name":"Sava","first_name":"Ioana","full_name":"Sava, Ioana"},{"full_name":"Guo, Hui","first_name":"Hui","last_name":"Guo"},{"full_name":"Ciazynska, Katarzyna A.","first_name":"Katarzyna A.","last_name":"Ciazynska"},{"full_name":"Zaccai, Nathan R.","first_name":"Nathan R.","last_name":"Zaccai"},{"full_name":"Gray, Sally R.","first_name":"Sally R.","last_name":"Gray"},{"id":"05A2795C-31B5-11EA-83A7-7DA23DDC885E","last_name":"Vallis","first_name":"Yvonne","full_name":"Vallis, Yvonne","orcid":"0000-0002-5408-5906"},{"full_name":"Höning, Stefan","last_name":"Höning","first_name":"Stefan"},{"first_name":"Bernard T.","last_name":"Kelly","full_name":"Kelly, Bernard T."},{"full_name":"Gershlick, David C.","last_name":"Gershlick","first_name":"David C."},{"full_name":"Briggs, John A.G.","first_name":"John A.G.","last_name":"Briggs"},{"last_name":"Owen","first_name":"David J.","full_name":"Owen, David J."}],"status":"public","volume":12,"researchdata_availability":"yes","doi":"10.1126/sciadv.aed1529","file":[{"checksum":"461b5f73941fe6b5df2a129c7563601f","date_created":"2026-07-14T06:45:37Z","success":1,"relation":"main_file","creator":"dernst","access_level":"open_access","file_id":"22331","file_size":8269526,"date_updated":"2026-07-14T06:45:37Z","content_type":"application/pdf","file_name":"2026_ScienceAdv_Kaufman.pdf"}],"article_number":"eaed1529","publisher":"AAAS","month":"05","department":[{"_id":"MaDe"}],"dataavailabilitystatement":"Structures determined by electron microscopy are deposited in the Electron\r\nMicroscopy Data Bank under accession codes EMD-54255,\r\nEMD-54256,\r\nEMD-54257,\r\nand\r\nEMD-54258.\r\nCorresponding molecular models are deposited in the Protein Data Bank under\r\naccession codes 9RTW, 9RTX, 9RTY, and 9RTZ. All additional data and code required to\r\nevaluate and reproduce the results in the paper are present in the paper and/or the\r\nsupplementary materials. Any code used is explicitly stated and available in the original\r\npublications. Plasmids and cell lines can be requested by writing to D.C.G. (dg553@ cam. ac. uk)\r\nor D.J.O. (djo30@ cam. ac. uk). All reasonable requests for materials will be honored.","day":"15","oa":1,"das_tickbox":"1","fulldoi":"https://doi.org/10.1126/sciadv.aed1529","has_accepted_license":"1","file_date_updated":"2026-07-14T06:45:37Z","date_published":"2026-05-15T00:00:00Z","article_processing_charge":"Yes","publication_status":"published","year":"2026","quality_controlled":"1","intvolume":"        12","ddc":["570"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"}},{"ddc":["530"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"intvolume":"        12","publication_status":"published","year":"2026","quality_controlled":"1","article_processing_charge":"Yes","has_accepted_license":"1","date_published":"2026-02-13T00:00:00Z","file_date_updated":"2026-02-24T07:23:32Z","acknowledged_ssus":[{"_id":"NanoFab"},{"_id":"M-Shop"}],"arxiv":1,"fulldoi":"https://doi.org/10.1126/sciadv.ady7222","corr_author":"1","oa":1,"day":"13","publisher":"AAAS","department":[{"_id":"MaSe"},{"_id":"AnHi"},{"_id":"GeKa"}],"month":"02","external_id":{"arxiv":["2504.09721"]},"article_number":"eady7222","doi":"10.1126/sciadv.ady7222","file":[{"file_id":"21353","file_size":2775975,"content_type":"application/pdf","date_updated":"2026-02-24T07:23:32Z","file_name":"2026_ScienceAdv_Bubis.pdf","checksum":"8402f322f8f0e858b1d9aac57e306e31","date_created":"2026-02-24T07:23:32Z","success":1,"relation":"main_file","creator":"dernst","access_level":"open_access"}],"volume":12,"author":[{"first_name":"Anton","last_name":"Bubis","id":"1f6212b5-f795-11ec-9c0c-de4780302890","full_name":"Bubis, Anton"},{"full_name":"Vigliotti, Lucia","id":"539e1e1a-e604-11ee-a1df-f02b018e5c8c","first_name":"Lucia","last_name":"Vigliotti"},{"full_name":"Serbyn, Maksym","orcid":"0000-0002-2399-5827","id":"47809E7E-F248-11E8-B48F-1D18A9856A87","first_name":"Maksym","last_name":"Serbyn"},{"orcid":"0000-0003-2607-2363","full_name":"Higginbotham, Andrew P","id":"4AD6785A-F248-11E8-B48F-1D18A9856A87","last_name":"Higginbotham","first_name":"Andrew P"}],"date_created":"2026-02-22T20:47:38Z","status":"public","title":"Non-equilibrium plasmon liquid in a Josephson junction chain","_id":"21340","abstract":[{"text":"Equilibrium quantum systems are often described by a gas of weakly interacting normal modes. Bringing such systems far from equilibrium, however, can drastically enhance mode-to-mode interactions. Understanding the resulting liquid is a fundamental question for quantum statistical mechanics and a practical question for engineering driven quantum devices. To tackle this question, we probe the non-equilibrium kinetics of one-dimensional plasmons in a long chain of Josephson junctions. We introduce multimode spectroscopy to controllably study the departure from equilibrium, witnessing the evolution from pairwise coupling between plasma modes at weak driving to dramatic, high-order, cascaded couplings at strong driving. Scaling to many-mode drives, we stimulate interactions between hundreds of modes, resulting in near-continuum internal dynamics. Imaging the resulting non-equilibrium plasmon populations, we then resolve the nonlocal redistribution of energy in the response to a weak perturbation—an explicit verification of the emergence of a strongly interacting, non-equilibrium liquid of plasmons.","lang":"eng"}],"oa_version":"Published Version","type":"journal_article","article_type":"original","DOAJ_listed":"1","citation":{"chicago":"Bubis, Anton, Lucia Vigliotti, Maksym Serbyn, and Andrew P Higginbotham. “Non-Equilibrium Plasmon Liquid in a Josephson Junction Chain.” <i>Science Advances</i>. AAAS, 2026. <a href=\"https://doi.org/10.1126/sciadv.ady7222\">https://doi.org/10.1126/sciadv.ady7222</a>.","apa":"Bubis, A., Vigliotti, L., Serbyn, M., &#38; Higginbotham, A. P. (2026). Non-equilibrium plasmon liquid in a Josephson junction chain. <i>Science Advances</i>. AAAS. <a href=\"https://doi.org/10.1126/sciadv.ady7222\">https://doi.org/10.1126/sciadv.ady7222</a>","ama":"Bubis A, Vigliotti L, Serbyn M, Higginbotham AP. Non-equilibrium plasmon liquid in a Josephson junction chain. <i>Science Advances</i>. 2026;12(7). doi:<a href=\"https://doi.org/10.1126/sciadv.ady7222\">10.1126/sciadv.ady7222</a>","mla":"Bubis, Anton, et al. “Non-Equilibrium Plasmon Liquid in a Josephson Junction Chain.” <i>Science Advances</i>, vol. 12, no. 7, eady7222, AAAS, 2026, doi:<a href=\"https://doi.org/10.1126/sciadv.ady7222\">10.1126/sciadv.ady7222</a>.","ista":"Bubis A, Vigliotti L, Serbyn M, Higginbotham AP. 2026. Non-equilibrium plasmon liquid in a Josephson junction chain. Science Advances. 12(7), eady7222.","ieee":"A. Bubis, L. Vigliotti, M. Serbyn, and A. P. Higginbotham, “Non-equilibrium plasmon liquid in a Josephson junction chain,” <i>Science Advances</i>, vol. 12, no. 7. AAAS, 2026.","short":"A. Bubis, L. Vigliotti, M. Serbyn, A.P. Higginbotham, Science Advances 12 (2026)."},"PlanS_conform":"1","date_updated":"2026-10-20T08:10:46Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","issue":"7","publication":"Science Advances","acknowledgement":"We thank V. Vitelli, M. Fruchart, and A. Burshstein for helpful input. We acknowledge technical support from the Nanofabrication Facility and the MIBA machine shop at IST Austria. This research was supported in part by grant NSF PHY-2309135 to the Kavli Institute for Theoretical Physics (KITP), by the Austrian Science Fund (FWF) SFB F86, and by the NOMIS foundation.","publication_identifier":{"eissn":["2375-2548"]},"OA_type":"gold","OA_place":"publisher","language":[{"iso":"eng"}]},{"title":"Extracellular vesicles mediate stem cell signaling and systemic RNAi in planarians","_id":"21383","status":"public","date_created":"2026-03-02T10:08:07Z","author":[{"full_name":"Sasidharan, Vidyanand","first_name":"Vidyanand","last_name":"Sasidharan"},{"full_name":"Ancellotti, Laura","first_name":"Laura","last_name":"Ancellotti"},{"full_name":"Doddihal, Viraj","id":"034e0824-174b-11ef-b32b-9366a0e70d1c","last_name":"Doddihal","first_name":"Viraj"},{"full_name":"Brewster, Carolyn","first_name":"Carolyn","last_name":"Brewster"},{"last_name":"Mann","first_name":"Frederick","full_name":"Mann, Frederick"},{"full_name":"McKinney, Mary Cathleen","first_name":"Mary Cathleen","last_name":"McKinney"},{"full_name":"Varberg, Joseph","first_name":"Joseph","last_name":"Varberg"},{"full_name":"Ross, Eric","first_name":"Eric","last_name":"Ross"},{"full_name":"Deng, Fengyan","last_name":"Deng","first_name":"Fengyan"},{"full_name":"Yi, Kexi","last_name":"Yi","first_name":"Kexi"},{"last_name":"Sánchez Alvarado","first_name":"Alejandro","full_name":"Sánchez Alvarado, Alejandro"}],"type":"journal_article","oa_version":"Published Version","article_type":"original","abstract":[{"lang":"eng","text":"Planarian flatworms are known for their remarkable regenerative capacity; however, the precise intercellular communication mechanisms underlying this process remain unsolved. Here, we report the discovery and characterization of abundant extracellular vesicles (EVs) in planarians. Using imaging and molecular analysis, we show conservation of biogenesis, morphology, and protein composition of planarian EVs. Environmental stressors significantly elevate EV release, indicating that planarians dynamically regulate vesicle production. Functionally, planarian EVs mediate intercellular communication by transferring regulatory signals: We find that they shuttle small RNAs that effect systemic RNA interference (RNAi) throughout the organism. Notably, gene knockdown experiments reveal a crucial role for AGO-3, a member of the Argonaute family of proteins, in modulating the association of small interfering RNAs with EVs, linking the intracellular RNAi machinery to EV-based signaling. These findings highlight EVs as pivotal mediators of cell-cell communication in planarians, with broad implications for understanding the coordination of gene regulation and tissue regeneration in animals."}],"license":"https://creativecommons.org/licenses/by-nc/4.0/","DOAJ_listed":"1","citation":{"apa":"Sasidharan, V., Ancellotti, L., Doddihal, V., Brewster, C., Mann, F., McKinney, M. C., … Sánchez Alvarado, A. (2026). Extracellular vesicles mediate stem cell signaling and systemic RNAi in planarians. <i>Science Advances</i>. AAAS. <a href=\"https://doi.org/10.1126/sciadv.ady1461\">https://doi.org/10.1126/sciadv.ady1461</a>","chicago":"Sasidharan, Vidyanand, Laura Ancellotti, Viraj Doddihal, Carolyn Brewster, Frederick Mann, Mary Cathleen McKinney, Joseph Varberg, et al. “Extracellular Vesicles Mediate Stem Cell Signaling and Systemic RNAi in Planarians.” <i>Science Advances</i>. AAAS, 2026. <a href=\"https://doi.org/10.1126/sciadv.ady1461\">https://doi.org/10.1126/sciadv.ady1461</a>.","short":"V. Sasidharan, L. Ancellotti, V. Doddihal, C. Brewster, F. Mann, M.C. McKinney, J. Varberg, E. Ross, F. Deng, K. Yi, A. Sánchez Alvarado, Science Advances 12 (2026).","ista":"Sasidharan V, Ancellotti L, Doddihal V, Brewster C, Mann F, McKinney MC, Varberg J, Ross E, Deng F, Yi K, Sánchez Alvarado A. 2026. Extracellular vesicles mediate stem cell signaling and systemic RNAi in planarians. Science Advances. 12(6), eady1461.","ieee":"V. Sasidharan <i>et al.</i>, “Extracellular vesicles mediate stem cell signaling and systemic RNAi in planarians,” <i>Science Advances</i>, vol. 12, no. 6. AAAS, 2026.","mla":"Sasidharan, Vidyanand, et al. “Extracellular Vesicles Mediate Stem Cell Signaling and Systemic RNAi in Planarians.” <i>Science Advances</i>, vol. 12, no. 6, eady1461, AAAS, 2026, doi:<a href=\"https://doi.org/10.1126/sciadv.ady1461\">10.1126/sciadv.ady1461</a>.","ama":"Sasidharan V, Ancellotti L, Doddihal V, et al. Extracellular vesicles mediate stem cell signaling and systemic RNAi in planarians. <i>Science Advances</i>. 2026;12(6). doi:<a href=\"https://doi.org/10.1126/sciadv.ady1461\">10.1126/sciadv.ady1461</a>"},"date_updated":"2026-10-20T08:11:11Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication":"Science Advances","scopus_import":"1","issue":"6","publication_identifier":{"eissn":["2375-2548"]},"acknowledgement":"We thank all the Sánchez Alvarado lab members for inputs and discussions. We are grateful to the Stowers Aquatics (particularly the Planarian team), Microscopy, and Molecular Biology core facilities for technical contributions and method development; e. n. lissek and A. Fujii from Oni US and S. Wang from the University of Missouri, Kansas city, for assistance with dStORM imaging; and d. Alburty and A. Page from innovaprep for assisting with the ntA. We also thank M. Miller for the illustrations. This work was supported by the hhMi and Stowers institute. ","OA_place":"publisher","OA_type":"gold","language":[{"iso":"eng"}],"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by-nc/4.0/legalcode","short":"CC BY-NC (4.0)","name":"Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)","image":"/images/cc_by_nc.png"},"ddc":["570"],"publication_status":"published","year":"2026","quality_controlled":"1","intvolume":"        12","has_accepted_license":"1","file_date_updated":"2026-03-02T14:19:35Z","date_published":"2026-02-01T00:00:00Z","article_processing_charge":"Yes","fulldoi":"https://doi.org/10.1126/sciadv.ady1461","day":"01","oa":1,"publisher":"AAAS","department":[{"_id":"CaHe"}],"month":"02","article_number":"eady1461","volume":12,"doi":"10.1126/sciadv.ady1461","file":[{"access_level":"open_access","creator":"dernst","relation":"main_file","success":1,"checksum":"fa9f6dafe3538e2d2872c098e06d1712","date_created":"2026-03-02T14:19:35Z","content_type":"application/pdf","date_updated":"2026-03-02T14:19:35Z","file_name":"2026_ScienceAdv_Sasidharan.pdf","file_size":2841345,"file_id":"21389"}]},{"scopus_import":"1","issue":"13","publication":"Science Advances","publication_identifier":{"eissn":["2375-2548"]},"acknowledgement":"We thank I. Salecker (Flybow), B. Altenhein (Fas2-Gal4Mz507), A. Nose (UAS-intra- and extra-Fas2::YFP), and C. S. Goodman (UAS-Fas2PEST+/−), as well as the Bloomington Stock Center for providing materials and fly stocks. We thank S. Waddell and the lab, especially B. Senapati, for providing the opportunity to conduct memory experiments at the CNCB, University of Oxford, and for supervision and discussions during this period. We also thank W. Kallina, S. Ilgerl, D. Bartel, A. Grimm, and A. Litin for technical support and the Hummel Lab for stimulating discussions and critical comments on the manuscript. We acknowledge the early exploratory work of A. Mattia, S. Trkulja, C. Schönherr, S. Bogner, B. Simpson, L. Tomasek, H. Roth, H. Vokač, R. Gredler, F. Kapelari, T. Kolarova, C. Ignitsch, Á. Bautista-Soldevila, and M. Kassem.\r\nThis research was funded by the University of Vienna, the Vienna Doctoral School Cognition, Behaviour and Neuroscience (uni:docs fellowship) (to J.W.M.) and by the Austrian Science Fund (FWF) (Cluster of Excellence Neuronal Circuits in Health and Disease, grant DOI 10.55776/COE16; https://www.fwf.ac.at/en/research-radar/10.55776/COE16) (to T.H.). For open access purposes, the author has applied a CC BY public copyright license to any author-accepted manuscript version arising from this submission.","OA_type":"gold","OA_place":"publisher","language":[{"iso":"eng"}],"status":"public","date_created":"2026-04-12T22:01:48Z","author":[{"first_name":"Johann W.","last_name":"Markovitsch","full_name":"Markovitsch, Johann W."},{"full_name":"Mitić, Daniel","first_name":"Daniel","last_name":"Mitić"},{"full_name":"Del Pilar Jiménez García, Alisa","first_name":"Alisa","last_name":"Del Pilar Jiménez García"},{"orcid":"0009-0003-0415-7603","full_name":"Zane, Alsberga","first_name":"Alsberga","last_name":"Zane","id":"60f7509a-f652-11ea-9d86-b963d6490d7c"},{"last_name":"Kainz","first_name":"Sarah","full_name":"Kainz, Sarah"},{"last_name":"Kaur","first_name":"Rashmit","full_name":"Kaur, Rashmit"},{"full_name":"Hummel, Thomas","first_name":"Thomas","last_name":"Hummel"}],"title":"Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity","_id":"21707","abstract":[{"lang":"eng","text":"Structural and functional differences between brain hemispheres are a common feature of animal nervous systems with reduced bilateral asymmetry often linked to impaired cognitive performance. How neuronal left-right asymmetry is initiated and integrated into a bilaterally symmetrical ground pattern is poorly understood. Here, we show that the directional asymmetry of a Drosophila central brain circuit originates from axonal interactions of two types of bilateral pioneer neurons. Subsequent recruitment of neighboring neurons into the asymmetric neuropil primordium results in hemisphere-specific microcircuits. Circuit lateralization requires dynamic expression of the cell adhesion molecule Fasciclin 2 to maintain structural plasticity in axonal remodeling. Reduced circuit asymmetry following cell type–specific Fasciclin 2 manipulation affects adult brain function. These results reveal an unexpected degree of developmental plasticity of late-born Drosophila neurons in the formation of a circuit node via the lateralized recruitment of symmetric circuit components."}],"type":"journal_article","oa_version":"Published Version","article_type":"original","DOAJ_listed":"1","citation":{"short":"J.W. Markovitsch, D. Mitić, A. Del Pilar Jiménez García, A. Zane, S. Kainz, R. Kaur, T. Hummel, Science Advances 12 (2026).","ista":"Markovitsch JW, Mitić D, Del Pilar Jiménez García A, Zane A, Kainz S, Kaur R, Hummel T. 2026. Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity. Science Advances. 12(13), eaea6020.","ieee":"J. W. Markovitsch <i>et al.</i>, “Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity,” <i>Science Advances</i>, vol. 12, no. 13. AAAS, 2026.","ama":"Markovitsch JW, Mitić D, Del Pilar Jiménez García A, et al. Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity. <i>Science Advances</i>. 2026;12(13). doi:<a href=\"https://doi.org/10.1126/sciadv.aea6020\">10.1126/sciadv.aea6020</a>","mla":"Markovitsch, Johann W., et al. “Sequential Formation of Drosophila Circuit Asymmetry via Prolonged Structural Plasticity.” <i>Science Advances</i>, vol. 12, no. 13, eaea6020, AAAS, 2026, doi:<a href=\"https://doi.org/10.1126/sciadv.aea6020\">10.1126/sciadv.aea6020</a>.","apa":"Markovitsch, J. W., Mitić, D., Del Pilar Jiménez García, A., Zane, A., Kainz, S., Kaur, R., &#38; Hummel, T. (2026). Sequential formation of Drosophila circuit asymmetry via prolonged structural plasticity. <i>Science Advances</i>. AAAS. <a href=\"https://doi.org/10.1126/sciadv.aea6020\">https://doi.org/10.1126/sciadv.aea6020</a>","chicago":"Markovitsch, Johann W., Daniel Mitić, Alisa Del Pilar Jiménez García, Alsberga Zane, Sarah Kainz, Rashmit Kaur, and Thomas Hummel. “Sequential Formation of Drosophila Circuit Asymmetry via Prolonged Structural Plasticity.” <i>Science Advances</i>. AAAS, 2026. <a href=\"https://doi.org/10.1126/sciadv.aea6020\">https://doi.org/10.1126/sciadv.aea6020</a>."},"date_updated":"2026-10-20T08:11:29Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa":1,"day":"27","publisher":"AAAS","department":[{"_id":"MiSi"},{"_id":"GradSch"}],"month":"03","article_number":"eaea6020","doi":"10.1126/sciadv.aea6020","file":[{"success":1,"date_created":"2026-05-04T09:16:36Z","checksum":"3eed470fe73e53d2a8d55d6fba6934e3","access_level":"open_access","relation":"main_file","creator":"dernst","file_id":"21786","date_updated":"2026-05-04T09:16:36Z","content_type":"application/pdf","file_name":"2026_ScienceAdv_Markovitsch.pdf","file_size":11101140}],"volume":12,"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"ddc":["570"],"intvolume":"        12","publication_status":"published","year":"2026","quality_controlled":"1","article_processing_charge":"Yes","has_accepted_license":"1","file_date_updated":"2026-05-04T09:16:36Z","date_published":"2026-03-27T00:00:00Z","fulldoi":"https://doi.org/10.1126/sciadv.aea6020"},{"related_material":{"link":[{"relation":"press_release","description":"News on ISTA website","url":"https://ista.ac.at/en/news/roots-steer-clear-of-plant-rot/"}]},"citation":{"short":"Z. Bao, H. Wang, A. Zhang, R. Gao, W. Gu, N. Fan, J. Friml, Y. Zhang, Science 393 (2026).","ista":"Bao Z, Wang H, Zhang A, Gao R, Gu W, Fan N, Friml J, Zhang Y. 2026. Roots navigate around decay regions by sensing local pH gradients. Science. 393(6807), eadw6568.","ieee":"Z. Bao <i>et al.</i>, “Roots navigate around decay regions by sensing local pH gradients,” <i>Science</i>, vol. 393, no. 6807. AAAS, 2026.","ama":"Bao Z, Wang H, Zhang A, et al. Roots navigate around decay regions by sensing local pH gradients. <i>Science</i>. 2026;393(6807). doi:<a href=\"https://doi.org/10.1126/science.adw6568\">10.1126/science.adw6568</a>","mla":"Bao, Zhulatai, et al. “Roots Navigate around Decay Regions by Sensing Local PH Gradients.” <i>Science</i>, vol. 393, no. 6807, eadw6568, AAAS, 2026, doi:<a href=\"https://doi.org/10.1126/science.adw6568\">10.1126/science.adw6568</a>.","apa":"Bao, Z., Wang, H., Zhang, A., Gao, R., Gu, W., Fan, N., … Zhang, Y. (2026). Roots navigate around decay regions by sensing local pH gradients. <i>Science</i>. AAAS. <a href=\"https://doi.org/10.1126/science.adw6568\">https://doi.org/10.1126/science.adw6568</a>","chicago":"Bao, Zhulatai, Huihui Wang, Ai Zhang, Ruxi Gao, Wen Gu, Ni Fan, Jiří Friml, and Yuzhou Zhang. “Roots Navigate around Decay Regions by Sensing Local PH Gradients.” <i>Science</i>. AAAS, 2026. <a href=\"https://doi.org/10.1126/science.adw6568\">https://doi.org/10.1126/science.adw6568</a>."},"project":[{"name":"Cyclic nucleotides as second messengers in plants","_id":"8f347782-16d5-11f0-9cad-8c19706ee739","grant_number":"101142681"},{"grant_number":"P37051","_id":"7bcece63-9f16-11ee-852c-ae94e099eeb6","name":"Guanylate cyclase activity of TIR1/AFBs auxin receptors"}],"date_updated":"2026-10-20T08:12:03Z","supplementarymaterial":"yes","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"Roots navigate around decay regions by sensing local pH gradients","_id":"22315","status":"public","date_created":"2026-07-13T14:57:10Z","author":[{"full_name":"Bao, Zhulatai","first_name":"Zhulatai","last_name":"Bao"},{"full_name":"Wang, Huihui","first_name":"Huihui","last_name":"Wang"},{"full_name":"Zhang, Ai","last_name":"Zhang","first_name":"Ai"},{"full_name":"Gao, Ruxi","first_name":"Ruxi","last_name":"Gao"},{"last_name":"Gu","first_name":"Wen","full_name":"Gu, Wen"},{"full_name":"Fan, Ni","last_name":"Fan","first_name":"Ni"},{"last_name":"Friml","first_name":"Jiří","id":"4159519E-F248-11E8-B48F-1D18A9856A87","full_name":"Friml, Jiří","orcid":"0000-0002-8302-7596"},{"full_name":"Zhang, Yuzhou","first_name":"Yuzhou","last_name":"Zhang"}],"oa_version":"None","type":"journal_article","article_type":"original","abstract":[{"lang":"eng","text":"Plant tropisms enable roots to navigate complex soils by responding to directional environmental cues. Biological decay, although central to nutrient cycling, also creates microbially active and potentially hostile niches. In this work, we identified “saprotropism,” a previously unrecognized growth response that enables roots to actively bend away from decaying plant-derived matter. Fungal-driven microbial decomposition released organic acids and formed stable pH gradients in surrounding soil, allowing roots to pinpoint decay without direct contact. Root epidermal cells sensed this acidic gradient through the root meristem growth factor peptide-receptor module, converting external pH asymmetry into asymmetric abscisic acid (ABA) distribution. ABA asymmetry drove microtubule reorganization, which was decoded into decay-avoidant root bending. Together, these findings establish microbial decay–derived chemical gradients as an instructive signal for root navigation and expand the framework of microbe-soil-plant communication."}],"OA_type":"closed access","language":[{"iso":"eng"}],"publication":"Science","scopus_import":"1","issue":"6807","publication_identifier":{"issn":["0036-8075"],"eissn":["1095-9203"]},"acknowledgement":"We are grateful to H. Guo and L. Liu (Department of Biology, Southern University of Science and Technology) for providing the rgf1/2/3, rgi1/2/3/4, tpst-1, and pepr1/2 lines. We thank K.-h. Liu (College of Life Science, Northwest A&F University) for generously providing the ABA biosensor nlsABACUS2-400n. We also thank J. Li and J. Chang (School of Life Sciences, Lanzhou University) for providing the ahk2-5/cre1-2, ahp1/2/3, arr16/arr17, and pTCSn::GFP lines. Our thanks further extend to D. Qian, also from the School of Life Sciences at Lanzhou University, for sharing Arabidopsis line pTUB6::mCherry-TUB6. We are grateful to Y. Zhao (CAS Center for Excellence in Molecular Plant Sciences, Chinese Academy of Sciences) for providing nced3/5, snrk2.2/2.3/2.6, and pyl duodecuple mutants. We also acknowledge the Teaching and Research Core Facility at the College of Life Sciences, Northwest A&F University, particularly N. Fan, for their invaluable technical assistance. We also thank Life Science Research Core Services (LSRCS), Northwest A&F University, for helping with characterization, including CLSM (X. Liu). Fundamental and Interdisciplinary Disciplines Breakthrough Plan of the Ministry of Education of China JYB2025XDXM706 (Y.Z.); Qin Chuangyuan High-level Innovation and Entrepreneurship Talent Program QCYRCXM-2022-237 (Y.Z.); Fundamental Research Funds for the Central Universities K20200168 (Y.Z.); National Natural Science Foundation of China 32570375 (Y.Z.); National Natural Science Foundation of China 32400699 (A.Z.); European Research Council (ERC, CYNIPS) 101142681 (J.F.); Austrian Science Fund (FWF): P 37051-B (J.F.).","date_published":"2026-07-09T00:00:00Z","article_processing_charge":"No","das_tickbox":"1","fulldoi":"https://doi.org/10.1126/science.adw6568","publication_status":"published","year":"2026","pmid":1,"quality_controlled":"1","intvolume":"       393","article_number":"eadw6568","volume":393,"doi":"10.1126/science.adw6568","researchdata_availability":"yes","dataavailabilitystatement":"All data are available in the manuscript or the supplementary materials. The raw RNA-seq data have been deposited in the NCBI Gene Expression Omnibus (GEO) under accession number GSE315473. Microbiome sequencing data have been deposited in the Sequence Read Archive (SRA) under BioProject number PRJNA1397137. Materials are available upon request from the corresponding author.","day":"09","external_id":{"pmid":["42424472"]},"publisher":"AAAS","month":"07","department":[{"_id":"JiFr"}]},{"dataavailabilitystatement":"This work has made use of Euclid data from the European Space Agency (ESA) mission Euclid. The quasar cutouts are available at https://doi.org/10.57780/esa-50769fd. The discovery spectra are available from the corresponding author upon reasonable request.","day":"01","oa":1,"external_id":{"arxiv":["2607.03432"]},"publisher":"EDP Sciences","department":[{"_id":"JoMa"}],"month":"07","article_number":"A104","volume":711,"doi":"10.1051/0004-6361/202658883","researchdata_availability":"no","file":[{"checksum":"055c80a2cd071884e2804ef17dcf1e16","date_created":"2026-10-12T06:20:29Z","success":1,"creator":"dernst","relation":"main_file","access_level":"open_access","file_id":"23097","file_size":14151909,"date_updated":"2026-10-12T06:20:29Z","content_type":"application/pdf","file_name":"2026_AstronomyAstrophysics_Yang.pdf"}],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"ddc":["520"],"publication_status":"published","year":"2026","quality_controlled":"1","intvolume":"       711","has_accepted_license":"1","file_date_updated":"2026-10-12T06:20:29Z","date_published":"2026-07-01T00:00:00Z","article_processing_charge":"No","das_tickbox":"1","fulldoi":"https://doi.org/10.1051/0004-6361/202658883","arxiv":1,"publication":"Astronomy & Astrophysics","scopus_import":"1","acknowledgement":"D. Yang acknowledges helpful discussions with members of the ENIGMA group at UC Santa Barbara and Leiden University, in particular Elia Pizzati, Silvia Onorato, and Diego González for their valuable feedback. D. Yang thanks Shane Bechtel for assistance during observations, and acknowledges the early contributions of Riccardo Nanni, which helped lay the foundation for this work. D. Yang and J. F. Hennawi acknowledge support from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement No 885301). J. F. Hennawi acknowledges support from NSF grant No. 2307180. F. Guarneri and J.-T. Schindler are supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – Project number 518006966. F. Wang acknowledges support from NSF award AST-2513040. R. Decarli acknowledges support from the INAF GO 2022 grant “The birth of the giants: JWST sheds light on the build-up of quasars at cosmic dawn”, INAF Minigrant 2024 “The interstellar medium at high redshift”, and by the PRIN MUR “2022935STW”, RFF M4.C2.1.1, CUP J53D23001570006 and C53D23000950006. S. E. I. Bosman is supported by the Deutsche Forschungsgemeinschaft (DFG) under Emmy Noether grant number BO 5771/1-1. Y. Harikane acknowledges support from the Japan Society for the Promotion of Science (JSPS) Grant-in-Aid for Scientific Research (24H00245), the JSPS Core-to-Core Program (JPJSCCA20210003), and the JSPS International Leading Research (22K21349). J. R. Weaver acknowledges that support for this work was provided by The Brinson Foundation through a Brinson Prize Fellowship grant. The Euclid Consortium acknowledges the European Space Agency and a number of agencies and institutes that have supported the development of Euclid, in particular the Agenzia Spaziale Italiana, the Austrian Forschungsförderungsgesellschaft funded through BMIMI, the Belgian Science Policy, the Canadian Euclid Consortium, the Deutsches Zentrum für Luft- und Raumfahrt, the DTU Space and the Niels Bohr Institute in Denmark, the French Centre National d’Etudes Spatiales, the Fundação para a Ciência e a Tecnologia, the Hungarian Academy of Sciences, the Ministerio de Ciencia, Innovación y Universidades, the National Aeronautics and Space Administration, the National Astronomical Observatory of Japan, the Netherlandse Onderzoekschool Voor Astronomie, the Norwegian Space Agency, the Research Council of Finland, the Romanian Space Agency, the State Secretariat for Education, Research, and Innovation (SERI) at the Swiss Space Office (SSO), and the United Kingdom Space Agency. A complete and detailed list is available on the Euclid web site (www.euclid-ec.org). Some of the data presented herein were obtained at Keck Observatory, which is a private 501(c)3 non-profit organization operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognise and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the Native Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. This paper includes data gathered with the 6.5 meter Magellan Telescopes located at Las Campanas Observatory, Chile. This work uses LBT data from programmes: MPIA-2025A-007 and MPIA-2025B-004. The LBT is an international collaboration among institutions in the United States, Italy and Germany. LBT Corporation partners are: The University of Arizona on behalf of the Arizona university system; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany, representing the Max-Planck Society, the Astrophysical Institute Potsdam, and Heidelberg University; The Ohio State University, and The Research Corporation, on behalf of The University of Notre Dame, University of Minnesota, and University of Virginia, LOFAR data products were provided by the LOFAR Surveys Key Science project (LSKSP; https://lofar-surveys.org/) and were derived from observations with the International LOFAR Telescope (ILT). LOFAR is the Low Frequency Array designed and constructed by ASTRON. It has observing, data processing, and data storage facilities in several countries, which are owned by various parties (each with their own funding sources), and which are collectively operated by the ILT foundation under a joint scientific policy. The efforts of the LSKSP have benefited from funding from the European Research Council, NOVA, NWO, CNRS-INSU, the SURF Co-operative, the UK Science and Technology Funding Council and the Jülich Supercomputing Centre. We make use of z-band imaging from the Wide Imaging with Subaru HSC of the Euclid Sky (WISHES) program operated by the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. We also make use of z-band imaging from the Dark Energy Survey (DES), based on observations obtained at the Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which is operated by AURA under a cooperative agreement with the National Science Foundation. This work made use of NumPy (Harris et al. 2020), SciPy (Virtanen et al. 2020), Astropy (Astropy Collaboration 2013, 2018, 2022), PypeIt (Prochaska et al. 2020), Sculptor (Schindler 2022), condXD (Kang et al. 2025), pysersic (Pasha & Miller 2023), Matplotlib (Hunter 2007), corner.py (Foreman-Mackey 2016), healpy (Zonca et al. 2020).","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"OA_type":"diamond","OA_place":"publisher","language":[{"iso":"eng"}],"title":"Euclid: Discovery of 31 new quasars at 6.6 < z < 7.8","_id":"23044","date_created":"2026-10-04T22:01:54Z","author":[{"last_name":"Yang","first_name":"D.","full_name":"Yang, D."},{"last_name":"Hennawi","first_name":"J. F.","full_name":"Hennawi, J. F."},{"full_name":"Guarneri, F.","last_name":"Guarneri","first_name":"F."},{"full_name":"Wolf, J.","last_name":"Wolf","first_name":"J."},{"last_name":"Belladitta","first_name":"S.","full_name":"Belladitta, S."},{"full_name":"Schindler, J. T.","first_name":"J. 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M.","full_name":"Zerbi, F. M."},{"full_name":"Zucca, E.","last_name":"Zucca","first_name":"E."},{"full_name":"Fabbian, G.","last_name":"Fabbian","first_name":"G."},{"first_name":"M.","last_name":"Huertas-Company","full_name":"Huertas-Company, M."},{"full_name":"Martín-Fleitas, J.","last_name":"Martín-Fleitas","first_name":"J."},{"last_name":"Monaco","first_name":"P.","full_name":"Monaco, P."},{"last_name":"Scottez","first_name":"V.","full_name":"Scottez, V."},{"full_name":"Viel, M.","last_name":"Viel","first_name":"M."}],"status":"public","oa_version":"Published Version","type":"journal_article","article_type":"original","abstract":[{"text":"We report the discovery of 31 new high-z quasars in the redshift range 6.6 < z < 7.8. These quasars were selected from approximately 3000 deg2 of sky covered during the first 1.5 years of the Euclid Wide Survey, representing the initial results of the Euclid high-z quasar search. Our candidate selection employed multiple machine-learning and probabilistic techniques applied to the EuclidIE, YE, JE, and HE images, supplemented by ancillary z-band data when available. Spectroscopic follow-up observations were carried out with Keck, Magellan, and the Large Binocular Telescope (LBT). Among the new discoveries, there are 12 quasars at z ≥ 7, more than doubling the number of previously known quasars at z ≥ 7. The newly discovered quasars exhibit 21.2 < JE < 23.2 (−25.5 < M1450 < −23.6), extending quasar studies to the faint end of the quasar luminosity function (QLF) at z ≳ 7. The quasar with the highest-z, EUCL J172902.75+641018.1 at z ≈ 7.77, sets the new redshift record for the most distant quasar ever reported. These discoveries demonstrate Euclid’s transformative role in high-z quasar discovery and set the stage for future follow-up studies of the early galaxies hosting quasars, supermassive black hole growth, and the intergalactic medium in the epoch of reionisation.","lang":"eng"}],"citation":{"ama":"Yang D, Hennawi JF, Guarneri F, et al. Euclid: Discovery of 31 new quasars at 6.6 &#60; z &#60; 7.8. <i>Astronomy &#38; Astrophysics</i>. 2026;711. doi:<a href=\"https://doi.org/10.1051/0004-6361/202658883\">10.1051/0004-6361/202658883</a>","mla":"Yang, D., et al. “Euclid: Discovery of 31 New Quasars at 6.6 &#60; z &#60; 7.8.” <i>Astronomy &#38; Astrophysics</i>, vol. 711, A104, EDP Sciences, 2026, doi:<a href=\"https://doi.org/10.1051/0004-6361/202658883\">10.1051/0004-6361/202658883</a>.","ista":"Yang D et al. 2026. Euclid: Discovery of 31 new quasars at 6.6 &#60; z &#60; 7.8. Astronomy &#38; Astrophysics. 711, A104.","ieee":"D. Yang <i>et al.</i>, “Euclid: Discovery of 31 new quasars at 6.6 &#60; z &#60; 7.8,” <i>Astronomy &#38; Astrophysics</i>, vol. 711. EDP Sciences, 2026.","short":"D. Yang, J.F. Hennawi, F. Guarneri, J. Wolf, S. Belladitta, J.T. Schindler, A.C.N. Hughes, E. Bañados, D.J. Mortlock, J. Yang, F. Wang, X. Fan, K. Jahnke, D. Stern, C.J. Willott, A.J. Barth, H.J.A. Rottgering, R.G. Varadaraj, R. Decarli, A.C. Eilers, M. Ezziati, Y. Fu, J. Huang, X. Jin, Y. Kang, L.N. Martinez-Ramirez, Y. Matsuoka, M. Onoue, R. Pello, R.P. Remigio, W.L. Tee, B. Venemans, G. Vietri, B. Wang, L.J. Abbo, H. Atek, S. Bisogni, S.E.I. Bosman, R.A.A. Bowler, C.J. Conselice, F.B. Davies, C.M. Gutierrez, Y. Harikane, K. Rubinur, C.C. Lovell, M. Magliocchetti, J.J. Matthee, F. Ricci, M. Scialpi, D. Scott, L. Spinoglio, F. Tarsitano, Y. Toba, F. Walter, J.R. Weaver, G. Zamorani, B. Altieri, A. Amara, S. Andreon, H. Aussel, C. Baccigalupi, M. Baldi, A. Balestra, S. Bardelli, P. Battaglia, A. Biviano, E. Branchini, M. Brescia, S. Camera, G. Cañas-Herrera, V. Capobianco, C. Carbone, J. Carretero, M. Castellano, G. Castignani, S. Cavuoti, K.C. Chambers, A. Cimatti, C. Colodro-Conde, G. Congedo, L. Conversi, Y. Copin, F. Courbin, H.M. Courtois, M. Cropper, J.C. Cuillandre, H. Degaudenzi, G. De Lucia, C. Dolding, H. Dole, M. Douspis, F. Dubath, X. Dupac, S. Dusini, S. Escoffier, M. Farina, R. Farinelli, S. Ferriol, F. Finelli, N. Fourmanoit, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, K. George, B. Gillis, C. Giocoli, P. Gómez-Alvarez, J. Gracia-Carpio, A. Grazian, F. Grupp, L. Guzzo, S. Gwyn, S.V.H. Haugan, H. Hoekstra, W. Holmes, I.M. Hook, F. Hormuth, A. Hornstrup, M. Jhabvala, S. Kermiche, B. Kubik, K. Kuijken, M. Kümmel, M. Kunz, H. Kurki-Suonio, A.M.C. Le Brun, S. Ligori, P.B. Lilje, V. Lindholm, I. Lloro, G. Mainetti, D. Maino, E. Maiorano, O. Mansutti, O. Marggraf, M. Martinelli, N. Martinet, F. Marulli, R.J. Massey, H.J. Mccracken, E. Medinaceli, S. Mei, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, J.J. Mohr, A. Mora, M. Moresco, L. Moscardini, E. Munari, R. Nakajima, C. Neissner, R.C. Nichol, S.M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W.J. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L.A. Popa, L. Pozzetti, G.D. Racca, F. Raison, R. Rebolo, A. Renzi, J. Rhodes, G. Riccio, H.W. Rix, E. Romelli, M. Roncarelli, C. Rosset, B. Rusholme, R. Saglia, Z. Sakr, D. Sapone, M. Sauvage, M. Schirmer, P. Schneider, T. Schrabback, A. Secroun, G. Seidel, S. Serrano, E. Sihvola, P. Simon, C. Sirignano, G. Sirri, L. Stanco, J. Steinwagner, P. Tallada-Crespí, I. Tereno, N. Tessore, S. Toft, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, L. Valenziano, J. Valiviita, T. Vassallo, Y. Wang, J. Weller, F.M. Zerbi, E. Zucca, G. Fabbian, M. Huertas-Company, J. Martín-Fleitas, P. Monaco, V. Scottez, M. Viel, Astronomy &#38; Astrophysics 711 (2026).","chicago":"Yang, D., J. F. Hennawi, F. Guarneri, J. Wolf, S. Belladitta, J. T. Schindler, A. C.N. Hughes, et al. “Euclid: Discovery of 31 New Quasars at 6.6 &#60; z &#60; 7.8.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2026. <a href=\"https://doi.org/10.1051/0004-6361/202658883\">https://doi.org/10.1051/0004-6361/202658883</a>.","apa":"Yang, D., Hennawi, J. F., Guarneri, F., Wolf, J., Belladitta, S., Schindler, J. T., … Viel, M. (2026). Euclid: Discovery of 31 new quasars at 6.6 &#60; z &#60; 7.8. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202658883\">https://doi.org/10.1051/0004-6361/202658883</a>"},"DOAJ_listed":"1","supplementarymaterial":"yes","date_updated":"2026-10-20T08:15:12Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","PlanS_conform":"1"},{"DOAJ_listed":"1","citation":{"chicago":"Llerena, M., L. Pentericci, R. Amorín, A. Ferrara, M. Dickinson, F. Arevalo-Gonzalez, A. Calabrò, et al. “Extreme Equivalent-Width-Selected Low-Mass Starbursts at z = 4 − 9: Insights into Their Role in Cosmic Reionization.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2026. <a href=\"https://doi.org/10.1051/0004-6361/202557897\">https://doi.org/10.1051/0004-6361/202557897</a>.","apa":"Llerena, M., Pentericci, L., Amorín, R., Ferrara, A., Dickinson, M., Arevalo-Gonzalez, F., … Yung, L. Y. A. (2026). Extreme equivalent-width-selected low-mass starbursts at z = 4 − 9: Insights into their role in cosmic reionization. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202557897\">https://doi.org/10.1051/0004-6361/202557897</a>","ama":"Llerena M, Pentericci L, Amorín R, et al. Extreme equivalent-width-selected low-mass starbursts at z = 4 − 9: Insights into their role in cosmic reionization. <i>Astronomy &#38; Astrophysics</i>. 2026;708. doi:<a href=\"https://doi.org/10.1051/0004-6361/202557897\">10.1051/0004-6361/202557897</a>","mla":"Llerena, M., et al. “Extreme Equivalent-Width-Selected Low-Mass Starbursts at z = 4 − 9: Insights into Their Role in Cosmic Reionization.” <i>Astronomy &#38; Astrophysics</i>, vol. 708, A152, EDP Sciences, 2026, doi:<a href=\"https://doi.org/10.1051/0004-6361/202557897\">10.1051/0004-6361/202557897</a>.","short":"M. Llerena, L. Pentericci, R. Amorín, A. Ferrara, M. Dickinson, F. Arevalo-Gonzalez, A. Calabrò, L. Napolitano, S. Mascia, P. Arrabal Haro, R. Begley, N.J. Cleri, K. Davis, W. Hu, J.S. Kartaltepe, A.M. Koekemoer, R.A. Lucas, E. Mcgrath, D.J. Mcleod, C. Papovich, T.M. Stanton, A.J. Taylor, R. Tripodi, X. Wang, L.Y.A. Yung, Astronomy &#38; Astrophysics 708 (2026).","ista":"Llerena M, Pentericci L, Amorín R, Ferrara A, Dickinson M, Arevalo-Gonzalez F, Calabrò A, Napolitano L, Mascia S, Arrabal Haro P, Begley R, Cleri NJ, Davis K, Hu W, Kartaltepe JS, Koekemoer AM, Lucas RA, Mcgrath E, Mcleod DJ, Papovich C, Stanton TM, Taylor AJ, Tripodi R, Wang X, Yung LYA. 2026. Extreme equivalent-width-selected low-mass starbursts at z = 4 − 9: Insights into their role in cosmic reionization. Astronomy &#38; Astrophysics. 708, A152.","ieee":"M. Llerena <i>et al.</i>, “Extreme equivalent-width-selected low-mass starbursts at z = 4 − 9: Insights into their role in cosmic reionization,” <i>Astronomy &#38; Astrophysics</i>, vol. 708. EDP Sciences, 2026."},"PlanS_conform":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2026-10-20T08:15:59Z","supplementarymaterial":"yes","date_created":"2026-10-04T22:01:55Z","status":"public","author":[{"last_name":"Llerena","first_name":"M.","full_name":"Llerena, M."},{"last_name":"Pentericci","first_name":"L.","full_name":"Pentericci, L."},{"first_name":"R.","last_name":"Amorín","full_name":"Amorín, R."},{"full_name":"Ferrara, A.","last_name":"Ferrara","first_name":"A."},{"last_name":"Dickinson","first_name":"M.","full_name":"Dickinson, M."},{"full_name":"Arevalo-Gonzalez, F.","first_name":"F.","last_name":"Arevalo-Gonzalez"},{"full_name":"Calabrò, A.","first_name":"A.","last_name":"Calabrò"},{"full_name":"Napolitano, L.","first_name":"L.","last_name":"Napolitano"},{"last_name":"Mascia","first_name":"Sara","id":"edaf889c-c7cd-11ef-ab1b-bb28c431bd29","full_name":"Mascia, Sara"},{"full_name":"Arrabal Haro, P.","last_name":"Arrabal Haro","first_name":"P."},{"full_name":"Begley, R.","last_name":"Begley","first_name":"R."},{"full_name":"Cleri, N. J.","last_name":"Cleri","first_name":"N. J."},{"full_name":"Davis, K.","last_name":"Davis","first_name":"K."},{"last_name":"Hu","first_name":"W.","full_name":"Hu, W."},{"last_name":"Kartaltepe","first_name":"J. S.","full_name":"Kartaltepe, J. S."},{"last_name":"Koekemoer","first_name":"A. M.","full_name":"Koekemoer, A. M."},{"first_name":"R. A.","last_name":"Lucas","full_name":"Lucas, R. A."},{"last_name":"Mcgrath","first_name":"E.","full_name":"Mcgrath, E."},{"full_name":"Mcleod, D. J.","last_name":"Mcleod","first_name":"D. J."},{"first_name":"C.","last_name":"Papovich","full_name":"Papovich, C."},{"last_name":"Stanton","first_name":"T. M.","full_name":"Stanton, T. M."},{"last_name":"Taylor","first_name":"A. J.","full_name":"Taylor, A. J."},{"full_name":"Tripodi, R.","last_name":"Tripodi","first_name":"R."},{"full_name":"Wang, X.","last_name":"Wang","first_name":"X."},{"full_name":"Yung, L. Y.A.","first_name":"L. Y.A.","last_name":"Yung"}],"_id":"23049","title":"Extreme equivalent-width-selected low-mass starbursts at z = 4 − 9: Insights into their role in cosmic reionization","abstract":[{"lang":"eng","text":"We investigate the properties of extreme emission line galaxies (EELGs) at z = 4 − 9 and their role in reionization. Compact, low-mass galaxies with intense optical emission lines are linked to elevated specific star formation rates (sSFRs) and recent bursts of star formation. Feedback in these systems may enable the leakage of ionizing radiation into the intergalactic medium. Using JWST/NIRSpec spectroscopy from the CAPERS, CEERS, and RUBIES surveys, we compiled 160 NIRCam-selected EELGs in the EGS field. These galaxies show extreme rest-frame equivalent widths (EWs), with a median EW([O III]+Hβ) = 1616 Å and EW(Hα) = 763 Å. They are low-mass (median log(M★/M⊙) = 8.26) with high sSFRs (median 43 Gyr−1), above the z ∼ 6 main sequence. UV slopes are diverse, with a median value of β = −2.0, and only 7% have extremely blue continua (β < −2.6). Emission-line diagnostics suggest stellar populations as the primary ionizing source, although an AGN fraction of 14% cannot be entirely ruled out. These galaxies are efficient ionizing photon producers, with median log(ξion [Hz erg−1]) = 25.37, exceeding typical values at similar redshifts. Escape fractions, however, are heterogeneous: 16% of EELGs at z < 7 show escape fractions > 5% for both Lyα and LyC photons, while 82% lack detectable Lyα emission. The median inferred LyC escape fraction is modest (5%) but enhanced in compact super-Eddington systems with sSFR > 25 Gyr−1. These results indicate that EELGs contribute approximately 16 − 40% of the total ionizing emissivity required to sustain hydrogen reionization. EELGs are extremely compact, with a median effective radius of 0.49 kpc, and exhibit a recent star formation burst. Our analysis indicates that sSFR and star formation rate surface density are the primary drivers of their extreme emission line strengths."}],"article_type":"original","type":"journal_article","oa_version":"Published Version","OA_place":"publisher","OA_type":"diamond","language":[{"iso":"eng"}],"scopus_import":"1","publication":"Astronomy & Astrophysics","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"acknowledgement":"We thank the anonymous referee for the thorough review and constructive suggestions that significantly improved this paper. We also thank Sophia Flury for valuable feedback and insightful comments, which helped refine our interpretation of the results. MLl acknowledges support from the INAF Large Grant 2022 “Extragalactic Surveys with JWST” (PI L. Pentericci), the PRIN 2022 MUR project 2022CB3PJ3 – First Light And Galaxy aSsembly (FLAGS) funded by the European Union – Next Generation EU, the INAF Mini-grant 2024 “Galaxies in the epoch of Reionization and their analogs at lower redshift” (PI M. Llerena), and the Large Grant RF 2023 F.O. 1.05.23.01.11 “The MOONS Extragalactic Survey”. RA acknowledges support of Grant PID2023-147386NB-I00 funded by MICIU/AEI/10.13039/501100011033 and by ERDF/EU, and the Severo Ochoa award to the IAA-CSIC CEX2021-001131-S. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-03127. Support for program number GO-6368 was provided through a grant from the STScI under NASA contract NAS5-03127. The data were obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute. These observations are associated with program #6368, and can be accessed via doi. Some of the data products presented herein were retrieved from the Dawn JWST Archive (DJA). DJA is an initiative of the Cosmic Dawn Center (DAWN), which is funded by the Danish National Research Foundation under grant DNRF140. These observations are associated with programs #1345, #2750, and #4233. This work has made extensive use of Python packages astropy (Astropy Collaboration 2018), numpy (Harris et al. 2020), Matplotlib (Hunter 2007) and LiMe (Fernández et al. 2024).","article_processing_charge":"No","date_published":"2026-04-01T00:00:00Z","file_date_updated":"2026-10-12T07:19:26Z","has_accepted_license":"1","arxiv":1,"fulldoi":"https://doi.org/10.1051/0004-6361/202557897","das_tickbox":"1","ddc":["520"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"intvolume":"       708","quality_controlled":"1","year":"2026","publication_status":"published","article_number":"A152","file":[{"file_id":"23100","file_name":"2026_AstronomyAstrophysics_Llerena.pdf","date_updated":"2026-10-12T07:19:26Z","content_type":"application/pdf","file_size":5918938,"success":1,"date_created":"2026-10-12T07:19:26Z","checksum":"d678534203385bec7579e68e12cc09b4","access_level":"open_access","creator":"dernst","relation":"main_file"}],"researchdata_availability":"no","doi":"10.1051/0004-6361/202557897","volume":708,"oa":1,"dataavailabilitystatement":"Table A.1 is available at the CDS via https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/708/A152","day":"01","month":"04","department":[{"_id":"JoMa"}],"publisher":"EDP Sciences","external_id":{"arxiv":["2510.25647"]}},{"oa":1,"day":"01","month":"04","department":[{"_id":"JoMa"}],"publisher":"EDP Sciences","external_id":{"arxiv":["2508.14171"]},"article_number":"A102","file":[{"access_level":"open_access","relation":"main_file","creator":"dernst","success":1,"date_created":"2026-10-12T07:09:27Z","checksum":"adff12137f194affedd27fa07c82e062","file_name":"2026_AstronomyAstrophysics_Napolitano.pdf","date_updated":"2026-10-12T07:09:27Z","content_type":"application/pdf","file_size":3265893,"file_id":"23099"}],"researchdata_availability":"no","doi":"10.1051/0004-6361/202556912","volume":708,"ddc":["520"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"intvolume":"       708","quality_controlled":"1","year":"2026","publication_status":"published","article_processing_charge":"No","file_date_updated":"2026-10-12T07:09:27Z","date_published":"2026-04-01T00:00:00Z","has_accepted_license":"1","arxiv":1,"fulldoi":"https://doi.org/10.1051/0004-6361/202556912","das_tickbox":"0","scopus_import":"1","publication":"Astronomy & Astrophysics","acknowledgement":"We thank the anonymous referee for the constructive feedback provided. LN acknowledges support from grant “Progetti per Avvio alla Ricerca – Tipo 1, Unveiling Cosmic Dawn: Galaxy Evolution with CAPERS” (AR1241906F947685) and from PRIN 2022 MUR project 2022CB3PJ3 – First Light And Galaxy aSsembly (FLAGS) funded by the European Union – Next Generation EU. LN, LP, AB, and BC acknowledge support from the ERC synergy grant 101166930 – RECAP. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-03127. These observations are associated with programs #6368, #4233, #1215, #2565, and #3543. Support for program number GO-6368 was provided through a grant from the STScI under NASA contract NAS5-03127. The data were obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute. These observations can be accessed via DOI. Some of the data products presented in this work were retrieved from the Dawn JWST Archive (DJA). DJA is an initiative of the Cosmic Dawn Center (DAWN), which is funded by the Danish National Research Foundation under grant DNRF140.","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"OA_place":"publisher","OA_type":"diamond","language":[{"iso":"eng"}],"status":"public","date_created":"2026-10-04T22:01:55Z","author":[{"full_name":"Napolitano, L.","first_name":"L.","last_name":"Napolitano"},{"full_name":"Pentericci, L.","first_name":"L.","last_name":"Pentericci"},{"full_name":"Dickinson, M.","first_name":"M.","last_name":"Dickinson"},{"last_name":"Arrabal Haro","first_name":"P.","full_name":"Arrabal Haro, P."},{"full_name":"Taylor, A. J.","last_name":"Taylor","first_name":"A. J."},{"first_name":"A.","last_name":"Calabrò","full_name":"Calabrò, A."},{"full_name":"Bhagwat, A.","last_name":"Bhagwat","first_name":"A."},{"full_name":"Santini, P.","first_name":"P.","last_name":"Santini"},{"last_name":"Arevalo-Gonzalez","first_name":"F.","full_name":"Arevalo-Gonzalez, F."},{"full_name":"Begley, R.","first_name":"R.","last_name":"Begley"},{"full_name":"Castellano, M.","first_name":"M.","last_name":"Castellano"},{"full_name":"Ciardi, B.","last_name":"Ciardi","first_name":"B."},{"first_name":"C. T.","last_name":"Donnan","full_name":"Donnan, C. T."},{"last_name":"Dottorini","first_name":"D.","full_name":"Dottorini, D."},{"first_name":"J. S.","last_name":"Dunlop","full_name":"Dunlop, J. S."},{"first_name":"S. L.","last_name":"Finkelstein","full_name":"Finkelstein, S. L."},{"full_name":"Fontana, A.","first_name":"A.","last_name":"Fontana"},{"first_name":"M.","last_name":"Giavalisco","full_name":"Giavalisco, M."},{"full_name":"Hirschmann, M.","first_name":"M.","last_name":"Hirschmann"},{"full_name":"Jung, I.","first_name":"I.","last_name":"Jung"},{"last_name":"Koekemoer","first_name":"A. M.","full_name":"Koekemoer, A. M."},{"full_name":"Kokorev, V.","last_name":"Kokorev","first_name":"V."},{"full_name":"Llerena, M.","last_name":"Llerena","first_name":"M."},{"last_name":"Lucas","first_name":"R. A.","full_name":"Lucas, R. A."},{"full_name":"Mascia, Sara","id":"edaf889c-c7cd-11ef-ab1b-bb28c431bd29","first_name":"Sara","last_name":"Mascia"},{"full_name":"Merlin, E.","last_name":"Merlin","first_name":"E."},{"last_name":"Pérez-González","first_name":"P. G.","full_name":"Pérez-González, P. G."},{"first_name":"T. M.","last_name":"Stanton","full_name":"Stanton, T. M."},{"last_name":"Tripodi","first_name":"R.","full_name":"Tripodi, R."},{"first_name":"X.","last_name":"Wang","full_name":"Wang, X."},{"first_name":"B. J.","last_name":"Weiner","full_name":"Weiner, B. J."}],"_id":"23050","title":"Lyα visibility from z = 4.5 to 11 in the UDS field: Evidence for a high neutral hydrogen fraction and small ionized bubbles at z ∼ 7","abstract":[{"lang":"eng","text":"The resonant scattering nature of Lyα photons interacting with neutral hydrogen makes Lyα emitters (LAEs) robust tracers of the intergalactic neutral hydrogen fraction, and thus sensitive probes of cosmic reionization. We present an extensive study of the Lyα evolution from galaxies at 4.5 ≤ z ≤ 11 in the UDS field, observed as part of the CAPERS survey, and complemented with spectra from the DAWN JWST Archive. The combined sample includes 651 spectroscopically confirmed Lyα-break galaxies, among which we find 73 S/N > 3 LAEs in JWST-NIRSpec PRISM spectra. We trace the redshift evolution of the LAE fraction with EW0 > 25 Å (XLyα) between z = 5 and z = 9, extending such an analysis to the UDS field for the first time. At z = 5 and 6, the UDS results agree with the average JWST XLyα values from multiple fields. However, JWST measurements are consistently lower than ground-based results. To investigate this, we compare JWST observations to a population of star-forming galaxies at z ∼ 6 observed with VLT-FORS2. We find that a Lyα slit-loss of 35 ± 10% in JWST spectra accounts for the offset, as the resonant Lyα emission is more spatially extended than the stellar continuum. From z = 6 to 7, the UDS field shows a significant drop in Lyα visibility, from which we infer a neutral hydrogen fraction of XHI = 0.7–0.9. Finally, we identify two robust ionized bubbles at z = 7.29 and 7.77, with radii of Rion = 0.6 and 0.5 physical Mpc and photometric overdensities of N/⟨N⟩ = 3 and 4, based on candidate counts down to the photometric completeness limit. Compared to the large ionized region at z ∼ 7 in the EGS field, these results indicate significant field-to-field variation, supporting a patchy, inhomogeneous reionization process."}],"article_type":"original","oa_version":"Published Version","type":"journal_article","citation":{"chicago":"Napolitano, L., L. Pentericci, M. Dickinson, P. Arrabal Haro, A. J. Taylor, A. Calabrò, A. Bhagwat, et al. “Lyα Visibility from z = 4.5 to 11 in the UDS Field: Evidence for a High Neutral Hydrogen Fraction and Small Ionized Bubbles at z ∼ 7.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2026. <a href=\"https://doi.org/10.1051/0004-6361/202556912\">https://doi.org/10.1051/0004-6361/202556912</a>.","apa":"Napolitano, L., Pentericci, L., Dickinson, M., Arrabal Haro, P., Taylor, A. J., Calabrò, A., … Weiner, B. J. (2026). Lyα visibility from z = 4.5 to 11 in the UDS field: Evidence for a high neutral hydrogen fraction and small ionized bubbles at z ∼ 7. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202556912\">https://doi.org/10.1051/0004-6361/202556912</a>","ama":"Napolitano L, Pentericci L, Dickinson M, et al. Lyα visibility from z = 4.5 to 11 in the UDS field: Evidence for a high neutral hydrogen fraction and small ionized bubbles at z ∼ 7. <i>Astronomy &#38; Astrophysics</i>. 2026;708. doi:<a href=\"https://doi.org/10.1051/0004-6361/202556912\">10.1051/0004-6361/202556912</a>","mla":"Napolitano, L., et al. “Lyα Visibility from z = 4.5 to 11 in the UDS Field: Evidence for a High Neutral Hydrogen Fraction and Small Ionized Bubbles at z ∼ 7.” <i>Astronomy &#38; Astrophysics</i>, vol. 708, A102, EDP Sciences, 2026, doi:<a href=\"https://doi.org/10.1051/0004-6361/202556912\">10.1051/0004-6361/202556912</a>.","short":"L. Napolitano, L. Pentericci, M. Dickinson, P. Arrabal Haro, A.J. Taylor, A. Calabrò, A. Bhagwat, P. Santini, F. Arevalo-Gonzalez, R. Begley, M. Castellano, B. Ciardi, C.T. Donnan, D. Dottorini, J.S. Dunlop, S.L. Finkelstein, A. Fontana, M. Giavalisco, M. Hirschmann, I. Jung, A.M. Koekemoer, V. Kokorev, M. Llerena, R.A. Lucas, S. Mascia, E. Merlin, P.G. Pérez-González, T.M. Stanton, R. Tripodi, X. Wang, B.J. Weiner, Astronomy &#38; Astrophysics 708 (2026).","ieee":"L. Napolitano <i>et al.</i>, “Lyα visibility from z = 4.5 to 11 in the UDS field: Evidence for a high neutral hydrogen fraction and small ionized bubbles at z ∼ 7,” <i>Astronomy &#38; Astrophysics</i>, vol. 708. EDP Sciences, 2026.","ista":"Napolitano L, Pentericci L, Dickinson M, Arrabal Haro P, Taylor AJ, Calabrò A, Bhagwat A, Santini P, Arevalo-Gonzalez F, Begley R, Castellano M, Ciardi B, Donnan CT, Dottorini D, Dunlop JS, Finkelstein SL, Fontana A, Giavalisco M, Hirschmann M, Jung I, Koekemoer AM, Kokorev V, Llerena M, Lucas RA, Mascia S, Merlin E, Pérez-González PG, Stanton TM, Tripodi R, Wang X, Weiner BJ. 2026. Lyα visibility from z = 4.5 to 11 in the UDS field: Evidence for a high neutral hydrogen fraction and small ionized bubbles at z ∼ 7. Astronomy &#38; Astrophysics. 708, A102."},"PlanS_conform":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2026-10-20T08:15:36Z","supplementarymaterial":"yes"},{"day":"01","oa":1,"external_id":{"arxiv":["2511.15792"]},"publisher":"EDP Sciences","month":"04","department":[{"_id":"JoMa"}],"article_number":"A33","volume":708,"researchdata_availability":"yes","doi":"10.1051/0004-6361/202558205","file":[{"file_id":"23101","file_size":587642,"content_type":"application/pdf","date_updated":"2026-10-12T07:31:23Z","file_name":"2026_AstronomyAstrophysics_Matharu.pdf","checksum":"875d217ea15192fa1208f3db34a7fad6","date_created":"2026-10-12T07:31:23Z","success":1,"creator":"dernst","relation":"main_file","access_level":"open_access"}],"ddc":["520"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"publication_status":"published","year":"2026","quality_controlled":"1","intvolume":"       708","has_accepted_license":"1","file_date_updated":"2026-10-12T07:31:23Z","date_published":"2026-04-01T00:00:00Z","article_processing_charge":"No","das_tickbox":"0","fulldoi":"https://doi.org/10.1051/0004-6361/202558205","arxiv":1,"publication":"Astronomy & Astrophysics","scopus_import":"1","acknowledgement":"JM is grateful to the Max Planck Society for the MPIA Prize Fellowship and to the Cosmic Dawn Center for the DAWN Fellowship. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The raw data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with JWST Cycle 1 GO programs #1895 and #2079. Support for both programs was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Associations of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant DNRF140. This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI) under contract number MB22.00072, as well as from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. This work benefited from support from the George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University. CP thanks Marsha and Ralph Schilling for generous support of this research.","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"OA_place":"publisher","OA_type":"diamond","language":[{"iso":"eng"}],"title":"A first look at a complete view of spatially resolved star formation at 1  <  z  <  1.8 with JWST NGDEEP+FRESCO slitless spectroscopy","_id":"23048","date_created":"2026-10-04T22:01:55Z","author":[{"first_name":"Jasleen","last_name":"Matharu","full_name":"Matharu, Jasleen"},{"last_name":"Shen","first_name":"Lu","full_name":"Shen, Lu"},{"first_name":"Irene","last_name":"Shivaei","full_name":"Shivaei, Irene"},{"full_name":"Oesch, Pascal A.","last_name":"Oesch","first_name":"Pascal A."},{"last_name":"Papovich","first_name":"Casey","full_name":"Papovich, Casey"},{"last_name":"Brammer","first_name":"Gabriel","full_name":"Brammer, Gabriel"},{"last_name":"Reddy","first_name":"Naveen A.","full_name":"Reddy, Naveen A."},{"first_name":"Yingjie","last_name":"Cheng","full_name":"Cheng, Yingjie"},{"last_name":"Van Dokkum","first_name":"Pieter","full_name":"Van Dokkum, Pieter"},{"full_name":"Finkelstein, Steven L.","last_name":"Finkelstein","first_name":"Steven L."},{"full_name":"Hathi, Nimish P.","first_name":"Nimish P.","last_name":"Hathi"},{"full_name":"Kartaltepe, Jeyhan S.","first_name":"Jeyhan S.","last_name":"Kartaltepe"},{"first_name":"Anton M.","last_name":"Koekemoer","full_name":"Koekemoer, Anton M."},{"orcid":"0000-0003-2871-127X","full_name":"Matthee, Jorryt J","last_name":"Matthee","first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"last_name":"Pirzkal","first_name":"Nor","full_name":"Pirzkal, Nor"},{"last_name":"Wilkins","first_name":"Stephen M.","full_name":"Wilkins, Stephen M."},{"full_name":"Wozniak, Michael A.","last_name":"Wozniak","first_name":"Michael A."},{"full_name":"Xiao, Mengyuan","last_name":"Xiao","first_name":"Mengyuan"}],"status":"public","type":"journal_article","oa_version":"Published Version","article_type":"original","abstract":[{"text":"The previously inaccessible star formation tracer Paschen-Alpha (Paα) can now be spatially resolved by JWST NIRCam slitless spectroscopy in distant galaxies up to cosmic noon. In the first study of its kind, we combine JWST NGDEEP NIRISS and FRESCO NIRCam slitless spectroscopy to provide the first direct comparison of spatially resolved dust-obscured (traced by Paα) versus unobscured (traced by Hα) star formation across the main sequence. We stacked Paα and Hα emission-line maps, along with stellar continuum images at both wavelengths of 31 galaxies at 1 < z < 1.8 in three bins of stellar mass spanning 7.7 ≤ log(M*/M⊙) < 11. Surface brightness profiles were measured and equivalent width (EW) profiles computed. Increasing Paα and Hα EW profiles with galactocentric radius across all stellar masses probed provides direct evidence for the inside-out growth of galaxies both via dust-obscured and unobscured star formation for the first time. For galaxies predominantly on the main sequence (log(M*/M⊙)≥8.8), a weakly positive (0.1 ± 0.1) Paα/Hα line profile gradient as a function of radius is found at 8.8 ≤ log(M*/M⊙) < 9.9, with a negative (−0.4 ± 0.1) Paα/Hα line profile gradient as a function of radius found at the highest stellar masses of 9.9 ≤ log(M*/M⊙) < 11.0. Low-mass galaxies (7.7 ≤ log(M*/M⊙) < 8.8) with predominantly high specific star formation rates relative to the main sequence are also found to have a negative (−0.5 ± 0.1) Paα/Hα line profile gradient as a function of radius. Our results demonstrate that while inside-out growth via star formation is ubiquitous across the main sequence just after cosmic noon, centrally concentrated dust attenuation is not. Along with other recent work in the literature, our findings now motivate future studies of resolved SFR and dust attenuation profiles in large samples of individual cosmic noon galaxies across the main sequence, aimed at understanding the intrinsic scatter in spatially resolved star formation.","lang":"eng"}],"DOAJ_listed":"1","citation":{"apa":"Matharu, J., Shen, L., Shivaei, I., Oesch, P. A., Papovich, C., Brammer, G., … Xiao, M. (2026). A first look at a complete view of spatially resolved star formation at 1  &#60;  z  &#60;  1.8 with JWST NGDEEP+FRESCO slitless spectroscopy. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202558205\">https://doi.org/10.1051/0004-6361/202558205</a>","chicago":"Matharu, Jasleen, Lu Shen, Irene Shivaei, Pascal A. Oesch, Casey Papovich, Gabriel Brammer, Naveen A. Reddy, et al. “A First Look at a Complete View of Spatially Resolved Star Formation at 1  &#60;  z  &#60;  1.8 with JWST NGDEEP+FRESCO Slitless Spectroscopy.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2026. <a href=\"https://doi.org/10.1051/0004-6361/202558205\">https://doi.org/10.1051/0004-6361/202558205</a>.","ista":"Matharu J, Shen L, Shivaei I, Oesch PA, Papovich C, Brammer G, Reddy NA, Cheng Y, Van Dokkum P, Finkelstein SL, Hathi NP, Kartaltepe JS, Koekemoer AM, Matthee JJ, Pirzkal N, Wilkins SM, Wozniak MA, Xiao M. 2026. A first look at a complete view of spatially resolved star formation at 1  &#60;  z  &#60;  1.8 with JWST NGDEEP+FRESCO slitless spectroscopy. Astronomy &#38; Astrophysics. 708, A33.","ieee":"J. Matharu <i>et al.</i>, “A first look at a complete view of spatially resolved star formation at 1  &#60;  z  &#60;  1.8 with JWST NGDEEP+FRESCO slitless spectroscopy,” <i>Astronomy &#38; Astrophysics</i>, vol. 708. EDP Sciences, 2026.","short":"J. Matharu, L. Shen, I. Shivaei, P.A. Oesch, C. Papovich, G. Brammer, N.A. Reddy, Y. Cheng, P. Van Dokkum, S.L. Finkelstein, N.P. Hathi, J.S. Kartaltepe, A.M. Koekemoer, J.J. Matthee, N. Pirzkal, S.M. Wilkins, M.A. Wozniak, M. Xiao, Astronomy &#38; Astrophysics 708 (2026).","mla":"Matharu, Jasleen, et al. “A First Look at a Complete View of Spatially Resolved Star Formation at 1  &#60;  z  &#60;  1.8 with JWST NGDEEP+FRESCO Slitless Spectroscopy.” <i>Astronomy &#38; Astrophysics</i>, vol. 708, A33, EDP Sciences, 2026, doi:<a href=\"https://doi.org/10.1051/0004-6361/202558205\">10.1051/0004-6361/202558205</a>.","ama":"Matharu J, Shen L, Shivaei I, et al. A first look at a complete view of spatially resolved star formation at 1  &#60;  z  &#60;  1.8 with JWST NGDEEP+FRESCO slitless spectroscopy. <i>Astronomy &#38; Astrophysics</i>. 2026;708. doi:<a href=\"https://doi.org/10.1051/0004-6361/202558205\">10.1051/0004-6361/202558205</a>"},"date_updated":"2026-10-20T08:16:24Z","supplementarymaterial":"no","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","PlanS_conform":"1"},{"publisher":"EDP Sciences","month":"05","department":[{"_id":"LiBu"}],"external_id":{"arxiv":["2603.16597"]},"oa":1,"day":"01","researchdata_availability":"no","doi":"10.1051/0004-6361/202557690","file":[{"access_level":"open_access","creator":"dernst","relation":"main_file","success":1,"date_created":"2026-10-07T12:35:39Z","checksum":"6f5d496ee876c8ff4bce6924be2cad19","file_name":"2026_AstronomyAstrophysics_Hekker.pdf","date_updated":"2026-10-07T12:35:39Z","content_type":"application/pdf","file_size":13650005,"file_id":"23077"}],"volume":709,"article_number":"A84","intvolume":"       709","publication_status":"published","year":"2026","quality_controlled":"1","ddc":["520"],"tmp":{"image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"arxiv":1,"das_tickbox":"0","fulldoi":"https://doi.org/10.1051/0004-6361/202557690","article_processing_charge":"No","has_accepted_license":"1","date_published":"2026-05-01T00:00:00Z","file_date_updated":"2026-10-07T12:35:39Z","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"acknowledgement":"We thank the referee and editor for their comments\r\nand work, which improved the manuscript significantly. We acknowledge funding from the ERC Consolidator Grant ‘DipolarSound’ (grant agreement #\r\n101000296). SB is partially supported by NSF grant AST-2205026. YE acknowledges funding from the Science and Technology Facilities Council (STFC)","scopus_import":"1","publication":"Astronomy & Astrophysics","language":[{"iso":"eng"}],"OA_place":"publisher","OA_type":"diamond","abstract":[{"lang":"eng","text":"Context. In the convective envelopes of relatively cool (surface temperature ≲6700 K) stars, oscillations are excited by turbulent convection. In these so-called solar-like oscillators, radial oscillation modes appear at nearly equally spaced frequencies. This spacing is referred to as the ‘large-frequency separation’. Deviations from equally spaced frequencies are a result of the internal structure of a star being different from a sphere of ideal gas at constant temperature. Hence, these deviations provide information on the internal structure of the star.\r\n\r\nAims. In this work, we investigate the second-order (quadratic) deviation from uniform spacing, referred to as curvature. We aim to provide homogeneous values for observed red-giant stars, understand differences between the results from observations and predictions from stellar models, and reveal the connection between curvature and stellar structure.\r\n\r\nMethods. We used Kepler data of red-giant stars and computed the curvature for several thousand stars. We compared these to the curvature derived from MESA models. We subsequently investigated the trends and differences between results from observations and models. Finally, we computed sensitivity kernels to identify the stellar region(s) to which the curvature is most sensitive and performed a glitch analysis.\r\n\r\nResults. We found that the curvature is sensitive to evolutionary phase and mass. Interestingly, the observed values and values from models show some discrepancies. Including the surface effect in the model frequencies reduces the discrepancies, though it introduces a frequency-dependent over- or under-estimation of the curvature from the models compared to the observations. From the kernels, we confirmed that the curvature is mostly sensitive to the near-surface layers of the star. The glitch analysis shows that in theory this provides information on the location and strength of the He I and H I ionisation layers.\r\n\r\nConclusions. The curvature provides a probe into the near-surface structure of the star. The deviations between the curvature derived from observations and models call for improvements in the near-surface layers of stellar models."}],"type":"journal_article","oa_version":"Published Version","article_type":"original","status":"public","author":[{"last_name":"Hekker","first_name":"S.","full_name":"Hekker, S."},{"full_name":"Elsworth, Y.","first_name":"Y.","last_name":"Elsworth"},{"last_name":"Basu","first_name":"S.","full_name":"Basu, S."},{"first_name":"F.","last_name":"Ahlborn","full_name":"Ahlborn, F."},{"last_name":"Ball","first_name":"W. H.","full_name":"Ball, W. H."},{"full_name":"Bellinger, E. P.","last_name":"Bellinger","first_name":"E. P."},{"id":"158c74c1-eed5-11ef-8c05-e45f52925cdc","last_name":"Buchele","first_name":"Lynn","full_name":"Buchele, Lynn"},{"full_name":"Espinoza-Rojas, F.","first_name":"F.","last_name":"Espinoza-Rojas"}],"date_created":"2026-10-04T22:01:54Z","title":"The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars","_id":"23045","PlanS_conform":"1","date_updated":"2026-10-20T08:14:24Z","supplementarymaterial":"yes","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"apa":"Hekker, S., Elsworth, Y., Basu, S., Ahlborn, F., Ball, W. H., Bellinger, E. P., … Espinoza-Rojas, F. (2026). The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202557690\">https://doi.org/10.1051/0004-6361/202557690</a>","chicago":"Hekker, S., Y. Elsworth, S. Basu, F. Ahlborn, W. H. Ball, E. P. Bellinger, Lynn Buchele, and F. Espinoza-Rojas. “The Sensitivity and Behaviour of the Curvature in the Échelle Diagram of Red-Giant Stars.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2026. <a href=\"https://doi.org/10.1051/0004-6361/202557690\">https://doi.org/10.1051/0004-6361/202557690</a>.","short":"S. Hekker, Y. Elsworth, S. Basu, F. Ahlborn, W.H. Ball, E.P. Bellinger, L. Buchele, F. Espinoza-Rojas, Astronomy &#38; Astrophysics 709 (2026).","ista":"Hekker S, Elsworth Y, Basu S, Ahlborn F, Ball WH, Bellinger EP, Buchele L, Espinoza-Rojas F. 2026. The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars. Astronomy &#38; Astrophysics. 709, A84.","ieee":"S. Hekker <i>et al.</i>, “The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars,” <i>Astronomy &#38; Astrophysics</i>, vol. 709. EDP Sciences, 2026.","mla":"Hekker, S., et al. “The Sensitivity and Behaviour of the Curvature in the Échelle Diagram of Red-Giant Stars.” <i>Astronomy &#38; Astrophysics</i>, vol. 709, A84, EDP Sciences, 2026, doi:<a href=\"https://doi.org/10.1051/0004-6361/202557690\">10.1051/0004-6361/202557690</a>.","ama":"Hekker S, Elsworth Y, Basu S, et al. The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars. <i>Astronomy &#38; Astrophysics</i>. 2026;709. doi:<a href=\"https://doi.org/10.1051/0004-6361/202557690\">10.1051/0004-6361/202557690</a>"},"DOAJ_listed":"1"}]