[{"article_number":"L053502","article_type":"letter_note","oa_version":"Published Version","arxiv":1,"author":[{"id":"b6798902-eea0-11ea-9cbc-a8e14286c631","last_name":"Diaz Melian","first_name":"Vicente L","full_name":"Diaz Melian, Vicente L"},{"full_name":"Lenton, Isaac C","first_name":"Isaac C","last_name":"Lenton","orcid":"0000-0002-5010-6984","id":"a550210f-223c-11ec-8182-e2d45e817efb"},{"full_name":"Binysh, Jack","first_name":"Jack","last_name":"Binysh"},{"last_name":"Souslov","first_name":"Anton","full_name":"Souslov, Anton"},{"orcid":"0000-0002-2299-3176","last_name":"Waitukaitis","id":"3A1FFC16-F248-11E8-B48F-1D18A9856A87","first_name":"Scott R","full_name":"Waitukaitis, Scott R"}],"publication_identifier":{"eissn":["2470-0053"],"issn":["2470-0045"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","corr_author":"1","acknowledgement":"This research was supported by the Scientific Service Units of The Institute of Science and Technology Austria (ISTA) through resources provided by the Miba Machine Shop and the Scientific Computing Facility. J.B. acknowledges funding from the European Union's Horizon research and innovation programme under the Marie Sklodowska-Curie Grant Agreement No. 101106500.","date_updated":"2026-06-16T11:24:18Z","publication":"Physical Review E","acknowledged_ssus":[{"_id":"M-Shop"},{"_id":"ScienComp"}],"day":"14","file_date_updated":"2026-06-16T11:21:53Z","PlanS_conform":"1","department":[{"_id":"ScWa"},{"_id":"GradSch"}],"type":"journal_article","date_published":"2026-05-14T00:00:00Z","publication_status":"published","file":[{"success":1,"date_created":"2026-06-16T11:21:53Z","date_updated":"2026-06-16T11:21:53Z","relation":"main_file","file_name":"2026_PhysicalReviewE_DiazMelian.pdf","file_size":3173197,"access_level":"open_access","file_id":"22014","content_type":"application/pdf","creator":"dernst","checksum":"902cc8d177c8d3ae9cfe07c30375c9a9"}],"intvolume":"       113","abstract":[{"lang":"eng","text":"A floating Leidenfrost droplet exhibits curvature inversion of its underside, due to the balance of vapor pressure and surface tension. Using interferometric imaging, we find different behavior for a levitated hydrogel sphere. Curvature inversion is observed briefly just after deposition, but quickly gives way to a steady state with no inversion. We show the essential role of vaporization in shaping the underbelly of the hydrogel, where changes due to direct mass loss are more significant than the balance of vapor pressure and elastic forces."}],"publisher":"American Physical Society","title":"Geometry of the vapor layer under a Leidenfrost hydrogel sphere","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"year":"2026","has_accepted_license":"1","scopus_import":"1","license":"https://creativecommons.org/licenses/by/4.0/","oa":1,"OA_type":"hybrid","external_id":{"arxiv":["2507.04982"]},"ddc":["530"],"article_processing_charge":"Yes (via OA deal)","_id":"21982","quality_controlled":"1","volume":113,"language":[{"iso":"eng"}],"OA_place":"publisher","doi":"10.1103/m7gr-2t6j","status":"public","date_created":"2026-06-10T07:36:41Z","month":"05","issue":"5","citation":{"chicago":"Diaz Melian, Vicente L, Isaac C Lenton, Jack Binysh, Anton Souslov, and Scott R Waitukaitis. “Geometry of the Vapor Layer under a Leidenfrost Hydrogel Sphere.” <i>Physical Review E</i>. American Physical Society, 2026. <a href=\"https://doi.org/10.1103/m7gr-2t6j\">https://doi.org/10.1103/m7gr-2t6j</a>.","ista":"Diaz Melian VL, Lenton IC, Binysh J, Souslov A, Waitukaitis SR. 2026. Geometry of the vapor layer under a Leidenfrost hydrogel sphere. Physical Review E. 113(5), L053502.","short":"V.L. Diaz Melian, I.C. Lenton, J. Binysh, A. Souslov, S.R. Waitukaitis, Physical Review E 113 (2026).","apa":"Diaz Melian, V. L., Lenton, I. C., Binysh, J., Souslov, A., &#38; Waitukaitis, S. R. (2026). Geometry of the vapor layer under a Leidenfrost hydrogel sphere. <i>Physical Review E</i>. American Physical Society. <a href=\"https://doi.org/10.1103/m7gr-2t6j\">https://doi.org/10.1103/m7gr-2t6j</a>","ieee":"V. L. Diaz Melian, I. C. Lenton, J. Binysh, A. Souslov, and S. R. Waitukaitis, “Geometry of the vapor layer under a Leidenfrost hydrogel sphere,” <i>Physical Review E</i>, vol. 113, no. 5. American Physical Society, 2026.","mla":"Diaz Melian, Vicente L., et al. “Geometry of the Vapor Layer under a Leidenfrost Hydrogel Sphere.” <i>Physical Review E</i>, vol. 113, no. 5, L053502, American Physical Society, 2026, doi:<a href=\"https://doi.org/10.1103/m7gr-2t6j\">10.1103/m7gr-2t6j</a>.","ama":"Diaz Melian VL, Lenton IC, Binysh J, Souslov A, Waitukaitis SR. Geometry of the vapor layer under a Leidenfrost hydrogel sphere. <i>Physical Review E</i>. 2026;113(5). doi:<a href=\"https://doi.org/10.1103/m7gr-2t6j\">10.1103/m7gr-2t6j</a>"}},{"publication_status":"published","intvolume":"        99","PlanS_conform":"1","day":"09","type":"journal_article","department":[{"_id":"GradSch"},{"_id":"CaGu"},{"_id":"GaTk"}],"date_published":"2026-05-09T00:00:00Z","corr_author":"1","date_updated":"2026-06-16T12:37:02Z","acknowledgement":"We thank Nick Barton and Noa Ottilie Borst for essential contributions to this manuscript.\r\nE.M. acknowledges support from the APART-USA fellowship, jointly funded by the Austrian Academy of Sciences (ÖAW) and the Institute of Science and Technology Austria (ISTA).\r\nThis study was supported by the European Molecular Biology Laboratory (J.C.); the European Molecular Biology Laboratory Interdisciplinary Postdoc Programme (EIPOD) under the Marie Skłodowska-Curie Actions cofund (S.H.A.).","publication":"Current Opinion in Genetics & Development","article_type":"original","article_number":"102483","arxiv":1,"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1016/j.gde.2026.102483"}],"oa_version":"Published Version","author":[{"orcid":"0000-0003-2977-7844","last_name":"Mascolo","id":"776a6ed0-a053-11f0-8635-80b95e0e0d53","first_name":"Elia","full_name":"Mascolo, Elia"},{"first_name":"Reka E","full_name":"Körei, Reka E","last_name":"Körei","id":"50FDE43E-AA30-11E9-A72B-8A12E6697425"},{"last_name":"Herrera-Álvarez","first_name":"Santiago","full_name":"Herrera-Álvarez, Santiago"},{"id":"47F8433E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-6220-2052","last_name":"Guet","first_name":"Calin C","full_name":"Guet, Calin C"},{"full_name":"Crocker, Justin","first_name":"Justin","last_name":"Crocker"},{"id":"3D494DCA-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-6699-1455","last_name":"Tkačik","full_name":"Tkačik, Gašper","first_name":"Gašper"}],"publication_identifier":{"issn":["0959-437X"],"eissn":["1879-0380"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","language":[{"iso":"eng"}],"volume":99,"doi":"10.1016/j.gde.2026.102483","OA_place":"publisher","date_created":"2026-06-10T07:37:12Z","status":"public","citation":{"ama":"Mascolo E, Körei RE, Herrera-Álvarez S, Guet CC, Crocker J, Tkačik G. Long-term evolution of regulatory DNA sequences. Part 1: Simulations on global, biophysically-realistic genotype–phenotype maps. <i>Current Opinion in Genetics &#38; Development</i>. 2026;99. doi:<a href=\"https://doi.org/10.1016/j.gde.2026.102483\">10.1016/j.gde.2026.102483</a>","ieee":"E. Mascolo, R. E. Körei, S. Herrera-Álvarez, C. C. Guet, J. Crocker, and G. Tkačik, “Long-term evolution of regulatory DNA sequences. Part 1: Simulations on global, biophysically-realistic genotype–phenotype maps,” <i>Current Opinion in Genetics &#38; Development</i>, vol. 99. Elsevier, 2026.","mla":"Mascolo, Elia, et al. “Long-Term Evolution of Regulatory DNA Sequences. Part 1: Simulations on Global, Biophysically-Realistic Genotype–Phenotype Maps.” <i>Current Opinion in Genetics &#38; Development</i>, vol. 99, 102483, Elsevier, 2026, doi:<a href=\"https://doi.org/10.1016/j.gde.2026.102483\">10.1016/j.gde.2026.102483</a>.","apa":"Mascolo, E., Körei, R. E., Herrera-Álvarez, S., Guet, C. C., Crocker, J., &#38; Tkačik, G. (2026). Long-term evolution of regulatory DNA sequences. Part 1: Simulations on global, biophysically-realistic genotype–phenotype maps. <i>Current Opinion in Genetics &#38; Development</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.gde.2026.102483\">https://doi.org/10.1016/j.gde.2026.102483</a>","short":"E. Mascolo, R.E. Körei, S. Herrera-Álvarez, C.C. Guet, J. Crocker, G. Tkačik, Current Opinion in Genetics &#38; Development 99 (2026).","ista":"Mascolo E, Körei RE, Herrera-Álvarez S, Guet CC, Crocker J, Tkačik G. 2026. Long-term evolution of regulatory DNA sequences. Part 1: Simulations on global, biophysically-realistic genotype–phenotype maps. Current Opinion in Genetics &#38; Development. 99, 102483.","chicago":"Mascolo, Elia, Reka E Körei, Santiago Herrera-Álvarez, Calin C Guet, Justin Crocker, and Gašper Tkačik. “Long-Term Evolution of Regulatory DNA Sequences. Part 1: Simulations on Global, Biophysically-Realistic Genotype–Phenotype Maps.” <i>Current Opinion in Genetics &#38; Development</i>. Elsevier, 2026. <a href=\"https://doi.org/10.1016/j.gde.2026.102483\">https://doi.org/10.1016/j.gde.2026.102483</a>."},"month":"05","oa":1,"OA_type":"hybrid","external_id":{"arxiv":["2601.19681"]},"ddc":["570"],"_id":"21983","quality_controlled":"1","article_processing_charge":"Yes (via OA deal)","scopus_import":"1","year":"2026","has_accepted_license":"1","abstract":[{"text":"Promoters and enhancers are cis-regulatory elements (CREs), DNA sequences that bind transcription factor (TF) proteins to up- or down-regulate target genes. Decades-long efforts yielded TF-DNA interaction models that predict how strongly an individual TF binds arbitrary DNA sequences and how individual binding events on the CRE combine to affect gene expression. These insights can be synthesized into a global, biophysically realistic, and quantitative genotype–phenotype map for gene regulation, a ‘holy grail’ for the application of evolutionary theory. A global map provides a rare opportunity to simulate the long-term evolution of regulatory sequences and pose several fundamental questions: How long does it take to evolve CREs de novo? How many non-trivial regulatory functions exist in sequence space? How connected are they? For which regulatory architecture is CRE evolution most rapid and evolvable? In this article, the first of a two-part series, we briefly review the pertinent modeling and simulation efforts for a unique system that enables close, quantitative, and mechanistic links between biophysics, as well as systems, synthetic, and evolutionary biology.","lang":"eng"}],"publisher":"Elsevier","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"title":"Long-term evolution of regulatory DNA sequences. Part 1: Simulations on global, biophysically-realistic genotype–phenotype maps"},{"oa":1,"OA_type":"green","ddc":["580"],"article_processing_charge":"No","_id":"21994","language":[{"iso":"eng"}],"doi":"10.1101/2025.10.07.680881","OA_place":"repository","date_created":"2026-06-13T16:57:07Z","project":[{"name":"Cyclic nucleotides as second messengers in plants","_id":"8f347782-16d5-11f0-9cad-8c19706ee739","grant_number":"101142681"},{"name":"Peptide receptors for auxin canalization in Arabidopsis","_id":"bd76d395-d553-11ed-ba76-f678c14f9033","grant_number":"I06123"},{"_id":"7bcece63-9f16-11ee-852c-ae94e099eeb6","grant_number":"P37051","name":"Guanylate cyclase activity of TIR1/AFBs auxin receptors"}],"status":"public","citation":{"apa":"Ge, Z., Koczka, L., Mazur, E., Molnar, G., Vladimirtsev, D., Kassem, N., … Friml, J. (n.d.). MAKR6 integrates TMK and CAMEL/CANAR signalling for auxin canalization in Arabidopsis. <i>bioRxiv</i>. <a href=\"https://doi.org/10.1101/2025.10.07.680881\">https://doi.org/10.1101/2025.10.07.680881</a>","mla":"Ge, Zengxiang, et al. “MAKR6 Integrates TMK and CAMEL/CANAR Signalling for Auxin Canalization in Arabidopsis.” <i>BioRxiv</i>, doi:<a href=\"https://doi.org/10.1101/2025.10.07.680881\">10.1101/2025.10.07.680881</a>.","ieee":"Z. Ge <i>et al.</i>, “MAKR6 integrates TMK and CAMEL/CANAR signalling for auxin canalization in Arabidopsis,” <i>bioRxiv</i>. .","ama":"Ge Z, Koczka L, Mazur E, et al. MAKR6 integrates TMK and CAMEL/CANAR signalling for auxin canalization in Arabidopsis. <i>bioRxiv</i>. doi:<a href=\"https://doi.org/10.1101/2025.10.07.680881\">10.1101/2025.10.07.680881</a>","ista":"Ge Z, Koczka L, Mazur E, Molnar G, Vladimirtsev D, Kassem N, Ait Ikene S, Fiedler L, Friml J. MAKR6 integrates TMK and CAMEL/CANAR signalling for auxin canalization in Arabidopsis. bioRxiv, <a href=\"https://doi.org/10.1101/2025.10.07.680881\">10.1101/2025.10.07.680881</a>.","chicago":"Ge, Zengxiang, Lilla Koczka, Ewa Mazur, Gergely Molnar, Dmitrii Vladimirtsev, Nada Kassem, Sara Ait Ikene, Lukas Fiedler, and Jiří Friml. “MAKR6 Integrates TMK and CAMEL/CANAR Signalling for Auxin Canalization in Arabidopsis.” <i>BioRxiv</i>, n.d. <a href=\"https://doi.org/10.1101/2025.10.07.680881\">https://doi.org/10.1101/2025.10.07.680881</a>.","short":"Z. Ge, L. Koczka, E. Mazur, G. Molnar, D. Vladimirtsev, N. Kassem, S. Ait Ikene, L. Fiedler, J. Friml, BioRxiv (n.d.)."},"month":"05","abstract":[{"text":"Adaptive plant development is orchestrated, among others, by directional, intercellular transport of the phytohormone auxin. Self-organizing development, such as flexible vasculature formation, depends on so-called auxin canalization, manifested by the gradual formation of auxin transport channels through feedback between auxin signalling and transport. Herein, we identify MAKR6 as an important, novel component in this feedback. MAKR6 expression accumulates strongly in vascular cells and is tightly regulated by auxin via the Aux/IAA-ARF-WRKY23 transcriptional network. MAKR6 is required for auxin canalization-dependent processes, including leaf venation, vasculature regeneration, and de novo auxin channel formation from local auxin sources. Mechanistically, MAKR6 interacts with the PIN1 auxin transporter, modulating its trafficking and polarization. MAKR6 also associates with and integrates two key receptor-like kinase complexes involved in canalization, TMK1/4 and the CAMEL-CANAR. Together, our study establishes MAKR6 as a multifaceted regulator that couples transcriptional auxin signalling to PIN1 repolarization and coordinates multiple RLK-mediated signalling pathways during canalization. This provides mechanistic insights into auxin canalization and exemplifies a framework for exploring similar regulatory nodes in other developmental contexts.","lang":"eng"}],"tmp":{"short":"CC BY-NC-ND (4.0)","image":"/images/cc_by_nc_nd.png","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)"},"title":"MAKR6 integrates TMK and CAMEL/CANAR signalling for auxin canalization in Arabidopsis","scopus_import":"1","has_accepted_license":"1","year":"2026","license":"https://creativecommons.org/licenses/by-nc-nd/4.0/","day":"30","type":"preprint","department":[{"_id":"GradSch"},{"_id":"JiFr"}],"date_published":"2026-05-30T00:00:00Z","publication_status":"submitted","oa_version":"Preprint","main_file_link":[{"url":"https://doi.org/10.1101/2025.10.07.680881","open_access":"1"}],"author":[{"full_name":"Ge, Zengxiang","first_name":"Zengxiang","orcid":"0000-0001-9381-3577","last_name":"Ge","id":"f43371a3-09ff-11eb-8013-bd0c6a2f6de8"},{"full_name":"Koczka, Lilla","first_name":"Lilla","last_name":"Koczka"},{"full_name":"Mazur, Ewa","first_name":"Ewa","last_name":"Mazur"},{"first_name":"Gergely","full_name":"Molnar, Gergely","last_name":"Molnar","id":"34F1AF46-F248-11E8-B48F-1D18A9856A87"},{"first_name":"Dmitrii","full_name":"Vladimirtsev, Dmitrii","id":"60466724-5355-11ee-ae5a-fa55e8f99c3d","last_name":"Vladimirtsev"},{"full_name":"Kassem, Nada","first_name":"Nada","last_name":"Kassem"},{"last_name":"Ait Ikene","id":"6a0bb896-6bad-11f1-9bef-906e9eb76034","first_name":"Sara","full_name":"Ait Ikene, Sara"},{"full_name":"Fiedler, Lukas","first_name":"Lukas","id":"7c417475-8972-11ed-ae7b-8b674ca26986","last_name":"Fiedler"},{"full_name":"Friml, Jiří","first_name":"Jiří","orcid":"0000-0002-8302-7596","last_name":"Friml","id":"4159519E-F248-11E8-B48F-1D18A9856A87"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","corr_author":"1","date_updated":"2026-06-19T07:14:01Z","acknowledgement":"We would like to thank Dr. Yvon Jaillais (ENS, Lyon) for sharing MAKR2 materials. This research was supported by the Scientific Service Units (SSU) of ISTA through resources provided by the Imaging & Optics Facility (IOF) and the Lab Support Facility (LSF). The research in the Friml group leading to these results was funded by the European Research Council (ERC): 101142681 CYNIPS; and the Austrian Science Fund (FWF): I 6123-B and P 37051-B. Ewa Mazur was supported by the National Science Centre (NCN), Poland, under the OPUS call in the WEAVE programme: 2021/43/I/NZ1/01835.","publication":"bioRxiv"},{"publisher":"Springer Nature","title":"One-milligram torsional pendulum toward experiments at the quantum-gravity interface","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"abstract":[{"lang":"eng","text":"Probing the possibility of entanglement generation through gravity offers a path to tackle the question of whether gravitational fields possess a quantum mechanical nature. A potential realization necessitates systems with low-frequency dynamics at an optimal mass scale, for which the microgram-to-milligram range is a strong contender. Here, after refining a figure-of-merit for the problem, we present a 1-milligram torsional pendulum operating at 18 Hz. We demonstrate laser cooling its motion from room temperature to 240 microkelvins, surpassing by over 20-fold the coldest motions attained for oscillators ranging from micrograms to kilograms. We quantify and contrast the utility of the current approach with other platforms. The achieved performance and large improvement potential highlight milligram-scale torsional pendulums as a powerful platform for precision measurements relevant to future studies at the quantum-gravity interface."}],"scopus_import":"1","year":"2026","has_accepted_license":"1","ddc":["530"],"_id":"20840","quality_controlled":"1","article_processing_charge":"Yes","oa":1,"external_id":{"arxiv":["2408.09445"]},"OA_type":"gold","date_created":"2025-12-21T11:39:04Z","project":[{"name":"A quantum hybrid of atoms and milligram-scale pendulums: towards gravitational quantum mechanics","_id":"bdb2a702-d553-11ed-ba76-f12e3e5a3bc6","grant_number":"101087907"}],"status":"public","citation":{"ista":"Agafonova S, Rosello P, Mekonnen M, Hosten O. 2026. One-milligram torsional pendulum toward experiments at the quantum-gravity interface. Communications Physics. 9, 80.","chicago":"Agafonova, Sofia, Pere Rosello, Manuel Mekonnen, and Onur Hosten. “One-Milligram Torsional Pendulum toward Experiments at the Quantum-Gravity Interface.” <i>Communications Physics</i>. Springer Nature, 2026. <a href=\"https://doi.org/10.1038/s42005-026-02514-w\">https://doi.org/10.1038/s42005-026-02514-w</a>.","short":"S. Agafonova, P. Rosello, M. Mekonnen, O. Hosten, Communications Physics 9 (2026).","apa":"Agafonova, S., Rosello, P., Mekonnen, M., &#38; Hosten, O. (2026). One-milligram torsional pendulum toward experiments at the quantum-gravity interface. <i>Communications Physics</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s42005-026-02514-w\">https://doi.org/10.1038/s42005-026-02514-w</a>","ieee":"S. Agafonova, P. Rosello, M. Mekonnen, and O. Hosten, “One-milligram torsional pendulum toward experiments at the quantum-gravity interface,” <i>Communications Physics</i>, vol. 9. Springer Nature, 2026.","mla":"Agafonova, Sofia, et al. “One-Milligram Torsional Pendulum toward Experiments at the Quantum-Gravity Interface.” <i>Communications Physics</i>, vol. 9, 80, Springer Nature, 2026, doi:<a href=\"https://doi.org/10.1038/s42005-026-02514-w\">10.1038/s42005-026-02514-w</a>.","ama":"Agafonova S, Rosello P, Mekonnen M, Hosten O. One-milligram torsional pendulum toward experiments at the quantum-gravity interface. <i>Communications Physics</i>. 2026;9. doi:<a href=\"https://doi.org/10.1038/s42005-026-02514-w\">10.1038/s42005-026-02514-w</a>"},"month":"03","language":[{"iso":"eng"}],"volume":9,"OA_place":"publisher","doi":"10.1038/s42005-026-02514-w","publication_identifier":{"eissn":["2399-3650"]},"author":[{"first_name":"Sofya","full_name":"Agafonova, Sofya","orcid":"0000-0003-0582-2946","last_name":"Agafonova","id":"09501ff6-dca7-11ea-a8ae-b3e0b9166e80"},{"last_name":"Rosello","full_name":"Rosello, Pere","first_name":"Pere"},{"last_name":"Mekonnen","full_name":"Mekonnen, Manuel","first_name":"Manuel"},{"first_name":"Onur","full_name":"Hosten, Onur","last_name":"Hosten","orcid":"0000-0002-2031-204X","id":"4C02D85E-F248-11E8-B48F-1D18A9856A87"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","article_number":"80","arxiv":1,"oa_version":"Published Version","related_material":{"record":[{"relation":"research_data","status":"public","id":"20842"}]},"publication":"Communications Physics","corr_author":"1","date_updated":"2026-06-10T08:36:06Z","acknowledgement":"We thank Gerard Higgins, Andrei Militaru, Nikolai Kiesel, and Markus Aspelmeyer for useful discussions on the topic of the figure-of-merit. We thank Teodor Strömberg for helping with the additional characterizations of the optical lever noise. We thank Johannes Fink and Scott Waitukaitis for their helpful feedback on the manuscript. This work was supported by Institute of Science and Technology Austria and the European Research Council under Grant No. 101087907 (ERC CoG QuHAMP).","date_published":"2026-03-04T00:00:00Z","PlanS_conform":"1","file_date_updated":"2026-03-16T10:07:46Z","day":"04","type":"journal_article","department":[{"_id":"GradSch"},{"_id":"OnHo"}],"publication_status":"published","intvolume":"         9","file":[{"relation":"main_file","date_updated":"2026-03-16T10:07:46Z","success":1,"date_created":"2026-03-16T10:07:46Z","creator":"dernst","checksum":"62e2175e7e3ad49260ae6a7b4e0860a2","content_type":"application/pdf","file_id":"21457","access_level":"open_access","file_size":1901772,"file_name":"2026_CommunicationsPhysics_Agafonova.pdf"}],"DOAJ_listed":"1"},{"date_published":"2026-01-14T00:00:00Z","page":"22","type":"dissertation","department":[{"_id":"GradSch"},{"_id":"JiFr"}],"day":"14","file_date_updated":"2026-01-28T12:38:19Z","alternative_title":["ISTA Master’s Thesis"],"file":[{"checksum":"812857b2fbe3f6113bef22fd04bccd3e","creator":"dvladimi","embargo":"2027-01-01","file_id":"21033","content_type":"application/pdf","file_name":"2026_Vladimirtsev_Dmitrii_Thesis.pdf","access_level":"closed","file_size":2867531,"date_updated":"2026-01-21T14:12:13Z","relation":"main_file","embargo_to":"open_access","date_created":"2026-01-21T14:12:13Z"},{"file_name":"Source Files.zip","access_level":"closed","file_size":25023066,"checksum":"2b969f97f8d7461bea3d255f48c2219c","creator":"dvladimi","content_type":"application/x-zip-compressed","file_id":"21034","date_created":"2026-01-21T14:41:58Z","date_updated":"2026-01-28T12:38:19Z","relation":"source_file"}],"publication_status":"published","user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","author":[{"first_name":"Dmitrii","full_name":"Vladimirtsev, Dmitrii","id":"60466724-5355-11ee-ae5a-fa55e8f99c3d","last_name":"Vladimirtsev"}],"publication_identifier":{"issn":["2791-4585"]},"oa_version":"Published Version","acknowledged_ssus":[{"_id":"LifeSc"},{"_id":"Bio"}],"related_material":{"record":[{"id":"20982","status":"public","relation":"part_of_dissertation"}]},"date_updated":"2026-04-07T11:41:44Z","corr_author":"1","article_processing_charge":"No","_id":"20964","ddc":["570"],"supervisor":[{"full_name":"Friml, Jiří","first_name":"Jiří","id":"4159519E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8302-7596","last_name":"Friml"}],"citation":{"chicago":"Vladimirtsev, Dmitrii. “Armadillo Repeat Only Proteins Are Master Regulators of Plant Cyclic-Nucleotide Gated Channels.” Institute of Science and Technology Austria, 2026. <a href=\"https://doi.org/10.15479/AT-ISTA-20964\">https://doi.org/10.15479/AT-ISTA-20964</a>.","ista":"Vladimirtsev D. 2026. Armadillo repeat only proteins are master regulators of plant cyclic-nucleotide gated channels. Institute of Science and Technology Austria.","short":"D. Vladimirtsev, Armadillo Repeat Only Proteins Are Master Regulators of Plant Cyclic-Nucleotide Gated Channels, Institute of Science and Technology Austria, 2026.","apa":"Vladimirtsev, D. (2026). <i>Armadillo repeat only proteins are master regulators of plant cyclic-nucleotide gated channels</i>. Institute of Science and Technology Austria. <a href=\"https://doi.org/10.15479/AT-ISTA-20964\">https://doi.org/10.15479/AT-ISTA-20964</a>","ama":"Vladimirtsev D. Armadillo repeat only proteins are master regulators of plant cyclic-nucleotide gated channels. 2026. doi:<a href=\"https://doi.org/10.15479/AT-ISTA-20964\">10.15479/AT-ISTA-20964</a>","mla":"Vladimirtsev, Dmitrii. <i>Armadillo Repeat Only Proteins Are Master Regulators of Plant Cyclic-Nucleotide Gated Channels</i>. Institute of Science and Technology Austria, 2026, doi:<a href=\"https://doi.org/10.15479/AT-ISTA-20964\">10.15479/AT-ISTA-20964</a>.","ieee":"D. Vladimirtsev, “Armadillo repeat only proteins are master regulators of plant cyclic-nucleotide gated channels,” Institute of Science and Technology Austria, 2026."},"month":"01","project":[{"_id":"8f347782-16d5-11f0-9cad-8c19706ee739","grant_number":"101142681","name":"Cyclic nucleotides as second messengers in plants"}],"date_created":"2026-01-09T09:22:48Z","status":"public","doi":"10.15479/AT-ISTA-20964","OA_place":"publisher","language":[{"iso":"eng"}],"degree_awarded":"MS","title":"Armadillo repeat only proteins are master regulators of plant cyclic-nucleotide gated channels","publisher":"Institute of Science and Technology Austria","has_accepted_license":"1","year":"2026"},{"author":[{"last_name":"Garcia Castillo","id":"ae681a14-dc74-11ea-a0a7-c6ef18161701","full_name":"Garcia Castillo, Diego Fernando","first_name":"Diego Fernando"}],"publication_identifier":{"isbn":["978-3-99078-077-0"],"issn":["2663-337X"]},"user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","oa_version":"Published Version","related_material":{"record":[{"id":"18498","status":"public","relation":"research_data"},{"id":"18491","status":"public","relation":"part_of_dissertation"}]},"corr_author":"1","acknowledgement":"I acknowledge the funding agencies 1Norwegian Research Council RCN project 315287.\r\n2The FIASCO project \"Illuminating range shifts through evolutionary FIASCO: contrasting\r\nFaIling And Successful ColOnizations in replicated wild populations\", funded by the\r\nEuropean Union - Next Generation EU (Piano Nazionale di Ripresa e Resilienza - MUR\r\ncode: P202229JBC, CUP: C53D23007100001). 3Ecotypic formation in Littorina saxatilis\r\nin the Western Atlantic and comparisons across the North Atlantic. University of\r\nGothenburg Research Travel Grant, Tjarno Marine Laboratory, Sweden. $3023 (2018).\r\n4JIN project (Young Researchers, Spanish Ministry of Science, RTI2018-101274-J-I00)","date_updated":"2026-04-16T12:20:37Z","date_published":"2026-01-16T00:00:00Z","file_date_updated":"2026-01-16T13:08:59Z","day":"16","department":[{"_id":"GradSch"},{"_id":"NiBa"}],"type":"dissertation","page":"199","publication_status":"published","file":[{"file_id":"20996","content_type":"application/vnd.openxmlformats-officedocument.wordprocessingml.document","checksum":"841f1bc073d667125729b2a017f8c37a","creator":"dgarciac","access_level":"closed","file_size":22456421,"file_name":"2026_Garcia_Diego_Thesis.docx","relation":"source_file","date_updated":"2026-01-16T12:25:13Z","date_created":"2026-01-16T12:25:13Z"},{"relation":"main_file","date_updated":"2026-01-16T12:25:13Z","date_created":"2026-01-16T12:25:13Z","success":1,"checksum":"a1f33d4f183ce7072eee42a6ccf5340b","creator":"dgarciac","file_id":"20997","content_type":"application/pdf","file_size":9556719,"access_level":"open_access","file_name":"2026_Garcia_Diego_Thesis.pdf"},{"date_created":"2026-01-16T13:08:14Z","date_updated":"2026-01-16T13:08:14Z","relation":"supplementary_material","file_name":"2026_DiegoGarcia_LittorinaDB Source Code and Protocols.rar","access_level":"closed","file_size":54491433,"creator":"dgarciac","checksum":"98a80691067174c30fe53f38ce7344e6","description":"Source code of the PostgreSQL database, front-end and back-end of the LittorinaDB web application developed as a product of the 4th chapter of the thesis.","content_type":"application/x-compressed","file_id":"20998"},{"date_created":"2026-01-16T13:08:14Z","relation":"supplementary_material","date_updated":"2026-01-16T13:08:14Z","file_size":7982811,"access_level":"open_access","file_name":"2026_DiegoGarcia_Thesis-Supplementary_Material.rar","checksum":"99a3cab2fa36666b9a92eefc27d586da","creator":"dgarciac","file_id":"20999","content_type":"application/x-compressed"},{"content_type":"text/plain","file_id":"21000","checksum":"255fdf56b2932c46bf27c63aa6106a4f","creator":"dgarciac","access_level":"open_access","file_size":732,"file_name":"README.txt","relation":"supplementary_material","date_updated":"2026-01-16T13:08:59Z","date_created":"2026-01-16T13:08:59Z"}],"alternative_title":["ISTA Thesis"],"publisher":"Institute of Science and Technology Austria","title":"The genomic architecture of local adaptation in introduced populations","tmp":{"short":"CC BY-NC-SA (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode","image":"/images/cc_by_nc_sa.png","name":"Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)"},"abstract":[{"text":"Rapid local adaptation to new environments is critical for species persistence, especially in introduced populations. The evolutionary success of these populations is fundamentally dictated by the organization of genetic variation—the genomic architecture—in the face of severe demographic constraints, such as the founder effects and genetic bottlenecks that frequently accompany colonization. A central question in evolutionary biology is whether rapid adaptation relies on major-effect loci, such as chromosomal inversions, or on many small-effect loci dispersed across the genome. Furthermore, the genomic architecture strongly influences the extent to which evolutionary outcomes are predictable. Using introduced populations of the marine snail, Littorina saxatilis, as a model, this thesis investigates how genetic variation and genomic structure drive adaptation following introduction. We employed a population genomics approach on experimentally and accidentally introduced populations to dissect the specific genomic features that underpin divergence in newly colonized environments.\r\n\r\nIn Chapter 2, we tested the predictability of local adaptation through an uncommon 30-year transplant experiment in nature. By distinguishing allele and chromosomal inversion frequency changes from neutral expectations, we found that evolutionary change was highly predictable at the macro-scale (phenotypes and chromosomal inversions), but less robust at the level of individual collinear loci. This result demonstrates that evolution can be predictable when a population possesses sufficient standing genetic variation (SGV), with chromosomal inversions acting as key integrated units that facilitate a rapid response to selection. Building on this, Chapter 3 applied whole-genome sequencing to three accidentally introduced populations (Venice, San Francisco, and Redwood City) to investigate their likely source and genomic patterns of divergence. We identified genomic regions of remarkable divergence potentially associated with local adaptation, and likely fuelled by SGV, while explicitly acknowledging the difficulty in disentangling selection signals from the genome-wide effects of demographic processes. Furthermore, we found that the divergence patterns relied extensively on the collinear genome in these introduced populations, and less clearly on the chromosomal inversions. This observation contrasts with local adaptation observed in the experimental system that relied on both collinear loci and highly selected chromosomal inversions, highlighting how demographic history and genomic architecture influence the detectable signature of local adaptation.\r\n\r\nA major limitation to conducting large-scale comparative evolutionary studies is the lack of data standardization, which prevents the integration of community knowledge and high-resolution environmental and genetic data. Chapter 4 addresses this by developing a community database for the Littorina system. This platform implements standardized protocols for the integration of diverse phenotypic and environmental data from multiple Littorina species. Likewise, the platform also centralizes the availability of associated genomic data through links to external repositories. This database represents a crucial tool to test complex, large-scale evolutionary hypotheses.\r\n\r\nCollectively, this thesis strongly reinforces the fundamental importance of SGV as the raw material for successful local adaptation, a conclusion supported by evidence in both experimental and accidental introductions. Furthermore, this work highlights the critical role of the genomic architecture—specifically chromosomal inversions—in driving the predictability and effectiveness of adaptive responses. Our findings underscore how the interplay between SGV and genomic architecture dictates the trajectory and detectability of evolution in colonizing populations, while simultaneously providing a necessary tool to advance comparative evolutionary genomics in emerging model organisms.","lang":"eng"}],"license":"https://creativecommons.org/licenses/by-nc-sa/4.0/","year":"2026","has_accepted_license":"1","supervisor":[{"full_name":"Barton, Nicholas H","first_name":"Nicholas H","last_name":"Barton","orcid":"0000-0002-8548-5240","id":"4880FE40-F248-11E8-B48F-1D18A9856A87"},{"orcid":"0000-0003-1050-4969","last_name":"Westram","id":"3C147470-F248-11E8-B48F-1D18A9856A87","first_name":"Anja M","full_name":"Westram, Anja M"}],"ddc":["576"],"_id":"20991","article_processing_charge":"No","oa":1,"status":"public","date_created":"2026-01-16T09:47:59Z","month":"01","citation":{"apa":"Garcia Castillo, D. F. (2026). <i>The genomic architecture of local adaptation in introduced populations</i>. Institute of Science and Technology Austria. <a href=\"https://doi.org/10.15479/AT-ISTA-20991\">https://doi.org/10.15479/AT-ISTA-20991</a>","mla":"Garcia Castillo, Diego Fernando. <i>The Genomic Architecture of Local Adaptation in Introduced Populations</i>. Institute of Science and Technology Austria, 2026, doi:<a href=\"https://doi.org/10.15479/AT-ISTA-20991\">10.15479/AT-ISTA-20991</a>.","ieee":"D. F. Garcia Castillo, “The genomic architecture of local adaptation in introduced populations,” Institute of Science and Technology Austria, 2026.","ama":"Garcia Castillo DF. The genomic architecture of local adaptation in introduced populations. 2026. doi:<a href=\"https://doi.org/10.15479/AT-ISTA-20991\">10.15479/AT-ISTA-20991</a>","chicago":"Garcia Castillo, Diego Fernando. “The Genomic Architecture of Local Adaptation in Introduced Populations.” Institute of Science and Technology Austria, 2026. <a href=\"https://doi.org/10.15479/AT-ISTA-20991\">https://doi.org/10.15479/AT-ISTA-20991</a>.","ista":"Garcia Castillo DF. 2026. The genomic architecture of local adaptation in introduced populations. Institute of Science and Technology Austria.","short":"D.F. Garcia Castillo, The Genomic Architecture of Local Adaptation in Introduced Populations, Institute of Science and Technology Austria, 2026."},"degree_awarded":"PhD","language":[{"iso":"eng"}],"OA_place":"publisher","doi":"10.15479/AT-ISTA-20991"},{"article_processing_charge":"No","_id":"21001","quality_controlled":"1","OA_type":"closed access","month":"01","issue":"1","citation":{"ista":"Patil NN, Wu R, Fiedler C, Kapuria N, Nan B, Jakhar N, Cabot A, Ibáñez M, Ryan KM, Ganose AM, Singh S. 2026. Layered alkali-copper selenides: Deciphering thermoelectric properties and reaction pathways for nanostructuring β-CsCu5Se3. ACS Energy Letters. 11(1), 481–488.","chicago":"Patil, Niraj Nitish, Ruiqi Wu, Christine Fiedler, Nilotpal Kapuria, Bingfei Nan, Navita Jakhar, Andreu Cabot, et al. “Layered Alkali-Copper Selenides: Deciphering Thermoelectric Properties and Reaction Pathways for Nanostructuring β-CsCu5Se3.” <i>ACS Energy Letters</i>. American Chemical Society, 2026. <a href=\"https://doi.org/10.1021/acsenergylett.5c02909\">https://doi.org/10.1021/acsenergylett.5c02909</a>.","short":"N.N. Patil, R. Wu, C. Fiedler, N. Kapuria, B. Nan, N. Jakhar, A. Cabot, M. Ibáñez, K.M. Ryan, A.M. Ganose, S. Singh, ACS Energy Letters 11 (2026) 481–488.","apa":"Patil, N. N., Wu, R., Fiedler, C., Kapuria, N., Nan, B., Jakhar, N., … Singh, S. (2026). Layered alkali-copper selenides: Deciphering thermoelectric properties and reaction pathways for nanostructuring β-CsCu5Se3. <i>ACS Energy Letters</i>. American Chemical Society. <a href=\"https://doi.org/10.1021/acsenergylett.5c02909\">https://doi.org/10.1021/acsenergylett.5c02909</a>","ama":"Patil NN, Wu R, Fiedler C, et al. Layered alkali-copper selenides: Deciphering thermoelectric properties and reaction pathways for nanostructuring β-CsCu5Se3. <i>ACS Energy Letters</i>. 2026;11(1):481-488. doi:<a href=\"https://doi.org/10.1021/acsenergylett.5c02909\">10.1021/acsenergylett.5c02909</a>","mla":"Patil, Niraj Nitish, et al. “Layered Alkali-Copper Selenides: Deciphering Thermoelectric Properties and Reaction Pathways for Nanostructuring β-CsCu5Se3.” <i>ACS Energy Letters</i>, vol. 11, no. 1, American Chemical Society, 2026, pp. 481–88, doi:<a href=\"https://doi.org/10.1021/acsenergylett.5c02909\">10.1021/acsenergylett.5c02909</a>.","ieee":"N. N. Patil <i>et al.</i>, “Layered alkali-copper selenides: Deciphering thermoelectric properties and reaction pathways for nanostructuring β-CsCu5Se3,” <i>ACS Energy Letters</i>, vol. 11, no. 1. American Chemical Society, pp. 481–488, 2026."},"status":"public","date_created":"2026-01-18T23:02:43Z","project":[{"_id":"9B8F7476-BA93-11EA-9121-9846C619BF3A","name":"HighTE: The Werner Siemens Laboratory for the High Throughput Discovery of Semiconductors for Waste Heat Recovery"}],"doi":"10.1021/acsenergylett.5c02909","volume":11,"language":[{"iso":"eng"}],"title":"Layered alkali-copper selenides: Deciphering thermoelectric properties and reaction pathways for nanostructuring β-CsCu5Se3","publisher":"American Chemical Society","abstract":[{"text":"Copper chalcogenides offer high charge mobility and low lattice thermal conductivity but suffer from structural instability due to dynamic Cu+ migration. Here, we report a colloidal hot-injection synthesis of ternary cesium copper selenide (CsCu5Se3) nanocrystals (NCs), achieving precise control over phase, size, and morphology through tailored precursor-ligand modulation. This strategy enabled systematic exploration of stable and metastable Cs–Cu–Se phases and mechanistic investigation of nucleation and growth, providing insight into phase modulation and dimensional control at the nanoscale. CsCu5Se3 NCs exhibit low lattice thermal conductivity (∼0.5 Wm–1K–1) and an experimental zT of 0.27 at 718 K. Complementary first-principles calculations, consistent with experimental electronic and optical responses, predict a zT of 1.05 at 1000 K. These findings elucidate the formation dynamics of CsCu5Se3 and establish ABZ (A = alkali, B = metal, Z = chalcogen) NCs as tunable platforms for advanced functional applications.","lang":"eng"}],"year":"2026","scopus_import":"1","date_published":"2026-01-09T00:00:00Z","department":[{"_id":"MaIb"},{"_id":"GradSch"}],"page":"481-488","type":"journal_article","day":"09","intvolume":"        11","publication_status":"published","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["2380-8195"]},"author":[{"last_name":"Patil","first_name":"Niraj Nitish","full_name":"Patil, Niraj Nitish"},{"last_name":"Wu","first_name":"Ruiqi","full_name":"Wu, Ruiqi"},{"full_name":"Fiedler, Christine","first_name":"Christine","id":"bd3fceba-dc74-11ea-a0a7-c17f71817366","last_name":"Fiedler"},{"first_name":"Nilotpal","full_name":"Kapuria, Nilotpal","last_name":"Kapuria"},{"first_name":"Bingfei","full_name":"Nan, Bingfei","last_name":"Nan"},{"full_name":"Navita, Navita","first_name":"Navita","orcid":"0000-0001-7408-8197","last_name":"Navita","id":"6ebe278d-ba0b-11ee-8184-f34cdc671de4"},{"full_name":"Cabot, Andreu","first_name":"Andreu","last_name":"Cabot"},{"last_name":"Ibáñez","orcid":"0000-0001-5013-2843","id":"43C61214-F248-11E8-B48F-1D18A9856A87","full_name":"Ibáñez, Maria","first_name":"Maria"},{"full_name":"Ryan, Kevin M.","first_name":"Kevin M.","last_name":"Ryan"},{"first_name":"Alex M.","full_name":"Ganose, Alex M.","last_name":"Ganose"},{"last_name":"Singh","first_name":"Shalini","full_name":"Singh, Shalini"}],"oa_version":"None","article_type":"letter_note","publication":"ACS Energy Letters","acknowledgement":"This publication has emanated from research conducted with the financial support of Taighde Éireann-Research Ireland under Grant number 22/FFP-P/11591. C.F. and M.I. would like to acknowledge the financial support of ISTA and the Werner Siemens Foundation. N.N.P. acknowledges the financial support of AMBER under grant number 12/rc/2278_p2.","date_updated":"2026-01-19T08:43:21Z"},{"ddc":["540"],"article_processing_charge":"Yes (via OA deal)","_id":"21008","quality_controlled":"1","oa":1,"OA_type":"hybrid","status":"public","project":[{"name":"Photoactive ligands for transformative nickel catalysis","grant_number":"PAT 1250924","_id":"8f1d607d-16d5-11f0-9cad-ab453295ba5e"}],"date_created":"2026-01-20T10:04:57Z","month":"01","issue":"2","citation":{"ieee":"A. Bena and B. Pieber, “Advances in NiI/NiIII-catalyzed C(sp2)–heteroatom cross-couplings,” <i>ACS Catalysis</i>, vol. 16, no. 2. American Chemical Society, pp. 866–881, 2026.","mla":"Bena, Aleksander, and Bartholomäus Pieber. “Advances in NiI/NiIII-Catalyzed C(Sp2)–Heteroatom Cross-Couplings.” <i>ACS Catalysis</i>, vol. 16, no. 2, American Chemical Society, 2026, pp. 866–81, doi:<a href=\"https://doi.org/10.1021/acscatal.5c07964\">10.1021/acscatal.5c07964</a>.","ama":"Bena A, Pieber B. Advances in NiI/NiIII-catalyzed C(sp2)–heteroatom cross-couplings. <i>ACS Catalysis</i>. 2026;16(2):866-881. doi:<a href=\"https://doi.org/10.1021/acscatal.5c07964\">10.1021/acscatal.5c07964</a>","apa":"Bena, A., &#38; Pieber, B. (2026). Advances in NiI/NiIII-catalyzed C(sp2)–heteroatom cross-couplings. <i>ACS Catalysis</i>. American Chemical Society. <a href=\"https://doi.org/10.1021/acscatal.5c07964\">https://doi.org/10.1021/acscatal.5c07964</a>","short":"A. Bena, B. Pieber, ACS Catalysis 16 (2026) 866–881.","chicago":"Bena, Aleksander, and Bartholomäus Pieber. “Advances in NiI/NiIII-Catalyzed C(Sp2)–Heteroatom Cross-Couplings.” <i>ACS Catalysis</i>. American Chemical Society, 2026. <a href=\"https://doi.org/10.1021/acscatal.5c07964\">https://doi.org/10.1021/acscatal.5c07964</a>.","ista":"Bena A, Pieber B. 2026. Advances in NiI/NiIII-catalyzed C(sp2)–heteroatom cross-couplings. ACS Catalysis. 16(2), 866–881."},"volume":16,"language":[{"iso":"eng"}],"OA_place":"publisher","doi":"10.1021/acscatal.5c07964","publisher":"American Chemical Society","title":"Advances in NiI/NiIII-catalyzed C(sp2)–heteroatom cross-couplings","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"abstract":[{"text":"C(sp2)–heteroatom couplings operating via NiI/NiIII catalysis have emerged as an alternative to canonical Pd0/PdII systems that require complex ligand architectures. Despite intensive research efforts during the past decade, catalytic methods employing this approach are still mostly confined to activated starting materials and require high catalyst loadings due to the low catalytic activity of NiI and undesired catalyst deactivation events. This article highlights recent advances in the field toward solving these long-standing challenges. We survey strategies that streamline the generation of catalytically competent NiI species from bench-stable NiII precatalysts, and discuss mechanistic studies that shed light on deactivation pathways and the rate-determining oxidative addition of aryl halides. In the final section, we highlight recently developed synthetic methodologies, which provide evidence that limitations can indeed be addressed by working at elevated temperatures, employing alternative electrophiles, harnessing the benefits of additives, or fine-tuning the metal’s reactivity through the ligand field.","lang":"eng"}],"year":"2026","has_accepted_license":"1","scopus_import":"1","date_published":"2026-01-16T00:00:00Z","file_date_updated":"2026-01-21T09:12:10Z","day":"16","PlanS_conform":"1","department":[{"_id":"BaPi"},{"_id":"GradSch"}],"page":"866-881","type":"journal_article","publication_status":"published","file":[{"file_size":3797064,"access_level":"open_access","file_name":"2026_ACSCatalysis_Bena.pdf","content_type":"application/pdf","file_id":"21030","checksum":"05743d6d7b4bae37aad1a91471123032","creator":"dernst","success":1,"date_created":"2026-01-21T09:12:10Z","relation":"main_file","date_updated":"2026-01-21T09:12:10Z"}],"intvolume":"        16","author":[{"full_name":"Bena, Aleksander","first_name":"Aleksander","last_name":"Bena","id":"4197c39e-e8ec-11ed-86cb-afed934cd664"},{"orcid":"0000-0001-8689-388X","last_name":"Pieber","id":"93e5e5b2-0da6-11ed-8a41-af589a024726","first_name":"Bartholomäus","full_name":"Pieber, Bartholomäus"}],"publication_identifier":{"eissn":["2155-5435"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","oa_version":"Published Version","publication":"ACS Catalysis","corr_author":"1","acknowledgement":"We gratefully acknowledge the Institute of Science and Technology Austria for generous financial support. B.P. acknowledges the Austrian Science Fund (PAT 1250924) for funding.","date_updated":"2026-01-21T09:15:16Z"},{"DOAJ_listed":"1","file":[{"date_updated":"2026-01-21T08:39:01Z","relation":"main_file","success":1,"date_created":"2026-01-21T08:39:01Z","content_type":"application/pdf","file_id":"21027","creator":"dernst","checksum":"6ea369e3b46bea58efab4f38b6c671a7","file_name":"2026_JAMES_Goswami.pdf","file_size":19509786,"access_level":"open_access"}],"intvolume":"        18","publication_status":"published","department":[{"_id":"CaMu"},{"_id":"BjHo"},{"_id":"GradSch"}],"type":"journal_article","day":"12","file_date_updated":"2026-01-21T08:39:01Z","PlanS_conform":"1","date_published":"2026-01-12T00:00:00Z","acknowledgement":"The authors gratefully acknowledge funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (Project CLUSTER, Grant Agreement No. 805041). This research was supported by the Scientific Service Units (SSU) of ISTA through resources provided by Scientific Computing (SciComp). We are grateful to three anonymous reviewer(s) for their insightful suggestions that have improved the quality of our manuscript. Open Access funding provided by Institute of Science and Technology Austria/KEMÖ.","date_updated":"2026-01-21T08:41:19Z","corr_author":"1","publication":"Journal of Advances in Modeling Earth Systems","acknowledged_ssus":[{"_id":"ScienComp"}],"oa_version":"Published Version","article_type":"original","article_number":"e2024MS004576","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","author":[{"first_name":"BIDYUT B","full_name":"GOSWAMI, BIDYUT B","id":"3a4ac09c-6d61-11ec-bf66-884cde66b64b","last_name":"GOSWAMI","orcid":"0000-0001-8602-3083"},{"id":"a6e549c6-8972-11ed-ae7b-a336d97ac043","last_name":"Lu","orcid":"0009-0008-5320-7730","full_name":"Lu, Ziyin","first_name":"Ziyin"},{"first_name":"Caroline J","full_name":"Muller, Caroline J","orcid":"0000-0001-5836-5350","last_name":"Muller","id":"f978ccb0-3f7f-11eb-b193-b0e2bd13182b"}],"publication_identifier":{"eissn":["1942-2466"]},"doi":"10.1029/2024ms004576","OA_place":"publisher","volume":18,"language":[{"iso":"eng"}],"month":"01","citation":{"short":"B.B. GOSWAMI, Z. Lu, C.J. Muller, Journal of Advances in Modeling Earth Systems 18 (2026).","ista":"GOSWAMI BB, Lu Z, Muller CJ. 2026. Convective self‐aggregation in diurnally oscillating sea surface temperature and solar forcing experiments. Journal of Advances in Modeling Earth Systems. 18(1), e2024MS004576.","chicago":"GOSWAMI, BIDYUT B, Ziyin Lu, and Caroline J Muller. “Convective Self‐aggregation in Diurnally Oscillating Sea Surface Temperature and Solar Forcing Experiments.” <i>Journal of Advances in Modeling Earth Systems</i>. Wiley, 2026. <a href=\"https://doi.org/10.1029/2024ms004576\">https://doi.org/10.1029/2024ms004576</a>.","ieee":"B. B. GOSWAMI, Z. Lu, and C. J. Muller, “Convective self‐aggregation in diurnally oscillating sea surface temperature and solar forcing experiments,” <i>Journal of Advances in Modeling Earth Systems</i>, vol. 18, no. 1. Wiley, 2026.","mla":"GOSWAMI, BIDYUT B., et al. “Convective Self‐aggregation in Diurnally Oscillating Sea Surface Temperature and Solar Forcing Experiments.” <i>Journal of Advances in Modeling Earth Systems</i>, vol. 18, no. 1, e2024MS004576, Wiley, 2026, doi:<a href=\"https://doi.org/10.1029/2024ms004576\">10.1029/2024ms004576</a>.","ama":"GOSWAMI BB, Lu Z, Muller CJ. Convective self‐aggregation in diurnally oscillating sea surface temperature and solar forcing experiments. <i>Journal of Advances in Modeling Earth Systems</i>. 2026;18(1). doi:<a href=\"https://doi.org/10.1029/2024ms004576\">10.1029/2024ms004576</a>","apa":"GOSWAMI, B. B., Lu, Z., &#38; Muller, C. J. (2026). Convective self‐aggregation in diurnally oscillating sea surface temperature and solar forcing experiments. <i>Journal of Advances in Modeling Earth Systems</i>. Wiley. <a href=\"https://doi.org/10.1029/2024ms004576\">https://doi.org/10.1029/2024ms004576</a>"},"issue":"1","status":"public","project":[{"name":"Organization of CLoUdS, and implications of Tropical  cyclones and for the Energetics of the tropics, in current and waRming climate","_id":"629205d8-2b32-11ec-9570-e1356ff73576","grant_number":"805041","call_identifier":"H2020"}],"date_created":"2026-01-20T10:08:54Z","OA_type":"gold","oa":1,"_id":"21013","quality_controlled":"1","article_processing_charge":"Yes","ddc":["550"],"year":"2026","ec_funded":1,"has_accepted_license":"1","scopus_import":"1","abstract":[{"lang":"eng","text":"We have addressed convective self‐aggregation (CSA) in steady and oscillating sea surface temperature (SST) and solar radiation (SOLIN) cloud‐resolving model simulations in a non‐rotating radiative‐convective equilibrium (RCE) framework. Our experiment designs are motivated by land‐ocean heterogeneity of atmospheric convection. The steady and oscillating forcings are idealizations of ocean and land conditions, respectively, based on their differences in heat capacities. In both kinds of simulations, the diurnal mean SST and SOLIN are the same, and both SST and SOLIN are only varied in time (i.e., they are spatially homogeneous at any given time). We find that diurnally oscillating forcing accelerates CSA. Stronger long‐wave cooling in dry regions at night and during the warm SST phase (late afternoon) both allow the long‐wave feedback, known to favor aggregation, to intensify compared to steady forcing simulations. In addition to the long‐wave, reduced short‐wave warming in dry regions (during the day) further enhances radiative cooling there compared to moist regions. Overall, the radiative cooling is enhanced in dry regions compared to neighboring moist convective regions. A dry subsidence is driven by this net radiative (short‐wave plus long‐wave) cooling, consistent with earlier work on CSA. Stronger radiative cooling allows stronger subsidence which allows low‐level circulation to more efficiently transport moisture and energy up‐gradient, driving convection to aggregate faster. We also note a sensitivity of our experimental setup to initial conditions, more so at warmer SST. This stochastic behavior might be critical in reconciling the differences of opinion regarding the response of convection aggregation to oscillating SST forcing."}],"title":"Convective self‐aggregation in diurnally oscillating sea surface temperature and solar forcing experiments","tmp":{"short":"CC BY-NC-ND (4.0)","image":"/images/cc_by_nc_nd.png","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)"},"publisher":"Wiley"},{"file":[{"date_updated":"2026-03-16T11:51:10Z","relation":"main_file","date_created":"2026-03-16T11:51:10Z","content_type":"application/zip","description":"Python3 library written in C++20 to integrate vertex models. Please read the readme at https://github.com/yketa/cells/blob/main/README.md for detailed instructions for installation and usage of the code in this repository. ","file_id":"21461","checksum":"5d1fda7e410f24c311fcf6bcf725698f","creator":"snaik","file_name":"cells-main.zip","access_level":"open_access","file_size":725916,"title":"Cell git repository"},{"success":1,"date_created":"2026-03-18T14:52:02Z","relation":"main_file","date_updated":"2026-03-18T14:52:02Z","file_size":282168895,"access_level":"open_access","file_name":"DevBranchDataRepo.zip","content_type":"application/x-zip-compressed","file_id":"21464","creator":"snaik","checksum":"ee350c8eaed99f3ca348c47c8b190d3c"},{"file_size":2231,"access_level":"open_access","file_name":"ReadMe.md","file_id":"21466","content_type":"text/markdown","creator":"snaik","checksum":"1ecaf2c1a2ce8ff9c75a128cc02d0b8f","date_created":"2026-03-18T15:01:32Z","success":1,"relation":"main_file","date_updated":"2026-03-18T15:01:32Z"},{"file_name":"PaperSchematics.svg","access_level":"open_access","file_size":1951210,"checksum":"da9a4687e5144b61a64ca341f922046a","creator":"snaik","content_type":"image/svg+xml","file_id":"21467","success":1,"date_created":"2026-03-18T15:12:57Z","date_updated":"2026-03-18T15:12:57Z","relation":"main_file"},{"date_updated":"2026-03-21T03:37:43Z","relation":"main_file","date_created":"2026-03-21T03:37:43Z","success":1,"content_type":"application/octet-stream","file_id":"21468","checksum":"9ac1054b16c212c6f34d402dce2c80e0","creator":"snaik","file_name":"maxwell_sketch.tex","file_size":1897,"access_level":"open_access"},{"date_updated":"2026-03-24T07:21:43Z","relation":"main_file","date_created":"2026-03-24T07:21:43Z","success":1,"content_type":"application/x-zip-compressed","file_id":"21495","creator":"snaik","checksum":"7c9ecf78e2593b3830d96fa94baa08df","file_name":"DataRepo.zip","file_size":749368723,"access_level":"open_access"}],"day":"24","file_date_updated":"2026-03-24T07:21:43Z","contributor":[{"last_name":"Keta","contributor_type":"researcher","first_name":"Yann-Edwin"},{"last_name":"Henkes","first_name":"Silke ","contributor_type":"supervisor"},{"orcid":"0000-0002-0912-4566","last_name":"Heisenberg","id":"39427864-F248-11E8-B48F-1D18A9856A87","first_name":"Carl-Philipp J","contributor_type":"supervisor"},{"contributor_type":"supervisor","first_name":"Edouard B","orcid":"0000-0001-6005-1561","last_name":"Hannezo","id":"3A9DB764-F248-11E8-B48F-1D18A9856A87"}],"department":[{"_id":"GradSch"},{"_id":"CaHe"},{"_id":"EdHa"}],"type":"research_data","date_published":"2026-03-24T00:00:00Z","corr_author":"1","acknowledgement":"We thank all members of the Heisenberg, Henkes, and Hannezo groups for their support. We are also grateful to the Imaging and Optics, Scientific Computing, Life Science Support, and Cryo-Electron Microscopy facilities at ISTA for their technical assistance and support. Numerical simulations were performed using the computational resources from Lorentz Institute and the Academic Leiden Interdisciplinary Cluster Environment (ALICE) provided by Leiden University, and from PMMH provided by Sorbonne Université. S.N has received funding from European Union’s Horizon 2020 research and innovation programme (grant agreement No. 665385). This work was supported by the Austrian Science Fund (FWF) under projects PAT5044023 and W1250 awarded to C.-P.H.","date_updated":"2026-06-10T09:44:10Z","acknowledged_ssus":[{"_id":"Bio"},{"_id":"EM-Fac"},{"_id":"ScienComp"},{"_id":"LifeSc"}],"oa_version":"Published Version","author":[{"full_name":"Naik, Suyash","first_name":"Suyash","last_name":"Naik","orcid":"0000-0001-8421-5508","id":"2C0B105C-F248-11E8-B48F-1D18A9856A87"}],"user_id":"68b8ca59-c5b3-11ee-8790-cd641c68093d","OA_place":"repository","doi":"10.15479/AT-ISTA-21137","status":"public","project":[{"grant_number":"665385","call_identifier":"H2020","_id":"2564DBCA-B435-11E9-9278-68D0E5697425","name":"International IST Doctoral Program"},{"name":"Keratins in epithelial tissue spreading","_id":"8f060199-16d5-11f0-9cad-f3253b266c46","grant_number":"PAT 5044023"},{"grant_number":"W1250-B20","call_identifier":"FWF","_id":"252C3B08-B435-11E9-9278-68D0E5697425","name":"Nano-Analytics of Cellular Systems"}],"date_created":"2026-02-04T16:38:02Z","month":"3","citation":{"chicago":"Naik, Suyash. “Data Associated with Keratins Coordinate Tissue Spreading .” Institute of Science and Technology Austria, 2026. <a href=\"https://doi.org/10.15479/AT-ISTA-21137\">https://doi.org/10.15479/AT-ISTA-21137</a>.","ista":"Naik S. 2026. Data associated with Keratins coordinate tissue spreading , Institute of Science and Technology Austria, <a href=\"https://doi.org/10.15479/AT-ISTA-21137\">10.15479/AT-ISTA-21137</a>.","short":"S. Naik, (2026).","apa":"Naik, S. (2026). Data associated with Keratins coordinate tissue spreading . Institute of Science and Technology Austria. <a href=\"https://doi.org/10.15479/AT-ISTA-21137\">https://doi.org/10.15479/AT-ISTA-21137</a>","ama":"Naik S. Data associated with Keratins coordinate tissue spreading . 2026. doi:<a href=\"https://doi.org/10.15479/AT-ISTA-21137\">10.15479/AT-ISTA-21137</a>","ieee":"S. Naik, “Data associated with Keratins coordinate tissue spreading .” Institute of Science and Technology Austria, 2026.","mla":"Naik, Suyash. <i>Data Associated with Keratins Coordinate Tissue Spreading </i>. Institute of Science and Technology Austria, 2026, doi:<a href=\"https://doi.org/10.15479/AT-ISTA-21137\">10.15479/AT-ISTA-21137</a>."},"oa":1,"article_processing_charge":"No","_id":"21137","ec_funded":1,"year":"2026","has_accepted_license":"1","license":"https://creativecommons.org/licenses/by-sa/4.0/","publisher":"Institute of Science and Technology Austria","title":"Data associated with Keratins coordinate tissue spreading ","tmp":{"short":"CC BY-SA (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-sa/4.0/legalcode","image":"/images/cc_by_sa.png","name":"Creative Commons Attribution-ShareAlike 4.0 International Public License (CC BY-SA 4.0)"}},{"publication_status":"published","intvolume":"        17","file":[{"date_updated":"2026-02-23T10:32:12Z","relation":"main_file","success":1,"date_created":"2026-02-23T10:32:12Z","checksum":"920e8edfd3b8b42f5bb6f86d4c66c54d","creator":"dernst","content_type":"application/pdf","file_id":"21349","file_name":"2026_CellSystems_GomezPascual.pdf","access_level":"open_access","file_size":10606778}],"date_published":"2026-02-18T00:00:00Z","PlanS_conform":"1","file_date_updated":"2026-02-23T10:32:12Z","day":"18","type":"journal_article","department":[{"_id":"GradSch"}],"publication":"Cell Systems","date_updated":"2026-02-23T10:35:01Z","acknowledgement":"We would like to thank the Summer School Systems Genetics of Neural Ageing for bringing us together and spurring our international collaboration. We would also like to acknowledge the funding for the Summer School 2022 from the e:Med Systems Medicine Program of the BMBF (Bundesministerium für Bildung und Forschung; German Ministry of Education and Research) to R.W.O. In addition, we would like to thank the FLI imaging core facility for their assistance. A.G.-P. is supported by Fundación Séneca, Región de Murcia, Spain (21259/FPI/19). D.E.M.d.B. is financed by a Rubicon scholarship (452021116) from the Dutch Research Council (NWO). This work was also supported by NIH NIA R01AG070913-01 (R.W.W.), R01AG075813-01 (D.G.A.), and R01AG075818 (C.K.). We acknowledge the help of Larry Mobraaten (Jackson Laboratory, Bar Harbor, MN) with the BXD strains and U. Obermüller for the help with the histology. For the purpose of open access, the authors have applied a CC BY public copyright license to all author-accepted manuscripts arising from this submission.","publication_identifier":{"issn":["2405-4712"]},"author":[{"full_name":"Gómez-Pascual, Alicia","first_name":"Alicia","last_name":"Gómez-Pascual"},{"last_name":"Glikman","id":"ab8acda1-91c1-11f0-aad8-f75d3d6424d8","full_name":"Glikman, Dow M","first_name":"Dow M"},{"first_name":"Hui Xin","full_name":"Ng, Hui Xin","last_name":"Ng"},{"first_name":"James E.","full_name":"Tomkins, James E.","last_name":"Tomkins"},{"last_name":"Lu","full_name":"Lu, Lu","first_name":"Lu"},{"last_name":"Xu","first_name":"Ying","full_name":"Xu, Ying"},{"full_name":"Ashbrook, David G.","first_name":"David G.","last_name":"Ashbrook"},{"last_name":"Kaczorowski","full_name":"Kaczorowski, Catherine","first_name":"Catherine"},{"last_name":"Kempermann","first_name":"Gerd","full_name":"Kempermann, Gerd"},{"first_name":"John","full_name":"Killmar, John","last_name":"Killmar"},{"last_name":"Mozhui","full_name":"Mozhui, Khyobeni","first_name":"Khyobeni"},{"last_name":"Ohlenschläger","first_name":"Oliver","full_name":"Ohlenschläger, Oliver"},{"full_name":"Aebersold, Rudolf","first_name":"Rudolf","last_name":"Aebersold"},{"full_name":"Ingram, Donald K.","first_name":"Donald K.","last_name":"Ingram"},{"full_name":"Williams, Evan G.","first_name":"Evan G.","last_name":"Williams"},{"last_name":"Jucker","first_name":"Mathias","full_name":"Jucker, Mathias"},{"first_name":"Rupert W.","full_name":"Overall, Rupert W.","last_name":"Overall"},{"last_name":"Williams","first_name":"Robert W.","full_name":"Williams, Robert W."},{"last_name":"de Bakker","full_name":"de Bakker, Dennis E.M.","first_name":"Dennis E.M."}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","article_number":"101488","oa_version":"Published Version","date_created":"2026-02-16T10:45:10Z","status":"public","issue":"2","citation":{"apa":"Gómez-Pascual, A., Glikman, D. M., Ng, H. X., Tomkins, J. E., Lu, L., Xu, Y., … de Bakker, D. E. M. (2026). The Smarcal1-Usp37 locus modulates glycogen aggregation in astrocytes of the aged hippocampus. <i>Cell Systems</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.cels.2025.101488\">https://doi.org/10.1016/j.cels.2025.101488</a>","ama":"Gómez-Pascual A, Glikman DM, Ng HX, et al. The Smarcal1-Usp37 locus modulates glycogen aggregation in astrocytes of the aged hippocampus. <i>Cell Systems</i>. 2026;17(2). doi:<a href=\"https://doi.org/10.1016/j.cels.2025.101488\">10.1016/j.cels.2025.101488</a>","mla":"Gómez-Pascual, Alicia, et al. “The Smarcal1-Usp37 Locus Modulates Glycogen Aggregation in Astrocytes of the Aged Hippocampus.” <i>Cell Systems</i>, vol. 17, no. 2, 101488, Elsevier, 2026, doi:<a href=\"https://doi.org/10.1016/j.cels.2025.101488\">10.1016/j.cels.2025.101488</a>.","ieee":"A. Gómez-Pascual <i>et al.</i>, “The Smarcal1-Usp37 locus modulates glycogen aggregation in astrocytes of the aged hippocampus,” <i>Cell Systems</i>, vol. 17, no. 2. Elsevier, 2026.","ista":"Gómez-Pascual A, Glikman DM, Ng HX, Tomkins JE, Lu L, Xu Y, Ashbrook DG, Kaczorowski C, Kempermann G, Killmar J, Mozhui K, Ohlenschläger O, Aebersold R, Ingram DK, Williams EG, Jucker M, Overall RW, Williams RW, de Bakker DEM. 2026. The Smarcal1-Usp37 locus modulates glycogen aggregation in astrocytes of the aged hippocampus. Cell Systems. 17(2), 101488.","chicago":"Gómez-Pascual, Alicia, Dow M Glikman, Hui Xin Ng, James E. Tomkins, Lu Lu, Ying Xu, David G. Ashbrook, et al. “The Smarcal1-Usp37 Locus Modulates Glycogen Aggregation in Astrocytes of the Aged Hippocampus.” <i>Cell Systems</i>. Elsevier, 2026. <a href=\"https://doi.org/10.1016/j.cels.2025.101488\">https://doi.org/10.1016/j.cels.2025.101488</a>.","short":"A. Gómez-Pascual, D.M. Glikman, H.X. Ng, J.E. Tomkins, L. Lu, Y. Xu, D.G. Ashbrook, C. Kaczorowski, G. Kempermann, J. Killmar, K. Mozhui, O. Ohlenschläger, R. Aebersold, D.K. Ingram, E.G. Williams, M. Jucker, R.W. Overall, R.W. Williams, D.E.M. de Bakker, Cell Systems 17 (2026)."},"month":"02","language":[{"iso":"eng"}],"volume":17,"doi":"10.1016/j.cels.2025.101488","OA_place":"publisher","ddc":["570"],"_id":"21234","article_processing_charge":"No","quality_controlled":"1","oa":1,"external_id":{"pmid":["41633365"]},"OA_type":"hybrid","pmid":1,"scopus_import":"1","has_accepted_license":"1","year":"2026","publisher":"Elsevier","title":"The Smarcal1-Usp37 locus modulates glycogen aggregation in astrocytes of the aged hippocampus","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"abstract":[{"text":"In aged humans and mice, hypobranched glycogen aggregates, known as polyglucosan bodies (PGBs), accumulate in hippocampal astrocytes. While PGBs are linked to cognitive decline in neurological diseases, they remain largely unstudied in the context of typical aging. We show that PGBs arise in autophagy-dysregulated astrocytes in the aged hippocampus, with substantial variation among 32 inbred BXD mouse strains. Genetic mapping through quantitative trait locus analysis identified a major locus (Pgb1) that modulates hippocampal PGB burden. Extensive transcriptomic and proteomic datasets were produced for the aged hippocampus of the BXD family to investigate the mechanism by which the Pgb1 locus modulates PGB burden. We identified that Pgb1 contains allelic Smarcal1 and Usp37 variants and influences PGB burden through trans-regulation of mRNA and protein expression levels, including abundance of glycogen-mobilizing factor PYGB. Furthermore, comprehensive phenome-wide association scans, transcriptomic analyses, and direct behavioral testing demonstrated that cognition remains intact despite age-related PGB burden. A record of this paper’s transparent peer review process is included in the supplemental information.","lang":"eng"}]},{"article_number":"A188","article_type":"original","oa_version":"Published Version","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"author":[{"last_name":"Cristea","id":"4d500bea-31f8-11ee-a48d-d4904fb363c7","first_name":"Andrei-Alexandru","full_name":"Cristea, Andrei-Alexandru"},{"first_name":"Ilaria","full_name":"Caiazzo, Ilaria","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","orcid":"0000-0002-4770-5388","last_name":"Caiazzo"},{"first_name":"Tim","full_name":"Cunningham, Tim","last_name":"Cunningham"},{"last_name":"Raymond","full_name":"Raymond, John C.","first_name":"John C."},{"last_name":"Vennes","full_name":"Vennes, Stephane","first_name":"Stephane"},{"first_name":"Adela","full_name":"Kawka, Adela","last_name":"Kawka"},{"first_name":"Aayush A","full_name":"Desai, Aayush A","last_name":"Desai","id":"502cfd30-32c1-11ee-a9a4-d8dad5c6739e"},{"last_name":"Miller","first_name":"David R.","full_name":"Miller, David R."},{"full_name":"Hermes, J. J.","first_name":"J. J.","last_name":"Hermes"},{"last_name":"Fuller","first_name":"Jim","full_name":"Fuller, Jim"},{"first_name":"Jeremy","full_name":"Heyl, Jeremy","last_name":"Heyl"},{"last_name":"van Roestel","full_name":"van Roestel, Jan","first_name":"Jan"},{"full_name":"Burdge, Kevin B.","first_name":"Kevin B.","last_name":"Burdge"},{"first_name":"Antonio C.","full_name":"Rodriguez, Antonio C.","last_name":"Rodriguez"},{"first_name":"Ingrid","full_name":"Pelisoli, Ingrid","last_name":"Pelisoli"},{"last_name":"Gänsicke","full_name":"Gänsicke, Boris T.","first_name":"Boris T."},{"last_name":"Szkody","first_name":"Paula","full_name":"Szkody, Paula"},{"full_name":"Kenyon, Scott J.","first_name":"Scott J.","last_name":"Kenyon"},{"full_name":"Vanderbosch, Zach","first_name":"Zach","last_name":"Vanderbosch"},{"last_name":"Drake","full_name":"Drake, Andrew","first_name":"Andrew"},{"first_name":"Lilia","full_name":"Ferrario, Lilia","last_name":"Ferrario"},{"first_name":"Dayal","full_name":"Wickramasinghe, Dayal","last_name":"Wickramasinghe"},{"last_name":"Karambelkar","full_name":"Karambelkar, Viraj R.","first_name":"Viraj R."},{"full_name":"Justham, Stephen","first_name":"Stephen","last_name":"Justham"},{"last_name":"Pakmor","full_name":"Pakmor, Ruediger","first_name":"Ruediger"},{"full_name":"El-Badry, Kareem","first_name":"Kareem","last_name":"El-Badry"},{"last_name":"Prince","first_name":"Thomas","full_name":"Prince, Thomas"},{"full_name":"Kulkarni, S. R.","first_name":"S. R.","last_name":"Kulkarni"},{"last_name":"Graham","first_name":"Matthew J.","full_name":"Graham, Matthew J."},{"last_name":"Masci","full_name":"Masci, Frank J.","first_name":"Frank J."},{"first_name":"Steven L.","full_name":"Groom, Steven L.","last_name":"Groom"},{"last_name":"Purdum","first_name":"Josiah","full_name":"Purdum, Josiah"},{"last_name":"Dekany","full_name":"Dekany, Richard","first_name":"Richard"},{"first_name":"Eric C.","full_name":"Bellm, Eric C.","last_name":"Bellm"}],"user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","corr_author":"1","date_updated":"2026-04-28T12:01:21Z","acknowledgement":"We thank Lynne Hillenbrand and Soumyadeep Bhattacharjee for helpful discussions, and Kishalay De for his help with the WIRC\r\nreduction pipeline. IC was supported by NASA through grants from the Space\r\nTelescope Science Institute, under NASA contracts NASA.22K1813, NAS5-\r\n26555 and NAS5-03127. TC was supported by NASA through the NASA Hubble\r\nFellowship grant HST-HF2-51527.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research\r\nin Astronomy, Inc., for NASA, under contract NAS5-26555. This project has\r\nreceived funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (Grant agreement No. 101020057). This work was based on observations obtained with the\r\nSamuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar\r\nObservatory as part of the Zwicky Transient Facility project. ZTF is supported\r\nby the National Science Foundation under Grants No. AST-1440341, AST2034437, and currently Award #2407588. ZTF receives additional funding from\r\nthe ZTF partnership. Current members include Caltech, USA; Caltech/IPAC,\r\nUSA; University of Maryland, USA; University of California, Berkeley, USA;\r\nUniversity of Wisconsin at Milwaukee, USA; Cornell University, USA; Drexel\r\nUniversity, USA; University of North Carolina at Chapel Hill, USA; Institute\r\nof Science and Technology, Austria; National Central University, Taiwan, and\r\nOKC, University of Stockholm, Sweden. Operations are conducted by Caltech’s\r\nOptical Observatory (COO), Caltech/IPAC, and the University of Washington at\r\nSeattle, USA. This work has made use of data from the European Space Agency\r\n(ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by\r\nthe Gaia Data Processing and Analysis Consortium (DPAC, https://www.\r\ncosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. The Pan-STARRS1 Surveys (PS1)\r\nand the PS1 public science archive have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, the PanSTARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck\r\nInstitute for Extraterrestrial Physics, Garching, The Johns Hopkins University,\r\nDurham University, the University of Edinburgh, the Queen’s University Belfast,\r\nthe Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through\r\nthe Planetary Science Division of the NASA Science Mission Directorate, the\r\nNational Science Foundation Grant No. AST–1238877, the University of Maryland, Eotvos Lorand University (ELTE), the Los Alamos National Laboratory,\r\nand the Gordon and Betty Moore Foundation. This work made use of Astropy\r\n(http://www.astropy.org): a community-developed core Python package\r\nand an ecosystem of tools and resources for astronomy (Astropy Collaboration\r\n2013, 2018, 2022).","related_material":{"link":[{"description":"News on ISTA website","url":"https://ista.ac.at/en/news/twos-company-new-class-of-star-remnants/","relation":"press_release"}]},"publication":"Astronomy & Astrophysics","PlanS_conform":"1","day":"10","file_date_updated":"2026-02-23T12:04:37Z","type":"journal_article","department":[{"_id":"IlCa"},{"_id":"GradSch"}],"date_published":"2026-02-10T00:00:00Z","DOAJ_listed":"1","publication_status":"published","intvolume":"       706","file":[{"file_id":"21350","content_type":"application/pdf","creator":"dernst","checksum":"229b688e6e78cab5bb8e2bac366d1575","file_name":"2026_AstronomyAstrophysics_Cristea.pdf","access_level":"open_access","file_size":5352853,"date_updated":"2026-02-23T12:04:37Z","relation":"main_file","success":1,"date_created":"2026-02-23T12:04:37Z"}],"abstract":[{"lang":"eng","text":"Many white dwarfs are observed in compact double white dwarf binaries, and through the emission of gravitational waves, a large fraction are destined to merge. The merger remnants that do not explode in a Type Ia supernova are expected to initially be rapidly rotating and highly magnetized. In this work, we present our discovery of the variable white dwarf ZTF J200832.79+444939.67, hereafter ZTF J2008+4449, as a likely merger remnant showing signs of circumstellar material without a stellar or substellar companion. The nature of ZTF J2008+4449 as a merger remnant is supported by its physical properties: it is hot (35 500 ± 300 K) and massive (1.12 ± 0.03 M\r\n                    <jats:sub>⊙</jats:sub>\r\n                    ), rapidly rotating with a period of ≈6.6 minutes, and likely possesses exceptionally strong magnetic fields (∼400−600 MG) at its surface. Remarkably, we detect a significant period derivative of (1.80 ± 0.09)×10\r\n                    <jats:sup>−12</jats:sup>\r\n                    s/s, indicating that the white dwarf is spinning down, and a soft X-ray emission that is inconsistent with photospheric emission. As the presence of a mass-transferring stellar or brown dwarf companion is excluded by infrared photometry, the detected spin-down and X-ray emission could be tell-tale signs of a magnetically driven wind or of interaction with circumstellar material, possibly originating from the fallback of gravitationally bound merger ejecta or from the tidal disruption of a planetary object. We also detect Balmer emission, which requires the presence of ionized hydrogen in the vicinity of the white dwarf, showing Doppler shifts as high as ≈2000 km s\r\n                    <jats:sup>−1</jats:sup>\r\n                    . The unusual variability of the Balmer emission on the spin period of the white dwarf is consistent with the trapping of a half ring of ionized gas in the magnetosphere of the white dwarf.\r\n                  </jats:p>"}],"publisher":"EDP Sciences","title":"A half ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"has_accepted_license":"1","year":"2026","oa":1,"OA_type":"gold","ddc":["520"],"quality_controlled":"1","_id":"21274","article_processing_charge":"Yes","language":[{"iso":"eng"}],"volume":706,"OA_place":"publisher","doi":"10.1051/0004-6361/202556432","date_created":"2026-02-17T08:12:05Z","status":"public","citation":{"apa":"Cristea, A.-A., Caiazzo, I., Cunningham, T., Raymond, J. C., Vennes, S., Kawka, A., … Bellm, E. C. (2026). A half ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202556432\">https://doi.org/10.1051/0004-6361/202556432</a>","mla":"Cristea, Andrei-Alexandru, et al. “A Half Ring of Ionized Circumstellar Material Trapped in the Magnetosphere of a White Dwarf Merger Remnant.” <i>Astronomy &#38; Astrophysics</i>, vol. 706, A188, EDP Sciences, 2026, doi:<a href=\"https://doi.org/10.1051/0004-6361/202556432\">10.1051/0004-6361/202556432</a>.","ieee":"A.-A. Cristea <i>et al.</i>, “A half ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant,” <i>Astronomy &#38; Astrophysics</i>, vol. 706. EDP Sciences, 2026.","ama":"Cristea A-A, Caiazzo I, Cunningham T, et al. A half ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant. <i>Astronomy &#38; Astrophysics</i>. 2026;706. doi:<a href=\"https://doi.org/10.1051/0004-6361/202556432\">10.1051/0004-6361/202556432</a>","ista":"Cristea A-A, Caiazzo I, Cunningham T, Raymond JC, Vennes S, Kawka A, Desai AA, Miller DR, Hermes JJ, Fuller J, Heyl J, van Roestel J, Burdge KB, Rodriguez AC, Pelisoli I, Gänsicke BT, Szkody P, Kenyon SJ, Vanderbosch Z, Drake A, Ferrario L, Wickramasinghe D, Karambelkar VR, Justham S, Pakmor R, El-Badry K, Prince T, Kulkarni SR, Graham MJ, Masci FJ, Groom SL, Purdum J, Dekany R, Bellm EC. 2026. A half ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant. Astronomy &#38; Astrophysics. 706, A188.","chicago":"Cristea, Andrei-Alexandru, Ilaria Caiazzo, Tim Cunningham, John C. Raymond, Stephane Vennes, Adela Kawka, Aayush A Desai, et al. “A Half Ring of Ionized Circumstellar Material Trapped in the Magnetosphere of a White Dwarf Merger Remnant.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2026. <a href=\"https://doi.org/10.1051/0004-6361/202556432\">https://doi.org/10.1051/0004-6361/202556432</a>.","short":"A.-A. Cristea, I. Caiazzo, T. Cunningham, J.C. Raymond, S. Vennes, A. Kawka, A.A. Desai, D.R. Miller, J.J. Hermes, J. Fuller, J. Heyl, J. van Roestel, K.B. Burdge, A.C. Rodriguez, I. Pelisoli, B.T. Gänsicke, P. Szkody, S.J. Kenyon, Z. Vanderbosch, A. Drake, L. Ferrario, D. Wickramasinghe, V.R. Karambelkar, S. Justham, R. Pakmor, K. El-Badry, T. Prince, S.R. Kulkarni, M.J. Graham, F.J. Masci, S.L. Groom, J. Purdum, R. Dekany, E.C. Bellm, Astronomy &#38; Astrophysics 706 (2026)."},"month":"02"},{"user_id":"68b8ca59-c5b3-11ee-8790-cd641c68093d","author":[{"full_name":"Becker, Lea Marie","first_name":"Lea Marie","last_name":"Becker","orcid":"0000-0002-6401-5151","id":"36336939-eb97-11eb-a6c2-c83f1214ca79"},{"id":"7B541462-FAF6-11E9-A490-E8DFE5697425","last_name":"Schanda","orcid":"0000-0002-9350-7606","full_name":"Schanda, Paul","first_name":"Paul"}],"oa_version":"Published Version","acknowledged_ssus":[{"_id":"NMR"},{"_id":"LifeSc"}],"date_updated":"2026-06-10T09:28:41Z","acknowledgement":"We thank Ben P. Tatman for insightful discussions. This research was supported by the Scientific Service Units (SSU) of Institute of Science and Technology Austria (ISTA) through resources provided by the Nuclear Magnetic Resonance Facility and the Lab Support Facility.","corr_author":"1","date_published":"2026-02-18T00:00:00Z","type":"research_data","department":[{"_id":"GradSch"},{"_id":"PaSc"}],"contributor":[{"first_name":"Giorgia","contributor_type":"researcher","id":"334a5e40-8747-11f0-b671-ba1f5154b4b4","last_name":"Toscano"},{"last_name":"Kapitonova","id":"9fb2a840-89e1-11ee-a8b7-cc5c7ba62471","contributor_type":"researcher","first_name":"Anna"},{"contributor_type":"researcher","first_name":"Rajkumar","last_name":"Singh","id":"a3089acd-6806-11ee-bacc-f0c7d500ad20"},{"last_name":"Guillerm","id":"bb74f472-ae54-11eb-9835-bc9c22fb1183","first_name":"Undina","contributor_type":"researcher"},{"last_name":"Lichtenecker","first_name":"Roman","contributor_type":"researcher"}],"file_date_updated":"2026-02-17T10:11:14Z","day":"18","file":[{"date_updated":"2026-02-17T10:11:14Z","relation":"main_file","date_created":"2026-02-17T10:11:14Z","success":1,"checksum":"2d3105f26be578073b88ee1f2ea0bdb1","creator":"lbecker","file_id":"21285","content_type":"application/zip","file_name":"Research_data.zip","file_size":36996027,"access_level":"open_access"},{"file_name":"README.txt","access_level":"open_access","file_size":1993,"content_type":"text/plain","file_id":"21286","checksum":"e24aebcdb8856cb181cbaa02de020ddb","creator":"lbecker","date_created":"2026-02-17T10:11:14Z","date_updated":"2026-02-17T10:11:14Z","relation":"table_of_contents"}],"title":"Research data for \"Accelerated 19F biomolecular magic-angle spinning NMR with paramagnetic dopants\"","tmp":{"short":"CC BY-NC (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc/4.0/legalcode","image":"/images/cc_by_nc.png","name":"Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)"},"publisher":"Institute of Science and Technology Austria","abstract":[{"text":"The advantageous characteristics attributed to the 19F nucleus have made it a popular target for NMR once again in recent years. Aside from solution NMR, an increasing number of studies have been conducted applying solid-state magic-angle-spinning NMR to fluorine-labeled samples. Here, the high chemical shift anisotropy and strong dipolar couplings can be utilized to get structural insights into proteins and measure long distances. Despite increasing popularity and promising benefits, the sensitivity of biomolecular 19F MAS NMR often suffers from slow longitudinal T1 relaxation and therefore long recycle delays. In this work, we expand paramagnetic doping, an approach commonly used to reduce proton T1 relaxation times, to 19F-labeled biological samples. We study the effect of Gd(DTPA) and Gd(DTPA-BMA) on 19F and 13C T1 and T2 relaxation in a [5-19F13C]-tryptophan-labeled protein via 19F-detected MAS NMR experiments. The observed paramagnetic relaxation enhancement substantially reduces measurement times of 19F MAS NMR experiments without compromising resolution. Additionally, we report the chemical-shift assignments of all four fluorotryptophan signals in the 12 × 39 kDa large protein using a mutagenesis approach.","lang":"eng"}],"license":"https://creativecommons.org/licenses/by-nc/4.0/","year":"2026","has_accepted_license":"1","article_processing_charge":"No","_id":"21284","ddc":["541"],"OA_type":"free access","oa":1,"citation":{"ama":"Becker LM, Schanda P. Research data for “Accelerated 19F biomolecular magic-angle spinning NMR with paramagnetic dopants.” 2026. doi:<a href=\"https://doi.org/10.15479/AT-ISTA-21284\">10.15479/AT-ISTA-21284</a>","mla":"Becker, Lea Marie, and Paul Schanda. <i>Research Data for “Accelerated 19F Biomolecular Magic-Angle Spinning NMR with Paramagnetic Dopants.”</i> Institute of Science and Technology Austria, 2026, doi:<a href=\"https://doi.org/10.15479/AT-ISTA-21284\">10.15479/AT-ISTA-21284</a>.","ieee":"L. M. Becker and P. Schanda, “Research data for ‘Accelerated 19F biomolecular magic-angle spinning NMR with paramagnetic dopants.’” Institute of Science and Technology Austria, 2026.","apa":"Becker, L. M., &#38; Schanda, P. (2026). Research data for “Accelerated 19F biomolecular magic-angle spinning NMR with paramagnetic dopants.” Institute of Science and Technology Austria. <a href=\"https://doi.org/10.15479/AT-ISTA-21284\">https://doi.org/10.15479/AT-ISTA-21284</a>","short":"L.M. Becker, P. Schanda, (2026).","chicago":"Becker, Lea Marie, and Paul Schanda. “Research Data for ‘Accelerated 19F Biomolecular Magic-Angle Spinning NMR with Paramagnetic Dopants.’” Institute of Science and Technology Austria, 2026. <a href=\"https://doi.org/10.15479/AT-ISTA-21284\">https://doi.org/10.15479/AT-ISTA-21284</a>.","ista":"Becker LM, Schanda P. 2026. Research data for ‘Accelerated 19F biomolecular magic-angle spinning NMR with paramagnetic dopants’, Institute of Science and Technology Austria, <a href=\"https://doi.org/10.15479/AT-ISTA-21284\">10.15479/AT-ISTA-21284</a>."},"month":"2","date_created":"2026-02-17T10:17:14Z","status":"public","doi":"10.15479/AT-ISTA-21284","OA_place":"repository"},{"DOAJ_listed":"1","publication_status":"published","file":[{"relation":"main_file","date_updated":"2026-02-24T07:46:47Z","success":1,"date_created":"2026-02-24T07:46:47Z","creator":"dernst","checksum":"6f5849d29ad43bee32f90152f6fc0294","file_id":"21355","content_type":"application/pdf","access_level":"open_access","file_size":6531719,"file_name":"2026_AstronomyAstrophysics_Kotiwale.pdf"}],"intvolume":"       706","file_date_updated":"2026-02-24T07:46:47Z","day":"01","PlanS_conform":"1","department":[{"_id":"JoMa"},{"_id":"GradSch"}],"type":"journal_article","date_published":"2026-02-01T00:00:00Z","corr_author":"1","acknowledgement":"We thank the anonymous referee for the insightful comments that helped improving this paper. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Associations of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations were taken under programmes # 1243, # 1933 and # 3516. Funded by the European Union (ERC, AGENTS, 101076224). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. GK acknowledges support from the Foundation MERAC. APV acknowledge support from the Sussex Astronomy Centre STFC Consolidated Grant (ST/X001040/1).","date_updated":"2026-02-24T07:49:42Z","publication":"Astronomy & Astrophysics","article_number":"A165","article_type":"original","arxiv":1,"oa_version":"Published Version","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"author":[{"id":"1438afc8-1ff6-11ee-9fa6-cd4a75d66875","last_name":"Kotiwale","full_name":"Kotiwale, Gauri","first_name":"Gauri"},{"first_name":"Jorryt J","full_name":"Matthee, Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","last_name":"Matthee","orcid":"0000-0003-2871-127X"},{"first_name":"Daichi","full_name":"Kashino, Daichi","last_name":"Kashino"},{"first_name":"Aswin P.","full_name":"Vijayan, Aswin P.","last_name":"Vijayan"},{"id":"018f0249-0e87-11f0-b167-cbce08fbd541","last_name":"Torralba Torregrosa","orcid":"0000-0001-5586-6950","first_name":"Alberto","full_name":"Torralba Torregrosa, Alberto"},{"last_name":"Di Cesare","id":"2d002343-372f-11ef-98ec-a164d20427cb","full_name":"Di Cesare, Claudia","first_name":"Claudia"},{"full_name":"Iani, Edoardo","first_name":"Edoardo","id":"4053390a-6b68-11ef-9828-a3b8adef8d0a","orcid":"0000-0001-8386-3546","last_name":"Iani"},{"last_name":"Bordoloi","first_name":"Rongmon","full_name":"Bordoloi, Rongmon"},{"first_name":"Joel","full_name":"Leja, Joel","last_name":"Leja"},{"last_name":"Maseda","full_name":"Maseda, Michael V.","first_name":"Michael V."},{"first_name":"Sandro","full_name":"Tacchella, Sandro","last_name":"Tacchella"},{"last_name":"Shivaei","first_name":"Irene","full_name":"Shivaei, Irene"},{"last_name":"Heintz","first_name":"Kasper E.","full_name":"Heintz, Kasper E."},{"first_name":"A. Lola","full_name":"Danhaive, A. Lola","last_name":"Danhaive"},{"first_name":"Sara","full_name":"Mascia, Sara","last_name":"Mascia","id":"edaf889c-c7cd-11ef-ab1b-bb28c431bd29"},{"id":"9a9394cb-3200-11ee-973b-f5ba2a8b16e4","orcid":"0000-0001-5346-6048","last_name":"Kramarenko","full_name":"Kramarenko, Ivan","first_name":"Ivan"},{"last_name":"Navarrete","id":"aa14a535-50c9-11ef-b52e-e0c373d10148","first_name":"Benjamín","full_name":"Navarrete, Benjamín"},{"last_name":"Mackenzie","first_name":"Ruari","full_name":"Mackenzie, Ruari"},{"last_name":"Naidu","full_name":"Naidu, Rohan P.","first_name":"Rohan P."},{"last_name":"Sobral","first_name":"David","full_name":"Sobral, David"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","volume":706,"language":[{"iso":"eng"}],"OA_place":"publisher","doi":"10.1051/0004-6361/202556597","status":"public","project":[{"_id":"bd9b2118-d553-11ed-ba76-db24564edfea","grant_number":"101076224","name":"Young galaxies as tracers and agents of cosmic reionization"}],"date_created":"2026-02-22T23:01:35Z","month":"02","citation":{"apa":"Kotiwale, G., Matthee, J. J., Kashino, D., Vijayan, A. P., Torralba Torregrosa, A., Di Cesare, C., … Sobral, D. (2026). Rapid, out-of-equilibrium metal enrichment indicated by a flat mass-metallicity relation at z ∼ 6 from NIRCam grism spectroscopy. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202556597\">https://doi.org/10.1051/0004-6361/202556597</a>","ama":"Kotiwale G, Matthee JJ, Kashino D, et al. Rapid, out-of-equilibrium metal enrichment indicated by a flat mass-metallicity relation at z ∼ 6 from NIRCam grism spectroscopy. <i>Astronomy &#38; Astrophysics</i>. 2026;706. doi:<a href=\"https://doi.org/10.1051/0004-6361/202556597\">10.1051/0004-6361/202556597</a>","ieee":"G. Kotiwale <i>et al.</i>, “Rapid, out-of-equilibrium metal enrichment indicated by a flat mass-metallicity relation at z ∼ 6 from NIRCam grism spectroscopy,” <i>Astronomy &#38; Astrophysics</i>, vol. 706. EDP Sciences, 2026.","mla":"Kotiwale, Gauri, et al. “Rapid, out-of-Equilibrium Metal Enrichment Indicated by a Flat Mass-Metallicity Relation at z ∼ 6 from NIRCam Grism Spectroscopy.” <i>Astronomy &#38; Astrophysics</i>, vol. 706, A165, EDP Sciences, 2026, doi:<a href=\"https://doi.org/10.1051/0004-6361/202556597\">10.1051/0004-6361/202556597</a>.","chicago":"Kotiwale, Gauri, Jorryt J Matthee, Daichi Kashino, Aswin P. Vijayan, Alberto Torralba Torregrosa, Claudia Di Cesare, Edoardo Iani, et al. “Rapid, out-of-Equilibrium Metal Enrichment Indicated by a Flat Mass-Metallicity Relation at z ∼ 6 from NIRCam Grism Spectroscopy.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2026. <a href=\"https://doi.org/10.1051/0004-6361/202556597\">https://doi.org/10.1051/0004-6361/202556597</a>.","ista":"Kotiwale G, Matthee JJ, Kashino D, Vijayan AP, Torralba Torregrosa A, Di Cesare C, Iani E, Bordoloi R, Leja J, Maseda MV, Tacchella S, Shivaei I, Heintz KE, Danhaive AL, Mascia S, Kramarenko I, Navarrete B, Mackenzie R, Naidu RP, Sobral D. 2026. Rapid, out-of-equilibrium metal enrichment indicated by a flat mass-metallicity relation at z ∼ 6 from NIRCam grism spectroscopy. Astronomy &#38; Astrophysics. 706, A165.","short":"G. Kotiwale, J.J. Matthee, D. Kashino, A.P. Vijayan, A. Torralba Torregrosa, C. Di Cesare, E. Iani, R. Bordoloi, J. Leja, M.V. Maseda, S. Tacchella, I. Shivaei, K.E. Heintz, A.L. Danhaive, S. Mascia, I. Kramarenko, B. Navarrete, R. Mackenzie, R.P. Naidu, D. Sobral, Astronomy &#38; Astrophysics 706 (2026)."},"oa":1,"OA_type":"diamond","external_id":{"arxiv":["2510.19959"]},"ddc":["520"],"_id":"21341","quality_controlled":"1","article_processing_charge":"No","has_accepted_license":"1","year":"2026","scopus_import":"1","abstract":[{"text":"We aim to characterise the mass-metallicity relation (MZR) and the 3D correlation between the stellar mass, metallicity, and star formation rate (SFR) known as the fundamental metallicity relation (FMR) for galaxies at 5 < z < 7. Using ∼800 [O III] selected galaxies from deep NIRCam grism surveys, we present our stacked measurements of direct-Te metallicities, which we used to test recent strong-line metallicity calibrations. Our measured direct-Te metallicities (0.1–0.2 Z⊙ for M★ ≈ 5 × 107 − 9 M⊙, respectively) match recent JWST/NIRSpec-based results. However, there are significant inconsistencies between observations and hydrodynamical simulations. We observe a flatter MZR slope than the SPHINX20 and FLARES simulations, which cannot be attributed to selection effects. With simple models, we show that the effect of an [O III] flux-limited sample on the observed shape of the MZR is strongly dependent on the FMR. If the FMR is similar to the one in the local Universe, the intrinsic high-redshift MZR should be even flatter than is observed. In turn, a 3D relation where SFR correlates positively with metallicity at fixed mass would imply an intrinsically steeper MZR. Our measurements indicate that metallicity variations at fixed mass show little dependence on the SFR, suggesting a flat intrinsic MZR. This could indicate that the low-mass galaxies at these redshifts are out of equilibrium and that metal enrichment occurs rapidly in low-mass galaxies. However, being limited by our stacking analysis, we are yet to probe the scatter in the MZR and its dependence on SFR. Large carefully selected samples of galaxies with robust metallicity measurements can put tight constraints on the high-redshift FMR and help us to understand the interplay between gas flows, star formation, and feedback in early galaxies.","lang":"eng"}],"publisher":"EDP Sciences","title":"Rapid, out-of-equilibrium metal enrichment indicated by a flat mass-metallicity relation at z ∼ 6 from NIRCam grism spectroscopy","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"}},{"publication":"arXiv","related_material":{"link":[{"relation":"supplementary_material","url":"https://ivan-sergeyev.github.io/seymour/blueprint.pdf"}]},"date_updated":"2026-03-09T15:14:18Z","year":"2026","corr_author":"1","title":"A blueprint for the formalization of Seymour's matroid decomposition theorem","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"user_id":"8b945eb4-e2f2-11eb-945a-df72226e66a9","author":[{"first_name":"Ivan","full_name":"Sergeev, Ivan","orcid":"0009-0004-9145-8785","last_name":"Sergeev","id":"ca3c9187-9a72-11ee-a009-8af825d896b0"},{"id":"40ED02A8-C8B4-11E9-A9C0-453BE6697425","last_name":"Dvorak","orcid":"0000-0001-5293-214X","first_name":"Martin","full_name":"Dvorak, Martin"},{"last_name":"Rampell","full_name":"Rampell, Cameron","first_name":"Cameron"},{"last_name":"Sandey","full_name":"Sandey, Mark","first_name":"Mark"},{"last_name":"Monticone","first_name":"Pietro","full_name":"Monticone, Pietro"}],"oa_version":"Preprint","arxiv":1,"main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2601.01255"}],"abstract":[{"lang":"eng","text":"This document is a blueprint for the formalization in Lean of the structural theory of regular matroids underlying Seymour's decomposition theorem. We present a modular account of regularity via totally unimodular representations, show that regularity is preserved under 1-, 2-, and 3-sums, and establish regularity for several special classes of matroids, including graphic, cographic, and the matroid R10. The blueprint records the logical structure of the proof, the precise dependencies between results, and their correspondence with Lean declarations. It is intended both as a guide for the ongoing formalization effort and as a human-readable reference for the organization of the proof."}],"citation":{"chicago":"Sergeev, Ivan, Martin Dvorak, Cameron Rampell, Mark Sandey, and Pietro Monticone. “A Blueprint for the Formalization of Seymour’s Matroid Decomposition Theorem.” <i>ArXiv</i>, n.d. <a href=\"https://doi.org/10.48550/arXiv.2601.01255\">https://doi.org/10.48550/arXiv.2601.01255</a>.","ista":"Sergeev I, Dvorak M, Rampell C, Sandey M, Monticone P. A blueprint for the formalization of Seymour’s matroid decomposition theorem. arXiv, <a href=\"https://doi.org/10.48550/arXiv.2601.01255\">10.48550/arXiv.2601.01255</a>.","short":"I. Sergeev, M. Dvorak, C. Rampell, M. Sandey, P. Monticone, ArXiv (n.d.).","apa":"Sergeev, I., Dvorak, M., Rampell, C., Sandey, M., &#38; Monticone, P. (n.d.). A blueprint for the formalization of Seymour’s matroid decomposition theorem. <i>arXiv</i>. <a href=\"https://doi.org/10.48550/arXiv.2601.01255\">https://doi.org/10.48550/arXiv.2601.01255</a>","ama":"Sergeev I, Dvorak M, Rampell C, Sandey M, Monticone P. A blueprint for the formalization of Seymour’s matroid decomposition theorem. <i>arXiv</i>. doi:<a href=\"https://doi.org/10.48550/arXiv.2601.01255\">10.48550/arXiv.2601.01255</a>","mla":"Sergeev, Ivan, et al. “A Blueprint for the Formalization of Seymour’s Matroid Decomposition Theorem.” <i>ArXiv</i>, doi:<a href=\"https://doi.org/10.48550/arXiv.2601.01255\">10.48550/arXiv.2601.01255</a>.","ieee":"I. Sergeev, M. Dvorak, C. Rampell, M. Sandey, and P. Monticone, “A blueprint for the formalization of Seymour’s matroid decomposition theorem,” <i>arXiv</i>. ."},"month":"01","publication_status":"submitted","date_created":"2026-03-04T12:09:26Z","status":"public","doi":"10.48550/arXiv.2601.01255","OA_place":"repository","language":[{"iso":"eng"}],"_id":"21400","article_processing_charge":"No","date_published":"2026-01-03T00:00:00Z","page":"18","external_id":{"arxiv":["2601.01255"]},"type":"preprint","department":[{"_id":"GradSch"},{"_id":"VlKo"}],"oa":1,"day":"03"},{"ec_funded":1,"has_accepted_license":"1","year":"2026","title":"Privacy-preserving runtime verification","publisher":"Institute of Science and Technology Austria","abstract":[{"text":"Runtime verification offers scalable solutions to improve the safety and reliability of systems. However, systems that require verification or monitoring by a third party to ensure compliance with a specification might contain sensitive information, causing privacy concerns when usual runtime verification approaches are used. Privacy is compromised if protected information about the system, or sensitive data that is processed by the system, is revealed. In addition, revealing the specification being monitored may undermine the essence of third-party verification.\r\n\r\nIn this thesis, we propose a protocol for privacy-preserving runtime verification of systems against formal sequential specifications. We develop the protocol in two steps. In the first step, the monitor verifies whether the system satisfies the specification without learning anything else, though both parties are aware of the specification. In the second step, we extend the protocol to ensure that the system remains oblivious to the monitored specification, while the monitor learns only whether the system satisfies the specification and nothing more. Our protocol adapts and improves existing techniques used in cryptography, and more specifically, multi-party computation.\r\n\r\nThe sequential specification defines the observation step of the monitor, whose granularity depends on the situation (e.g., banks may be monitored on a daily basis). Our protocol exchanges a single message per observation step, after an initialization phase. This design minimizes communication overhead, enabling relatively lightweight privacy-preserving monitoring. We implement our approach for monitoring specifications described by register automata and evaluate it experimentally.\r\n","lang":"eng"}],"keyword":["Privacy-preserving verification","Runtime verification","Monitoring","Reactive functionalities","Cryptographic protocols"],"month":"03","citation":{"apa":"Karimi, M. (2026). <i>Privacy-preserving runtime verification</i>. Institute of Science and Technology Austria. <a href=\"https://doi.org/10.15479/AT-ISTA-21401\">https://doi.org/10.15479/AT-ISTA-21401</a>","ieee":"M. Karimi, “Privacy-preserving runtime verification,” Institute of Science and Technology Austria, 2026.","mla":"Karimi, Mahyar. <i>Privacy-Preserving Runtime Verification</i>. Institute of Science and Technology Austria, 2026, doi:<a href=\"https://doi.org/10.15479/AT-ISTA-21401\">10.15479/AT-ISTA-21401</a>.","ama":"Karimi M. Privacy-preserving runtime verification. 2026. doi:<a href=\"https://doi.org/10.15479/AT-ISTA-21401\">10.15479/AT-ISTA-21401</a>","ista":"Karimi M. 2026. Privacy-preserving runtime verification. Institute of Science and Technology Austria.","chicago":"Karimi, Mahyar. “Privacy-Preserving Runtime Verification.” Institute of Science and Technology Austria, 2026. <a href=\"https://doi.org/10.15479/AT-ISTA-21401\">https://doi.org/10.15479/AT-ISTA-21401</a>.","short":"M. Karimi, Privacy-Preserving Runtime Verification, Institute of Science and Technology Austria, 2026."},"status":"public","project":[{"name":"Vigilant Algorithmic Monitoring of Software","grant_number":"101020093","call_identifier":"H2020","_id":"62781420-2b32-11ec-9570-8d9b63373d4d"},{"grant_number":"F8512","_id":"34a4ce89-11ca-11ed-8bc3-8cc37fb6e11f","name":"Security and Privacy by Design for Complex Systems"}],"date_created":"2026-03-05T15:20:47Z","doi":"10.15479/AT-ISTA-21401","OA_place":"repository","degree_awarded":"MS","language":[{"iso":"eng"}],"_id":"21401","article_processing_charge":"No","supervisor":[{"first_name":"Thomas A","full_name":"Henzinger, Thomas A","id":"40876CD8-F248-11E8-B48F-1D18A9856A87","last_name":"Henzinger","orcid":"0000-0002-2985-7724"}],"ddc":["000"],"oa":1,"related_material":{"record":[{"relation":"part_of_dissertation","status":"public","id":"21020"}]},"acknowledgement":"This work is part of the project VAMOS, which has received funding from the European\r\nResearch Council (ERC) under grant agreement No. 101020093, and the Austrian Science\r\nFund (FWF) SFB project SpyCoDe F8502.\r\n","date_updated":"2026-03-13T13:37:20Z","corr_author":"1","user_id":"8b945eb4-e2f2-11eb-945a-df72226e66a9","publication_identifier":{"issn":["2791-4585"]},"author":[{"id":"6e5417ba-5355-11ee-ae5a-94c2e510b26b","last_name":"Karimi","orcid":"0009-0005-0820-1696","first_name":"Mahyar","full_name":"Karimi, Mahyar"}],"oa_version":"Published Version","file":[{"file_name":"2026_Karimi_Mahyar_Thesis.pdf","file_size":766048,"access_level":"open_access","creator":"mkarimi","checksum":"3f49f05c9d123e14d7adb73d3bc50fe2","content_type":"application/pdf","file_id":"21404","date_created":"2026-03-06T14:06:25Z","date_updated":"2026-03-10T15:20:09Z","relation":"main_file"},{"relation":"source_file","date_updated":"2026-03-06T14:06:25Z","date_created":"2026-03-06T14:06:25Z","checksum":"8fb9db4b4187e26443369a993427a5ff","creator":"mkarimi","file_id":"21405","content_type":"application/zip","file_size":1243394,"access_level":"closed","file_name":"2026_Karimi_Mahyar_Thesis_src.zip"}],"alternative_title":["ISTA Master’s Thesis"],"publication_status":"published","date_published":"2026-03-05T00:00:00Z","department":[{"_id":"GradSch"},{"_id":"ToHe"}],"page":"60","type":"dissertation","day":"05","file_date_updated":"2026-03-10T15:20:09Z"},{"has_accepted_license":"1","year":"2026","scopus_import":"1","abstract":[{"lang":"eng","text":"Rational design strategies for self-assembly require a detailed understanding of both the equilibrium state and the assembly kinetics. While the former is starting to be well understood, the latter remains a major theoretical challenge, especially in programmable systems and the so-called semi-addressable regime, where binding is often nondeterministic and the formation of off-target structures negatively influences the assembly. Here, we show that it is possible to simultaneously sculpt the assembly outcome and the assembly kinetics through the underexplored design space of binding energies and particle concentrations. By formulating the assembly process as a complex reaction network, we calculate and optimize the tradeoff between assembly speed and quality and show that parameter optimization can speed up assembly by many orders of magnitude without lowering the yield of the target structure. Although the exact speedup varies from design to design, we find the largest speedups for nondeterministic systems where unoptimized assembly is the slowest, sometimes even making them assemble faster than optimized, fully addressable designs. Therefore, these results not only solve a key challenge in semi-addressable self-assembly but further emphasize the utility of semi-addressability, where designs have the potential to be faster as well as cheaper (fewer particle species) and better (higher yield). More broadly, our results highlight the importance of parameter optimization in programmable self-assembly and provide practical tools for simultaneous optimization of kinetics and yield in a wide range of systems."}],"title":"Simultaneous optimization of assembly time and yield in programmable self-assembly","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"publisher":"AIP Publishing","OA_place":"publisher","doi":"10.1063/5.0304731","volume":164,"language":[{"iso":"eng"}],"month":"02","citation":{"ista":"Hübl M, Goodrich CP. 2026. Simultaneous optimization of assembly time and yield in programmable self-assembly. Journal of Chemical Physics. 164(8), 084904.","chicago":"Hübl, Maximilian, and Carl Peter Goodrich. “Simultaneous Optimization of Assembly Time and Yield in Programmable Self-Assembly.” <i>Journal of Chemical Physics</i>. AIP Publishing, 2026. <a href=\"https://doi.org/10.1063/5.0304731\">https://doi.org/10.1063/5.0304731</a>.","short":"M. Hübl, C.P. Goodrich, Journal of Chemical Physics 164 (2026).","apa":"Hübl, M., &#38; Goodrich, C. P. (2026). Simultaneous optimization of assembly time and yield in programmable self-assembly. <i>Journal of Chemical Physics</i>. AIP Publishing. <a href=\"https://doi.org/10.1063/5.0304731\">https://doi.org/10.1063/5.0304731</a>","ama":"Hübl M, Goodrich CP. Simultaneous optimization of assembly time and yield in programmable self-assembly. <i>Journal of Chemical Physics</i>. 2026;164(8). doi:<a href=\"https://doi.org/10.1063/5.0304731\">10.1063/5.0304731</a>","mla":"Hübl, Maximilian, and Carl Peter Goodrich. “Simultaneous Optimization of Assembly Time and Yield in Programmable Self-Assembly.” <i>Journal of Chemical Physics</i>, vol. 164, no. 8, 084904, AIP Publishing, 2026, doi:<a href=\"https://doi.org/10.1063/5.0304731\">10.1063/5.0304731</a>.","ieee":"M. Hübl and C. P. Goodrich, “Simultaneous optimization of assembly time and yield in programmable self-assembly,” <i>Journal of Chemical Physics</i>, vol. 164, no. 8. AIP Publishing, 2026."},"issue":"8","status":"public","project":[{"name":"Dynamically reconfigurable self-assembly with triangular DNA-origami bricks","_id":"8dd93da8-16d5-11f0-9cad-d2c70200d9a5","grant_number":"FTI23-G-011"}],"date_created":"2026-03-08T23:01:45Z","OA_type":"hybrid","external_id":{"arxiv":["2510.07876"]},"oa":1,"article_processing_charge":"Yes (via OA deal)","_id":"21408","quality_controlled":"1","ddc":["540"],"acknowledgement":"The research was supported by the Gesellschaft für Forschungsförderung Niederösterreich under Project No. FTI23-G-011.","date_updated":"2026-03-09T10:40:41Z","corr_author":"1","publication":"Journal of Chemical Physics","oa_version":"Published Version","arxiv":1,"article_type":"original","article_number":"084904","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","author":[{"full_name":"Hübl, Maximilian","first_name":"Maximilian","last_name":"Hübl","id":"5eb8629e-15b2-11ec-abd3-e6f3e5e01f32"},{"id":"EB352CD2-F68A-11E9-89C5-A432E6697425","last_name":"Goodrich","orcid":"0000-0002-1307-5074","full_name":"Goodrich, Carl Peter","first_name":"Carl Peter"}],"publication_identifier":{"eissn":["1089-7690"],"issn":["0021-9606"]},"file":[{"access_level":"open_access","file_size":6903766,"file_name":"2026_JourChemPhysics_Huebl.pdf","creator":"dernst","checksum":"9bdb8870930e83edb973408da3038559","file_id":"21415","content_type":"application/pdf","date_created":"2026-03-09T10:38:55Z","success":1,"relation":"main_file","date_updated":"2026-03-09T10:38:55Z"}],"intvolume":"       164","publication_status":"published","department":[{"_id":"CaGo"},{"_id":"GradSch"}],"type":"journal_article","day":"28","file_date_updated":"2026-03-09T10:38:55Z","date_published":"2026-02-28T00:00:00Z"},{"abstract":[{"text":"Three-dimensional (3D) crystals offer a route to scaling up trapped-ion systems for quantum sensing and quantum simulation applications; however, engineering coherent spin-motion couplings and effective spin-spin interactions in large crystals poses technical challenges associated with decoherence and prolonged timescales to generate appreciable entanglement. Here, we explore the possibility of speeding up these interactions in 3D crystals via parametric amplification. For this purpose, we derive a general Hamiltonian for the parametric amplification of spin-motion coupling that is broadly applicable to normal modes with motion transverse to or along the spatial extent of the crystal. Unlike in lower-dimensional crystals, we find that the ability to faithfully (uniformly) amplify the spin-spin interactions in 3D crystals depends on the physical implementation of the spin-motion coupling. We consider the light-shift gate, and the so-called phase-insensitive and phase-sensitive Mølmer-Sørensen (MS) gates, and we find that only the phase-sensitive MS gate can be faithfully amplified in general 3D crystals. We discuss a situation where nonuniform amplification can be advantageous. We also reconsider the effect of counter-rotating terms on parametric amplification and find that they are not as detrimental as previous studies suggest.","lang":"eng"}],"title":"Parametric amplification of spin-motion coupling in three-dimensional trapped-ion crystals","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"publisher":"American Physical Society","has_accepted_license":"1","year":"2026","scopus_import":"1","OA_type":"hybrid","external_id":{"arxiv":["2507.16741"]},"oa":1,"article_processing_charge":"Yes (via OA deal)","_id":"21449","quality_controlled":"1","ddc":["530"],"OA_place":"publisher","doi":"10.1103/h1m9-h3yw","volume":25,"language":[{"iso":"eng"}],"month":"03","issue":"3","citation":{"chicago":"Hawaldar, Samarth, N. Nikhil, Ana Maria Rey, John J. Bollinger, and Athreya Shankar. “Parametric Amplification of Spin-Motion Coupling in Three-Dimensional Trapped-Ion Crystals.” <i>Physical Review Applied</i>. American Physical Society, 2026. <a href=\"https://doi.org/10.1103/h1m9-h3yw\">https://doi.org/10.1103/h1m9-h3yw</a>.","ista":"Hawaldar S, Nikhil N, Rey AM, Bollinger JJ, Shankar A. 2026. Parametric amplification of spin-motion coupling in three-dimensional trapped-ion crystals. Physical Review Applied. 25(3), 034004.","short":"S. Hawaldar, N. Nikhil, A.M. Rey, J.J. Bollinger, A. Shankar, Physical Review Applied 25 (2026).","apa":"Hawaldar, S., Nikhil, N., Rey, A. M., Bollinger, J. J., &#38; Shankar, A. (2026). Parametric amplification of spin-motion coupling in three-dimensional trapped-ion crystals. <i>Physical Review Applied</i>. American Physical Society. <a href=\"https://doi.org/10.1103/h1m9-h3yw\">https://doi.org/10.1103/h1m9-h3yw</a>","ama":"Hawaldar S, Nikhil N, Rey AM, Bollinger JJ, Shankar A. Parametric amplification of spin-motion coupling in three-dimensional trapped-ion crystals. <i>Physical Review Applied</i>. 2026;25(3). doi:<a href=\"https://doi.org/10.1103/h1m9-h3yw\">10.1103/h1m9-h3yw</a>","ieee":"S. Hawaldar, N. Nikhil, A. M. Rey, J. J. Bollinger, and A. Shankar, “Parametric amplification of spin-motion coupling in three-dimensional trapped-ion crystals,” <i>Physical Review Applied</i>, vol. 25, no. 3. American Physical Society, 2026.","mla":"Hawaldar, Samarth, et al. “Parametric Amplification of Spin-Motion Coupling in Three-Dimensional Trapped-Ion Crystals.” <i>Physical Review Applied</i>, vol. 25, no. 3, 034004, American Physical Society, 2026, doi:<a href=\"https://doi.org/10.1103/h1m9-h3yw\">10.1103/h1m9-h3yw</a>."},"status":"public","project":[{"name":"QUANTUM INFORMATION SYSTEMS BEYOND CLASSICAL CAPABILITIES / P5- Integration of Superconducting Quantum Circuits","grant_number":"F07105","_id":"bdb108fd-d553-11ed-ba76-83dc74a9864f"}],"date_created":"2026-03-15T23:01:35Z","arxiv":1,"oa_version":"Published Version","article_type":"original","article_number":"034004","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","author":[{"id":"221708e1-1ff6-11ee-9fa6-85146607433e","orcid":"0000-0002-1965-4309","last_name":"Hawaldar","full_name":"Hawaldar, Samarth","first_name":"Samarth"},{"last_name":"Nikhil","first_name":"N.","full_name":"Nikhil, N."},{"last_name":"Rey","first_name":"Ana Maria","full_name":"Rey, Ana Maria"},{"full_name":"Bollinger, John J.","first_name":"John J.","last_name":"Bollinger"},{"first_name":"Athreya","full_name":"Shankar, Athreya","last_name":"Shankar"}],"publication_identifier":{"eissn":["2331-7019"]},"acknowledgement":"We thank Wenchao Ge and Allison Carter for feedback on the manuscript. We also thank Wenchao Ge for sharing the numerical simulation data that we have used in Fig. 5 of this paper. N.N. would like to thank Perimeter Institute and Boston University for support during this research. S.H. acknowledges partial support from the Institute of Science and Technology Austria and the Austrian Science Fund (FWF) DOI 10.55776/F71 for the duration of this project. This work was supported by DOE Quantum Systems Accelerator, ARO W911NF24-1-0128, and NSF JILA-PFC PHY-2317149. J.J.B. and A.M.R. acknowledge support through AFOSR Grant No. FA9550-25-1-0080. A.S. acknowledges support by the Department of Science and Technology, Govt. of India through the INSPIRE Faculty Award (DST/INSPIRE/04/2023/001486), by the Anusandhan National Research Foundation (ANRF), Govt. of India through the Prime Minister’s Early Career Research Grant (PMECRG) (ANRF/ECRG/2024/001160/PMS) and by IIT Madras through the New Faculty Initiation Grant (NFIG).","date_updated":"2026-04-14T09:04:08Z","corr_author":"1","publication":"Physical Review Applied","department":[{"_id":"JoFi"},{"_id":"GradSch"}],"type":"journal_article","day":"01","file_date_updated":"2026-03-16T09:24:53Z","PlanS_conform":"1","date_published":"2026-03-01T00:00:00Z","file":[{"date_updated":"2026-03-16T09:24:53Z","relation":"main_file","date_created":"2026-03-16T09:24:53Z","success":1,"creator":"dernst","checksum":"f0dc6a50222b778fd75cc72a28d38689","content_type":"application/pdf","file_id":"21456","file_name":"2026_PhysicalReviewApplied_Hawaldar.pdf","access_level":"open_access","file_size":1421954}],"intvolume":"        25","publication_status":"published"},{"doi":"10.1051/0004-6361/202557790","OA_place":"publisher","volume":707,"language":[{"iso":"eng"}],"month":"03","citation":{"ista":"Di Cesare C, Matthee JJ, Naidu RP, Torralba A, Kotiwale G, Kramarenko I, Blaizot J, Rosdahl J, Leja J, Iani E, Adamo A, Covelo-Paz A, Furtak LJ, Heintz KE, Mascia S, Navarrete B, Oesch PA, Romano M, Shivaei I, Tacchella S. 2026. The slope and scatter of the star-forming main sequence at z ∼ 5: Reconciling observations with simulations. Astronomy &#38; Astrophysics. 707, A129.","chicago":"Di Cesare, Claudia, Jorryt J Matthee, Rohan P. Naidu, Alberto Torralba, Gauri Kotiwale, Ivan Kramarenko, Jeremy Blaizot, et al. “The Slope and Scatter of the Star-Forming Main Sequence at z ∼ 5: Reconciling Observations with Simulations.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2026. <a href=\"https://doi.org/10.1051/0004-6361/202557790\">https://doi.org/10.1051/0004-6361/202557790</a>.","short":"C. Di Cesare, J.J. Matthee, R.P. Naidu, A. Torralba, G. Kotiwale, I. Kramarenko, J. Blaizot, J. Rosdahl, J. Leja, E. Iani, A. Adamo, A. Covelo-Paz, L.J. Furtak, K.E. Heintz, S. Mascia, B. Navarrete, P.A. Oesch, M. Romano, I. Shivaei, S. Tacchella, Astronomy &#38; Astrophysics 707 (2026).","apa":"Di Cesare, C., Matthee, J. J., Naidu, R. P., Torralba, A., Kotiwale, G., Kramarenko, I., … Tacchella, S. (2026). The slope and scatter of the star-forming main sequence at z ∼ 5: Reconciling observations with simulations. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202557790\">https://doi.org/10.1051/0004-6361/202557790</a>","mla":"Di Cesare, Claudia, et al. “The Slope and Scatter of the Star-Forming Main Sequence at z ∼ 5: Reconciling Observations with Simulations.” <i>Astronomy &#38; Astrophysics</i>, vol. 707, A129, EDP Sciences, 2026, doi:<a href=\"https://doi.org/10.1051/0004-6361/202557790\">10.1051/0004-6361/202557790</a>.","ieee":"C. Di Cesare <i>et al.</i>, “The slope and scatter of the star-forming main sequence at z ∼ 5: Reconciling observations with simulations,” <i>Astronomy &#38; Astrophysics</i>, vol. 707. EDP Sciences, 2026.","ama":"Di Cesare C, Matthee JJ, Naidu RP, et al. The slope and scatter of the star-forming main sequence at z ∼ 5: Reconciling observations with simulations. <i>Astronomy &#38; Astrophysics</i>. 2026;707. doi:<a href=\"https://doi.org/10.1051/0004-6361/202557790\">10.1051/0004-6361/202557790</a>"},"status":"public","project":[{"_id":"bd9b2118-d553-11ed-ba76-db24564edfea","grant_number":"101076224","name":"Young galaxies as tracers and agents of cosmic reionization"}],"date_created":"2026-03-15T23:01:36Z","OA_type":"diamond","external_id":{"arxiv":["2510.19044"]},"oa":1,"article_processing_charge":"No","_id":"21452","quality_controlled":"1","ddc":["520"],"year":"2026","has_accepted_license":"1","scopus_import":"1","abstract":[{"text":"Galaxies exhibit a tight correlation between their star formation rate (SFR) and stellar mass over a wide redshift range known as the star-forming main sequence (SFMS). With JWST, the SFMS can now be investigated at high redshifts down to masses of ∼106 M⊙, using sensitive star formation rate tracers such as the Hα emission, which allow us to probe the variability in the star formation histories. We present inferences of the SFMS based on 316 Hα-selected galaxies at z ∼ 4 − 5 with log(M★/M⊙) = 6.4 − 10.6. These galaxies were identified behind the Abell 2744 lensing cluster with NIRCam grism spectroscopy from the survey All the Little Things (ALT). At face value, our data suggest a shallow slope in the SFMS (SFR ∝ M★α, with α = 0.45). After we corrected this for the Hα-flux limited nature of our survey using a Bayesian framework, the slope steepened to α = 0.59+0.10−0.09, whereas current data on their own are inconclusive on the mass dependence of the scatter. These slopes differ significantly from the slope of ∼1 that is expected from the observed evolution of the galaxy stellar mass function and from simulations. When we fixed the slope to α = 1, we found evidence for a decreasing intrinsic scatter with stellar mass (from ∼0.5 dex at M★ = 108 M⊙ to 0.4 dex at M★ = 1010 M⊙). This difference might be explained by a (combination of) luminosity-dependent SFR(Hα) calibration, a population of (mini)-quenched low-mass galaxies, or underestimated dust attenuation in high-mass galaxies. Future deep observations with different facilities can quantify these processes, which will enable us to achieve better insights into the variability of the star formation histories.","lang":"eng"}],"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"title":"The slope and scatter of the star-forming main sequence at z ∼ 5: Reconciling observations with simulations","publisher":"EDP Sciences","DOAJ_listed":"1","file":[{"date_created":"2026-03-16T10:48:07Z","success":1,"relation":"main_file","date_updated":"2026-03-16T10:48:07Z","access_level":"open_access","file_size":1821411,"file_name":"2026_AstronomyAstrophysics_DiCesare.pdf","creator":"dernst","checksum":"c056b00ce7324849754521fde10fb7ca","file_id":"21459","content_type":"application/pdf"}],"intvolume":"       707","publication_status":"published","department":[{"_id":"JoMa"},{"_id":"GradSch"}],"type":"journal_article","day":"01","file_date_updated":"2026-03-16T10:48:07Z","PlanS_conform":"1","date_published":"2026-03-01T00:00:00Z","acknowledgement":"We thank the anonymous referee for the insightful comments that helped improving the manuscript. We thank Romain. A. Meyer for valuable discussion, Pierluigi Rinaldi for his help with data handling and Luca Graziani and William McClymont for providing the dustyGadget and\r\nTHESAN-ZOOM data, respectively. Funded by the European Union (ERC, AGENTS, 101076224). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program # 3516. We acknowledge funding from JWST program GO-3516. Software used in developing this work includes: matplotlib (Hunter 2007), numpy (Oliphant 2007), scipy (Virtanen et al. 2020), TOPCAT (Taylor 2005), and Astropy (Astropy Collaboration 2013).","date_updated":"2026-03-16T10:52:44Z","corr_author":"1","publication":"Astronomy & Astrophysics","oa_version":"Published Version","arxiv":1,"article_type":"original","article_number":"A129","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","author":[{"id":"2d002343-372f-11ef-98ec-a164d20427cb","last_name":"Di Cesare","first_name":"Claudia","full_name":"Di Cesare, Claudia"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X","last_name":"Matthee","first_name":"Jorryt J","full_name":"Matthee, Jorryt J"},{"last_name":"Naidu","full_name":"Naidu, Rohan P.","first_name":"Rohan P."},{"first_name":"Alberto","full_name":"Torralba, Alberto","last_name":"Torralba"},{"full_name":"Kotiwale, Gauri","first_name":"Gauri","last_name":"Kotiwale","id":"1438afc8-1ff6-11ee-9fa6-cd4a75d66875"},{"id":"9a9394cb-3200-11ee-973b-f5ba2a8b16e4","last_name":"Kramarenko","orcid":"0000-0001-5346-6048","full_name":"Kramarenko, Ivan","first_name":"Ivan"},{"last_name":"Blaizot","first_name":"Jeremy","full_name":"Blaizot, Jeremy"},{"full_name":"Rosdahl, Joakim","first_name":"Joakim","last_name":"Rosdahl"},{"full_name":"Leja, Joel","first_name":"Joel","last_name":"Leja"},{"first_name":"Edoardo","full_name":"Iani, Edoardo","id":"4053390a-6b68-11ef-9828-a3b8adef8d0a","last_name":"Iani","orcid":"0000-0001-8386-3546"},{"first_name":"Angela","full_name":"Adamo, Angela","last_name":"Adamo"},{"last_name":"Covelo-Paz","first_name":"Alba","full_name":"Covelo-Paz, Alba"},{"full_name":"Furtak, Lukas J.","first_name":"Lukas J.","last_name":"Furtak"},{"first_name":"Kasper E.","full_name":"Heintz, Kasper E.","last_name":"Heintz"},{"id":"edaf889c-c7cd-11ef-ab1b-bb28c431bd29","last_name":"Mascia","first_name":"Sara","full_name":"Mascia, Sara"},{"full_name":"Navarrete, Benjamín","first_name":"Benjamín","last_name":"Navarrete","id":"aa14a535-50c9-11ef-b52e-e0c373d10148"},{"last_name":"Oesch","first_name":"Pascal A.","full_name":"Oesch, Pascal A."},{"last_name":"Romano","first_name":"Michael","full_name":"Romano, Michael"},{"first_name":"Irene","full_name":"Shivaei, Irene","last_name":"Shivaei"},{"first_name":"Sandro","full_name":"Tacchella, Sandro","last_name":"Tacchella"}],"publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]}},{"doi":"10.1103/1c5k-9z82","OA_place":"publisher","language":[{"iso":"eng"}],"volume":136,"citation":{"chicago":"Shen, Chao, Maximilian Frenzel, Sebastian F. Maehrlein, and Zhanybek Alpichshev. “Disentangling Electronic and Ionic Nonlinear Polarization Effects in Bulk THz Kerr Response.” <i>Physical Review Letters</i>. American Physical Society, 2026. <a href=\"https://doi.org/10.1103/1c5k-9z82\">https://doi.org/10.1103/1c5k-9z82</a>.","ista":"Shen C, Frenzel M, Maehrlein SF, Alpichshev Z. 2026. Disentangling electronic and ionic nonlinear polarization effects in bulk THz Kerr response. Physical Review Letters. 136(10), 106901.","short":"C. Shen, M. Frenzel, S.F. Maehrlein, Z. Alpichshev, Physical Review Letters 136 (2026).","apa":"Shen, C., Frenzel, M., Maehrlein, S. F., &#38; Alpichshev, Z. (2026). Disentangling electronic and ionic nonlinear polarization effects in bulk THz Kerr response. <i>Physical Review Letters</i>. American Physical Society. <a href=\"https://doi.org/10.1103/1c5k-9z82\">https://doi.org/10.1103/1c5k-9z82</a>","ama":"Shen C, Frenzel M, Maehrlein SF, Alpichshev Z. Disentangling electronic and ionic nonlinear polarization effects in bulk THz Kerr response. <i>Physical Review Letters</i>. 2026;136(10). doi:<a href=\"https://doi.org/10.1103/1c5k-9z82\">10.1103/1c5k-9z82</a>","ieee":"C. Shen, M. Frenzel, S. F. Maehrlein, and Z. Alpichshev, “Disentangling electronic and ionic nonlinear polarization effects in bulk THz Kerr response,” <i>Physical Review Letters</i>, vol. 136, no. 10. American Physical Society, 2026.","mla":"Shen, Chao, et al. “Disentangling Electronic and Ionic Nonlinear Polarization Effects in Bulk THz Kerr Response.” <i>Physical Review Letters</i>, vol. 136, no. 10, 106901, American Physical Society, 2026, doi:<a href=\"https://doi.org/10.1103/1c5k-9z82\">10.1103/1c5k-9z82</a>."},"issue":"10","month":"03","date_created":"2026-03-22T23:04:31Z","project":[{"name":"Center for Correlated Quantum Materials and Solid State Quantum Systems: Nonlinear THz spectroscopy of quantum critical materials","grant_number":"F8602","_id":"34a97cc6-11ca-11ed-8bc3-9acbba792f33"}],"status":"public","OA_type":"hybrid","oa":1,"_id":"21469","quality_controlled":"1","article_processing_charge":"Yes (via OA deal)","ddc":["530"],"scopus_import":"1","has_accepted_license":"1","year":"2026","abstract":[{"lang":"eng","text":"Terahertz (THz) spectroscopy is a powerful probe of low-energy excitations in complex materials. Extending it into the nonlinear regime broadens its scope and can provide valuable insight into interactions among these modes. However, interpreting nonlinear spectra is challenging because resonant features in this case do not always reflect intrinsic material dynamics. Here, we study nonlinear THz-induced Kerr effect in a generic material LaAlO3. After detailed analysis of temporal oscillations of the Kerr signal, we identify an 𝐸𝑔 Raman mode at 1.1 THz excited through a two-photon process, while two additional peaks (0.86 and 0.36 THz) arise from phase matching of the near-infrared probe beam with co- and counterpropagating THz pump fields, mediated by off-resonant electronic hyperpolarizability. These results demonstrate the crucial role of kinematic effects in shaping THz-induced Kerr response and establish a framework for interpreting nonlinear spectroscopies in complex materials."}],"title":"Disentangling electronic and ionic nonlinear polarization effects in bulk THz Kerr response","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)"},"publisher":"American Physical Society","intvolume":"       136","file":[{"success":1,"date_created":"2026-03-23T13:08:06Z","date_updated":"2026-03-23T13:08:06Z","relation":"main_file","file_name":"2026_PhysicalReviewLetters_Shen.pdf","access_level":"open_access","file_size":1375532,"content_type":"application/pdf","file_id":"21475","creator":"dernst","checksum":"712b05b4b0e0fbe9fd426a8c9d41ce20"}],"publication_status":"published","type":"journal_article","department":[{"_id":"ZhAl"},{"_id":"GradSch"}],"PlanS_conform":"1","day":"13","file_date_updated":"2026-03-23T13:08:06Z","date_published":"2026-03-13T00:00:00Z","date_updated":"2026-03-23T13:11:09Z","acknowledgement":"Z. A. acknowledges support from the collaborative research project SFB Q-M&S funded by the Austrian Science Fund (FWF, Grant No. PR1050F8602). S. F. M. acknowledges support and funding from the Deutsche Forschungsgemeinschaft (DFG, Grant No. 469405347).","corr_author":"1","publication":"Physical Review Letters","oa_version":"Published Version","article_number":"106901","article_type":"original","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"issn":["0031-9007"],"eissn":["1079-7114"]},"author":[{"first_name":"Chao","full_name":"Shen, Chao","last_name":"Shen","id":"f84c083e-dc8d-11ea-abe3-aaf3d822a8bb"},{"last_name":"Frenzel","full_name":"Frenzel, Maximilian","first_name":"Maximilian"},{"last_name":"Maehrlein","full_name":"Maehrlein, Sebastian F.","first_name":"Sebastian F."},{"id":"45E67A2A-F248-11E8-B48F-1D18A9856A87","last_name":"Alpichshev","orcid":"0000-0002-7183-5203","full_name":"Alpichshev, Zhanybek","first_name":"Zhanybek"}]}]