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C., Marhavá, P., Benková, E., Yoshida, S., & Friml, J. (2020). Wounding-induced changes in cellular pressure and localized auxin signalling spatially coordinate restorative divisions in roots. Proceedings of the National Academy of Sciences of the United States of America. National Academy of Sciences. https://doi.org/10.1073/pnas.2003346117","ama":"Hörmayer L, Montesinos López JC, Marhavá P, Benková E, Yoshida S, Friml J. Wounding-induced changes in cellular pressure and localized auxin signalling spatially coordinate restorative divisions in roots. Proceedings of the National Academy of Sciences of the United States of America. 2020;117(26). doi:10.1073/pnas.2003346117","mla":"Hörmayer, Lukas, et al. “Wounding-Induced Changes in Cellular Pressure and Localized Auxin Signalling Spatially Coordinate Restorative Divisions in Roots.” Proceedings of the National Academy of Sciences of the United States of America, vol. 117, no. 26, 202003346, National Academy of Sciences, 2020, doi:10.1073/pnas.2003346117.","ieee":"L. Hörmayer, J. C. Montesinos López, P. Marhavá, E. Benková, S. Yoshida, and J. Friml, “Wounding-induced changes in cellular pressure and localized auxin signalling spatially coordinate restorative divisions in roots,” Proceedings of the National Academy of Sciences of the United States of America, vol. 117, no. 26. National Academy of Sciences, 2020.","chicago":"Hörmayer, Lukas, Juan C Montesinos López, Petra Marhavá, Eva Benková, Saiko Yoshida, and Jiří Friml. “Wounding-Induced Changes in Cellular Pressure and Localized Auxin Signalling Spatially Coordinate Restorative Divisions in Roots.” Proceedings of the National Academy of Sciences of the United States of America. National Academy of Sciences, 2020. https://doi.org/10.1073/pnas.2003346117.","short":"L. Hörmayer, J.C. Montesinos López, P. Marhavá, E. Benková, S. Yoshida, J. Friml, Proceedings of the National Academy of Sciences of the United States of America 117 (2020).","ista":"Hörmayer L, Montesinos López JC, Marhavá P, Benková E, Yoshida S, Friml J. 2020. Wounding-induced changes in cellular pressure and localized auxin signalling spatially coordinate restorative divisions in roots. Proceedings of the National Academy of Sciences of the United States of America. 117(26), 202003346."},"publication":"Proceedings of the National Academy of Sciences of the United States of America","type":"journal_article","project":[{"_id":"261099A6-B435-11E9-9278-68D0E5697425","call_identifier":"H2020","grant_number":"742985","name":"Tracing Evolution of Auxin Transport and Polarity in Plants"},{"grant_number":"P29988","call_identifier":"FWF","name":"RNA-directed DNA methylation in plant development","_id":"262EF96E-B435-11E9-9278-68D0E5697425"}],"_id":"8002","doi":"10.1073/pnas.2003346117","author":[{"full_name":"Hörmayer, Lukas","first_name":"Lukas","id":"2EEE7A2A-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8295-2926","last_name":"Hörmayer"},{"id":"310A8E3E-F248-11E8-B48F-1D18A9856A87","first_name":"Juan C","full_name":"Montesinos López, Juan C","last_name":"Montesinos López","orcid":"0000-0001-9179-6099"},{"full_name":"Marhavá, Petra","first_name":"Petra","id":"44E59624-F248-11E8-B48F-1D18A9856A87","last_name":"Marhavá"},{"id":"38F4F166-F248-11E8-B48F-1D18A9856A87","first_name":"Eva","full_name":"Benková, Eva","last_name":"Benková","orcid":"0000-0002-8510-9739"},{"first_name":"Saiko","full_name":"Yoshida, Saiko","id":"2E46069C-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-6111-9353","last_name":"Yoshida"},{"full_name":"Friml, Jiří","first_name":"Jiří","id":"4159519E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8302-7596","last_name":"Friml"}],"quality_controlled":"1","pmid":1,"isi":1,"scopus_import":"1","date_created":"2020-06-22T13:33:52Z","abstract":[{"text":"Wound healing in plant tissues, consisting of rigid cell wall-encapsulated cells, represents a considerable challenge and occurs through largely unknown mechanisms distinct from those in animals. Owing to their inability to migrate, plant cells rely on targeted cell division and expansion to regenerate wounds. Strict coordination of these wound-induced responses is essential to ensure efficient, spatially restricted wound healing. Single-cell tracking by live imaging allowed us to gain mechanistic insight into the wound perception and coordination of wound responses after laser-based wounding in Arabidopsis root. We revealed a crucial contribution of the collapse of damaged cells in wound perception and detected an auxin increase specific to cells immediately adjacent to the wound. This localized auxin increase balances wound-induced cell expansion and restorative division rates in a dose-dependent manner, leading to tumorous overproliferation when the canonical TIR1 auxin signaling is disrupted. Auxin and wound-induced turgor pressure changes together also spatially define the activation of key components of regeneration, such as the transcription regulator ERF115. Our observations suggest that the wound signaling involves the sensing of collapse of damaged cells and a local auxin signaling activation to coordinate the downstream transcriptional responses in the immediate wound vicinity.","lang":"eng"}],"day":"30","volume":117,"file_date_updated":"2020-07-14T12:48:07Z","related_material":{"record":[{"relation":"dissertation_contains","id":"9992","status":"public"}],"link":[{"description":"News on IST Homepage","url":"https://ist.ac.at/en/news/how-wounded-plants-coordinate-their-healing/","relation":"press_release"}]},"language":[{"iso":"eng"}],"title":"Wounding-induced changes in cellular pressure and localized auxin signalling spatially coordinate restorative divisions in roots"},{"date_created":"2020-01-12T16:07:26Z","day":"13","abstract":[{"lang":"eng","text":"Many flows encountered in nature and applications are characterized by a chaotic motion known as turbulence. Turbulent flows generate intense friction with pipe walls and are responsible for considerable amounts of energy losses at world scale. The nature of turbulent friction and techniques aimed at reducing it have been subject of extensive research over the last century, but no definite answer has been found yet. In this thesis we show that in pipes at moderate turbulent Reynolds numbers friction is better described by the power law first introduced by Blasius and not by the Prandtl–von Kármán formula. At higher Reynolds numbers, large scale motions gradually become more important in the flow and can be related to the change in scaling of friction. Next, we present a series of new techniques that can relaminarize turbulence by suppressing a key mechanism that regenerates it at walls, the lift–up effect. In addition, we investigate the process of turbulence decay in several experiments and discuss the drag reduction potential. Finally, we examine the behavior of friction under pulsating conditions inspired by the human heart cycle and we show that under such circumstances turbulent friction can be reduced to produce energy savings."}],"language":[{"iso":"eng"}],"related_material":{"record":[{"status":"public","relation":"part_of_dissertation","id":"422"},{"relation":"part_of_dissertation","id":"461","status":"public"},{"status":"public","relation":"part_of_dissertation","id":"6228"},{"id":"6486","relation":"part_of_dissertation","status":"public"}]},"title":"New approaches to reduce friction in turbulent pipe flow","file_date_updated":"2021-01-13T23:30:05Z","supervisor":[{"id":"3A374330-F248-11E8-B48F-1D18A9856A87","full_name":"Hof, Björn","first_name":"Björn","last_name":"Hof","orcid":"0000-0003-2057-2754"}],"_id":"7258","doi":"10.15479/AT:ISTA:7258","project":[{"_id":"25152F3A-B435-11E9-9278-68D0E5697425","name":"Decoding the complexity of turbulence at its origin","call_identifier":"FP7","grant_number":"306589"},{"call_identifier":"H2020","grant_number":"737549","name":"Eliminating turbulence in oil pipelines","_id":"25104D44-B435-11E9-9278-68D0E5697425"},{"name":"Experimental studies of the turbulence transition and transport processes in turbulent Taylor-Couette currents","grant_number":"HO 4393/1-2","_id":"25136C54-B435-11E9-9278-68D0E5697425"}],"page":"174","author":[{"full_name":"Scarselli, Davide","first_name":"Davide","id":"40315C30-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-5227-4271","last_name":"Scarselli"}],"ddc":["532"],"citation":{"apa":"Scarselli, D. (2020). New approaches to reduce friction in turbulent pipe flow. Institute of Science and Technology Austria. https://doi.org/10.15479/AT:ISTA:7258","ama":"Scarselli D. New approaches to reduce friction in turbulent pipe flow. 2020. doi:10.15479/AT:ISTA:7258","ieee":"D. Scarselli, “New approaches to reduce friction in turbulent pipe flow,” Institute of Science and Technology Austria, 2020.","mla":"Scarselli, Davide. New Approaches to Reduce Friction in Turbulent Pipe Flow. Institute of Science and Technology Austria, 2020, doi:10.15479/AT:ISTA:7258.","chicago":"Scarselli, Davide. “New Approaches to Reduce Friction in Turbulent Pipe Flow.” Institute of Science and Technology Austria, 2020. https://doi.org/10.15479/AT:ISTA:7258.","short":"D. Scarselli, New Approaches to Reduce Friction in Turbulent Pipe Flow, Institute of Science and Technology Austria, 2020.","ista":"Scarselli D. 2020. New approaches to reduce friction in turbulent pipe flow. Institute of Science and Technology Austria."},"type":"dissertation","article_processing_charge":"No","department":[{"_id":"BjHo"}],"oa":1,"publisher":"Institute of Science and Technology Austria","ec_funded":1,"date_updated":"2026-04-08T07:28:22Z","publication_status":"published","date_published":"2020-01-13T00:00:00Z","month":"01","has_accepted_license":"1","corr_author":"1","status":"public","year":"2020","degree_awarded":"PhD","oa_version":"None","alternative_title":["ISTA Thesis"],"file":[{"file_id":"7259","relation":"source_file","file_name":"2020_Scarselli_Thesis.zip","date_created":"2020-01-12T15:57:14Z","date_updated":"2021-01-13T23:30:05Z","embargo_to":"open_access","creator":"dscarsel","file_size":26640830,"access_level":"closed","content_type":"application/zip","checksum":"4df1ab24e9896635106adde5a54615bf"},{"creator":"dscarsel","access_level":"open_access","content_type":"application/pdf","checksum":"48659ab98e3414293c7a721385c2fd1c","file_size":8515844,"date_updated":"2021-01-13T23:30:05Z","relation":"main_file","file_name":"2020_Scarselli_Thesis.pdf","date_created":"2020-01-12T15:56:14Z","embargo":"2021-01-12","file_id":"7260"}],"publication_identifier":{"issn":["2663-337X"]},"OA_place":"publisher","user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd"},{"type":"journal_article","publication":"Frontiers in Cell and Developmental Biology","intvolume":" 8","external_id":{"pmid":["33102480"],"isi":["000577915900001"]},"ddc":["570"],"citation":{"ama":"Hansen AH, Hippenmeyer S. Non-cell-autonomous mechanisms in radial projection neuron migration in the developing cerebral cortex. Frontiers in Cell and Developmental Biology. 2020;8(9). doi:10.3389/fcell.2020.574382","apa":"Hansen, A. H., & Hippenmeyer, S. (2020). Non-cell-autonomous mechanisms in radial projection neuron migration in the developing cerebral cortex. Frontiers in Cell and Developmental Biology. Frontiers. https://doi.org/10.3389/fcell.2020.574382","mla":"Hansen, Andi H., and Simon Hippenmeyer. “Non-Cell-Autonomous Mechanisms in Radial Projection Neuron Migration in the Developing Cerebral Cortex.” Frontiers in Cell and Developmental Biology, vol. 8, no. 9, 574382, Frontiers, 2020, doi:10.3389/fcell.2020.574382.","ieee":"A. H. Hansen and S. Hippenmeyer, “Non-cell-autonomous mechanisms in radial projection neuron migration in the developing cerebral cortex,” Frontiers in Cell and Developmental Biology, vol. 8, no. 9. Frontiers, 2020.","short":"A.H. Hansen, S. Hippenmeyer, Frontiers in Cell and Developmental Biology 8 (2020).","chicago":"Hansen, Andi H, and Simon Hippenmeyer. “Non-Cell-Autonomous Mechanisms in Radial Projection Neuron Migration in the Developing Cerebral Cortex.” Frontiers in Cell and Developmental Biology. Frontiers, 2020. https://doi.org/10.3389/fcell.2020.574382.","ista":"Hansen AH, Hippenmeyer S. 2020. Non-cell-autonomous mechanisms in radial projection neuron migration in the developing cerebral cortex. Frontiers in Cell and Developmental Biology. 8(9), 574382."},"acknowledgement":"AH was a recipient of a DOC Fellowship (24812) of the Austrian Academy of Sciences. This work also received support from IST Austria institutional funds; the People Programme (Marie Curie Actions) of the European Union’s Seventh Framework Programme (FP7/2007–2013) under REA Grant Agreement No. 618444 to SH.","author":[{"last_name":"Hansen","first_name":"Andi H","full_name":"Hansen, Andi H","id":"38853E16-F248-11E8-B48F-1D18A9856A87"},{"first_name":"Simon","full_name":"Hippenmeyer, Simon","id":"37B36620-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0003-2279-1061","last_name":"Hippenmeyer"}],"quality_controlled":"1","project":[{"grant_number":"24812","name":"Molecular mechanisms of radial neuronal migration","_id":"2625A13E-B435-11E9-9278-68D0E5697425"},{"call_identifier":"FP7","grant_number":"618444","name":"Molecular Mechanisms of Cerebral Cortex Development","_id":"25D61E48-B435-11E9-9278-68D0E5697425"}],"_id":"8569","doi":"10.3389/fcell.2020.574382","isi":1,"scopus_import":"1","pmid":1,"volume":8,"file_date_updated":"2020-09-28T13:11:17Z","related_material":{"record":[{"id":"9962","relation":"dissertation_contains","status":"public"}]},"language":[{"iso":"eng"}],"title":"Non-cell-autonomous mechanisms in radial projection neuron migration in the developing cerebral cortex","date_created":"2020-09-26T06:11:07Z","abstract":[{"text":"Concerted radial migration of newly born cortical projection neurons, from their birthplace to their final target lamina, is a key step in the assembly of the cerebral cortex. The cellular and molecular mechanisms regulating the specific sequential steps of radial neuronal migration in vivo are however still unclear, let alone the effects and interactions with the extracellular environment. In any in vivo context, cells will always be exposed to a complex extracellular environment consisting of (1) secreted factors acting as potential signaling cues, (2) the extracellular matrix, and (3) other cells providing cell–cell interaction through receptors and/or direct physical stimuli. Most studies so far have described and focused mainly on intrinsic cell-autonomous gene functions in neuronal migration but there is accumulating evidence that non-cell-autonomous-, local-, systemic-, and/or whole tissue-wide effects substantially contribute to the regulation of radial neuronal migration. These non-cell-autonomous effects may differentially affect cortical neuron migration in distinct cellular environments. However, the cellular and molecular natures of such non-cell-autonomous mechanisms are mostly unknown. Furthermore, physical forces due to collective migration and/or community effects (i.e., interactions with surrounding cells) may play important roles in neocortical projection neuron migration. In this concise review, we first outline distinct models of non-cell-autonomous interactions of cortical projection neurons along their radial migration trajectory during development. We then summarize experimental assays and platforms that can be utilized to visualize and potentially probe non-cell-autonomous mechanisms. Lastly, we define key questions to address in the future.","lang":"eng"}],"day":"25","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","publication_identifier":{"issn":["2296-634X"]},"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"oa_version":"Published Version","file":[{"date_updated":"2020-09-28T13:11:17Z","success":1,"file_size":5527139,"access_level":"open_access","checksum":"01f731824194c94c81a5da360d997073","content_type":"application/pdf","creator":"dernst","file_id":"8584","relation":"main_file","date_created":"2020-09-28T13:11:17Z","file_name":"2020_Frontiers_Hansen.pdf"}],"status":"public","year":"2020","issue":"9","corr_author":"1","has_accepted_license":"1","date_updated":"2026-06-29T22:31:18Z","publication_status":"published","date_published":"2020-09-25T00:00:00Z","month":"09","article_type":"original","ec_funded":1,"publisher":"Frontiers","oa":1,"department":[{"_id":"SiHi"}],"article_number":"574382","article_processing_charge":"Yes (via OA deal)"},{"quality_controlled":"1","page":"135-163","author":[{"last_name":"Angelopoulos","first_name":"Yannis","full_name":"Angelopoulos, Yannis"},{"last_name":"Killip","first_name":"Rowan","full_name":"Killip, Rowan"},{"last_name":"Visan","full_name":"Visan, Monica","first_name":"Monica","id":"056daca0-b8d1-11f0-964f-f91054abf8ca"}],"_id":"22080","doi":"10.1137/19m1265314","type":"journal_article","publication":"SIAM Journal on Mathematical Analysis","external_id":{"arxiv":["1807.08801"]},"citation":{"ieee":"Y. Angelopoulos, R. Killip, and M. Vişan, “Invariant measures for integrable spin chains and an integrable discrete nonlinear Schrödinger equation,” SIAM Journal on Mathematical Analysis, vol. 52, no. 1. Society for Industrial & Applied Mathematics, pp. 135–163, 2020.","mla":"Angelopoulos, Yannis, et al. “Invariant Measures for Integrable Spin Chains and an Integrable Discrete Nonlinear Schrödinger Equation.” SIAM Journal on Mathematical Analysis, vol. 52, no. 1, Society for Industrial & Applied Mathematics, 2020, pp. 135–63, doi:10.1137/19m1265314.","apa":"Angelopoulos, Y., Killip, R., & Vişan, M. (2020). Invariant measures for integrable spin chains and an integrable discrete nonlinear Schrödinger equation. SIAM Journal on Mathematical Analysis. Society for Industrial & Applied Mathematics. https://doi.org/10.1137/19m1265314","ama":"Angelopoulos Y, Killip R, Vişan M. Invariant measures for integrable spin chains and an integrable discrete nonlinear Schrödinger equation. SIAM Journal on Mathematical Analysis. 2020;52(1):135-163. doi:10.1137/19m1265314","ista":"Angelopoulos Y, Killip R, Vişan M. 2020. Invariant measures for integrable spin chains and an integrable discrete nonlinear Schrödinger equation. SIAM Journal on Mathematical Analysis. 52(1), 135–163.","chicago":"Angelopoulos, Yannis, Rowan Killip, and Monica Vişan. “Invariant Measures for Integrable Spin Chains and an Integrable Discrete Nonlinear Schrödinger Equation.” SIAM Journal on Mathematical Analysis. Society for Industrial & Applied Mathematics, 2020. https://doi.org/10.1137/19m1265314.","short":"Y. Angelopoulos, R. Killip, M. Vişan, SIAM Journal on Mathematical Analysis 52 (2020) 135–163."},"intvolume":" 52","arxiv":1,"language":[{"iso":"eng"}],"main_file_link":[{"url":"https://doi.org/10.48550/arXiv.1807.08801","open_access":"1"}],"title":"Invariant measures for integrable spin chains and an integrable discrete nonlinear Schrödinger equation","volume":52,"date_created":"2026-06-19T08:26:32Z","day":"01","abstract":[{"lang":"eng","text":"We consider discrete analogues of two well-known open problems regarding invariant measures for dispersive PDE, namely, the invariance of the Gibbs measure for the continuum (classical) Heisenberg model and the invariance of white noise under focusing cubic nonlinear Schrödinger equation. These continuum models are completely integrable and connected by the Hasimoto transform; correspondingly, we focus our attention on discretizations that are also completely integrable and also connected by a discrete Hasimoto transform. We consider these models on the infinite lattice ℤ. Concretely, for a completely integrable variant of the classical Heisenberg spin chain model (introduced independently by Haldane, Ishimori, and Sklyanin) we prove the existence and uniqueness of solutions for initial data following a Gibbs law (which we show is unique) and show that the Gibbs measure is preserved under these dynamics. In the setting of the focusing Ablowitz--Ladik system, we prove invariance of a measure that we will show is the appropriate discrete analogue of white noise. We also include a thorough discussion of the Poisson geometry associated to the discrete Hasimoto transform introduced by Ishimori that connects the two models studied in this article."}],"extern":"1","scopus_import":"1","status":"public","year":"2020","issue":"1","publication_identifier":{"issn":["0036-1410"],"eissn":["1095-7154"]},"OA_place":"repository","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Preprint","OA_type":"green","oa":1,"mathsc":["35Q55","35Q51","35Q82"],"article_processing_charge":"No","date_updated":"2026-06-30T12:21:20Z","publication_status":"published","month":"01","article_type":"original","date_published":"2020-01-01T00:00:00Z","publisher":"Society for Industrial & Applied Mathematics","das_tickbox":"1"},{"year":"2019","status":"public","oa_version":"Preprint","publication_identifier":{"eissn":["2363-9555"],"issn":["2522-0160"]},"user_id":"c635000d-4b10-11ee-a964-aac5a93f6ac1","article_processing_charge":"No","department":[{"_id":"TiBr"}],"article_number":"9","oa":1,"publisher":"Springer Nature","date_updated":"2023-09-05T15:39:31Z","publication_status":"published","month":"01","article_type":"original","date_published":"2019-01-02T00:00:00Z","_id":"10874","doi":"10.1007/s40993-018-0146-6","quality_controlled":"1","author":[{"last_name":"Ionica","first_name":"Sorina","full_name":"Ionica, Sorina"},{"last_name":"Kılıçer","first_name":"Pınar","full_name":"Kılıçer, Pınar"},{"first_name":"Kristin","full_name":"Lauter, Kristin","last_name":"Lauter"},{"last_name":"Lorenzo García","full_name":"Lorenzo García, Elisa","first_name":"Elisa"},{"last_name":"Manzateanu","id":"be8d652e-a908-11ec-82a4-e2867729459c","first_name":"Maria-Adelina","full_name":"Manzateanu, Maria-Adelina"},{"last_name":"Massierer","first_name":"Maike","full_name":"Massierer, Maike"},{"last_name":"Vincent","full_name":"Vincent, Christelle","first_name":"Christelle"}],"external_id":{"arxiv":["1807.08986"]},"acknowledgement":"The authors would like to thank the Lorentz Center in Leiden for hosting the Women in Numbers Europe 2 workshop and providing a productive and enjoyable environment for our initial work on this project. We are grateful to the organizers of WIN-E2, Irene Bouw, Rachel Newton and Ekin Ozman, for making this conference and this collaboration possible. We\r\nthank Irene Bouw and Christophe Ritzenhaler for helpful discussions. Ionica acknowledges support from the Thomas Jefferson Fund of the Embassy of France in the United States and the FACE Foundation. Most of Kılıçer’s work was carried out during her stay in Universiteit Leiden and Carl von Ossietzky Universität Oldenburg. Massierer was supported by the Australian Research Council (DP150101689). Vincent is supported by the National Science Foundation under Grant No. DMS-1802323 and by the Thomas Jefferson Fund of the Embassy of France in the United States and the FACE Foundation. ","citation":{"mla":"Ionica, Sorina, et al. “Modular Invariants for Genus 3 Hyperelliptic Curves.” Research in Number Theory, vol. 5, 9, Springer Nature, 2019, doi:10.1007/s40993-018-0146-6.","ieee":"S. Ionica et al., “Modular invariants for genus 3 hyperelliptic curves,” Research in Number Theory, vol. 5. Springer Nature, 2019.","ama":"Ionica S, Kılıçer P, Lauter K, et al. Modular invariants for genus 3 hyperelliptic curves. Research in Number Theory. 2019;5. doi:10.1007/s40993-018-0146-6","apa":"Ionica, S., Kılıçer, P., Lauter, K., Lorenzo García, E., Manzateanu, M.-A., Massierer, M., & Vincent, C. (2019). Modular invariants for genus 3 hyperelliptic curves. Research in Number Theory. Springer Nature. https://doi.org/10.1007/s40993-018-0146-6","ista":"Ionica S, Kılıçer P, Lauter K, Lorenzo García E, Manzateanu M-A, Massierer M, Vincent C. 2019. Modular invariants for genus 3 hyperelliptic curves. Research in Number Theory. 5, 9.","short":"S. Ionica, P. Kılıçer, K. Lauter, E. Lorenzo García, M.-A. Manzateanu, M. Massierer, C. Vincent, Research in Number Theory 5 (2019).","chicago":"Ionica, Sorina, Pınar Kılıçer, Kristin Lauter, Elisa Lorenzo García, Maria-Adelina Manzateanu, Maike Massierer, and Christelle Vincent. “Modular Invariants for Genus 3 Hyperelliptic Curves.” Research in Number Theory. Springer Nature, 2019. https://doi.org/10.1007/s40993-018-0146-6."},"intvolume":" 5","arxiv":1,"type":"journal_article","publication":"Research in Number Theory","date_created":"2022-03-18T12:09:48Z","day":"02","abstract":[{"lang":"eng","text":"In this article we prove an analogue of a theorem of Lachaud, Ritzenthaler, and Zykin, which allows us to connect invariants of binary octics to Siegel modular forms of genus 3. We use this connection to show that certain modular functions, when restricted to the hyperelliptic locus, assume values whose denominators are products of powers of primes of bad reduction for the associated hyperelliptic curves. We illustrate our theorem with explicit computations. This work is motivated by the study of the values of these modular functions at CM points of the Siegel upper half-space, which, if their denominators are known, can be used to effectively compute models of (hyperelliptic, in our case) curves with CM."}],"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1807.08986"}],"language":[{"iso":"eng"}],"title":"Modular invariants for genus 3 hyperelliptic curves","volume":5,"keyword":["Algebra and Number Theory"],"scopus_import":"1"},{"publisher":"EasyChair","date_published":"2019-05-25T00:00:00Z","month":"05","publication_status":"published","date_updated":"2022-05-17T07:09:47Z","article_processing_charge":"No","department":[{"_id":"ToHe"}],"conference":{"end_date":"2019-04-15","location":"Montreal, Canada","start_date":"2019-04-15","name":"ARCH: International Workshop on Applied Verification on Continuous and Hybrid Systems"},"oa":1,"alternative_title":["EPiC Series in Computing"],"file":[{"file_id":"11391","relation":"main_file","date_created":"2022-05-17T06:55:49Z","file_name":"2019_EPiCs_Frehse.pdf","date_updated":"2022-05-17T06:55:49Z","success":1,"access_level":"open_access","content_type":"application/pdf","checksum":"4b92e333db7b4e2349501a804dfede69","file_size":346415,"creator":"dernst"}],"oa_version":"Published Version","publication_identifier":{"issn":["2398-7340"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","editor":[{"last_name":"Frehse","first_name":"Goran","full_name":"Frehse, Goran"},{"last_name":"Althoff","full_name":"Althoff, Matthias","first_name":"Matthias"}],"has_accepted_license":"1","year":"2019","status":"public","scopus_import":"1","abstract":[{"lang":"eng","text":"This report presents the results of a friendly competition for formal verification of continuous and hybrid systems with piecewise constant dynamics. The friendly competition took place as part of the workshop Applied Verification for Continuous and Hybrid Systems (ARCH) in 2019. In this third edition, six tools have been applied to solve five different benchmark problems in the category for piecewise constant dynamics: BACH, Lyse, Hy- COMP, PHAVer/SX, PHAVerLite, and VeriSiMPL. Compared to last year, a new tool has participated (HyCOMP) and PHAVerLite has replaced PHAVer-lite. The result is a snap- shot of the current landscape of tools and the types of benchmarks they are particularly suited for. Due to the diversity of problems, we are not ranking tools, yet the presented results probably provide the most complete assessment of tools for the safety verification of continuous and hybrid systems with piecewise constant dynamics up to this date."}],"day":"25","date_created":"2022-03-18T12:29:23Z","title":"ARCH-COMP19 Category Report: Hybrid systems with piecewise constant dynamics","language":[{"iso":"eng"}],"file_date_updated":"2022-05-17T06:55:49Z","volume":61,"acknowledgement":"The authors gratefully acknowledge \fnancial support by the European Commission project\r\nUnCoVerCPS under grant number 643921. Lei Bu is supported by the National Natural Science\r\nFoundation of China (No.61572249).","citation":{"chicago":"Frehse, Goran, Alessandro Abate, Dieky Adzkiya, Anna Becchi, Lei Bu, Alessandro Cimatti, Mirco Giacobbe, et al. “ARCH-COMP19 Category Report: Hybrid Systems with Piecewise Constant Dynamics.” In ARCH19. 6th International Workshop on Applied Verification of Continuous and Hybrid Systems, edited by Goran Frehse and Matthias Althoff, 61:1–13. EasyChair, 2019. https://doi.org/10.29007/rjwn.","short":"G. Frehse, A. Abate, D. Adzkiya, A. Becchi, L. Bu, A. Cimatti, M. Giacobbe, A. Griggio, S. Mover, M.S. Mufid, I. Riouak, S. Tonetta, E. Zaffanella, in:, G. Frehse, M. Althoff (Eds.), ARCH19. 6th International Workshop on Applied Verification of Continuous and Hybrid Systems, EasyChair, 2019, pp. 1–13.","ista":"Frehse G, Abate A, Adzkiya D, Becchi A, Bu L, Cimatti A, Giacobbe M, Griggio A, Mover S, Mufid MS, Riouak I, Tonetta S, Zaffanella E. 2019. ARCH-COMP19 Category Report: Hybrid systems with piecewise constant dynamics. ARCH19. 6th International Workshop on Applied Verification of Continuous and Hybrid Systems. ARCH: International Workshop on Applied Verification on Continuous and Hybrid Systems, EPiC Series in Computing, vol. 61, 1–13.","apa":"Frehse, G., Abate, A., Adzkiya, D., Becchi, A., Bu, L., Cimatti, A., … Zaffanella, E. (2019). ARCH-COMP19 Category Report: Hybrid systems with piecewise constant dynamics. In G. Frehse & M. Althoff (Eds.), ARCH19. 6th International Workshop on Applied Verification of Continuous and Hybrid Systems (Vol. 61, pp. 1–13). Montreal, Canada: EasyChair. https://doi.org/10.29007/rjwn","ama":"Frehse G, Abate A, Adzkiya D, et al. ARCH-COMP19 Category Report: Hybrid systems with piecewise constant dynamics. In: Frehse G, Althoff M, eds. ARCH19. 6th International Workshop on Applied Verification of Continuous and Hybrid Systems. Vol 61. EasyChair; 2019:1-13. doi:10.29007/rjwn","ieee":"G. Frehse et al., “ARCH-COMP19 Category Report: Hybrid systems with piecewise constant dynamics,” in ARCH19. 6th International Workshop on Applied Verification of Continuous and Hybrid Systems, Montreal, Canada, 2019, vol. 61, pp. 1–13.","mla":"Frehse, Goran, et al. “ARCH-COMP19 Category Report: Hybrid Systems with Piecewise Constant Dynamics.” ARCH19. 6th International Workshop on Applied Verification of Continuous and Hybrid Systems, edited by Goran Frehse and Matthias Althoff, vol. 61, EasyChair, 2019, pp. 1–13, doi:10.29007/rjwn."},"ddc":["000"],"intvolume":" 61","publication":"ARCH19. 6th International Workshop on Applied Verification of Continuous and Hybrid Systems","type":"conference","doi":"10.29007/rjwn","_id":"10877","quality_controlled":"1","page":"1-13","author":[{"full_name":"Frehse, Goran","first_name":"Goran","last_name":"Frehse"},{"first_name":"Alessandro","full_name":"Abate, Alessandro","last_name":"Abate"},{"last_name":"Adzkiya","first_name":"Dieky","full_name":"Adzkiya, Dieky"},{"first_name":"Anna","full_name":"Becchi, Anna","last_name":"Becchi"},{"last_name":"Bu","full_name":"Bu, Lei","first_name":"Lei"},{"first_name":"Alessandro","full_name":"Cimatti, Alessandro","last_name":"Cimatti"},{"first_name":"Mirco","full_name":"Giacobbe, Mirco","id":"3444EA5E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8180-0904","last_name":"Giacobbe"},{"last_name":"Griggio","first_name":"Alberto","full_name":"Griggio, Alberto"},{"last_name":"Mover","first_name":"Sergio","full_name":"Mover, Sergio"},{"first_name":"Muhammad Syifa'ul","full_name":"Mufid, Muhammad Syifa'ul","last_name":"Mufid"},{"full_name":"Riouak, Idriss","first_name":"Idriss","last_name":"Riouak"},{"last_name":"Tonetta","first_name":"Stefano","full_name":"Tonetta, Stefano"},{"last_name":"Zaffanella","full_name":"Zaffanella, Enea","first_name":"Enea"}]},{"issue":"6","status":"public","year":"2019","corr_author":"1","publication_identifier":{"issn":["1553-5231"]},"user_id":"c635000d-4b10-11ee-a964-aac5a93f6ac1","oa_version":"Preprint","oa":1,"article_processing_charge":"No","department":[{"_id":"JaMa"}],"publication_status":"published","date_updated":"2025-04-15T08:31:32Z","date_published":"2019-06-01T00:00:00Z","month":"06","article_type":"original","publisher":"American Institute of Mathematical Sciences","quality_controlled":"1","page":"3037-3067","author":[{"last_name":"Flandoli","first_name":"Franco","full_name":"Flandoli, Franco"},{"first_name":"Enrico","full_name":"Priola, Enrico","last_name":"Priola"},{"id":"47491882-F248-11E8-B48F-1D18A9856A87","first_name":"Giovanni A","full_name":"Zanco, Giovanni A","last_name":"Zanco"}],"_id":"10878","doi":"10.3934/dcds.2019126","project":[{"_id":"fc31cba2-9c52-11eb-aca3-ff467d239cd2","grant_number":"F6504","name":"Taming Complexity in Partial Differential Systems"}],"type":"journal_article","publication":"Discrete and Continuous Dynamical Systems","external_id":{"isi":["000459954800003"],"arxiv":["1708.04156"]},"acknowledgement":"The second author has been partially supported by INdAM through the GNAMPA Research\r\nProject (2017) “Sistemi stocastici singolari: buona posizione e problemi di controllo”. The third\r\nauthor was partly funded by the Austrian Science Fund (FWF) project F 65.","citation":{"ista":"Flandoli F, Priola E, Zanco GA. 2019. A mean-field model with discontinuous coefficients for neurons with spatial interaction. Discrete and Continuous Dynamical Systems. 39(6), 3037–3067.","chicago":"Flandoli, Franco, Enrico Priola, and Giovanni A Zanco. “A Mean-Field Model with Discontinuous Coefficients for Neurons with Spatial Interaction.” Discrete and Continuous Dynamical Systems. American Institute of Mathematical Sciences, 2019. https://doi.org/10.3934/dcds.2019126.","short":"F. Flandoli, E. Priola, G.A. Zanco, Discrete and Continuous Dynamical Systems 39 (2019) 3037–3067.","mla":"Flandoli, Franco, et al. “A Mean-Field Model with Discontinuous Coefficients for Neurons with Spatial Interaction.” Discrete and Continuous Dynamical Systems, vol. 39, no. 6, American Institute of Mathematical Sciences, 2019, pp. 3037–67, doi:10.3934/dcds.2019126.","ieee":"F. Flandoli, E. Priola, and G. A. Zanco, “A mean-field model with discontinuous coefficients for neurons with spatial interaction,” Discrete and Continuous Dynamical Systems, vol. 39, no. 6. American Institute of Mathematical Sciences, pp. 3037–3067, 2019.","apa":"Flandoli, F., Priola, E., & Zanco, G. A. (2019). A mean-field model with discontinuous coefficients for neurons with spatial interaction. Discrete and Continuous Dynamical Systems. American Institute of Mathematical Sciences. https://doi.org/10.3934/dcds.2019126","ama":"Flandoli F, Priola E, Zanco GA. A mean-field model with discontinuous coefficients for neurons with spatial interaction. Discrete and Continuous Dynamical Systems. 2019;39(6):3037-3067. doi:10.3934/dcds.2019126"},"intvolume":" 39","arxiv":1,"language":[{"iso":"eng"}],"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1708.04156"}],"title":"A mean-field model with discontinuous coefficients for neurons with spatial interaction","keyword":["Applied Mathematics","Discrete Mathematics and Combinatorics","Analysis"],"volume":39,"date_created":"2022-03-18T12:33:34Z","abstract":[{"lang":"eng","text":"Starting from a microscopic model for a system of neurons evolving in time which individually follow a stochastic integrate-and-fire type model, we study a mean-field limit of the system. Our model is described by a system of SDEs with discontinuous coefficients for the action potential of each neuron and takes into account the (random) spatial configuration of neurons allowing the interaction to depend on it. In the limit as the number of particles tends to infinity, we obtain a nonlinear Fokker-Planck type PDE in two variables, with derivatives only with respect to one variable and discontinuous coefficients. We also study strong well-posedness of the system of SDEs and prove the existence and uniqueness of a weak measure-valued solution to the PDE, obtained as the limit of the laws of the empirical measures for the system of particles."}],"day":"01","scopus_import":"1","isi":1},{"oa":1,"article_processing_charge":"No","department":[{"_id":"LaEr"}],"date_published":"2019-03-01T00:00:00Z","article_type":"original","month":"03","publication_status":"published","date_updated":"2024-12-11T11:49:15Z","publisher":"European Mathematical Society","issue":"3","status":"public","year":"2019","publication_identifier":{"issn":["1664-039X"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Preprint","title":"Perturbations of continuum random Schrödinger operators with applications to Anderson orthogonality and the spectral shift function","language":[{"iso":"eng"}],"main_file_link":[{"url":"https://arxiv.org/abs/1701.02956","open_access":"1"}],"volume":9,"keyword":["Random Schrödinger operators","spectral shift function","Anderson orthogonality"],"abstract":[{"lang":"eng","text":"We study effects of a bounded and compactly supported perturbation on multidimensional continuum random Schrödinger operators in the region of complete localisation. Our main emphasis is on Anderson orthogonality for random Schrödinger operators. Among others, we prove that Anderson orthogonality does occur for Fermi energies in the region of complete localisation with a non-zero probability. This partially confirms recent non-rigorous findings [V. Khemani et al., Nature Phys. 11 (2015), 560–565]. The spectral shift function plays an important role in our analysis of Anderson orthogonality. We identify it with the index of the corresponding pair of spectral projections and explore the consequences thereof. All our results rely on the main technical estimate of this paper which guarantees separate exponential decay of the disorder-averaged Schatten p-norm of χa(f(H)−f(Hτ))χb in a and b. Here, Hτ is a perturbation of the random Schrödinger operator H, χa is the multiplication operator corresponding to the indicator function of a unit cube centred about a∈Rd, and f is in a suitable class of functions of bounded variation with distributional derivative supported in the region of complete localisation for H."}],"day":"01","date_created":"2022-03-18T12:36:42Z","scopus_import":"1","isi":1,"quality_controlled":"1","page":"921-965","author":[{"last_name":"Dietlein","full_name":"Dietlein, Adrian M","first_name":"Adrian M","id":"317CB464-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Gebert, Martin","first_name":"Martin","last_name":"Gebert"},{"last_name":"Müller","full_name":"Müller, Peter","first_name":"Peter"}],"doi":"10.4171/jst/267","_id":"10879","type":"journal_article","publication":"Journal of Spectral Theory","citation":{"apa":"Dietlein, A. M., Gebert, M., & Müller, P. (2019). Perturbations of continuum random Schrödinger operators with applications to Anderson orthogonality and the spectral shift function. Journal of Spectral Theory. European Mathematical Society. https://doi.org/10.4171/jst/267","ama":"Dietlein AM, Gebert M, Müller P. Perturbations of continuum random Schrödinger operators with applications to Anderson orthogonality and the spectral shift function. Journal of Spectral Theory. 2019;9(3):921-965. doi:10.4171/jst/267","mla":"Dietlein, Adrian M., et al. “Perturbations of Continuum Random Schrödinger Operators with Applications to Anderson Orthogonality and the Spectral Shift Function.” Journal of Spectral Theory, vol. 9, no. 3, European Mathematical Society, 2019, pp. 921–65, doi:10.4171/jst/267.","ieee":"A. M. Dietlein, M. Gebert, and P. Müller, “Perturbations of continuum random Schrödinger operators with applications to Anderson orthogonality and the spectral shift function,” Journal of Spectral Theory, vol. 9, no. 3. European Mathematical Society, pp. 921–965, 2019.","chicago":"Dietlein, Adrian M, Martin Gebert, and Peter Müller. “Perturbations of Continuum Random Schrödinger Operators with Applications to Anderson Orthogonality and the Spectral Shift Function.” Journal of Spectral Theory. European Mathematical Society, 2019. https://doi.org/10.4171/jst/267.","short":"A.M. Dietlein, M. Gebert, P. Müller, Journal of Spectral Theory 9 (2019) 921–965.","ista":"Dietlein AM, Gebert M, Müller P. 2019. Perturbations of continuum random Schrödinger operators with applications to Anderson orthogonality and the spectral shift function. Journal of Spectral Theory. 9(3), 921–965."},"acknowledgement":"M.G. was supported by the DFG under grant GE 2871/1-1.","external_id":{"arxiv":["1701.02956"],"isi":["000484709400006"]},"arxiv":1,"intvolume":" 9"},{"status":"public","issue":"1","year":"2019","publication_identifier":{"eissn":["1471-0064"],"issn":["1471-0056"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"None","article_processing_charge":"No","publication_status":"published","date_updated":"2024-10-14T11:18:54Z","month":"01","article_type":"review","date_published":"2019-01-01T00:00:00Z","publisher":"Springer Nature","quality_controlled":"1","page":"39-50","author":[{"full_name":"Buchwalter, Abigail","first_name":"Abigail","last_name":"Buchwalter"},{"last_name":"Kaneshiro","first_name":"Jeanae M.","full_name":"Kaneshiro, Jeanae M."},{"orcid":"0000-0002-2111-992X","last_name":"HETZER","first_name":"Martin W","full_name":"HETZER, Martin W","id":"86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed"}],"_id":"11059","doi":"10.1038/s41576-018-0063-5","publication":"Nature Reviews Genetics","type":"journal_article","external_id":{"pmid":["30356165"]},"citation":{"mla":"Buchwalter, Abigail, et al. “Coaching from the Sidelines: The Nuclear Periphery in Genome Regulation.” Nature Reviews Genetics, vol. 20, no. 1, Springer Nature, 2019, pp. 39–50, doi:10.1038/s41576-018-0063-5.","ieee":"A. Buchwalter, J. M. Kaneshiro, and M. Hetzer, “Coaching from the sidelines: The nuclear periphery in genome regulation,” Nature Reviews Genetics, vol. 20, no. 1. Springer Nature, pp. 39–50, 2019.","apa":"Buchwalter, A., Kaneshiro, J. M., & Hetzer, M. (2019). Coaching from the sidelines: The nuclear periphery in genome regulation. Nature Reviews Genetics. Springer Nature. https://doi.org/10.1038/s41576-018-0063-5","ama":"Buchwalter A, Kaneshiro JM, Hetzer M. Coaching from the sidelines: The nuclear periphery in genome regulation. Nature Reviews Genetics. 2019;20(1):39-50. doi:10.1038/s41576-018-0063-5","ista":"Buchwalter A, Kaneshiro JM, Hetzer M. 2019. Coaching from the sidelines: The nuclear periphery in genome regulation. Nature Reviews Genetics. 20(1), 39–50.","chicago":"Buchwalter, Abigail, Jeanae M. Kaneshiro, and Martin Hetzer. “Coaching from the Sidelines: The Nuclear Periphery in Genome Regulation.” Nature Reviews Genetics. Springer Nature, 2019. https://doi.org/10.1038/s41576-018-0063-5.","short":"A. Buchwalter, J.M. Kaneshiro, M. Hetzer, Nature Reviews Genetics 20 (2019) 39–50."},"intvolume":" 20","language":[{"iso":"eng"}],"title":"Coaching from the sidelines: The nuclear periphery in genome regulation","volume":20,"keyword":["Genetics (clinical)","Genetics","Molecular Biology"],"date_created":"2022-04-07T07:44:45Z","abstract":[{"lang":"eng","text":"The genome is packaged and organized nonrandomly within the 3D space of the nucleus to promote efficient gene expression and to faithfully maintain silencing of heterochromatin. The genome is enclosed within the nucleus by the nuclear envelope membrane, which contains a set of proteins that actively participate in chromatin organization and gene regulation. Technological advances are providing views of genome organization at unprecedented resolution and are beginning to reveal the ways that cells co-opt the structures of the nuclear periphery for nuclear organization and gene regulation. These genome regulatory roles of proteins of the nuclear periphery have important influences on development, disease and ageing."}],"day":"01","scopus_import":"1","extern":"1","pmid":1},{"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"file":[{"date_created":"2022-04-08T08:18:01Z","file_name":"2019_eLife_Buchwalter.pdf","relation":"main_file","file_id":"11138","content_type":"application/pdf","checksum":"1e8672a1e9c3dc0a2d3d0dad89673616","access_level":"open_access","file_size":6984654,"creator":"dernst","success":1,"date_updated":"2022-04-08T08:18:01Z"}],"oa_version":"Published Version","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"issn":["2050-084X"]},"has_accepted_license":"1","year":"2019","status":"public","publisher":"eLife Sciences Publications","article_type":"original","month":"10","date_published":"2019-10-10T00:00:00Z","publication_status":"published","date_updated":"2024-10-14T12:08:36Z","article_number":"e49796","article_processing_charge":"No","oa":1,"intvolume":" 8","citation":{"ista":"Buchwalter A, Schulte R, Tsai H, Capitanio J, Hetzer M. 2019. Selective clearance of the inner nuclear membrane protein emerin by vesicular transport during ER stress. eLife. 8, e49796.","short":"A. Buchwalter, R. Schulte, H. Tsai, J. Capitanio, M. Hetzer, ELife 8 (2019).","chicago":"Buchwalter, Abigail, Roberta Schulte, Hsiao Tsai, Juliana Capitanio, and Martin Hetzer. “Selective Clearance of the Inner Nuclear Membrane Protein Emerin by Vesicular Transport during ER Stress.” ELife. eLife Sciences Publications, 2019. https://doi.org/10.7554/elife.49796.","ieee":"A. Buchwalter, R. Schulte, H. Tsai, J. Capitanio, and M. Hetzer, “Selective clearance of the inner nuclear membrane protein emerin by vesicular transport during ER stress,” eLife, vol. 8. eLife Sciences Publications, 2019.","mla":"Buchwalter, Abigail, et al. “Selective Clearance of the Inner Nuclear Membrane Protein Emerin by Vesicular Transport during ER Stress.” ELife, vol. 8, e49796, eLife Sciences Publications, 2019, doi:10.7554/elife.49796.","ama":"Buchwalter A, Schulte R, Tsai H, Capitanio J, Hetzer M. Selective clearance of the inner nuclear membrane protein emerin by vesicular transport during ER stress. eLife. 2019;8. doi:10.7554/elife.49796","apa":"Buchwalter, A., Schulte, R., Tsai, H., Capitanio, J., & Hetzer, M. (2019). Selective clearance of the inner nuclear membrane protein emerin by vesicular transport during ER stress. ELife. eLife Sciences Publications. https://doi.org/10.7554/elife.49796"},"external_id":{"pmid":["31599721"]},"ddc":["570"],"publication":"eLife","type":"journal_article","doi":"10.7554/elife.49796","_id":"11060","author":[{"full_name":"Buchwalter, Abigail","first_name":"Abigail","last_name":"Buchwalter"},{"first_name":"Roberta","full_name":"Schulte, Roberta","last_name":"Schulte"},{"last_name":"Tsai","first_name":"Hsiao","full_name":"Tsai, Hsiao"},{"last_name":"Capitanio","full_name":"Capitanio, Juliana","first_name":"Juliana"},{"id":"86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed","full_name":"HETZER, Martin W","first_name":"Martin W","last_name":"HETZER","orcid":"0000-0002-2111-992X"}],"quality_controlled":"1","pmid":1,"extern":"1","scopus_import":"1","abstract":[{"lang":"eng","text":"The inner nuclear membrane (INM) is a subdomain of the endoplasmic reticulum (ER) that is gated by the nuclear pore complex. It is unknown whether proteins of the INM and ER are degraded through shared or distinct pathways in mammalian cells. We applied dynamic proteomics to profile protein half-lives and report that INM and ER residents turn over at similar rates, indicating that the INM’s unique topology is not a barrier to turnover. Using a microscopy approach, we observed that the proteasome can degrade INM proteins in situ. However, we also uncovered evidence for selective, vesicular transport-mediated turnover of a single INM protein, emerin, that is potentiated by ER stress. Emerin is rapidly cleared from the INM by a mechanism that requires emerin’s LEM domain to mediate vesicular trafficking to lysosomes. This work demonstrates that the INM can be dynamically remodeled in response to environmental inputs."}],"day":"10","date_created":"2022-04-07T07:45:02Z","file_date_updated":"2022-04-08T08:18:01Z","keyword":["General Immunology and Microbiology","General Biochemistry","Genetics and Molecular Biology","General Medicine","General Neuroscience"],"volume":8,"title":"Selective clearance of the inner nuclear membrane protein emerin by vesicular transport during ER stress","related_material":{"record":[{"id":"13079","relation":"research_data","status":"public"}]},"language":[{"iso":"eng"}]},{"doi":"10.1083/jcb.201809123","_id":"11061","quality_controlled":"1","page":"433-444","author":[{"last_name":"Toyama","full_name":"Toyama, Brandon H.","first_name":"Brandon H."},{"last_name":"Arrojo e Drigo","first_name":"Rafael","full_name":"Arrojo e Drigo, Rafael"},{"full_name":"Lev-Ram, Varda","first_name":"Varda","last_name":"Lev-Ram"},{"last_name":"Ramachandra","first_name":"Ranjan","full_name":"Ramachandra, Ranjan"},{"last_name":"Deerinck","first_name":"Thomas J.","full_name":"Deerinck, Thomas J."},{"full_name":"Lechene, Claude","first_name":"Claude","last_name":"Lechene"},{"full_name":"Ellisman, Mark H.","first_name":"Mark H.","last_name":"Ellisman"},{"orcid":"0000-0002-2111-992X","last_name":"HETZER","first_name":"Martin W","full_name":"HETZER, Martin W","id":"86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed"}],"citation":{"ieee":"B. H. Toyama et al., “Visualization of long-lived proteins reveals age mosaicism within nuclei of postmitotic cells,” Journal of Cell Biology, vol. 218, no. 2. Rockefeller University Press, pp. 433–444, 2019.","mla":"Toyama, Brandon H., et al. “Visualization of Long-Lived Proteins Reveals Age Mosaicism within Nuclei of Postmitotic Cells.” Journal of Cell Biology, vol. 218, no. 2, Rockefeller University Press, 2019, pp. 433–44, doi:10.1083/jcb.201809123.","apa":"Toyama, B. H., Arrojo e Drigo, R., Lev-Ram, V., Ramachandra, R., Deerinck, T. J., Lechene, C., … Hetzer, M. (2019). Visualization of long-lived proteins reveals age mosaicism within nuclei of postmitotic cells. Journal of Cell Biology. Rockefeller University Press. https://doi.org/10.1083/jcb.201809123","ama":"Toyama BH, Arrojo e Drigo R, Lev-Ram V, et al. Visualization of long-lived proteins reveals age mosaicism within nuclei of postmitotic cells. Journal of Cell Biology. 2019;218(2):433-444. doi:10.1083/jcb.201809123","ista":"Toyama BH, Arrojo e Drigo R, Lev-Ram V, Ramachandra R, Deerinck TJ, Lechene C, Ellisman MH, Hetzer M. 2019. Visualization of long-lived proteins reveals age mosaicism within nuclei of postmitotic cells. Journal of Cell Biology. 218(2), 433–444.","chicago":"Toyama, Brandon H., Rafael Arrojo e Drigo, Varda Lev-Ram, Ranjan Ramachandra, Thomas J. Deerinck, Claude Lechene, Mark H. Ellisman, and Martin Hetzer. “Visualization of Long-Lived Proteins Reveals Age Mosaicism within Nuclei of Postmitotic Cells.” Journal of Cell Biology. Rockefeller University Press, 2019. https://doi.org/10.1083/jcb.201809123.","short":"B.H. Toyama, R. Arrojo e Drigo, V. Lev-Ram, R. Ramachandra, T.J. Deerinck, C. Lechene, M.H. Ellisman, M. Hetzer, Journal of Cell Biology 218 (2019) 433–444."},"external_id":{"pmid":["30552100"]},"ddc":["570"],"intvolume":" 218","publication":"Journal of Cell Biology","type":"journal_article","abstract":[{"text":"Many adult tissues contain postmitotic cells as old as the host organism. The only organelle that does not turn over in these cells is the nucleus, and its maintenance represents a formidable challenge, as it harbors regulatory proteins that persist throughout adulthood. Here we developed strategies to visualize two classes of such long-lived proteins, histones and nucleoporins, to understand the function of protein longevity in nuclear maintenance. Genome-wide mapping of histones revealed specific enrichment of long-lived variants at silent gene loci. Interestingly, nuclear pores are maintained by piecemeal replacement of subunits, resulting in mosaic complexes composed of polypeptides with vastly different ages. In contrast, nondividing quiescent cells remove old nuclear pores in an ESCRT-dependent manner. Our findings reveal distinct molecular strategies of nuclear maintenance, linking lifelong protein persistence to gene regulation and nuclear integrity.","lang":"eng"}],"day":"04","date_created":"2022-04-07T07:45:11Z","title":"Visualization of long-lived proteins reveals age mosaicism within nuclei of postmitotic cells","language":[{"iso":"eng"}],"file_date_updated":"2022-04-08T08:26:32Z","volume":218,"keyword":["Cell Biology"],"pmid":1,"extern":"1","scopus_import":"1","has_accepted_license":"1","status":"public","year":"2019","issue":"2","file":[{"file_id":"11139","relation":"main_file","file_name":"2019_JCB_Toyama.pdf","date_created":"2022-04-08T08:26:32Z","date_updated":"2022-04-08T08:26:32Z","success":1,"creator":"dernst","file_size":2503838,"content_type":"application/pdf","access_level":"open_access","checksum":"7964ebbf833b0b35f9fba840eea9531d"}],"oa_version":"Published Version","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode","short":"CC BY-NC-SA (4.0)","image":"/images/cc_by_nc_sa.png","name":"Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)"},"publication_identifier":{"issn":["0021-9525"],"eissn":["1540-8140"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","oa":1,"publisher":"Rockefeller University Press","month":"02","date_published":"2019-02-04T00:00:00Z","article_type":"original","publication_status":"published","date_updated":"2024-10-14T11:19:21Z"},{"intvolume":" 30","external_id":{"pmid":["31178361"]},"citation":{"ama":"Arrojo e Drigo R, Lev-Ram V, Tyagi S, et al. Age mosaicism across multiple scales in adult tissues. Cell Metabolism. 2019;30(2):343-351.e3. doi:10.1016/j.cmet.2019.05.010","apa":"Arrojo e Drigo, R., Lev-Ram, V., Tyagi, S., Ramachandra, R., Deerinck, T., Bushong, E., … Hetzer, M. (2019). Age mosaicism across multiple scales in adult tissues. Cell Metabolism. Elsevier. https://doi.org/10.1016/j.cmet.2019.05.010","mla":"Arrojo e Drigo, Rafael, et al. “Age Mosaicism across Multiple Scales in Adult Tissues.” Cell Metabolism, vol. 30, no. 2, Elsevier, 2019, p. 343–351.e3, doi:10.1016/j.cmet.2019.05.010.","ieee":"R. Arrojo e Drigo et al., “Age mosaicism across multiple scales in adult tissues,” Cell Metabolism, vol. 30, no. 2. Elsevier, p. 343–351.e3, 2019.","short":"R. Arrojo e Drigo, V. Lev-Ram, S. Tyagi, R. Ramachandra, T. Deerinck, E. Bushong, S. Phan, V. Orphan, C. Lechene, M.H. Ellisman, M. Hetzer, Cell Metabolism 30 (2019) 343–351.e3.","chicago":"Arrojo e Drigo, Rafael, Varda Lev-Ram, Swati Tyagi, Ranjan Ramachandra, Thomas Deerinck, Eric Bushong, Sebastien Phan, et al. “Age Mosaicism across Multiple Scales in Adult Tissues.” Cell Metabolism. Elsevier, 2019. https://doi.org/10.1016/j.cmet.2019.05.010.","ista":"Arrojo e Drigo R, Lev-Ram V, Tyagi S, Ramachandra R, Deerinck T, Bushong E, Phan S, Orphan V, Lechene C, Ellisman MH, Hetzer M. 2019. Age mosaicism across multiple scales in adult tissues. Cell Metabolism. 30(2), 343–351.e3."},"type":"journal_article","publication":"Cell Metabolism","_id":"11062","doi":"10.1016/j.cmet.2019.05.010","author":[{"last_name":"Arrojo e Drigo","full_name":"Arrojo e Drigo, Rafael","first_name":"Rafael"},{"full_name":"Lev-Ram, Varda","first_name":"Varda","last_name":"Lev-Ram"},{"last_name":"Tyagi","full_name":"Tyagi, Swati","first_name":"Swati"},{"first_name":"Ranjan","full_name":"Ramachandra, Ranjan","last_name":"Ramachandra"},{"last_name":"Deerinck","full_name":"Deerinck, Thomas","first_name":"Thomas"},{"full_name":"Bushong, Eric","first_name":"Eric","last_name":"Bushong"},{"last_name":"Phan","first_name":"Sebastien","full_name":"Phan, Sebastien"},{"last_name":"Orphan","first_name":"Victoria","full_name":"Orphan, Victoria"},{"first_name":"Claude","full_name":"Lechene, Claude","last_name":"Lechene"},{"full_name":"Ellisman, Mark H.","first_name":"Mark H.","last_name":"Ellisman"},{"id":"86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed","full_name":"HETZER, Martin W","first_name":"Martin W","last_name":"HETZER","orcid":"0000-0002-2111-992X"}],"page":"343-351.e3","quality_controlled":"1","pmid":1,"scopus_import":"1","extern":"1","date_created":"2022-04-07T07:45:21Z","day":"06","abstract":[{"lang":"eng","text":"Most neurons are not replaced during an animal’s lifetime. This nondividing state is characterized by extreme longevity and age-dependent decline of key regulatory proteins. To study the lifespans of cells and proteins in adult tissues, we combined isotope labeling of mice with a hybrid imaging method (MIMS-EM). Using 15N mapping, we show that liver and pancreas are composed of cells with vastly different ages, many as old as the animal. Strikingly, we also found that a subset of fibroblasts and endothelial cells, both known for their replicative potential, are characterized by the absence of cell division during adulthood. In addition, we show that the primary cilia of beta cells and neurons contains different structural regions with vastly different lifespans. Based on these results, we propose that age mosaicism across multiple scales is a fundamental principle of adult tissue, cell, and protein complex organization."}],"volume":30,"keyword":["Cell Biology","Molecular Biology","Physiology"],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1016/j.cmet.2019.05.010"}],"language":[{"iso":"eng"}],"title":"Age mosaicism across multiple scales in adult tissues","oa_version":"Published Version","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"issn":["1550-4131"]},"year":"2019","status":"public","issue":"2","publisher":"Elsevier","publication_status":"published","date_updated":"2025-12-15T10:02:11Z","date_published":"2019-08-06T00:00:00Z","month":"08","article_type":"original","department":[{"_id":"MaHe"}],"article_processing_charge":"No","oa":1},{"title":"Exploring He II λ1640 emission line properties at z ∼2−4","language":[{"iso":"eng"}],"related_material":{"link":[{"url":"https://doi.org/10.1051/0004-6361/201834565e","relation":"erratum"}]},"main_file_link":[{"url":"https://arxiv.org/abs/1902.05960","open_access":"1"}],"keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: ISM / galaxies: star formation / galaxies: evolution / galaxies: high-redshift"],"volume":648,"abstract":[{"text":"Deep optical spectroscopic surveys of galaxies provide a unique opportunity to investigate rest-frame ultra-violet (UV) emission line properties of galaxies at z ∼ 2 − 4.5. Here we combine VLT/MUSE Guaranteed Time Observations of the Hubble Deep Field South, Ultra Deep Field, COSMOS, and several quasar fields with other publicly available data from VLT/VIMOS and VLT/FORS2 to construct a catalogue of He II λ1640 emitters at z ≳ 2. The deepest areas of our MUSE pointings reach a 3σ line flux limit of 3.1 × 10−19 erg s−1 cm−2. After discarding broad-line active galactic nuclei, we find 13 He II λ1640 detections from MUSE with a median MUV = −20.1 and 21 tentative He II λ1640 detections from other public surveys. Excluding Lyα, all except two galaxies in our sample show at least one other rest-UV emission line, with C III] λ1907, λ1909 being the most prominent. We use multi-wavelength data available in the Hubble legacy fields to derive basic galaxy properties of our sample through spectral energy distribution fitting techniques. Taking advantage of the high-quality spectra obtained by MUSE (∼10 − 30 h of exposure time per pointing), we use photo-ionisation models to study the rest-UV emission line diagnostics of the He II λ1640 emitters. Line ratios of our sample can be reproduced by moderately sub-solar photo-ionisation models, however, we find that including effects of binary stars lead to degeneracies in most free parameters. Even after considering extra ionising photons produced by extreme sub-solar metallicity binary stellar models, photo-ionisation models are unable to reproduce rest-frame He II λ1640 equivalent widths (∼0.2 − 10 Å), thus additional mechanisms are necessary in models to match the observed He II λ1640 properties.","lang":"eng"}],"day":"16","date_created":"2022-07-06T09:07:06Z","extern":"1","scopus_import":"1","quality_controlled":"1","author":[{"first_name":"Themiya","full_name":"Nanayakkara, Themiya","last_name":"Nanayakkara"},{"first_name":"Jarle","full_name":"Brinchmann, Jarle","last_name":"Brinchmann"},{"first_name":"Leindert","full_name":"Boogaard, Leindert","last_name":"Boogaard"},{"last_name":"Bouwens","first_name":"Rychard","full_name":"Bouwens, Rychard"},{"last_name":"Cantalupo","first_name":"Sebastiano","full_name":"Cantalupo, Sebastiano"},{"last_name":"Feltre","first_name":"Anna","full_name":"Feltre, Anna"},{"first_name":"Wolfram","full_name":"Kollatschny, Wolfram","last_name":"Kollatschny"},{"full_name":"Marino, Raffaella Anna","first_name":"Raffaella Anna","last_name":"Marino"},{"last_name":"Maseda","first_name":"Michael","full_name":"Maseda, Michael"},{"orcid":"0000-0003-2871-127X","last_name":"Matthee","full_name":"Matthee, Jorryt J","first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"last_name":"Paalvast","first_name":"Mieke","full_name":"Paalvast, Mieke"},{"last_name":"Richard","first_name":"Johan","full_name":"Richard, Johan"},{"full_name":"Verhamme, Anne","first_name":"Anne","last_name":"Verhamme"}],"doi":"10.1051/0004-6361/201834565","_id":"11499","type":"journal_article","publication":"Astronomy & Astrophysics","acknowledgement":"The authors wish to thank the referee for constructive comments that improved the paper substantially. We thank the BPASS team for making the stellar population models available. We thank Elizabeth Stanway, Claus Leitherer, Daniel Schaerer, Jorick Vink, and Nell Byler for insightful discussions. We thank the Lorentz Centre and the scientific organizers of the Characterizing galaxies with spectroscopy with a view for JWST workshop held at the Lorentz Centre in 2017 October, which promoted useful discussions in the wider community. TN, JB, and RB acknowledges the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) top grant TOP1.16.057. AF acknowledges support from the ERC via an Advanced Grant under grant agreement no. 339659-MUSICOS. JB acknowledges support by Fundação para a Ciência e a Tecnologia (FCT) through national funds (UID/FIS/04434/2013) and Investigador FCT contract IF/01654/2014/CP1215/CT0003, and by FEDER through COMPETE2020 (POCI-01-0145-FEDER-007672). JR acknowledges support from the ERC Starting grant 336736 (CALENDS). This research made use of astropy (http://www.astropy.org) a community-developed core Python package for Astronomy (Astropy Collaboration 2013, 2018) and pandas (McKinney 2010). Figures were generated using matplotlib (Hunter 2007) and seaborn (https://seaborn.pydata.org). Facilities: VLT (MUSE).","citation":{"chicago":"Nanayakkara, Themiya, Jarle Brinchmann, Leindert Boogaard, Rychard Bouwens, Sebastiano Cantalupo, Anna Feltre, Wolfram Kollatschny, et al. “Exploring He II Λ1640 Emission Line Properties at z ∼2−4.” Astronomy & Astrophysics. EDP Sciences, 2019. https://doi.org/10.1051/0004-6361/201834565.","short":"T. Nanayakkara, J. Brinchmann, L. Boogaard, R. Bouwens, S. Cantalupo, A. Feltre, W. Kollatschny, R.A. Marino, M. Maseda, J.J. Matthee, M. Paalvast, J. Richard, A. Verhamme, Astronomy & Astrophysics 648 (2019).","ista":"Nanayakkara T, Brinchmann J, Boogaard L, Bouwens R, Cantalupo S, Feltre A, Kollatschny W, Marino RA, Maseda M, Matthee JJ, Paalvast M, Richard J, Verhamme A. 2019. Exploring He II λ1640 emission line properties at z ∼2−4. Astronomy & Astrophysics. 648, A89.","apa":"Nanayakkara, T., Brinchmann, J., Boogaard, L., Bouwens, R., Cantalupo, S., Feltre, A., … Verhamme, A. (2019). Exploring He II λ1640 emission line properties at z ∼2−4. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/201834565","ama":"Nanayakkara T, Brinchmann J, Boogaard L, et al. Exploring He II λ1640 emission line properties at z ∼2−4. Astronomy & Astrophysics. 2019;648. doi:10.1051/0004-6361/201834565","mla":"Nanayakkara, Themiya, et al. “Exploring He II Λ1640 Emission Line Properties at z ∼2−4.” Astronomy & Astrophysics, vol. 648, A89, EDP Sciences, 2019, doi:10.1051/0004-6361/201834565.","ieee":"T. Nanayakkara et al., “Exploring He II λ1640 emission line properties at z ∼2−4,” Astronomy & Astrophysics, vol. 648. EDP Sciences, 2019."},"external_id":{"arxiv":["1902.05960"]},"arxiv":1,"intvolume":" 648","oa":1,"article_processing_charge":"No","article_number":"A89","date_published":"2019-04-16T00:00:00Z","article_type":"original","month":"04","date_updated":"2022-07-19T09:36:08Z","publication_status":"published","publisher":"EDP Sciences","status":"public","year":"2019","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Published Version"},{"year":"2019","status":"public","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"oa_version":"Published Version","oa":1,"article_number":"A3","article_processing_charge":"No","publication_status":"published","date_updated":"2022-07-19T09:36:31Z","article_type":"original","month":"07","date_published":"2019-07-25T00:00:00Z","publisher":"EDP Sciences","author":[{"last_name":"de La Vieuville","full_name":"de La Vieuville, G.","first_name":"G."},{"last_name":"Bina","first_name":"D.","full_name":"Bina, D."},{"last_name":"Pello","full_name":"Pello, R.","first_name":"R."},{"first_name":"G.","full_name":"Mahler, G.","last_name":"Mahler"},{"last_name":"Richard","full_name":"Richard, J.","first_name":"J."},{"last_name":"Drake","first_name":"A. B.","full_name":"Drake, A. B."},{"last_name":"Herenz","full_name":"Herenz, E. C.","first_name":"E. C."},{"first_name":"F. E.","full_name":"Bauer, F. E.","last_name":"Bauer"},{"last_name":"Clément","full_name":"Clément, B.","first_name":"B."},{"full_name":"Lagattuta, D.","first_name":"D.","last_name":"Lagattuta"},{"full_name":"Laporte, N.","first_name":"N.","last_name":"Laporte"},{"first_name":"J.","full_name":"Martinez, J.","last_name":"Martinez"},{"last_name":"Patrício","first_name":"V.","full_name":"Patrício, V."},{"last_name":"Wisotzki","full_name":"Wisotzki, L.","first_name":"L."},{"last_name":"Zabl","first_name":"J.","full_name":"Zabl, J."},{"first_name":"R. J.","full_name":"Bouwens, R. J.","last_name":"Bouwens"},{"first_name":"T.","full_name":"Contini, T.","last_name":"Contini"},{"last_name":"Garel","full_name":"Garel, T.","first_name":"T."},{"full_name":"Guiderdoni, B.","first_name":"B.","last_name":"Guiderdoni"},{"last_name":"Marino","first_name":"R. A.","full_name":"Marino, R. A."},{"full_name":"Maseda, M. V.","first_name":"M. V.","last_name":"Maseda"},{"orcid":"0000-0003-2871-127X","last_name":"Matthee","first_name":"Jorryt J","full_name":"Matthee, Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"full_name":"Schaye, J.","first_name":"J.","last_name":"Schaye"},{"last_name":"Soucail","full_name":"Soucail, G.","first_name":"G."}],"quality_controlled":"1","_id":"11505","doi":"10.1051/0004-6361/201834471","publication":"Astronomy & Astrophysics","type":"journal_article","intvolume":" 628","arxiv":1,"external_id":{"arxiv":["1905.13696"]},"acknowledgement":"We thank the anonymous referee for their critical review and useful suggestions. This work has been carried out thanks to the support of the OCEVU Labex (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02) funded by the “Investissements d’Avenir” French government programme managed by the ANR. Partially funded by the ERC starting grant CALENDS (JR, VP, BC, JM), the Agence Nationale de la recherche bearing the reference ANR-13-BS05-0010-02 (FOGHAR), and the “Programme National de Cosmologie and Galaxies” (PNCG) of CNRS/INSU, France. GdV, RP, JR, GM, JM, BC, and VP also acknowledge support by the Programa de Cooperacion Cientifica – ECOS SUD Program C16U02. NL acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 669253), ABD acknowledges support from the ERC advanced grant “Cosmic Gas”. LW acknowledges support by the Competitive Fund of the Leibniz Association through grant SAW-2015-AIP-2, and TG acknowledges support from the European Research Council under grant agreement ERC-stg-757258 (TRIPLE).. Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme IDs 060.A-9345, 094.A-0115, 095.A-0181, 096.A-0710, 097.A0269, 100.A-0249, and 294.A-5032. Also based on observations obtained with the NASA/ESA Hubble Space Telescope, retrieved from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute (STScI). STScI is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5-26555. This research made use of Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration 2013). All plots in this paper were created using Matplotlib (Hunter 2007).","citation":{"ista":"de La Vieuville G, Bina D, Pello R, Mahler G, Richard J, Drake AB, Herenz EC, Bauer FE, Clément B, Lagattuta D, Laporte N, Martinez J, Patrício V, Wisotzki L, Zabl J, Bouwens RJ, Contini T, Garel T, Guiderdoni B, Marino RA, Maseda MV, Matthee JJ, Schaye J, Soucail G. 2019. Faint end of the z ∼ 3–7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE. Astronomy & Astrophysics. 628, A3.","short":"G. de La Vieuville, D. Bina, R. Pello, G. Mahler, J. Richard, A.B. Drake, E.C. Herenz, F.E. Bauer, B. Clément, D. Lagattuta, N. Laporte, J. Martinez, V. Patrício, L. Wisotzki, J. Zabl, R.J. Bouwens, T. Contini, T. Garel, B. Guiderdoni, R.A. Marino, M.V. Maseda, J.J. Matthee, J. Schaye, G. Soucail, Astronomy & Astrophysics 628 (2019).","chicago":"La Vieuville, G. de, D. Bina, R. Pello, G. Mahler, J. Richard, A. B. Drake, E. C. Herenz, et al. “Faint End of the z ∼ 3–7 Luminosity Function of Lyman-Alpha Emitters behind Lensing Clusters Observed with MUSE.” Astronomy & Astrophysics. EDP Sciences, 2019. https://doi.org/10.1051/0004-6361/201834471.","ieee":"G. de La Vieuville et al., “Faint end of the z ∼ 3–7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE,” Astronomy & Astrophysics, vol. 628. EDP Sciences, 2019.","mla":"de La Vieuville, G., et al. “Faint End of the z ∼ 3–7 Luminosity Function of Lyman-Alpha Emitters behind Lensing Clusters Observed with MUSE.” Astronomy & Astrophysics, vol. 628, A3, EDP Sciences, 2019, doi:10.1051/0004-6361/201834471.","ama":"de La Vieuville G, Bina D, Pello R, et al. Faint end of the z ∼ 3–7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE. Astronomy & Astrophysics. 2019;628. doi:10.1051/0004-6361/201834471","apa":"de La Vieuville, G., Bina, D., Pello, R., Mahler, G., Richard, J., Drake, A. B., … Soucail, G. (2019). Faint end of the z ∼ 3–7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/201834471"},"volume":628,"keyword":["Space and Planetary Science","Astronomy and Astrophysics","gravitational lensing: strong / galaxies: high-redshift / dark ages","reionization","first stars / galaxies: clusters: general / galaxies: luminosity function","mass function"],"language":[{"iso":"eng"}],"main_file_link":[{"url":"https://arxiv.org/abs/1905.13696","open_access":"1"}],"title":"Faint end of the z ∼ 3–7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE","date_created":"2022-07-06T10:09:36Z","day":"25","abstract":[{"lang":"eng","text":"Contact. This paper presents the results obtained with the Multi-Unit Spectroscopic Explorer (MUSE) at the ESO Very Large Telescope on the faint end of the Lyman-alpha luminosity function (LF) based on deep observations of four lensing clusters. The goal of our project is to set strong constraints on the relative contribution of the Lyman-alpha emitter (LAE) population to cosmic reionization.\r\n\r\nAims. The precise aim of the present study is to further constrain the abundance of LAEs by taking advantage of the magnification provided by lensing clusters to build a blindly selected sample of galaxies which is less biased than current blank field samples in redshift and luminosity. By construction, this sample of LAEs is complementary to those built from deep blank fields, whether observed by MUSE or by other facilities, and makes it possible to determine the shape of the LF at fainter levels, as well as its evolution with redshift.\r\n\r\nMethods. We selected a sample of 156 LAEs with redshifts between 2.9 ≤ z ≤ 6.7 and magnification-corrected luminosities in the range 39 ≲ log LLyα [erg s−1] ≲43. To properly take into account the individual differences in detection conditions between the LAEs when computing the LF, including lensing configurations, and spatial and spectral morphologies, the non-parametric 1/Vmax method was adopted. The price to pay to benefit from magnification is a reduction of the effective volume of the survey, together with a more complex analysis procedure to properly determine the effective volume Vmax for each galaxy. In this paper we present a complete procedure for the determination of the LF based on IFU detections in lensing clusters. This procedure, including some new methods for masking, effective volume integration and (individual) completeness determinations, has been fully automated when possible, and it can be easily generalized to the analysis of IFU observations in blank fields.\r\n\r\nResults. As a result of this analysis, the Lyman-alpha LF has been obtained in four different redshift bins: 2.9 < z < 6, 7, 2.9 < z < 4.0, 4.0 < z < 5.0, and 5.0 < z < 6.7 with constraints down to log LLyα = 40.5. From our data only, no significant evolution of LF mean slope can be found. When performing a Schechter analysis also including data from the literature to complete the present sample towards the brightest luminosities, a steep faint end slope was measured varying from α = −1.69−0.08+0.08 to α = −1.87−0.12+0.12 between the lowest and the highest redshift bins.\r\n\r\nConclusions. The contribution of the LAE population to the star formation rate density at z ∼ 6 is ≲50% depending on the luminosity limit considered, which is of the same order as the Lyman-break galaxy (LBG) contribution. The evolution of the LAE contribution with redshift depends on the assumed escape fraction of Lyman-alpha photons, and appears to slightly increase with increasing redshift when this fraction is conservatively set to one. Depending on the intersection between the LAE/LBG populations, the contribution of the observed galaxies to the ionizing flux may suffice to keep the universe ionized at z ∼ 6."}],"scopus_import":"1","extern":"1"},{"quality_controlled":"1","author":[{"full_name":"Sobral, David","first_name":"David","last_name":"Sobral"},{"orcid":"0000-0003-2871-127X","last_name":"Matthee","full_name":"Matthee, Jorryt J","first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720"}],"_id":"11507","doi":"10.1051/0004-6361/201833075","type":"journal_article","publication":"Astronomy & Astrophysics","external_id":{"arxiv":["1803.08923"]},"citation":{"mla":"Sobral, David, and Jorryt J. Matthee. “Predicting Lyα Escape Fractions with a Simple Observable: Lyα in Emission as an Empirically Calibrated Star Formation Rate Indicator.” Astronomy & Astrophysics, vol. 623, A157, EDP Sciences, 2019, doi:10.1051/0004-6361/201833075.","ieee":"D. Sobral and J. J. Matthee, “Predicting Lyα escape fractions with a simple observable: Lyα in emission as an empirically calibrated star formation rate indicator,” Astronomy & Astrophysics, vol. 623. EDP Sciences, 2019.","ama":"Sobral D, Matthee JJ. Predicting Lyα escape fractions with a simple observable: Lyα in emission as an empirically calibrated star formation rate indicator. Astronomy & Astrophysics. 2019;623. doi:10.1051/0004-6361/201833075","apa":"Sobral, D., & Matthee, J. J. (2019). Predicting Lyα escape fractions with a simple observable: Lyα in emission as an empirically calibrated star formation rate indicator. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/201833075","ista":"Sobral D, Matthee JJ. 2019. Predicting Lyα escape fractions with a simple observable: Lyα in emission as an empirically calibrated star formation rate indicator. Astronomy & Astrophysics. 623, A157.","short":"D. Sobral, J.J. Matthee, Astronomy & Astrophysics 623 (2019).","chicago":"Sobral, David, and Jorryt J Matthee. “Predicting Lyα Escape Fractions with a Simple Observable: Lyα in Emission as an Empirically Calibrated Star Formation Rate Indicator.” Astronomy & Astrophysics. EDP Sciences, 2019. https://doi.org/10.1051/0004-6361/201833075."},"acknowledgement":"We thank the anonymous referees for multiple comments and suggestions which have improved the manuscript. JM acknowledges the support of a Huygens PhD fellowship from Leiden University. We have benefited greatly from the publicly available programming language PYTHON, including the NUMPY & SCIPY (Van Der Walt et al. 2011; Jones et al. 2001), MATPLOTLIB (Hunter 2007) and ASTROPY (Astropy Collaboration 2013) packages, and the TOPCAT analysis program (Taylor 2013). The results and samples of LAEs used for this paper are publicly available (see e.g. Sobral et al. 2017, 2018a) and we also provide the toy model used as a PYTHON script.","intvolume":" 623","arxiv":1,"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1803.08923"}],"language":[{"iso":"eng"}],"title":"Predicting Lyα escape fractions with a simple observable: Lyα in emission as an empirically calibrated star formation rate indicator","volume":623,"keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: high-redshift / galaxies: star formation / galaxies: statistics / galaxies: evolution / galaxies: formation / galaxies: ISM"],"date_created":"2022-07-06T11:08:16Z","day":"26","abstract":[{"lang":"eng","text":"Lyman-α (Lyα) is intrinsically the brightest line emitted from active galaxies. While it originates from many physical processes, for star-forming galaxies the intrinsic Lyα luminosity is a direct tracer of the Lyman-continuum (LyC) radiation produced by the most massive O- and early-type B-stars (M⋆ ≳ 10 M⊙) with lifetimes of a few Myrs. As such, Lyα luminosity should be an excellent instantaneous star formation rate (SFR) indicator. However, its resonant nature and susceptibility to dust as a rest-frame UV photon makes Lyα very hard to interpret due to the uncertain Lyα escape fraction, fesc, Lyα. Here we explore results from the CAlibrating LYMan-α with Hα (CALYMHA) survey at z = 2.2, follow-up of Lyα emitters (LAEs) at z = 2.2 − 2.6 and a z ∼ 0−0.3 compilation of LAEs to directly measure fesc, Lyα with Hα. We derive a simple empirical relation that robustly retrieves fesc, Lyα as a function of Lyα rest-frame EW (EW0): fesc,Lyα = 0.0048 EW0[Å] ± 0.05 and we show that it constrains a well-defined anti-correlation between ionisation efficiency (ξion) and dust extinction in LAEs. Observed Lyα luminosities and EW0 are easy measurable quantities at high redshift, thus making our relation a practical tool to estimate intrinsic Lyα and LyC luminosities under well controlled and simple assumptions. Our results allow observed Lyα luminosities to be used to compute SFRs for LAEs at z ∼ 0−2.6 within ±0.2 dex of the Hα dust corrected SFRs. We apply our empirical SFR(Lyα,EW0) calibration to several sources at z ≥ 2.6 to find that star-forming LAEs have SFRs typically ranging from 0.1 to 20 M⊙ yr−1 and that our calibration might be even applicable for the most luminous LAEs within the epoch of re-ionisation. Our results imply high ionisation efficiencies (log10[ξion/Hz erg−1] = 25.4−25.6) and low dust content in LAEs across cosmic time, and will be easily tested with future observations with JWST which can obtain Hα and Hβ measurements for high-redshift LAEs."}],"scopus_import":"1","extern":"1","status":"public","year":"2019","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Published Version","oa":1,"article_processing_charge":"No","article_number":"A157","date_updated":"2022-07-19T09:37:20Z","publication_status":"published","date_published":"2019-03-26T00:00:00Z","month":"03","article_type":"original","publisher":"EDP Sciences"},{"external_id":{"arxiv":["1903.09167"]},"citation":{"ista":"Boogaard LA, Decarli R, González-López J, van der Werf P, Walter F, Bouwens R, Aravena M, Carilli C, Bauer FE, Brinchmann J, Contini T, Cox P, da Cunha E, Daddi E, Díaz-Santos T, Hodge J, Inami H, Ivison R, Maseda M, Matthee JJ, Oesch P, Popping G, Riechers D, Schaye J, Schouws S, Smail I, Weiss A, Wisotzki L, Bacon R, Cortes PC, Rix H-W, Somerville RS, Swinbank M, Wagg J. 2019. The ALMA spectroscopic survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy. The Astrophysical Journal. 882(2), 140.","short":"L.A. Boogaard, R. Decarli, J. González-López, P. van der Werf, F. Walter, R. Bouwens, M. Aravena, C. Carilli, F.E. Bauer, J. Brinchmann, T. Contini, P. Cox, E. da Cunha, E. Daddi, T. Díaz-Santos, J. Hodge, H. Inami, R. Ivison, M. Maseda, J.J. Matthee, P. Oesch, G. Popping, D. Riechers, J. Schaye, S. Schouws, I. Smail, A. Weiss, L. Wisotzki, R. Bacon, P.C. Cortes, H.-W. Rix, R.S. Somerville, M. Swinbank, J. Wagg, The Astrophysical Journal 882 (2019).","chicago":"Boogaard, Leindert A., Roberto Decarli, Jorge González-López, Paul van der Werf, Fabian Walter, Rychard Bouwens, Manuel Aravena, et al. “The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-Mass Selected Galaxies Using MUSE Spectroscopy.” The Astrophysical Journal. IOP Publishing, 2019. https://doi.org/10.3847/1538-4357/ab3102.","ieee":"L. A. Boogaard et al., “The ALMA spectroscopic survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy,” The Astrophysical Journal, vol. 882, no. 2. IOP Publishing, 2019.","mla":"Boogaard, Leindert A., et al. “The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-Mass Selected Galaxies Using MUSE Spectroscopy.” The Astrophysical Journal, vol. 882, no. 2, 140, IOP Publishing, 2019, doi:10.3847/1538-4357/ab3102.","ama":"Boogaard LA, Decarli R, González-López J, et al. The ALMA spectroscopic survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy. The Astrophysical Journal. 2019;882(2). doi:10.3847/1538-4357/ab3102","apa":"Boogaard, L. A., Decarli, R., González-López, J., van der Werf, P., Walter, F., Bouwens, R., … Wagg, J. (2019). The ALMA spectroscopic survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ab3102"},"acknowledgement":"We are grateful to the referee for providing a constructive report. L.A.B. wants to thank Madusha L.P. Gunawardhana for her help with platefit. Based on observations collected at the European Southern Observatory under ESO programme(s): 094.A-2089(B), 095.A-0010(A), 096.A-0045(A), and 096.A-0045(B). This paper makes use of the following ALMA data: ADS/JAO.ALMA#2016.1.00324.L. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.\r\n\r\n\"Este trabajo contó con el apoyo de CONICYT+Programa de Astronomía+ Fondo CHINA-CONICYT\" J.G-L. acknowledges partial support from ALMA-CONICYT project 31160033. F.E.B. acknowledges support from CONICYT grant Basal AFB-170002 (FEB), and the Ministry of Economy, Development, and Tourism's Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS (FEB). J.B. acknowledges support by Fundação para a Ciência e a Tecnologia (FCT) through national funds (UID/FIS/04434/2013) and Investigador FCT contract IF/01654/2014/CP1215/CT0003., and by FEDER through COMPETE2020 (POCI-01-0145-FEDER-007672). T.D-S. acknowledges support from ALMA-CONYCIT project 31130005 and FONDECYT project 1151239. J.H. acknowledges support of the VIDI research programme with project number 639.042.611, which is (partly) financed by the Netherlands Organization for Scientific Research (NWO). D.R. acknowledges support from the National Science Foundation under grant No. AST-1614213. I.R.S. acknowledges support from the ERC Advanced Grant DUSTYGAL (321334) and STFC (ST/P000541/1)\r\n\r\nWork on Gnuastro has been funded by the Japanese MEXT scholarship and its Grant-in-Aid for Scientific Research (21244012, 24253003), the ERC advanced grant 339659-MUSICOS, European Union's Horizon 2020 research and innovation programme under Marie Sklodowska-Curie grant agreement No. 721463 to the SUNDIAL ITN, and from the Spanish MINECO under grant No. AYA2016-76219-P.","intvolume":" 882","arxiv":1,"type":"journal_article","publication":"The Astrophysical Journal","_id":"11514","doi":"10.3847/1538-4357/ab3102","quality_controlled":"1","author":[{"full_name":"Boogaard, Leindert A.","first_name":"Leindert A.","last_name":"Boogaard"},{"last_name":"Decarli","first_name":"Roberto","full_name":"Decarli, Roberto"},{"last_name":"González-López","full_name":"González-López, Jorge","first_name":"Jorge"},{"last_name":"van der Werf","full_name":"van der Werf, Paul","first_name":"Paul"},{"first_name":"Fabian","full_name":"Walter, Fabian","last_name":"Walter"},{"last_name":"Bouwens","first_name":"Rychard","full_name":"Bouwens, Rychard"},{"last_name":"Aravena","first_name":"Manuel","full_name":"Aravena, Manuel"},{"last_name":"Carilli","full_name":"Carilli, Chris","first_name":"Chris"},{"full_name":"Bauer, Franz Erik","first_name":"Franz Erik","last_name":"Bauer"},{"last_name":"Brinchmann","first_name":"Jarle","full_name":"Brinchmann, Jarle"},{"first_name":"Thierry","full_name":"Contini, Thierry","last_name":"Contini"},{"last_name":"Cox","first_name":"Pierre","full_name":"Cox, Pierre"},{"full_name":"da Cunha, Elisabete","first_name":"Elisabete","last_name":"da Cunha"},{"full_name":"Daddi, Emanuele","first_name":"Emanuele","last_name":"Daddi"},{"full_name":"Díaz-Santos, Tanio","first_name":"Tanio","last_name":"Díaz-Santos"},{"last_name":"Hodge","full_name":"Hodge, Jacqueline","first_name":"Jacqueline"},{"first_name":"Hanae","full_name":"Inami, Hanae","last_name":"Inami"},{"last_name":"Ivison","full_name":"Ivison, Rob","first_name":"Rob"},{"full_name":"Maseda, Michael","first_name":"Michael","last_name":"Maseda"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","full_name":"Matthee, Jorryt J","first_name":"Jorryt J","last_name":"Matthee","orcid":"0000-0003-2871-127X"},{"last_name":"Oesch","first_name":"Pascal","full_name":"Oesch, Pascal"},{"last_name":"Popping","first_name":"Gergö","full_name":"Popping, Gergö"},{"first_name":"Dominik","full_name":"Riechers, Dominik","last_name":"Riechers"},{"full_name":"Schaye, Joop","first_name":"Joop","last_name":"Schaye"},{"last_name":"Schouws","first_name":"Sander","full_name":"Schouws, Sander"},{"last_name":"Smail","full_name":"Smail, Ian","first_name":"Ian"},{"last_name":"Weiss","full_name":"Weiss, Axel","first_name":"Axel"},{"first_name":"Lutz","full_name":"Wisotzki, Lutz","last_name":"Wisotzki"},{"last_name":"Bacon","full_name":"Bacon, Roland","first_name":"Roland"},{"first_name":"Paulo C.","full_name":"Cortes, Paulo C.","last_name":"Cortes"},{"first_name":"Hans-Walter","full_name":"Rix, Hans-Walter","last_name":"Rix"},{"last_name":"Somerville","full_name":"Somerville, Rachel S.","first_name":"Rachel S."},{"last_name":"Swinbank","first_name":"Mark","full_name":"Swinbank, Mark"},{"full_name":"Wagg, Jeff","first_name":"Jeff","last_name":"Wagg"}],"extern":"1","scopus_import":"1","date_created":"2022-07-06T13:31:35Z","day":"11","abstract":[{"text":"We discuss the nature and physical properties of gas-mass selected galaxies in the ALMA spectroscopic survey (ASPECS) of the Hubble Ultra Deep Field (HUDF). We capitalize on the deep optical integral-field spectroscopy from the Multi Unit Spectroscopic Explorer (MUSE) HUDF Survey and multiwavelength data to uniquely associate all 16 line emitters, detected in the ALMA data without preselection, with rotational transitions of carbon monoxide (CO). We identify 10 as CO(2–1) at 1 < z < 2, 5 as CO(3–2) at 2 < z < 3, and 1 as CO(4–3) at z = 3.6. Using the MUSE data as a prior, we identify two additional CO(2–1) emitters, increasing the total sample size to 18. We infer metallicities consistent with (super-)solar for the CO-detected galaxies at z ≤ 1.5, motivating our choice of a Galactic conversion factor between CO luminosity and molecular gas mass for these galaxies. Using deep Chandra imaging of the HUDF, we determine an X-ray AGN fraction of 20% and 60% among the CO emitters at z ∼ 1.4 and z ∼ 2.6, respectively. Being a CO-flux-limited survey, ASPECS-LP detects molecular gas in galaxies on, above, and below the main sequence (MS) at z ∼ 1.4. For stellar masses ≥1010 (1010.5) ${M}_{\\odot }$, we detect about 40% (50%) of all galaxies in the HUDF at 1 < z < 2 (2 < z < 3). The combination of ALMA and MUSE integral-field spectroscopy thus enables an unprecedented view of MS galaxies during the peak of galaxy formation.","lang":"eng"}],"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1903.09167"}],"language":[{"iso":"eng"}],"title":"The ALMA spectroscopic survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"volume":882,"oa_version":"Preprint","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","issue":"2","status":"public","year":"2019","publisher":"IOP Publishing","date_updated":"2022-07-19T09:50:55Z","publication_status":"published","month":"09","date_published":"2019-09-11T00:00:00Z","article_type":"original","article_processing_charge":"No","article_number":"140","oa":1},{"publisher":"IOP Publishing","date_updated":"2024-10-14T11:32:02Z","publication_status":"published","article_type":"original","date_published":"2019-08-21T00:00:00Z","month":"08","article_number":"124","article_processing_charge":"No","oa":1,"oa_version":"Preprint","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"year":"2019","status":"public","issue":"2","extern":"1","scopus_import":"1","date_created":"2022-07-06T13:38:15Z","abstract":[{"lang":"eng","text":"We present new deep ALMA and Hubble Space Telescope (HST)/WFC3 observations of MASOSA and VR7, two luminous Lyα emitters (LAEs) at z = 6.5, for which the UV continuum levels differ by a factor of four. No IR dust continuum emission is detected in either, indicating little amounts of obscured star formation and/or high dust temperatures. MASOSA, with a UV luminosity M1500 = −20.9, compact size, and very high Lyα ${\\mathrm{EW}}_{0}\\approx 145\\,\\mathring{\\rm A} $, is undetected in [C ii] to a limit of L[C ii] < 2.2 × 107 L⊙, implying a metallicity Z ≲ 0.07 Z⊙. Intriguingly, our HST data indicate a red UV slope β = −1.1 ± 0.7, at odds with the low dust content. VR7, which is a bright (M1500 = −22.4) galaxy with moderate color (β = −1.4 ± 0.3) and Lyα EW0 = 34 Å, is clearly detected in [C ii] emission (S/N = 15). VR7's rest-frame UV morphology can be described by two components separated by ≈1.5 kpc and is globally more compact than the [C ii] emission. The global [C ii]/UV ratio indicates Z ≈ 0.2 Z⊙, but there are large variations in the UV/[C ii] ratio on kiloparsec scales. We also identify diffuse, possibly outflowing, [C ii]-emitting gas at ≈100 km s−1 with respect to the peak. VR7 appears to be assembling its components at a slightly more evolved stage than other luminous LAEs, with outflows already shaping its direct environment at z ∼ 7. Our results further indicate that the global [C ii]−UV relation steepens at SFR < 30 M⊙ yr−1, naturally explaining why the [C ii]/UV ratio is anticorrelated with Lyα EW in many, but not all, observed LAEs."}],"day":"21","volume":881,"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1903.08171"}],"language":[{"iso":"eng"}],"title":"Resolved UV and [C ii] structures of luminous galaxies within the epoch of reionization","intvolume":" 881","arxiv":1,"external_id":{"arxiv":["1903.08171"]},"acknowledgement":"We thank the anonymous referee for constructive comments and suggestions. We thank Max Gronke for comments on an earlier version of this paper. L.V. acknowledges funding from the European Union’s Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement No. 746119. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2017.1.01451.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. Based on observations obtained with the Very Large Telescope, programs 294.A-5018, 097.A-0943, and 99.A-0462. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained (from the Data Archive) at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program No. 14699.","citation":{"mla":"Matthee, Jorryt J., et al. “Resolved UV and [C Ii] Structures of Luminous Galaxies within the Epoch of Reionization.” The Astrophysical Journal, vol. 881, no. 2, 124, IOP Publishing, 2019, doi:10.3847/1538-4357/ab2f81.","ieee":"J. J. Matthee et al., “Resolved UV and [C ii] structures of luminous galaxies within the epoch of reionization,” The Astrophysical Journal, vol. 881, no. 2. IOP Publishing, 2019.","apa":"Matthee, J. J., Sobral, D., Boogaard, L. A., Röttgering, H., Vallini, L., Ferrara, A., … Mobasher, B. (2019). Resolved UV and [C ii] structures of luminous galaxies within the epoch of reionization. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ab2f81","ama":"Matthee JJ, Sobral D, Boogaard LA, et al. Resolved UV and [C ii] structures of luminous galaxies within the epoch of reionization. The Astrophysical Journal. 2019;881(2). doi:10.3847/1538-4357/ab2f81","ista":"Matthee JJ, Sobral D, Boogaard LA, Röttgering H, Vallini L, Ferrara A, Paulino-Afonso A, Boone F, Schaerer D, Mobasher B. 2019. Resolved UV and [C ii] structures of luminous galaxies within the epoch of reionization. The Astrophysical Journal. 881(2), 124.","chicago":"Matthee, Jorryt J, D. Sobral, L. A. Boogaard, H. Röttgering, L. Vallini, A. Ferrara, A. Paulino-Afonso, F. Boone, D. Schaerer, and B. Mobasher. “Resolved UV and [C Ii] Structures of Luminous Galaxies within the Epoch of Reionization.” The Astrophysical Journal. IOP Publishing, 2019. https://doi.org/10.3847/1538-4357/ab2f81.","short":"J.J. Matthee, D. Sobral, L.A. Boogaard, H. Röttgering, L. Vallini, A. Ferrara, A. Paulino-Afonso, F. Boone, D. Schaerer, B. Mobasher, The Astrophysical Journal 881 (2019)."},"type":"journal_article","publication":"The Astrophysical Journal","_id":"11515","doi":"10.3847/1538-4357/ab2f81","author":[{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","full_name":"Matthee, Jorryt J","first_name":"Jorryt J","last_name":"Matthee","orcid":"0000-0003-2871-127X"},{"last_name":"Sobral","first_name":"D.","full_name":"Sobral, D."},{"full_name":"Boogaard, L. A.","first_name":"L. A.","last_name":"Boogaard"},{"first_name":"H.","full_name":"Röttgering, H.","last_name":"Röttgering"},{"first_name":"L.","full_name":"Vallini, L.","last_name":"Vallini"},{"full_name":"Ferrara, A.","first_name":"A.","last_name":"Ferrara"},{"full_name":"Paulino-Afonso, A.","first_name":"A.","last_name":"Paulino-Afonso"},{"full_name":"Boone, F.","first_name":"F.","last_name":"Boone"},{"full_name":"Schaerer, D.","first_name":"D.","last_name":"Schaerer"},{"last_name":"Mobasher","full_name":"Mobasher, B.","first_name":"B."}],"quality_controlled":"1"},{"extern":"1","scopus_import":"1","volume":880,"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"title":"A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE","language":[{"iso":"eng"}],"main_file_link":[{"url":"https://arxiv.org/abs/1906.06347","open_access":"1"}],"day":"24","abstract":[{"lang":"eng","text":"The well-known quasar SDSS J095253.83+011421.9 (J0952+0114) at z = 3.02 has one of the most peculiar spectra discovered so far, showing the presence of narrow Lyα and broad metal emission lines. Although recent studies have suggested that a proximate damped Lyα absorption (PDLA) system causes this peculiar spectrum, the origin of the gas associated with the PDLA is unknown. Here we report the results of observations with the Multi Unit Spectroscopic Explorer (MUSE) that reveal a new giant (≈100 physical kpc) Lyα nebula. The detailed analysis of the Lyα velocity, velocity dispersion, and surface brightness profiles suggests that the J0952+0114 Lyα nebula shares similar properties with other QSO nebulae previously detected with MUSE, implying that the PDLA in J0952+0144 is covering only a small fraction of the solid angle of the QSO emission. We also detected bright and spectrally narrow C iv λ1550 and He ii λ1640 extended emission around J0952+0114 with velocity centroids similar to the peak of the extended and central narrow Lyα emission. The presence of a peculiarly bright, unresolved, and relatively broad He ii λ1640 emission in the central region at exactly the same PDLA redshift hints at the possibility that the PDLA originates in a clumpy outflow with a bulk velocity of about 500 km s−1. The smaller velocity dispersion of the large-scale Lyα emission suggests that the high-speed outflow is confined to the central region. Lastly, the derived spatially resolved He ii/Lyα and C iv/Lyα maps show a positive gradient with the distance to the QSO, hinting at a non-homogeneous distribution of the ionization parameter."}],"date_created":"2022-07-06T13:50:33Z","publication":"The Astrophysical Journal","type":"journal_article","arxiv":1,"intvolume":" 880","citation":{"apa":"Marino, R. A., Cantalupo, S., Pezzulli, G., Lilly, S. J., Gallego, S., Mackenzie, R., … Nanayakkara, T. (2019). A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ab2881","ama":"Marino RA, Cantalupo S, Pezzulli G, et al. A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE. The Astrophysical Journal. 2019;880(1). doi:10.3847/1538-4357/ab2881","ieee":"R. A. Marino et al., “A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE,” The Astrophysical Journal, vol. 880, no. 1. IOP Publishing, 2019.","mla":"Marino, Raffaella Anna, et al. “A Giant Lyα Nebula and a Small-Scale Clumpy Outflow in the System of the Exotic Quasar J0952+0114 Unveiled by MUSE.” The Astrophysical Journal, vol. 880, no. 1, 47, IOP Publishing, 2019, doi:10.3847/1538-4357/ab2881.","chicago":"Marino, Raffaella Anna, Sebastiano Cantalupo, Gabriele Pezzulli, Simon J. Lilly, Sofia Gallego, Ruari Mackenzie, Jorryt J Matthee, et al. “A Giant Lyα Nebula and a Small-Scale Clumpy Outflow in the System of the Exotic Quasar J0952+0114 Unveiled by MUSE.” The Astrophysical Journal. IOP Publishing, 2019. https://doi.org/10.3847/1538-4357/ab2881.","short":"R.A. Marino, S. Cantalupo, G. Pezzulli, S.J. Lilly, S. Gallego, R. Mackenzie, J.J. Matthee, J. Brinchmann, N. Bouché, A. Feltre, S. Muzahid, I. Schroetter, S.D. Johnson, T. Nanayakkara, The Astrophysical Journal 880 (2019).","ista":"Marino RA, Cantalupo S, Pezzulli G, Lilly SJ, Gallego S, Mackenzie R, Matthee JJ, Brinchmann J, Bouché N, Feltre A, Muzahid S, Schroetter I, Johnson SD, Nanayakkara T. 2019. A giant Lyα nebula and a small-scale clumpy outflow in the system of the exotic quasar J0952+0114 unveiled by MUSE. The Astrophysical Journal. 880(1), 47."},"acknowledgement":"We thank Lutz Wisotzki for stimulating discussions. This work is based on observations taken at ESO/VLT in Paranal and we would like to thank the ESO staff for their assistance and support during the MUSE GTO campaigns. This work was supported by the Swiss National Science Foundation. This research made use of Astropy, a community-developed core PYTHON package for astronomy (Astropy Collaboration et al. 2013), NumPy and SciPy (Oliphant 2007), Matplotlib (Hunter 2007), IPython (Perez & Granger 2007), and of the NASA Astrophysics Data System Bibliographic Services. S.C. and G.P. gratefully acknowledge support from Swiss National Science Foundation grant PP00P2−163824. A.F. acknowledges support from the ERC via Advanced Grant under grants agreement no. 339659-MUSICOS. J.B. acknowledges support by FCT/MCTES through national funds by grant UID/FIS/04434/2019 and through Investigador FCT Contract No. IF/01654/2014/CP1215/CT0003. S.D.J. is supported by a NASA Hubble Fellowship (HST-HF2-51375.001-A). T.N. acknowledges the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) top grant TOP1.16.057.","external_id":{"arxiv":["1906.06347"]},"author":[{"last_name":"Marino","full_name":"Marino, Raffaella Anna","first_name":"Raffaella Anna"},{"full_name":"Cantalupo, Sebastiano","first_name":"Sebastiano","last_name":"Cantalupo"},{"full_name":"Pezzulli, Gabriele","first_name":"Gabriele","last_name":"Pezzulli"},{"full_name":"Lilly, Simon J.","first_name":"Simon J.","last_name":"Lilly"},{"last_name":"Gallego","first_name":"Sofia","full_name":"Gallego, Sofia"},{"full_name":"Mackenzie, Ruari","first_name":"Ruari","last_name":"Mackenzie"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","first_name":"Jorryt J","full_name":"Matthee, Jorryt J","last_name":"Matthee","orcid":"0000-0003-2871-127X"},{"last_name":"Brinchmann","full_name":"Brinchmann, Jarle","first_name":"Jarle"},{"full_name":"Bouché, Nicolas","first_name":"Nicolas","last_name":"Bouché"},{"first_name":"Anna","full_name":"Feltre, Anna","last_name":"Feltre"},{"last_name":"Muzahid","first_name":"Sowgat","full_name":"Muzahid, Sowgat"},{"last_name":"Schroetter","full_name":"Schroetter, Ilane","first_name":"Ilane"},{"full_name":"Johnson, Sean D.","first_name":"Sean D.","last_name":"Johnson"},{"last_name":"Nanayakkara","first_name":"Themiya","full_name":"Nanayakkara, Themiya"}],"quality_controlled":"1","doi":"10.3847/1538-4357/ab2881","_id":"11516","month":"07","article_type":"original","date_published":"2019-07-24T00:00:00Z","date_updated":"2022-08-18T10:20:18Z","publication_status":"published","publisher":"IOP Publishing","oa":1,"article_number":"47","article_processing_charge":"No","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"oa_version":"Preprint","issue":"1","year":"2019","status":"public"},{"publisher":"IOP Publishing","publication_status":"published","date_updated":"2022-08-18T10:19:08Z","month":"06","article_type":"original","date_published":"2019-06-04T00:00:00Z","article_processing_charge":"No","article_number":"132","oa":1,"oa_version":"Preprint","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","year":"2019","status":"public","issue":"2","extern":"1","scopus_import":"1","date_created":"2022-07-07T08:38:24Z","day":"04","abstract":[{"lang":"eng","text":"To understand star formation in galaxies, we investigate the star formation rate (SFR) surface density (ΣSFR) profiles for galaxies, based on a well-defined sample of 976 star-forming MaNGA galaxies. We find that the typical ΣSFR profiles within 1.5Re of normal SF galaxies can be well described by an exponential function for different stellar mass intervals, while the sSFR profile shows positive gradients, especially for more massive SF galaxies. This is due to the more pronounced central cores or bulges rather than the onset of a `quenching' process. While galaxies that lie significantly above (or below) the star formation main sequence (SFMS) show overall an elevation (or suppression) of ΣSFR at all radii, this central elevation (or suppression) is more pronounced in more massive galaxies. The degree of central enhancement and suppression is quite symmetric, suggesting that both the elevation and suppression of star formation are following the same physical processes. Furthermore, we find that the dispersion in ΣSFR within and across the population is found to be tightly correlated with the inferred gas depletion time, whether based on the stellar surface mass density or the orbital dynamical time. This suggests that we are seeing the response of a simple gas-regulator system to variations in the accretion rate. This is explored using a heuristic model that can quantitatively explain the dependence of σ(ΣSFR) on gas depletion timescale. Variations in accretion rate are progressively more damped out in regions of low star-formation efficiency leading to a reduced amplitude of variations in star-formation."}],"language":[{"iso":"eng"}],"main_file_link":[{"url":"https://arxiv.org/abs/1901.10276","open_access":"1"}],"title":"On the elevation and suppression of star formation within galaxies","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"volume":877,"external_id":{"arxiv":["1901.10276"]},"acknowledgement":"We are grateful to the anonymous referee for their thoughtful and constructive review of the paper and their several suggestions (including the analysis of Section 3.4), which have improved the paper. This research has been supported by the Swiss National Science Foundation.\r\n\r\nFunding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS website is www.sdss.org.\r\n\r\nSDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration, including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofísica de Canarias, the Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatory of China, New Mexico State University, New York University, University of Notre Dame, Observatário Nacional/MCTI, the Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University","citation":{"ama":"Wang E, Lilly SJ, Pezzulli G, Matthee JJ. On the elevation and suppression of star formation within galaxies. The Astrophysical Journal. 2019;877(2). doi:10.3847/1538-4357/ab1c5b","apa":"Wang, E., Lilly, S. J., Pezzulli, G., & Matthee, J. J. (2019). On the elevation and suppression of star formation within galaxies. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ab1c5b","ieee":"E. Wang, S. J. Lilly, G. Pezzulli, and J. J. Matthee, “On the elevation and suppression of star formation within galaxies,” The Astrophysical Journal, vol. 877, no. 2. IOP Publishing, 2019.","mla":"Wang, Enci, et al. “On the Elevation and Suppression of Star Formation within Galaxies.” The Astrophysical Journal, vol. 877, no. 2, 132, IOP Publishing, 2019, doi:10.3847/1538-4357/ab1c5b.","short":"E. Wang, S.J. Lilly, G. Pezzulli, J.J. Matthee, The Astrophysical Journal 877 (2019).","chicago":"Wang, Enci, Simon J. Lilly, Gabriele Pezzulli, and Jorryt J Matthee. “On the Elevation and Suppression of Star Formation within Galaxies.” The Astrophysical Journal. IOP Publishing, 2019. https://doi.org/10.3847/1538-4357/ab1c5b.","ista":"Wang E, Lilly SJ, Pezzulli G, Matthee JJ. 2019. On the elevation and suppression of star formation within galaxies. The Astrophysical Journal. 877(2), 132."},"intvolume":" 877","arxiv":1,"publication":"The Astrophysical Journal","type":"journal_article","_id":"11517","doi":"10.3847/1538-4357/ab1c5b","quality_controlled":"1","author":[{"last_name":"Wang","first_name":"Enci","full_name":"Wang, Enci"},{"last_name":"Lilly","full_name":"Lilly, Simon J.","first_name":"Simon J."},{"first_name":"Gabriele","full_name":"Pezzulli, Gabriele","last_name":"Pezzulli"},{"last_name":"Matthee","orcid":"0000-0003-2871-127X","id":"7439a258-f3c0-11ec-9501-9df22fe06720","first_name":"Jorryt J","full_name":"Matthee, Jorryt J"}]},{"extern":"1","scopus_import":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: evolution","galaxies: haloes","galaxies: high-redshift","galaxies: star formation","cosmology: observations","large-scale structure of Universe"],"volume":489,"title":"The clustering of typical Ly α emitters from z ∼ 2.5–6: Host halo masses depend on Ly α and UV luminosities","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1811.00556"}],"language":[{"iso":"eng"}],"day":"01","abstract":[{"text":"We investigate the clustering and halo properties of ∼5000 Ly α-selected emission-line galaxies (LAEs) from the Slicing COSMOS 4K (SC4K) and from archival NB497 imaging of SA22 split in 15 discrete redshift slices between z ∼ 2.5 and 6. We measure clustering lengths of r0 ∼ 3–6 h−1 Mpc and typical halo masses of ∼1011 M⊙ for our narrowband-selected LAEs with typical LLy α ∼ 1042–43 erg s−1. The intermediate-band-selected LAEs are observed to have r0 ∼ 3.5–15 h−1 Mpc with typical halo masses of ∼1011–12 M⊙ and typical LLy α ∼ 1043–43.6 erg s−1. We find a strong, redshift-independent correlation between halo mass and Ly α luminosity normalized by the characteristic Ly α luminosity, L⋆(z). The faintest LAEs (L ∼ 0.1 L⋆(z)) typically identified by deep narrowband surveys are found in 1010 M⊙ haloes and the brightest LAEs (L ∼ 7 L⋆(z)) are found in ∼5 × 1012 M⊙ haloes. A dependency on the rest-frame 1500 Å UV luminosity, MUV, is also observed where the halo masses increase from 1011 to 1013 M⊙ for MUV ∼ −19 to −23.5 mag. Halo mass is also observed to increase from 109.8 to 1012 M⊙ for dust-corrected UV star formation rates from ∼0.6 to 10 M⊙ yr−1 and continues to increase up to 1013 M⊙ in halo mass, where the majority of those sources are active galactic nuclei. All the trends we observe are found to be redshift independent. Our results reveal that LAEs are the likely progenitors of a wide range of galaxies depending on their luminosity, from dwarf-like, to Milky Way-type, to bright cluster galaxies. LAEs therefore provide unique insight into the early formation and evolution of the galaxies we observe in the local Universe.","lang":"eng"}],"date_created":"2022-07-07T13:01:03Z","type":"journal_article","publication":"Monthly Notices of the Royal Astronomical Society","arxiv":1,"intvolume":" 489","citation":{"apa":"Khostovan, A. A., Sobral, D., Mobasher, B., Matthee, J. J., Cochrane, R. K., Chartab, N., … Calhau, J. (2019). The clustering of typical Ly α emitters from z ∼ 2.5–6: Host halo masses depend on Ly α and UV luminosities. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stz2149","ama":"Khostovan AA, Sobral D, Mobasher B, et al. The clustering of typical Ly α emitters from z ∼ 2.5–6: Host halo masses depend on Ly α and UV luminosities. Monthly Notices of the Royal Astronomical Society. 2019;489(1):555-573. doi:10.1093/mnras/stz2149","mla":"Khostovan, A. A., et al. “The Clustering of Typical Ly α Emitters from z ∼ 2.5–6: Host Halo Masses Depend on Ly α and UV Luminosities.” Monthly Notices of the Royal Astronomical Society, vol. 489, no. 1, Oxford University Press, 2019, pp. 555–73, doi:10.1093/mnras/stz2149.","ieee":"A. A. Khostovan et al., “The clustering of typical Ly α emitters from z ∼ 2.5–6: Host halo masses depend on Ly α and UV luminosities,” Monthly Notices of the Royal Astronomical Society, vol. 489, no. 1. Oxford University Press, pp. 555–573, 2019.","chicago":"Khostovan, A A, D Sobral, B Mobasher, Jorryt J Matthee, R K Cochrane, N Chartab, M Jafariyazani, A Paulino-Afonso, S Santos, and J Calhau. “The Clustering of Typical Ly α Emitters from z ∼ 2.5–6: Host Halo Masses Depend on Ly α and UV Luminosities.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2019. https://doi.org/10.1093/mnras/stz2149.","short":"A.A. Khostovan, D. Sobral, B. Mobasher, J.J. Matthee, R.K. Cochrane, N. Chartab, M. Jafariyazani, A. Paulino-Afonso, S. Santos, J. Calhau, Monthly Notices of the Royal Astronomical Society 489 (2019) 555–573.","ista":"Khostovan AA, Sobral D, Mobasher B, Matthee JJ, Cochrane RK, Chartab N, Jafariyazani M, Paulino-Afonso A, Santos S, Calhau J. 2019. The clustering of typical Ly α emitters from z ∼ 2.5–6: Host halo masses depend on Ly α and UV luminosities. Monthly Notices of the Royal Astronomical Society. 489(1), 555–573."},"acknowledgement":"We thank the anonymous referee for their useful comments and suggestions that helped improve this study. AAK acknowledges that this work was supported by NASA Headquarters under the NASA Earth and Space Science Fellowship Program – Grant NNX16AO92H. JM acknowledges support from the ETH Zwicky fellowship. RKC acknowledges funding from STFC via a studentship. APA acknowledges support from the Fundac¸ao para a Ci ˜ encia e a Tecnologia FCT through the fellowship PD/BD/52706/2014 and the research grant UID/FIS/04434/2013. JC and SS both acknowledge their support from the Lancaster University PhD Fellowship. We have benefited greatly from the publicly available programming language PYTHON, including the NUMPY, SCIPY, MATPLOTLIB, SCIKIT-LEARN, and ASTROPY packages, as well as the TOPCAT analysis program. The SC4K samples used in this paper are all publicly available for use by the community (Sobral et al. 2018a). The catalogue is also available on the COSMOS IPAC website (https://irsa.ipac.caltech.edu/data/COSMOS/overview.html).","external_id":{"arxiv":["1811.00556"]},"page":"555-573","author":[{"last_name":"Khostovan","first_name":"A A","full_name":"Khostovan, A A"},{"last_name":"Sobral","first_name":"D","full_name":"Sobral, D"},{"full_name":"Mobasher, B","first_name":"B","last_name":"Mobasher"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","full_name":"Matthee, Jorryt J","first_name":"Jorryt J","last_name":"Matthee","orcid":"0000-0003-2871-127X"},{"last_name":"Cochrane","first_name":"R K","full_name":"Cochrane, R K"},{"first_name":"N","full_name":"Chartab, N","last_name":"Chartab"},{"full_name":"Jafariyazani, M","first_name":"M","last_name":"Jafariyazani"},{"first_name":"A","full_name":"Paulino-Afonso, A","last_name":"Paulino-Afonso"},{"last_name":"Santos","full_name":"Santos, S","first_name":"S"},{"last_name":"Calhau","first_name":"J","full_name":"Calhau, J"}],"quality_controlled":"1","doi":"10.1093/mnras/stz2149","_id":"11535","date_published":"2019-10-01T00:00:00Z","month":"10","article_type":"original","publication_status":"published","date_updated":"2022-08-19T06:38:42Z","publisher":"Oxford University Press","oa":1,"article_processing_charge":"No","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"oa_version":"Preprint","year":"2019","status":"public","issue":"1"}]