[{"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"research_data_reference","_id":"13063","main_file_link":[{"url":"https://doi.org/10.5061/dryad.sqv9s4n51","open_access":"1"}],"year":"2021","oa":1,"status":"public","ddc":["570"],"day":"04","citation":{"ama":"Robinson MR. Probabilistic inference of the genetic architecture of functional enrichment of complex traits. 2021. doi:<a href=\"https://doi.org/10.5061/dryad.sqv9s4n51\">10.5061/dryad.sqv9s4n51</a>","mla":"Robinson, Matthew Richard. <i>Probabilistic Inference of the Genetic Architecture of Functional Enrichment of Complex Traits</i>. Dryad, 2021, doi:<a href=\"https://doi.org/10.5061/dryad.sqv9s4n51\">10.5061/dryad.sqv9s4n51</a>.","short":"M.R. Robinson, (2021).","ista":"Robinson MR. 2021. Probabilistic inference of the genetic architecture of functional enrichment of complex traits, Dryad, <a href=\"https://doi.org/10.5061/dryad.sqv9s4n51\">10.5061/dryad.sqv9s4n51</a>.","ieee":"M. R. Robinson, “Probabilistic inference of the genetic architecture of functional enrichment of complex traits.” Dryad, 2021.","chicago":"Robinson, Matthew Richard. “Probabilistic Inference of the Genetic Architecture of Functional Enrichment of Complex Traits.” Dryad, 2021. <a href=\"https://doi.org/10.5061/dryad.sqv9s4n51\">https://doi.org/10.5061/dryad.sqv9s4n51</a>.","apa":"Robinson, M. R. (2021). Probabilistic inference of the genetic architecture of functional enrichment of complex traits. Dryad. <a href=\"https://doi.org/10.5061/dryad.sqv9s4n51\">https://doi.org/10.5061/dryad.sqv9s4n51</a>"},"month":"11","department":[{"_id":"MaRo"}],"title":"Probabilistic inference of the genetic architecture of functional enrichment of complex traits","publisher":"Dryad","date_created":"2023-05-23T16:20:16Z","oa_version":"Published Version","tmp":{"short":"CC0 (1.0)","image":"/images/cc_0.png","legal_code_url":"https://creativecommons.org/publicdomain/zero/1.0/legalcode","name":"Creative Commons Public Domain Dedication (CC0 1.0)"},"date_published":"2021-11-04T00:00:00Z","author":[{"full_name":"Robinson, Matthew Richard","id":"E5D42276-F5DA-11E9-8E24-6303E6697425","first_name":"Matthew Richard","orcid":"0000-0001-8982-8813","last_name":"Robinson"}],"article_processing_charge":"No","date_updated":"2023-09-26T10:36:15Z","related_material":{"record":[{"id":"8429","status":"public","relation":"used_in_publication"}],"link":[{"relation":"software","url":"https://github.com/medical-genomics-group/gmrm"}]},"doi":"10.5061/dryad.sqv9s4n51","abstract":[{"text":"We develop a Bayesian model (BayesRR-RC) that provides robust SNP-heritability estimation, an alternative to marker discovery, and accurate genomic prediction, taking 22 seconds per iteration to estimate 8.4 million SNP-effects and 78 SNP-heritability parameters in the UK Biobank. We find that only $\\leq$ 10\\% of the genetic variation captured for height, body mass index, cardiovascular disease, and type 2 diabetes is attributable to proximal regulatory regions within 10kb upstream of genes, while 12-25% is attributed to coding regions, 32-44% to introns, and 22-28% to distal 10-500kb upstream regions. Up to 24% of all cis and coding regions of each chromosome are associated with each trait, with over 3,100 independent exonic and intronic regions and over 5,400 independent regulatory regions having &gt;95% probability of contributing &gt;0.001% to the genetic variance of these four traits. Our open-source software (GMRM) provides a scalable alternative to current approaches for biobank data.","lang":"eng"}]},{"abstract":[{"text":"Source data and source code for the graphs in \"Spatiotemporal dynamics of self-organized branching pancreatic cancer-derived organoids\".","lang":"eng"}],"date_published":"2021-07-30T00:00:00Z","author":[{"last_name":"Randriamanantsoa","first_name":"Samuel","full_name":"Randriamanantsoa, Samuel"},{"first_name":"Aristeidis","last_name":"Papargyriou","full_name":"Papargyriou, Aristeidis"},{"first_name":"Carlo","last_name":"Maurer","full_name":"Maurer, Carlo"},{"last_name":"Peschke","first_name":"Katja","full_name":"Peschke, Katja"},{"full_name":"Schuster, Maximilian","first_name":"Maximilian","last_name":"Schuster"},{"full_name":"Zecchin, Giulia","first_name":"Giulia","last_name":"Zecchin"},{"first_name":"Katja","last_name":"Steiger","full_name":"Steiger, Katja"},{"first_name":"Rupert","last_name":"Öllinger","full_name":"Öllinger, Rupert"},{"first_name":"Dieter","last_name":"Saur","full_name":"Saur, Dieter"},{"last_name":"Scheel","first_name":"Christina","full_name":"Scheel, Christina"},{"first_name":"Roland","last_name":"Rad","full_name":"Rad, Roland"},{"first_name":"Edouard B","last_name":"Hannezo","orcid":"0000-0001-6005-1561","full_name":"Hannezo, Edouard B","id":"3A9DB764-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Reichert, Maximilian","last_name":"Reichert","first_name":"Maximilian"},{"first_name":"Andreas R.","last_name":"Bausch","full_name":"Bausch, Andreas R."}],"article_processing_charge":"No","date_updated":"2023-08-04T09:25:23Z","doi":"10.5281/ZENODO.5148117","related_material":{"record":[{"id":"12217","relation":"used_in_publication","status":"public"}]},"date_created":"2023-05-23T16:39:24Z","tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"oa_version":"Published Version","department":[{"_id":"EdHa"}],"title":"Spatiotemporal dynamics of self-organized branching in pancreas-derived organoids","publisher":"Zenodo","citation":{"short":"S. Randriamanantsoa, A. Papargyriou, C. Maurer, K. Peschke, M. Schuster, G. Zecchin, K. Steiger, R. Öllinger, D. Saur, C. Scheel, R. Rad, E.B. Hannezo, M. Reichert, A.R. Bausch, (2021).","ista":"Randriamanantsoa S, Papargyriou A, Maurer C, Peschke K, Schuster M, Zecchin G, Steiger K, Öllinger R, Saur D, Scheel C, Rad R, Hannezo EB, Reichert M, Bausch AR. 2021. Spatiotemporal dynamics of self-organized branching in pancreas-derived organoids, Zenodo, <a href=\"https://doi.org/10.5281/ZENODO.5148117\">10.5281/ZENODO.5148117</a>.","mla":"Randriamanantsoa, Samuel, et al. <i>Spatiotemporal Dynamics of Self-Organized Branching in Pancreas-Derived Organoids</i>. Zenodo, 2021, doi:<a href=\"https://doi.org/10.5281/ZENODO.5148117\">10.5281/ZENODO.5148117</a>.","ama":"Randriamanantsoa S, Papargyriou A, Maurer C, et al. Spatiotemporal dynamics of self-organized branching in pancreas-derived organoids. 2021. doi:<a href=\"https://doi.org/10.5281/ZENODO.5148117\">10.5281/ZENODO.5148117</a>","apa":"Randriamanantsoa, S., Papargyriou, A., Maurer, C., Peschke, K., Schuster, M., Zecchin, G., … Bausch, A. R. (2021). Spatiotemporal dynamics of self-organized branching in pancreas-derived organoids. Zenodo. <a href=\"https://doi.org/10.5281/ZENODO.5148117\">https://doi.org/10.5281/ZENODO.5148117</a>","chicago":"Randriamanantsoa, Samuel, Aristeidis Papargyriou, Carlo Maurer, Katja Peschke, Maximilian Schuster, Giulia Zecchin, Katja Steiger, et al. “Spatiotemporal Dynamics of Self-Organized Branching in Pancreas-Derived Organoids.” Zenodo, 2021. <a href=\"https://doi.org/10.5281/ZENODO.5148117\">https://doi.org/10.5281/ZENODO.5148117</a>.","ieee":"S. Randriamanantsoa <i>et al.</i>, “Spatiotemporal dynamics of self-organized branching in pancreas-derived organoids.” Zenodo, 2021."},"month":"07","status":"public","oa":1,"ddc":["570"],"day":"30","main_file_link":[{"url":"https://doi.org/10.5281/zenodo.6577226","open_access":"1"}],"_id":"13068","year":"2021","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"research_data_reference"},{"abstract":[{"text":"To survive elevated temperatures, ectotherms adjust the fluidity of membranes by fine-tuning lipid desaturation levels in a process previously described to be cell-autonomous. We have discovered that, in Caenorhabditis elegans, neuronal Heat shock Factor 1 (HSF-1), the conserved master regulator of the heat shock response (HSR)- causes extensive fat remodelling in peripheral tissues. These changes include a decrease in fat desaturase and acid lipase expression in the intestine, and a global shift in the saturation levels of plasma membrane’s phospholipids. The observed remodelling of plasma membrane is in line with ectothermic adaptive responses and gives worms a cumulative advantage to warm temperatures. We have determined that at least six TAX-2/TAX-4 cGMP gated channel expressing sensory neurons and TGF-β/BMP are required for signalling across tissues to modulate fat desaturation. We also find neuronal hsf-1  is not only sufficient but also partially necessary to control the fat remodelling response and for survival at warm temperatures. This is the first study to show that a thermostat-based mechanism can cell non-autonomously coordinate membrane saturation and composition across tissues in a multicellular animal.","lang":"eng"}],"article_processing_charge":"No","doi":"10.5281/ZENODO.5519410","related_material":{"record":[{"id":"10322","status":"public","relation":"used_in_publication"}]},"date_updated":"2023-08-14T11:53:26Z","date_published":"2021-12-25T00:00:00Z","author":[{"full_name":"Chauve, Laetitia","last_name":"Chauve","first_name":"Laetitia"},{"full_name":"Hodge, Francesca","last_name":"Hodge","first_name":"Francesca"},{"full_name":"Murdoch, Sharlene","first_name":"Sharlene","last_name":"Murdoch"},{"full_name":"Masoudzadeh, Fatemah","last_name":"Masoudzadeh","first_name":"Fatemah"},{"full_name":"Mann, Harry-Jack","last_name":"Mann","first_name":"Harry-Jack"},{"last_name":"Lopez-Clavijo","first_name":"Andrea","full_name":"Lopez-Clavijo, Andrea"},{"first_name":"Hanneke","last_name":"Okkenhaug","full_name":"Okkenhaug, Hanneke"},{"first_name":"Greg","last_name":"West","full_name":"West, Greg"},{"last_name":"Sousa","first_name":"Bebiana C.","full_name":"Sousa, Bebiana C."},{"last_name":"Segonds-Pichon","first_name":"Anne","full_name":"Segonds-Pichon, Anne"},{"last_name":"Li","first_name":"Cheryl","full_name":"Li, Cheryl"},{"first_name":"Steven","last_name":"Wingett","full_name":"Wingett, Steven"},{"full_name":"Kienberger, Hermine","first_name":"Hermine","last_name":"Kienberger"},{"full_name":"Kleigrewe, Karin","last_name":"Kleigrewe","first_name":"Karin"},{"full_name":"de Bono, Mario","id":"4E3FF80E-F248-11E8-B48F-1D18A9856A87","first_name":"Mario","last_name":"de Bono","orcid":"0000-0001-8347-0443"},{"first_name":"Michael","last_name":"Wakelam","full_name":"Wakelam, Michael"},{"first_name":"Olivia","last_name":"Casanueva","full_name":"Casanueva, Olivia"}],"date_created":"2023-05-23T16:40:56Z","oa_version":"Published Version","tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"publisher":"Zenodo","department":[{"_id":"MaDe"}],"title":"Neuronal HSF-1 coordinates the propagation of fat desaturation across tissues to enable adaptation to high temperatures in C. elegans","month":"12","citation":{"ista":"Chauve L, Hodge F, Murdoch S, Masoudzadeh F, Mann H-J, Lopez-Clavijo A, Okkenhaug H, West G, Sousa BC, Segonds-Pichon A, Li C, Wingett S, Kienberger H, Kleigrewe K, de Bono M, Wakelam M, Casanueva O. 2021. Neuronal HSF-1 coordinates the propagation of fat desaturation across tissues to enable adaptation to high temperatures in C. elegans, Zenodo, <a href=\"https://doi.org/10.5281/ZENODO.5519410\">10.5281/ZENODO.5519410</a>.","short":"L. Chauve, F. Hodge, S. Murdoch, F. Masoudzadeh, H.-J. Mann, A. Lopez-Clavijo, H. Okkenhaug, G. West, B.C. Sousa, A. Segonds-Pichon, C. Li, S. Wingett, H. Kienberger, K. Kleigrewe, M. de Bono, M. Wakelam, O. Casanueva, (2021).","mla":"Chauve, Laetitia, et al. <i>Neuronal HSF-1 Coordinates the Propagation of Fat Desaturation across Tissues to Enable Adaptation to High Temperatures in C. Elegans</i>. Zenodo, 2021, doi:<a href=\"https://doi.org/10.5281/ZENODO.5519410\">10.5281/ZENODO.5519410</a>.","ama":"Chauve L, Hodge F, Murdoch S, et al. Neuronal HSF-1 coordinates the propagation of fat desaturation across tissues to enable adaptation to high temperatures in C. elegans. 2021. doi:<a href=\"https://doi.org/10.5281/ZENODO.5519410\">10.5281/ZENODO.5519410</a>","apa":"Chauve, L., Hodge, F., Murdoch, S., Masoudzadeh, F., Mann, H.-J., Lopez-Clavijo, A., … Casanueva, O. (2021). Neuronal HSF-1 coordinates the propagation of fat desaturation across tissues to enable adaptation to high temperatures in C. elegans. Zenodo. <a href=\"https://doi.org/10.5281/ZENODO.5519410\">https://doi.org/10.5281/ZENODO.5519410</a>","ieee":"L. Chauve <i>et al.</i>, “Neuronal HSF-1 coordinates the propagation of fat desaturation across tissues to enable adaptation to high temperatures in C. elegans.” Zenodo, 2021.","chicago":"Chauve, Laetitia, Francesca Hodge, Sharlene Murdoch, Fatemah Masoudzadeh, Harry-Jack Mann, Andrea Lopez-Clavijo, Hanneke Okkenhaug, et al. “Neuronal HSF-1 Coordinates the Propagation of Fat Desaturation across Tissues to Enable Adaptation to High Temperatures in C. Elegans.” Zenodo, 2021. <a href=\"https://doi.org/10.5281/ZENODO.5519410\">https://doi.org/10.5281/ZENODO.5519410</a>."},"ddc":["570"],"day":"25","oa":1,"status":"public","year":"2021","main_file_link":[{"open_access":"1","url":"https://doi.org/10.5281/zenodo.5547464"}],"_id":"13069","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"research_data_reference"},{"tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"oa_version":"Published Version","date_created":"2023-05-23T16:46:20Z","department":[{"_id":"MaRo"}],"title":"Blood-based epigenome-wide analyses of cognitive abilities","publisher":"Zenodo","abstract":[{"text":"CpGs and corresponding mean weights for DNAm-based prediction of cognitive abilities (6 traits)","lang":"eng"}],"date_published":"2021-12-20T00:00:00Z","author":[{"full_name":"McCartney, Daniel L","last_name":"McCartney","first_name":"Daniel L"},{"last_name":"Hillary","first_name":"Robert F","full_name":"Hillary, Robert F"},{"full_name":"Conole, Eleanor LS","first_name":"Eleanor LS","last_name":"Conole"},{"full_name":"Trejo Banos, Daniel","first_name":"Daniel","last_name":"Trejo Banos"},{"full_name":"Gadd, Danni A","first_name":"Danni A","last_name":"Gadd"},{"full_name":"Walker, Rosie M","last_name":"Walker","first_name":"Rosie M"},{"first_name":"Cliff","last_name":"Nangle","full_name":"Nangle, Cliff"},{"full_name":"Flaig, Robin","last_name":"Flaig","first_name":"Robin"},{"last_name":"Campbell","first_name":"Archie","full_name":"Campbell, Archie"},{"last_name":"Murray","first_name":"Alison D","full_name":"Murray, Alison D"},{"first_name":"Susana","last_name":"Munoz Maniega","full_name":"Munoz Maniega, Susana"},{"full_name":"del C Valdes-Hernandez, Maria","last_name":"del C Valdes-Hernandez","first_name":"Maria"},{"full_name":"Harris, Mathew A","first_name":"Mathew A","last_name":"Harris"},{"last_name":"Bastin","first_name":"Mark E","full_name":"Bastin, Mark E"},{"full_name":"Wardlaw, Joanna M","first_name":"Joanna M","last_name":"Wardlaw"},{"first_name":"Sarah E","last_name":"Harris","full_name":"Harris, Sarah E"},{"full_name":"Porteous, David J","last_name":"Porteous","first_name":"David J"},{"last_name":"Tucker-Drob","first_name":"Elliot M","full_name":"Tucker-Drob, Elliot M"},{"full_name":"McIntosh, Andrew M","first_name":"Andrew M","last_name":"McIntosh"},{"full_name":"Evans, Kathryn L","last_name":"Evans","first_name":"Kathryn L"},{"full_name":"Deary, Ian J","first_name":"Ian J","last_name":"Deary"},{"full_name":"Cox, Simon R","last_name":"Cox","first_name":"Simon R"},{"full_name":"Robinson, Matthew Richard","id":"E5D42276-F5DA-11E9-8E24-6303E6697425","first_name":"Matthew Richard","orcid":"0000-0001-8982-8813","last_name":"Robinson"},{"full_name":"Marioni, Riccardo E","first_name":"Riccardo E","last_name":"Marioni"}],"date_updated":"2023-08-02T14:05:12Z","related_material":{"record":[{"id":"10702","status":"public","relation":"used_in_publication"}]},"doi":"10.5281/ZENODO.5794028","article_processing_charge":"No","main_file_link":[{"url":"https://doi.org/10.5281/zenodo.5794029","open_access":"1"}],"_id":"13072","year":"2021","type":"research_data_reference","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"ieee":"D. L. McCartney <i>et al.</i>, “Blood-based epigenome-wide analyses of cognitive abilities.” Zenodo, 2021.","chicago":"McCartney, Daniel L, Robert F Hillary, Eleanor LS Conole, Daniel Trejo Banos, Danni A Gadd, Rosie M Walker, Cliff Nangle, et al. “Blood-Based Epigenome-Wide Analyses of Cognitive Abilities.” Zenodo, 2021. <a href=\"https://doi.org/10.5281/ZENODO.5794028\">https://doi.org/10.5281/ZENODO.5794028</a>.","apa":"McCartney, D. L., Hillary, R. F., Conole, E. L., Trejo Banos, D., Gadd, D. A., Walker, R. M., … Marioni, R. E. (2021). Blood-based epigenome-wide analyses of cognitive abilities. Zenodo. <a href=\"https://doi.org/10.5281/ZENODO.5794028\">https://doi.org/10.5281/ZENODO.5794028</a>","ama":"McCartney DL, Hillary RF, Conole EL, et al. Blood-based epigenome-wide analyses of cognitive abilities. 2021. doi:<a href=\"https://doi.org/10.5281/ZENODO.5794028\">10.5281/ZENODO.5794028</a>","mla":"McCartney, Daniel L., et al. <i>Blood-Based Epigenome-Wide Analyses of Cognitive Abilities</i>. Zenodo, 2021, doi:<a href=\"https://doi.org/10.5281/ZENODO.5794028\">10.5281/ZENODO.5794028</a>.","short":"D.L. McCartney, R.F. Hillary, E.L. Conole, D. Trejo Banos, D.A. Gadd, R.M. Walker, C. Nangle, R. Flaig, A. Campbell, A.D. Murray, S. Munoz Maniega, M. del C Valdes-Hernandez, M.A. Harris, M.E. Bastin, J.M. Wardlaw, S.E. Harris, D.J. Porteous, E.M. Tucker-Drob, A.M. McIntosh, K.L. Evans, I.J. Deary, S.R. Cox, M.R. Robinson, R.E. Marioni, (2021).","ista":"McCartney DL, Hillary RF, Conole EL, Trejo Banos D, Gadd DA, Walker RM, Nangle C, Flaig R, Campbell A, Murray AD, Munoz Maniega S, del C Valdes-Hernandez M, Harris MA, Bastin ME, Wardlaw JM, Harris SE, Porteous DJ, Tucker-Drob EM, McIntosh AM, Evans KL, Deary IJ, Cox SR, Robinson MR, Marioni RE. 2021. Blood-based epigenome-wide analyses of cognitive abilities, Zenodo, <a href=\"https://doi.org/10.5281/ZENODO.5794028\">10.5281/ZENODO.5794028</a>."},"month":"12","oa":1,"status":"public","day":"20","ddc":["570"]},{"oa_version":"Published Version","date_created":"2023-05-23T17:11:28Z","publisher":"Zenodo","department":[{"_id":"AnHi"}],"title":"Data for 'Closing of the Induced Gap in a Hybrid Superconductor-Semiconductor Nanowire","abstract":[{"text":"Data for the manuscript 'Closing of the Induced Gap in a Hybrid Superconductor-Semiconductor Nanowire' ([2006.01275] Closing of the Induced Gap in a Hybrid Superconductor-Semiconductor Nanowire (arxiv.org))\r\n\r\nWe upload a pdf with extended data sets, and the raw data for these extended datasets as well.","lang":"eng"}],"related_material":{"record":[{"relation":"used_in_publication","status":"public","id":"9570"}],"link":[{"relation":"software","url":"https://github.com/caslu85/Induced-Gap-Closing-Shared/tree/1.1.3"}]},"doi":"10.5281/ZENODO.4592435","date_updated":"2023-08-08T14:08:07Z","article_processing_charge":"No","author":[{"id":"4D495994-AE37-11E9-AC72-31CAE5697425","full_name":"Puglia, Denise","last_name":"Puglia","first_name":"Denise"},{"first_name":"Esteban","last_name":"Martinez","full_name":"Martinez, Esteban"},{"last_name":"Menard","first_name":"Gerbold","full_name":"Menard, Gerbold"},{"full_name":"Pöschl, Andreas","first_name":"Andreas","last_name":"Pöschl"},{"full_name":"Gronin, Sergei","first_name":"Sergei","last_name":"Gronin"},{"first_name":"Geoffrey","last_name":"Gardner","full_name":"Gardner, Geoffrey"},{"first_name":"Ray","last_name":"Kallaher","full_name":"Kallaher, Ray"},{"first_name":"Michael","last_name":"Manfra","full_name":"Manfra, Michael"},{"full_name":"Marcus, Charles","first_name":"Charles","last_name":"Marcus"},{"last_name":"Higginbotham","orcid":"0000-0003-2607-2363","first_name":"Andrew P","id":"4AD6785A-F248-11E8-B48F-1D18A9856A87","full_name":"Higginbotham, Andrew P"},{"first_name":"Lucas","last_name":"Casparis","full_name":"Casparis, Lucas"}],"date_published":"2021-03-09T00:00:00Z","year":"2021","main_file_link":[{"open_access":"1","url":"https://doi.org/10.5281/zenodo.4592460"}],"_id":"13080","type":"research_data_reference","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"03","citation":{"mla":"Puglia, Denise, et al. <i>Data for ’Closing of the Induced Gap in a Hybrid Superconductor-Semiconductor Nanowire</i>. Zenodo, 2021, doi:<a href=\"https://doi.org/10.5281/ZENODO.4592435\">10.5281/ZENODO.4592435</a>.","short":"D. Puglia, E. Martinez, G. Menard, A. Pöschl, S. Gronin, G. Gardner, R. Kallaher, M. Manfra, C. Marcus, A.P. Higginbotham, L. Casparis, (2021).","ista":"Puglia D, Martinez E, Menard G, Pöschl A, Gronin S, Gardner G, Kallaher R, Manfra M, Marcus C, Higginbotham AP, Casparis L. 2021. Data for ’Closing of the Induced Gap in a Hybrid Superconductor-Semiconductor Nanowire, Zenodo, <a href=\"https://doi.org/10.5281/ZENODO.4592435\">10.5281/ZENODO.4592435</a>.","ama":"Puglia D, Martinez E, Menard G, et al. Data for ’Closing of the Induced Gap in a Hybrid Superconductor-Semiconductor Nanowire. 2021. doi:<a href=\"https://doi.org/10.5281/ZENODO.4592435\">10.5281/ZENODO.4592435</a>","apa":"Puglia, D., Martinez, E., Menard, G., Pöschl, A., Gronin, S., Gardner, G., … Casparis, L. (2021). Data for ’Closing of the Induced Gap in a Hybrid Superconductor-Semiconductor Nanowire. Zenodo. <a href=\"https://doi.org/10.5281/ZENODO.4592435\">https://doi.org/10.5281/ZENODO.4592435</a>","ieee":"D. Puglia <i>et al.</i>, “Data for ’Closing of the Induced Gap in a Hybrid Superconductor-Semiconductor Nanowire.” Zenodo, 2021.","chicago":"Puglia, Denise, Esteban Martinez, Gerbold Menard, Andreas Pöschl, Sergei Gronin, Geoffrey Gardner, Ray Kallaher, et al. “Data for ’Closing of the Induced Gap in a Hybrid Superconductor-Semiconductor Nanowire.” Zenodo, 2021. <a href=\"https://doi.org/10.5281/ZENODO.4592435\">https://doi.org/10.5281/ZENODO.4592435</a>."},"day":"09","ddc":["530"],"status":"public","oa":1},{"conference":{"start_date":"2021-07-18","location":"Virtual","end_date":"2021-07-24","name":"International Conference on Machine Learning"},"tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"file_date_updated":"2023-06-19T10:49:12Z","scopus_import":"1","quality_controlled":"1","author":[{"full_name":"Nguyen, Quynh","first_name":"Quynh","last_name":"Nguyen"},{"first_name":"Marco","last_name":"Mondelli","orcid":"0000-0002-3242-7020","full_name":"Mondelli, Marco","id":"27EB676C-8706-11E9-9510-7717E6697425"},{"last_name":"Montufar","first_name":"Guido","full_name":"Montufar, Guido"}],"date_published":"2021-07-01T00:00:00Z","article_processing_charge":"No","date_updated":"2024-09-10T13:03:17Z","intvolume":"       139","file":[{"success":1,"date_created":"2023-06-19T10:49:12Z","content_type":"application/pdf","creator":"dernst","access_level":"open_access","relation":"main_file","file_name":"2021_PMLR_Nguyen.pdf","checksum":"19489cf5e16a0596b1f92e317d97c9b0","file_size":591332,"date_updated":"2023-06-19T10:49:12Z","file_id":"13155"}],"publication_status":"published","month":"07","project":[{"_id":"059876FA-7A3F-11EA-A408-12923DDC885E","name":"Prix Lopez-Loretta 2019 - Marco Mondelli"}],"language":[{"iso":"eng"}],"ddc":["000"],"day":"01","date_created":"2023-06-18T22:00:48Z","oa_version":"Published Version","publication":"Proceedings of the 38th International Conference on Machine Learning","department":[{"_id":"MaMo"}],"title":"Tight bounds on the smallest Eigenvalue of the neural tangent kernel for deep ReLU networks","publisher":"ML Research Press","abstract":[{"text":"A recent line of work has analyzed the theoretical properties of deep neural networks via the Neural Tangent Kernel (NTK). In particular, the smallest eigenvalue of the NTK has been related to the memorization capacity, the global convergence of gradient descent algorithms and the generalization of deep nets. However, existing results either provide bounds in the two-layer setting or assume that the spectrum of the NTK matrices is bounded away from 0 for multi-layer networks. In this paper, we provide tight bounds on the smallest eigenvalue of NTK matrices for deep ReLU nets, both in the limiting case of infinite widths and for finite widths. In the finite-width setting, the network architectures we consider are fairly general: we require the existence of a wide layer with roughly order of N neurons, N being the number of data samples; and the scaling of the remaining layer widths is arbitrary (up to logarithmic factors). To obtain our results, we analyze various quantities of independent interest: we give lower bounds on the smallest singular value of hidden feature matrices, and upper bounds on the Lipschitz constant of input-output feature maps.","lang":"eng"}],"arxiv":1,"_id":"13146","has_accepted_license":"1","year":"2021","volume":139,"page":"8119-8129","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"conference","citation":{"apa":"Nguyen, Q., Mondelli, M., &#38; Montufar, G. (2021). Tight bounds on the smallest Eigenvalue of the neural tangent kernel for deep ReLU networks. In <i>Proceedings of the 38th International Conference on Machine Learning</i> (Vol. 139, pp. 8119–8129). Virtual: ML Research Press.","ieee":"Q. Nguyen, M. Mondelli, and G. Montufar, “Tight bounds on the smallest Eigenvalue of the neural tangent kernel for deep ReLU networks,” in <i>Proceedings of the 38th International Conference on Machine Learning</i>, Virtual, 2021, vol. 139, pp. 8119–8129.","chicago":"Nguyen, Quynh, Marco Mondelli, and Guido Montufar. “Tight Bounds on the Smallest Eigenvalue of the Neural Tangent Kernel for Deep ReLU Networks.” In <i>Proceedings of the 38th International Conference on Machine Learning</i>, 139:8119–29. ML Research Press, 2021.","ista":"Nguyen Q, Mondelli M, Montufar G. 2021. Tight bounds on the smallest Eigenvalue of the neural tangent kernel for deep ReLU networks. Proceedings of the 38th International Conference on Machine Learning. International Conference on Machine Learning vol. 139, 8119–8129.","short":"Q. Nguyen, M. Mondelli, G. Montufar, in:, Proceedings of the 38th International Conference on Machine Learning, ML Research Press, 2021, pp. 8119–8129.","mla":"Nguyen, Quynh, et al. “Tight Bounds on the Smallest Eigenvalue of the Neural Tangent Kernel for Deep ReLU Networks.” <i>Proceedings of the 38th International Conference on Machine Learning</i>, vol. 139, ML Research Press, 2021, pp. 8119–29.","ama":"Nguyen Q, Mondelli M, Montufar G. Tight bounds on the smallest Eigenvalue of the neural tangent kernel for deep ReLU networks. In: <i>Proceedings of the 38th International Conference on Machine Learning</i>. Vol 139. ML Research Press; 2021:8119-8129."},"publication_identifier":{"eissn":["2640-3498"],"isbn":["9781713845065"]},"acknowledgement":"The authors would like to thank the anonymous reviewers for their helpful comments. MM was partially supported by the 2019 Lopez-Loreta Prize. QN and GM acknowledge support from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement no 757983).","oa":1,"status":"public","external_id":{"arxiv":["2012.11654"]}},{"intvolume":"       139","publication_status":"published","file":[{"relation":"main_file","access_level":"open_access","creator":"dernst","content_type":"application/pdf","date_created":"2023-06-19T10:41:05Z","success":1,"date_updated":"2023-06-19T10:41:05Z","file_id":"13154","file_size":429087,"checksum":"7ec0d59bac268b49c76bf2e036dedd7a","file_name":"2021_PMLR_Alimisis.pdf"}],"day":"01","ddc":["000"],"project":[{"call_identifier":"H2020","_id":"268A44D6-B435-11E9-9278-68D0E5697425","grant_number":"805223","name":"Elastic Coordination for Scalable Machine Learning"},{"call_identifier":"H2020","grant_number":"754411","name":"ISTplus - Postdoctoral Fellowships","_id":"260C2330-B435-11E9-9278-68D0E5697425"}],"language":[{"iso":"eng"}],"month":"07","file_date_updated":"2023-06-19T10:41:05Z","tmp":{"image":"/images/cc_by.png","short":"CC BY (4.0)","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"conference":{"start_date":"2021-07-18","location":"Virtual","end_date":"2021-07-24","name":"International Conference on Machine Learning"},"author":[{"full_name":"Alimisis, Foivos","last_name":"Alimisis","first_name":"Foivos"},{"first_name":"Peter","last_name":"Davies","orcid":"0000-0002-5646-9524","full_name":"Davies, Peter","id":"11396234-BB50-11E9-B24C-90FCE5697425"},{"orcid":"0000-0003-3650-940X","last_name":"Alistarh","first_name":"Dan-Adrian","id":"4A899BFC-F248-11E8-B48F-1D18A9856A87","full_name":"Alistarh, Dan-Adrian"}],"date_published":"2021-07-01T00:00:00Z","date_updated":"2023-06-19T10:44:38Z","article_processing_charge":"No","scopus_import":"1","quality_controlled":"1","page":"196-206","volume":139,"type":"conference","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13147","year":"2021","has_accepted_license":"1","acknowledgement":"The authors would like to thank Janne Korhonen, Aurelien Lucchi, Celestine MendlerDunner and Antonio Orvieto for helpful discussions. FA ¨and DA were supported during this work by the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 805223 ScaleML). PD was supported by the European Union’s Horizon 2020 programme under the Marie Skłodowska-Curie grant agreement No. 754411.","status":"public","oa":1,"external_id":{"arxiv":["2102.07214"]},"citation":{"ama":"Alimisis F, Davies P, Alistarh D-A. Communication-efficient distributed optimization with quantized preconditioners. In: <i>Proceedings of the 38th International Conference on Machine Learning</i>. Vol 139. ML Research Press; 2021:196-206.","mla":"Alimisis, Foivos, et al. “Communication-Efficient Distributed Optimization with Quantized Preconditioners.” <i>Proceedings of the 38th International Conference on Machine Learning</i>, vol. 139, ML Research Press, 2021, pp. 196–206.","ista":"Alimisis F, Davies P, Alistarh D-A. 2021. Communication-efficient distributed optimization with quantized preconditioners. Proceedings of the 38th International Conference on Machine Learning. International Conference on Machine Learning vol. 139, 196–206.","short":"F. Alimisis, P. Davies, D.-A. Alistarh, in:, Proceedings of the 38th International Conference on Machine Learning, ML Research Press, 2021, pp. 196–206.","chicago":"Alimisis, Foivos, Peter Davies, and Dan-Adrian Alistarh. “Communication-Efficient Distributed Optimization with Quantized Preconditioners.” In <i>Proceedings of the 38th International Conference on Machine Learning</i>, 139:196–206. ML Research Press, 2021.","ieee":"F. Alimisis, P. Davies, and D.-A. Alistarh, “Communication-efficient distributed optimization with quantized preconditioners,” in <i>Proceedings of the 38th International Conference on Machine Learning</i>, Virtual, 2021, vol. 139, pp. 196–206.","apa":"Alimisis, F., Davies, P., &#38; Alistarh, D.-A. (2021). Communication-efficient distributed optimization with quantized preconditioners. In <i>Proceedings of the 38th International Conference on Machine Learning</i> (Vol. 139, pp. 196–206). Virtual: ML Research Press."},"publication_identifier":{"isbn":["9781713845065"],"eissn":["2640-3498"]},"title":"Communication-efficient distributed optimization with quantized preconditioners","department":[{"_id":"DaAl"}],"publication":"Proceedings of the 38th International Conference on Machine Learning","publisher":"ML Research Press","oa_version":"Published Version","date_created":"2023-06-18T22:00:48Z","ec_funded":1,"arxiv":1,"abstract":[{"lang":"eng","text":"We investigate fast and communication-efficient algorithms for the classic problem of minimizing a sum of strongly convex and smooth functions that are distributed among n\r\n different nodes, which can communicate using a limited number of bits. Most previous communication-efficient approaches for this problem are limited to first-order optimization, and therefore have \\emph{linear} dependence on the condition number in their communication complexity. We show that this dependence is not inherent: communication-efficient methods can in fact have sublinear dependence on the condition number. For this, we design and analyze the first communication-efficient distributed variants of preconditioned gradient descent for Generalized Linear Models, and for Newton’s method. Our results rely on a new technique for quantizing both the preconditioner and the descent direction at each step of the algorithms, while controlling their convergence rate. We also validate our findings experimentally, showing faster convergence and reduced communication relative to previous methods."}]},{"author":[{"last_name":"Bian","first_name":"Tong","full_name":"Bian, Tong"},{"first_name":"Rafal","last_name":"Klajn","full_name":"Klajn, Rafal","id":"8e84690e-1e48-11ed-a02b-a1e6fb8bb53b"}],"date_published":"2021-12-01T00:00:00Z","date_updated":"2023-08-07T10:01:10Z","doi":"10.1111/nyas.14674","article_processing_charge":"No","scopus_import":"1","keyword":["History and Philosophy of Science","General Biochemistry","Genetics and Molecular Biology","General Neuroscience"],"quality_controlled":"1","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1111/nyas.14674"}],"intvolume":"      1505","publication_status":"published","pmid":1,"day":"01","ddc":["540"],"language":[{"iso":"eng"}],"month":"12","title":"Morphology control in crystalline nanoparticle–polymer aggregates","publication":"Annals of the New York Academy of Sciences","publisher":"Wiley","oa_version":"Published Version","date_created":"2023-08-01T09:33:39Z","abstract":[{"lang":"eng","text":"Self-assembly of nanoparticles can be mediated by polymers, but has so far led almost exclusively to nanoparticle aggregates that are amorphous. Here, we employed Coulombic interactions to generate a range of composite materials from mixtures of charged nanoparticles and oppositely charged polymers. The assembly behavior of these nanoparticle/polymer composites depends on their order of addition: polymers added to nanoparticles give rise to stable aggregates, but nanoparticles added to polymers disassemble the initially formed aggregates. The amorphous aggregates were transformed into crystalline ones by transiently increasing the ionic strength of the solution. The morphology of the resulting crystals depended on the length of the polymer: short polymer chains mediated the self-assembly of nanoparticles into strongly faceted crystals, whereas long chains led to pseudospherical nanoparticle/polymer assemblies, within which the crystalline order of nanoparticles was retained."}],"extern":"1","page":"191-201","volume":1505,"type":"journal_article","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13356","year":"2021","oa":1,"status":"public","article_type":"original","external_id":{"pmid":["34427923"]},"issue":"1","citation":{"apa":"Bian, T., &#38; Klajn, R. (2021). Morphology control in crystalline nanoparticle–polymer aggregates. <i>Annals of the New York Academy of Sciences</i>. Wiley. <a href=\"https://doi.org/10.1111/nyas.14674\">https://doi.org/10.1111/nyas.14674</a>","chicago":"Bian, Tong, and Rafal Klajn. “Morphology Control in Crystalline Nanoparticle–Polymer Aggregates.” <i>Annals of the New York Academy of Sciences</i>. Wiley, 2021. <a href=\"https://doi.org/10.1111/nyas.14674\">https://doi.org/10.1111/nyas.14674</a>.","ieee":"T. Bian and R. Klajn, “Morphology control in crystalline nanoparticle–polymer aggregates,” <i>Annals of the New York Academy of Sciences</i>, vol. 1505, no. 1. Wiley, pp. 191–201, 2021.","ista":"Bian T, Klajn R. 2021. Morphology control in crystalline nanoparticle–polymer aggregates. Annals of the New York Academy of Sciences. 1505(1), 191–201.","short":"T. Bian, R. Klajn, Annals of the New York Academy of Sciences 1505 (2021) 191–201.","mla":"Bian, Tong, and Rafal Klajn. “Morphology Control in Crystalline Nanoparticle–Polymer Aggregates.” <i>Annals of the New York Academy of Sciences</i>, vol. 1505, no. 1, Wiley, 2021, pp. 191–201, doi:<a href=\"https://doi.org/10.1111/nyas.14674\">10.1111/nyas.14674</a>.","ama":"Bian T, Klajn R. Morphology control in crystalline nanoparticle–polymer aggregates. <i>Annals of the New York Academy of Sciences</i>. 2021;1505(1):191-201. doi:<a href=\"https://doi.org/10.1111/nyas.14674\">10.1111/nyas.14674</a>"},"publication_identifier":{"eissn":["1749-6632"],"issn":["0077-8923"]}},{"date_created":"2023-08-01T09:34:54Z","oa_version":"Published Version","publication":"Nature Chemistry","title":"Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures","publisher":"Springer Nature","abstract":[{"text":"Coulombic interactions can be used to assemble charged nanoparticles into higher-order structures, but the process requires oppositely charged partners that are similarly sized. The ability to mediate the assembly of such charged nanoparticles using structurally simple small molecules would greatly facilitate the fabrication of nanostructured materials and harnessing their applications in catalysis, sensing and photonics. Here we show that small molecules with as few as three electric charges can effectively induce attractive interactions between oppositely charged nanoparticles in water. These interactions can guide the assembly of charged nanoparticles into colloidal crystals of a quality previously only thought to result from their co-crystallization with oppositely charged nanoparticles of a similar size. Transient nanoparticle assemblies can be generated using positively charged nanoparticles and multiply charged anions that are enzymatically hydrolysed into mono- and/or dianions. Our findings demonstrate an approach for the facile fabrication, manipulation and further investigation of static and dynamic nanostructured materials in aqueous environments.","lang":"eng"}],"extern":"1","_id":"13357","year":"2021","volume":13,"page":"940-949","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"journal_article","citation":{"ama":"Bian T, Gardin A, Gemen J, et al. Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures. <i>Nature Chemistry</i>. 2021;13(10):940-949. doi:<a href=\"https://doi.org/10.1038/s41557-021-00752-9\">10.1038/s41557-021-00752-9</a>","mla":"Bian, Tong, et al. “Electrostatic Co-Assembly of Nanoparticles with Oppositely Charged Small Molecules into Static and Dynamic Superstructures.” <i>Nature Chemistry</i>, vol. 13, no. 10, Springer Nature, 2021, pp. 940–49, doi:<a href=\"https://doi.org/10.1038/s41557-021-00752-9\">10.1038/s41557-021-00752-9</a>.","ista":"Bian T, Gardin A, Gemen J, Houben L, Perego C, Lee B, Elad N, Chu Z, Pavan GM, Klajn R. 2021. Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures. Nature Chemistry. 13(10), 940–949.","short":"T. Bian, A. Gardin, J. Gemen, L. Houben, C. Perego, B. Lee, N. Elad, Z. Chu, G.M. Pavan, R. Klajn, Nature Chemistry 13 (2021) 940–949.","chicago":"Bian, Tong, Andrea Gardin, Julius Gemen, Lothar Houben, Claudio Perego, Byeongdu Lee, Nadav Elad, Zonglin Chu, Giovanni M. Pavan, and Rafal Klajn. “Electrostatic Co-Assembly of Nanoparticles with Oppositely Charged Small Molecules into Static and Dynamic Superstructures.” <i>Nature Chemistry</i>. Springer Nature, 2021. <a href=\"https://doi.org/10.1038/s41557-021-00752-9\">https://doi.org/10.1038/s41557-021-00752-9</a>.","ieee":"T. Bian <i>et al.</i>, “Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures,” <i>Nature Chemistry</i>, vol. 13, no. 10. Springer Nature, pp. 940–949, 2021.","apa":"Bian, T., Gardin, A., Gemen, J., Houben, L., Perego, C., Lee, B., … Klajn, R. (2021). Electrostatic co-assembly of nanoparticles with oppositely charged small molecules into static and dynamic superstructures. <i>Nature Chemistry</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41557-021-00752-9\">https://doi.org/10.1038/s41557-021-00752-9</a>"},"publication_identifier":{"eissn":["1755-4349"],"issn":["1755-4330"]},"oa":1,"status":"public","issue":"10","article_type":"original","external_id":{"pmid":["34489564"]},"keyword":["General Chemical Engineering","General Chemistry"],"scopus_import":"1","quality_controlled":"1","date_published":"2021-10-01T00:00:00Z","author":[{"last_name":"Bian","first_name":"Tong","full_name":"Bian, Tong"},{"full_name":"Gardin, Andrea","first_name":"Andrea","last_name":"Gardin"},{"full_name":"Gemen, Julius","last_name":"Gemen","first_name":"Julius"},{"full_name":"Houben, Lothar","last_name":"Houben","first_name":"Lothar"},{"full_name":"Perego, Claudio","last_name":"Perego","first_name":"Claudio"},{"full_name":"Lee, Byeongdu","first_name":"Byeongdu","last_name":"Lee"},{"first_name":"Nadav","last_name":"Elad","full_name":"Elad, Nadav"},{"full_name":"Chu, Zonglin","first_name":"Zonglin","last_name":"Chu"},{"full_name":"Pavan, Giovanni M.","last_name":"Pavan","first_name":"Giovanni M."},{"full_name":"Klajn, Rafal","id":"8e84690e-1e48-11ed-a02b-a1e6fb8bb53b","first_name":"Rafal","last_name":"Klajn"}],"article_processing_charge":"No","doi":"10.1038/s41557-021-00752-9","date_updated":"2023-08-02T10:55:29Z","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1038/s41557-021-00752-9"}],"intvolume":"        13","publication_status":"published","month":"10","language":[{"iso":"eng"}],"pmid":1,"day":"01"},{"intvolume":"        60","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1002/anie.202014963"}],"publication_status":"published","day":"08","month":"03","language":[{"iso":"eng"}],"author":[{"last_name":"Ryssy","first_name":"Joonas","full_name":"Ryssy, Joonas"},{"full_name":"Natarajan, Ashwin K.","first_name":"Ashwin K.","last_name":"Natarajan"},{"last_name":"Wang","first_name":"Jinhua","full_name":"Wang, Jinhua"},{"last_name":"Lehtonen","first_name":"Arttu J.","full_name":"Lehtonen, Arttu J."},{"full_name":"Nguyen, Minh‐Kha","first_name":"Minh‐Kha","last_name":"Nguyen"},{"full_name":"Klajn, Rafal","id":"8e84690e-1e48-11ed-a02b-a1e6fb8bb53b","first_name":"Rafal","last_name":"Klajn"},{"full_name":"Kuzyk, Anton","last_name":"Kuzyk","first_name":"Anton"}],"date_published":"2021-03-08T00:00:00Z","article_processing_charge":"No","related_material":{"link":[{"relation":"erratum","url":"https://doi.org/10.1002/anie.202210394"}]},"doi":"10.1002/anie.202014963","date_updated":"2023-08-02T07:22:23Z","keyword":["General Chemistry","Catalysis"],"scopus_import":"1","quality_controlled":"1","volume":60,"page":"5859-5863","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"journal_article","_id":"13358","year":"2021","oa":1,"status":"public","issue":"11","article_type":"original","citation":{"ieee":"J. Ryssy <i>et al.</i>, “Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies,” <i>Angewandte Chemie International Edition</i>, vol. 60, no. 11. Wiley, pp. 5859–5863, 2021.","chicago":"Ryssy, Joonas, Ashwin K. Natarajan, Jinhua Wang, Arttu J. Lehtonen, Minh‐Kha Nguyen, Rafal Klajn, and Anton Kuzyk. “Light‐responsive Dynamic DNA‐origami‐based Plasmonic Assemblies.” <i>Angewandte Chemie International Edition</i>. Wiley, 2021. <a href=\"https://doi.org/10.1002/anie.202014963\">https://doi.org/10.1002/anie.202014963</a>.","apa":"Ryssy, J., Natarajan, A. K., Wang, J., Lehtonen, A. J., Nguyen, M., Klajn, R., &#38; Kuzyk, A. (2021). Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies. <i>Angewandte Chemie International Edition</i>. Wiley. <a href=\"https://doi.org/10.1002/anie.202014963\">https://doi.org/10.1002/anie.202014963</a>","ama":"Ryssy J, Natarajan AK, Wang J, et al. Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies. <i>Angewandte Chemie International Edition</i>. 2021;60(11):5859-5863. doi:<a href=\"https://doi.org/10.1002/anie.202014963\">10.1002/anie.202014963</a>","ista":"Ryssy J, Natarajan AK, Wang J, Lehtonen AJ, Nguyen M, Klajn R, Kuzyk A. 2021. Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies. Angewandte Chemie International Edition. 60(11), 5859–5863.","mla":"Ryssy, Joonas, et al. “Light‐responsive Dynamic DNA‐origami‐based Plasmonic Assemblies.” <i>Angewandte Chemie International Edition</i>, vol. 60, no. 11, Wiley, 2021, pp. 5859–63, doi:<a href=\"https://doi.org/10.1002/anie.202014963\">10.1002/anie.202014963</a>.","short":"J. Ryssy, A.K. Natarajan, J. Wang, A.J. Lehtonen, M. Nguyen, R. Klajn, A. Kuzyk, Angewandte Chemie International Edition 60 (2021) 5859–5863."},"publication_identifier":{"issn":["1433-7851"],"eissn":["1521-3773"]},"publication":"Angewandte Chemie International Edition","title":"Light‐responsive dynamic DNA‐origami‐based plasmonic assemblies","publisher":"Wiley","date_created":"2023-08-01T09:35:06Z","oa_version":"Published Version","abstract":[{"text":"DNA nanotechnology offers a versatile toolbox for precise spatial and temporal manipulation of matter on the nanoscale. However, rendering DNA-based systems responsive to light has remained challenging. Herein, we describe the remote manipulation of native (non-photoresponsive) chiral plasmonic molecules (CPMs) using light. Our strategy is based on the use of a photoresponsive medium comprising a merocyanine-based photoacid. Upon exposure to visible light, the medium decreases its pH, inducing the formation of DNA triplex links, leading to a spatial reconfiguration of the CPMs. The process can be reversed simply by turning the light off and it can be repeated for multiple cycles. The degree of the overall chirality change in an ensemble of CPMs depends on the CPM fraction undergoing reconfiguration, which, remarkably, depends on and can be tuned by the intensity of incident light. Such a dynamic, remotely controlled system could aid in further advancing DNA-based devices and nanomaterials.","lang":"eng"}],"extern":"1"},{"year":"2021","_id":"13359","type":"journal_article","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","page":"23-37","volume":7,"publication_identifier":{"issn":["2451-9294"]},"citation":{"short":"M. Weißenfels, J. Gemen, R. Klajn, Chem 7 (2021) 23–37.","mla":"Weißenfels, Maren, et al. “Dissipative Self-Assembly: Fueling with Chemicals versus Light.” <i>Chem</i>, vol. 7, no. 1, Elsevier, 2021, pp. 23–37, doi:<a href=\"https://doi.org/10.1016/j.chempr.2020.11.025\">10.1016/j.chempr.2020.11.025</a>.","ista":"Weißenfels M, Gemen J, Klajn R. 2021. Dissipative self-assembly: Fueling with chemicals versus light. Chem. 7(1), 23–37.","ama":"Weißenfels M, Gemen J, Klajn R. Dissipative self-assembly: Fueling with chemicals versus light. <i>Chem</i>. 2021;7(1):23-37. doi:<a href=\"https://doi.org/10.1016/j.chempr.2020.11.025\">10.1016/j.chempr.2020.11.025</a>","apa":"Weißenfels, M., Gemen, J., &#38; Klajn, R. (2021). Dissipative self-assembly: Fueling with chemicals versus light. <i>Chem</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.chempr.2020.11.025\">https://doi.org/10.1016/j.chempr.2020.11.025</a>","chicago":"Weißenfels, Maren, Julius Gemen, and Rafal Klajn. “Dissipative Self-Assembly: Fueling with Chemicals versus Light.” <i>Chem</i>. Elsevier, 2021. <a href=\"https://doi.org/10.1016/j.chempr.2020.11.025\">https://doi.org/10.1016/j.chempr.2020.11.025</a>.","ieee":"M. Weißenfels, J. Gemen, and R. Klajn, “Dissipative self-assembly: Fueling with chemicals versus light,” <i>Chem</i>, vol. 7, no. 1. Elsevier, pp. 23–37, 2021."},"article_type":"original","issue":"1","status":"public","oa":1,"oa_version":"Published Version","date_created":"2023-08-01T09:35:19Z","publisher":"Elsevier","title":"Dissipative self-assembly: Fueling with chemicals versus light","publication":"Chem","extern":"1","abstract":[{"lang":"eng","text":"Dissipative self-assembly is ubiquitous in nature, where it gives rise to complex structures and functions such as self-healing, homeostasis, and camouflage. These phenomena are enabled by the continuous conversion of energy stored in chemical fuels, such as ATP. Over the past decade, an increasing number of synthetic chemically driven systems have been reported that mimic the features of their natural counterparts. At the same time, it has been shown that dissipative self-assembly can also be fueled by light; these optically fueled systems have been developed in parallel to the chemically fueled ones. In this perspective, we critically compare these two classes of systems. Despite the complementarity and fundamental differences between these two modes of dissipative self-assembly, our analysis reveals that multiple analogies exist between chemically and light-fueled systems. We hope that these considerations will facilitate further development of the field of dissipative self-assembly."}],"publication_status":"published","intvolume":"         7","main_file_link":[{"url":"https://doi.org/10.1016/j.chempr.2020.11.025","open_access":"1"}],"language":[{"iso":"eng"}],"month":"01","day":"14","quality_controlled":"1","scopus_import":"1","keyword":["Materials Chemistry","Biochemistry (medical)","General Chemical Engineering","Environmental Chemistry","Biochemistry","General Chemistry"],"date_updated":"2023-08-07T10:04:28Z","doi":"10.1016/j.chempr.2020.11.025","article_processing_charge":"No","author":[{"full_name":"Weißenfels, Maren","first_name":"Maren","last_name":"Weißenfels"},{"full_name":"Gemen, Julius","first_name":"Julius","last_name":"Gemen"},{"id":"8e84690e-1e48-11ed-a02b-a1e6fb8bb53b","full_name":"Klajn, Rafal","last_name":"Klajn","first_name":"Rafal"}],"date_published":"2021-01-14T00:00:00Z"},{"publisher":"Wiley","publication":"Out‐of‐Equilibrium (Supra)molecular Systems and Materials","title":"Controlling Self‐Assembly of Nanoparticles Using Light","date_created":"2023-08-01T09:35:35Z","oa_version":"None","article_processing_charge":"No","date_updated":"2023-08-02T07:28:09Z","doi":"10.1002/9783527821990.ch9","date_published":"2021-04-19T00:00:00Z","author":[{"full_name":"Bian, Tong","first_name":"Tong","last_name":"Bian"},{"last_name":"Chu","first_name":"Zonglin","full_name":"Chu, Zonglin"},{"last_name":"Klajn","first_name":"Rafal","id":"8e84690e-1e48-11ed-a02b-a1e6fb8bb53b","full_name":"Klajn, Rafal"}],"editor":[{"last_name":"Giuseppone","first_name":"Nicolas","full_name":"Giuseppone, Nicolas"},{"full_name":"Walther, Andreas","last_name":"Walther","first_name":"Andreas"}],"extern":"1","quality_controlled":"1","scopus_import":"1","abstract":[{"text":"Inorganic nanoparticles (NPs) exhibit a wide range of fascinating physicochemical properties, many of which can be controlled by modulating the NP–NP coupling. Controlling the self-assembly of NPs using light has traditionally been achieved by functionalizing their surfaces with monolayers of photoswitchable molecules, which can be reversibly isomerized between two or more states upon exposure to different wavelengths of light. NPs whose assembly can be controlled by light in a reversible fashion can find interesting applications. The chapter deals with systems comprising mixtures of non-photoswitchable NPs and small-molecule photoacids and photobases. Examples of light-controlled self-assembly of NPs hitherto reported have been categorized into six distinct approaches. These are: functionalizing NPs with monolayers of photoswitchable molecules, light-controlled adsorption/desorption of photoswitchable molecules onto NPs, and light-induced electron transfer between the particle's inorganic core and the NP-bound ligands.","lang":"eng"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"book_chapter","page":"241-273","year":"2021","publication_status":"published","_id":"13360","day":"19","status":"public","month":"04","publication_identifier":{"eisbn":["9783527821990"],"isbn":["9783527346158"]},"language":[{"iso":"eng"}],"citation":{"ama":"Bian T, Chu Z, Klajn R. Controlling Self‐Assembly of Nanoparticles Using Light. In: Giuseppone N, Walther A, eds. <i>Out‐of‐Equilibrium (Supra)Molecular Systems and Materials</i>. Wiley; 2021:241-273. doi:<a href=\"https://doi.org/10.1002/9783527821990.ch9\">10.1002/9783527821990.ch9</a>","ista":"Bian T, Chu Z, Klajn R. 2021.Controlling Self‐Assembly of Nanoparticles Using Light. In: Out‐of‐Equilibrium (Supra)molecular Systems and Materials. , 241–273.","mla":"Bian, Tong, et al. “Controlling Self‐Assembly of Nanoparticles Using Light.” <i>Out‐of‐Equilibrium (Supra)Molecular Systems and Materials</i>, edited by Nicolas Giuseppone and Andreas Walther, Wiley, 2021, pp. 241–73, doi:<a href=\"https://doi.org/10.1002/9783527821990.ch9\">10.1002/9783527821990.ch9</a>.","short":"T. Bian, Z. Chu, R. Klajn, in:, N. Giuseppone, A. Walther (Eds.), Out‐of‐Equilibrium (Supra)Molecular Systems and Materials, Wiley, 2021, pp. 241–273.","chicago":"Bian, Tong, Zonglin Chu, and Rafal Klajn. “Controlling Self‐Assembly of Nanoparticles Using Light.” In <i>Out‐of‐Equilibrium (Supra)Molecular Systems and Materials</i>, edited by Nicolas Giuseppone and Andreas Walther, 241–73. Wiley, 2021. <a href=\"https://doi.org/10.1002/9783527821990.ch9\">https://doi.org/10.1002/9783527821990.ch9</a>.","ieee":"T. Bian, Z. Chu, and R. Klajn, “Controlling Self‐Assembly of Nanoparticles Using Light,” in <i>Out‐of‐Equilibrium (Supra)molecular Systems and Materials</i>, N. Giuseppone and A. Walther, Eds. Wiley, 2021, pp. 241–273.","apa":"Bian, T., Chu, Z., &#38; Klajn, R. (2021). Controlling Self‐Assembly of Nanoparticles Using Light. In N. Giuseppone &#38; A. Walther (Eds.), <i>Out‐of‐Equilibrium (Supra)molecular Systems and Materials</i> (pp. 241–273). Wiley. <a href=\"https://doi.org/10.1002/9783527821990.ch9\">https://doi.org/10.1002/9783527821990.ch9</a>"}},{"arxiv":1,"extern":"1","abstract":[{"lang":"eng","text":"Most massive stars are born in binaries close enough for mass transfer episodes. These modify the appearance, structure, and future evolution of both stars. We compute the evolution of a 100-day-period binary, consisting initially of a 25 M⊙ star and a 17 M⊙ star, which experiences stable mass transfer. We focus on the impact of mass accretion on the surface composition, internal rotation, and structure of the accretor. To anchor our models, we show that our accretor broadly reproduces the properties of ζ Ophiuchi, which has long been proposed to have accreted mass before being ejected as a runaway star when the companion exploded. We compare our accretor to models of single rotating stars and find that the later and stronger spin-up provided by mass accretion produces significant differences. Specifically, the core of the accretor retains higher spin at the end of the main sequence, and a convective layer develops that changes its density profile. Moreover, the surface of the accretor star is polluted by CNO-processed material donated by the companion. Our models show effects of mass accretion in binaries that are not captured in single rotating stellar models. This possibly impacts the further evolution (either in a binary or as single stars), the final collapse, and the resulting spin of the compact object."}],"publisher":"American Astronomical Society","title":"Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi","publication":"The Astrophysical Journal","oa_version":"Preprint","date_created":"2023-08-03T10:10:48Z","article_type":"original","external_id":{"arxiv":["2107.10933"]},"issue":"2","status":"public","oa":1,"publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"citation":{"ista":"Renzo M, Götberg YLL. 2021. Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi. The Astrophysical Journal. 923(2), 277.","short":"M. Renzo, Y.L.L. Götberg, The Astrophysical Journal 923 (2021).","mla":"Renzo, M., and Ylva Louise Linsdotter Götberg. “Evolution of Accretor Stars in Massive Binaries: Broader Implications from Modeling ζ Ophiuchi.” <i>The Astrophysical Journal</i>, vol. 923, no. 2, 277, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-4357/ac29c5\">10.3847/1538-4357/ac29c5</a>.","ama":"Renzo M, Götberg YLL. Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi. <i>The Astrophysical Journal</i>. 2021;923(2). doi:<a href=\"https://doi.org/10.3847/1538-4357/ac29c5\">10.3847/1538-4357/ac29c5</a>","apa":"Renzo, M., &#38; Götberg, Y. L. L. (2021). Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ac29c5\">https://doi.org/10.3847/1538-4357/ac29c5</a>","ieee":"M. Renzo and Y. L. L. Götberg, “Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi,” <i>The Astrophysical Journal</i>, vol. 923, no. 2. American Astronomical Society, 2021.","chicago":"Renzo, M., and Ylva Louise Linsdotter Götberg. “Evolution of Accretor Stars in Massive Binaries: Broader Implications from Modeling ζ Ophiuchi.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-4357/ac29c5\">https://doi.org/10.3847/1538-4357/ac29c5</a>."},"type":"journal_article","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","volume":923,"year":"2021","_id":"13453","doi":"10.3847/1538-4357/ac29c5","date_updated":"2023-08-21T11:59:34Z","article_processing_charge":"No","date_published":"2021-12-29T00:00:00Z","author":[{"full_name":"Renzo, M.","first_name":"M.","last_name":"Renzo"},{"id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","full_name":"Götberg, Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","last_name":"Götberg","first_name":"Ylva Louise Linsdotter"}],"quality_controlled":"1","scopus_import":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"article_number":"277","day":"29","language":[{"iso":"eng"}],"month":"12","publication_status":"published","main_file_link":[{"url":"https://arxiv.org/abs/2107.10933","open_access":"1"}],"intvolume":"       923"},{"publication_status":"published","intvolume":"       922","main_file_link":[{"url":"https://arxiv.org/abs/2109.14817","open_access":"1"}],"day":"03","month":"12","language":[{"iso":"eng"}],"article_number":"241","article_processing_charge":"No","date_updated":"2023-08-21T11:52:05Z","doi":"10.3847/1538-4357/ac27ae","date_published":"2021-12-03T00:00:00Z","author":[{"last_name":"Wong","first_name":"Tin Long Sunny","full_name":"Wong, Tin Long Sunny"},{"last_name":"Schwab","first_name":"Josiah","full_name":"Schwab, Josiah"},{"full_name":"Götberg, Ylva Louise Linsdotter","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","first_name":"Ylva Louise Linsdotter","last_name":"Götberg","orcid":"0000-0002-6960-6911"}],"quality_controlled":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"scopus_import":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"journal_article","volume":922,"year":"2021","_id":"13454","issue":"2","article_type":"original","external_id":{"arxiv":["2109.14817"]},"oa":1,"status":"public","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"citation":{"chicago":"Wong, Tin Long Sunny, Josiah Schwab, and Ylva Louise Linsdotter Götberg. “Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-4357/ac27ae\">https://doi.org/10.3847/1538-4357/ac27ae</a>.","ieee":"T. L. S. Wong, J. Schwab, and Y. L. L. Götberg, “Pre-explosion properties of Helium star donors to thermonuclear supernovae,” <i>The Astrophysical Journal</i>, vol. 922, no. 2. American Astronomical Society, 2021.","apa":"Wong, T. L. S., Schwab, J., &#38; Götberg, Y. L. L. (2021). Pre-explosion properties of Helium star donors to thermonuclear supernovae. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ac27ae\">https://doi.org/10.3847/1538-4357/ac27ae</a>","ama":"Wong TLS, Schwab J, Götberg YLL. Pre-explosion properties of Helium star donors to thermonuclear supernovae. <i>The Astrophysical Journal</i>. 2021;922(2). doi:<a href=\"https://doi.org/10.3847/1538-4357/ac27ae\">10.3847/1538-4357/ac27ae</a>","mla":"Wong, Tin Long Sunny, et al. “Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae.” <i>The Astrophysical Journal</i>, vol. 922, no. 2, 241, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-4357/ac27ae\">10.3847/1538-4357/ac27ae</a>.","short":"T.L.S. Wong, J. Schwab, Y.L.L. Götberg, The Astrophysical Journal 922 (2021).","ista":"Wong TLS, Schwab J, Götberg YLL. 2021. Pre-explosion properties of Helium star donors to thermonuclear supernovae. The Astrophysical Journal. 922(2), 241."},"publisher":"American Astronomical Society","publication":"The Astrophysical Journal","title":"Pre-explosion properties of Helium star donors to thermonuclear supernovae","date_created":"2023-08-03T10:10:58Z","oa_version":"Preprint","arxiv":1,"extern":"1","abstract":[{"lang":"eng","text":"Helium star–carbon-oxygen white dwarf (CO WD) binaries are potential single-degenerate progenitor systems of thermonuclear supernovae. Revisiting a set of binary evolution calculations using the stellar evolution code MESA, we refine our previous predictions about which systems can lead to a thermonuclear supernova and then characterize the properties of the helium star donor at the time of explosion. We convert these model properties to near-UV/optical magnitudes assuming a blackbody spectrum and support this approach using a matched stellar atmosphere model. These models will be valuable to compare with pre-explosion imaging for future supernovae, though we emphasize the observational difficulty of detecting extremely blue companions. The pre-explosion source detected in association with SN 2012Z has been interpreted as a helium star binary containing an initially ultra-massive WD in a multiday orbit. However, extending our binary models to initial CO WD masses of up to 1.2 M⊙, we find that these systems undergo off-center carbon ignitions and thus are not expected to produce thermonuclear supernovae. This tension suggests that, if SN 2012Z is associated with a helium star–WD binary, then the pre-explosion optical light from the system must be significantly modified by the binary environment and/or the WD does not have a carbon-rich interior composition."}]},{"quality_controlled":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"scopus_import":"1","article_processing_charge":"No","doi":"10.1051/0004-6361/202140506","date_updated":"2023-08-21T11:49:15Z","author":[{"full_name":"Laplace, E.","last_name":"Laplace","first_name":"E."},{"full_name":"Justham, S.","last_name":"Justham","first_name":"S."},{"first_name":"M.","last_name":"Renzo","full_name":"Renzo, M."},{"first_name":"Ylva Louise Linsdotter","last_name":"Götberg","orcid":"0000-0002-6960-6911","full_name":"Götberg, Ylva Louise Linsdotter","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d"},{"first_name":"R.","last_name":"Farmer","full_name":"Farmer, R."},{"first_name":"D.","last_name":"Vartanyan","full_name":"Vartanyan, D."},{"last_name":"de Mink","first_name":"S. E.","full_name":"de Mink, S. E."}],"date_published":"2021-12-02T00:00:00Z","article_number":"A58","month":"12","language":[{"iso":"eng"}],"day":"02","publication_status":"published","intvolume":"       656","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1051/0004-6361/202140506"}],"abstract":[{"lang":"eng","text":"The majority of massive stars live in binary or multiple systems and will interact with a companion during their lifetimes, which helps to explain the observed diversity of core-collapse supernovae. Donor stars in binary systems can lose most of their hydrogen-rich envelopes through mass transfer. As a result, not only are the surface properties affected, but so is the core structure. However, most calculations of the core-collapse properties of massive stars rely on single-star models. We present a systematic study of the difference between the pre-supernova structures of single stars and stars of the same initial mass (11–21 M⊙) that have been stripped due to stable post-main-sequence mass transfer at solar metallicity. We present the pre-supernova core composition with novel diagrams that give an intuitive representation of the isotope distribution. As shown in previous studies, at the edge of the carbon-oxygen core, the binary-stripped star models contain an extended gradient of carbon, oxygen, and neon. This layer remains until core collapse and is more extended in mass for higher initial stellar masses. It originates from the receding of the convective helium core during core helium burning in binary-stripped stars, which does not occur in single-star models. We find that this same evolutionary phase leads to systematic differences in the final density and nuclear energy generation profiles. Binary-stripped star models have systematically higher total masses of carbon at the moment of core collapse compared to single-star models, which likely results in systematically different supernova yields. In about half of our models, the silicon-burning and oxygen-rich layers merge after core silicon burning. We discuss the implications of our findings for the “explodability”, supernova observations, and nucleosynthesis of these stars. Our models are publicly available and can be readily used as input for detailed supernova simulations."}],"arxiv":1,"date_created":"2023-08-03T10:11:09Z","oa_version":"Published Version","publisher":"EDP Sciences","publication":"Astronomy & Astrophysics","title":"Different to the core: The pre-supernova structures of massive single and binary-stripped stars","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"citation":{"short":"E. Laplace, S. Justham, M. Renzo, Y.L.L. Götberg, R. Farmer, D. Vartanyan, S.E. de Mink, Astronomy &#38; Astrophysics 656 (2021).","ista":"Laplace E, Justham S, Renzo M, Götberg YLL, Farmer R, Vartanyan D, de Mink SE. 2021. Different to the core: The pre-supernova structures of massive single and binary-stripped stars. Astronomy &#38; Astrophysics. 656, A58.","mla":"Laplace, E., et al. “Different to the Core: The Pre-Supernova Structures of Massive Single and Binary-Stripped Stars.” <i>Astronomy &#38; Astrophysics</i>, vol. 656, A58, EDP Sciences, 2021, doi:<a href=\"https://doi.org/10.1051/0004-6361/202140506\">10.1051/0004-6361/202140506</a>.","ama":"Laplace E, Justham S, Renzo M, et al. Different to the core: The pre-supernova structures of massive single and binary-stripped stars. <i>Astronomy &#38; Astrophysics</i>. 2021;656. doi:<a href=\"https://doi.org/10.1051/0004-6361/202140506\">10.1051/0004-6361/202140506</a>","apa":"Laplace, E., Justham, S., Renzo, M., Götberg, Y. L. L., Farmer, R., Vartanyan, D., &#38; de Mink, S. E. (2021). Different to the core: The pre-supernova structures of massive single and binary-stripped stars. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202140506\">https://doi.org/10.1051/0004-6361/202140506</a>","chicago":"Laplace, E., S. Justham, M. Renzo, Ylva Louise Linsdotter Götberg, R. Farmer, D. Vartanyan, and S. E. de Mink. “Different to the Core: The Pre-Supernova Structures of Massive Single and Binary-Stripped Stars.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2021. <a href=\"https://doi.org/10.1051/0004-6361/202140506\">https://doi.org/10.1051/0004-6361/202140506</a>.","ieee":"E. Laplace <i>et al.</i>, “Different to the core: The pre-supernova structures of massive single and binary-stripped stars,” <i>Astronomy &#38; Astrophysics</i>, vol. 656. EDP Sciences, 2021."},"external_id":{"arxiv":["2102.05036"]},"article_type":"original","status":"public","oa":1,"year":"2021","_id":"13455","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"journal_article","volume":656},{"article_number":"5","quality_controlled":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"scopus_import":"1","article_processing_charge":"No","doi":"10.3847/1538-4357/ac0af6","date_updated":"2023-08-21T11:44:50Z","author":[{"full_name":"Berzin, Elizabeth","first_name":"Elizabeth","last_name":"Berzin"},{"last_name":"Secunda","first_name":"Amy","full_name":"Secunda, Amy"},{"full_name":"Cen, Renyue","last_name":"Cen","first_name":"Renyue"},{"first_name":"Alexander","last_name":"Menegas","full_name":"Menegas, Alexander"},{"last_name":"Götberg","orcid":"0000-0002-6960-6911","first_name":"Ylva Louise Linsdotter","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","full_name":"Götberg, Ylva Louise Linsdotter"}],"date_published":"2021-08-27T00:00:00Z","publication_status":"published","intvolume":"       918","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/ac0af6"}],"month":"08","language":[{"iso":"eng"}],"day":"27","date_created":"2023-08-03T10:11:24Z","oa_version":"Published Version","publisher":"American Astronomical Society","publication":"The Astrophysical Journal","title":"Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization","extern":"1","abstract":[{"lang":"eng","text":"While most simulations of the epoch of reionization have focused on single-stellar populations in star-forming dwarf galaxies, products of binary evolution are expected to significantly contribute to emissions of hydrogen-ionizing photons. Among these products are stripped stars (or helium stars), which have their envelopes stripped from interactions with binary companions, leaving an exposed helium core. Previous work has suggested these stripped stars can dominate the Lyman Continuum (LyC) photon output of high-redshift, low-luminosity galaxies post-starburst. Other sources of hard radiation in the early universe include zero-metallicity Population iii stars, which may have similar spectral energy distribution (SED) properties to galaxies with radiation dominated by stripped-star emissions. Here, we use four metrics (the power-law exponent over wavelength intervals 240–500 Å, 600–900 Å, and 1200–2000 Å, and the ratio of total luminosity in FUV wavelengths to LyC wavelengths) to compare the SEDs of simulated galaxies with only single-stellar evolution, galaxies containing stripped stars, and galaxies containing Population iii stars, with four different initial mass functions (IMFs). We find that stripped stars significantly alter SEDs in the LyC range of galaxies at the epoch of reionization. SEDs in galaxies with stripped stars have lower power-law indices in the LyC range and lower FUV to LyC luminosity ratios. These differences in SEDs are present at all considered luminosities (${M}_{\\mathrm{UV}}\\gt -15$, AB system), and are most pronounced for lower-luminosity galaxies. Intrinsic SEDs as well as those with interstellar medium absorption of galaxies with stripped stars and Population iii stars are found to be distinct for all tested Population iii IMFs."}],"arxiv":1,"year":"2021","_id":"13456","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"journal_article","volume":918,"publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"citation":{"mla":"Berzin, Elizabeth, et al. “Spectral Signatures of Population III and Envelope-Stripped Stars in Galaxies at the Epoch of Reionization.” <i>The Astrophysical Journal</i>, vol. 918, no. 1, 5, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-4357/ac0af6\">10.3847/1538-4357/ac0af6</a>.","short":"E. Berzin, A. Secunda, R. Cen, A. Menegas, Y.L.L. Götberg, The Astrophysical Journal 918 (2021).","ista":"Berzin E, Secunda A, Cen R, Menegas A, Götberg YLL. 2021. Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization. The Astrophysical Journal. 918(1), 5.","ama":"Berzin E, Secunda A, Cen R, Menegas A, Götberg YLL. Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization. <i>The Astrophysical Journal</i>. 2021;918(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/ac0af6\">10.3847/1538-4357/ac0af6</a>","apa":"Berzin, E., Secunda, A., Cen, R., Menegas, A., &#38; Götberg, Y. L. L. (2021). Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ac0af6\">https://doi.org/10.3847/1538-4357/ac0af6</a>","ieee":"E. Berzin, A. Secunda, R. Cen, A. Menegas, and Y. L. L. Götberg, “Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization,” <i>The Astrophysical Journal</i>, vol. 918, no. 1. American Astronomical Society, 2021.","chicago":"Berzin, Elizabeth, Amy Secunda, Renyue Cen, Alexander Menegas, and Ylva Louise Linsdotter Götberg. “Spectral Signatures of Population III and Envelope-Stripped Stars in Galaxies at the Epoch of Reionization.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-4357/ac0af6\">https://doi.org/10.3847/1538-4357/ac0af6</a>."},"issue":"1","external_id":{"arxiv":["2102.08408"]},"article_type":"original","oa":1,"status":"public"},{"day":"12","language":[{"iso":"eng"}],"month":"08","publication_status":"published","main_file_link":[{"url":"https://doi.org/10.1051/0004-6361/202140507","open_access":"1"}],"intvolume":"       652","doi":"10.1051/0004-6361/202140507","date_updated":"2023-08-21T11:49:36Z","article_processing_charge":"No","date_published":"2021-08-12T00:00:00Z","author":[{"full_name":"Bodensteiner, J.","last_name":"Bodensteiner","first_name":"J."},{"first_name":"H.","last_name":"Sana","full_name":"Sana, H."},{"full_name":"Wang, C.","first_name":"C.","last_name":"Wang"},{"full_name":"Langer, N.","last_name":"Langer","first_name":"N."},{"full_name":"Mahy, L.","last_name":"Mahy","first_name":"L."},{"full_name":"Banyard, G.","first_name":"G.","last_name":"Banyard"},{"last_name":"de Koter","first_name":"A.","full_name":"de Koter, A."},{"full_name":"de Mink, S. E.","first_name":"S. E.","last_name":"de Mink"},{"first_name":"C. J.","last_name":"Evans","full_name":"Evans, C. J."},{"full_name":"Götberg, Ylva Louise Linsdotter","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","first_name":"Ylva Louise Linsdotter","last_name":"Götberg","orcid":"0000-0002-6960-6911"},{"last_name":"Patrick","first_name":"L. R.","full_name":"Patrick, L. R."},{"full_name":"Schneider, F. R. N.","last_name":"Schneider","first_name":"F. R. N."},{"full_name":"Tramper, F.","last_name":"Tramper","first_name":"F."}],"quality_controlled":"1","scopus_import":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"article_number":"A70","external_id":{"arxiv":["2104.13409"]},"article_type":"original","status":"public","oa":1,"publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"citation":{"chicago":"Bodensteiner, J., H. Sana, C. Wang, N. Langer, L. Mahy, G. Banyard, A. de Koter, et al. “The Young Massive SMC Cluster NGC 330 Seen by MUSE. II. Multiplicity Properties of the Massive-Star Population.” <i>Astronomy &#38; Astrophysics</i>. EDP Sciences, 2021. <a href=\"https://doi.org/10.1051/0004-6361/202140507\">https://doi.org/10.1051/0004-6361/202140507</a>.","ieee":"J. Bodensteiner <i>et al.</i>, “The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population,” <i>Astronomy &#38; Astrophysics</i>, vol. 652. EDP Sciences, 2021.","apa":"Bodensteiner, J., Sana, H., Wang, C., Langer, N., Mahy, L., Banyard, G., … Tramper, F. (2021). The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. <i>Astronomy &#38; Astrophysics</i>. EDP Sciences. <a href=\"https://doi.org/10.1051/0004-6361/202140507\">https://doi.org/10.1051/0004-6361/202140507</a>","ama":"Bodensteiner J, Sana H, Wang C, et al. The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. <i>Astronomy &#38; Astrophysics</i>. 2021;652. doi:<a href=\"https://doi.org/10.1051/0004-6361/202140507\">10.1051/0004-6361/202140507</a>","mla":"Bodensteiner, J., et al. “The Young Massive SMC Cluster NGC 330 Seen by MUSE. II. Multiplicity Properties of the Massive-Star Population.” <i>Astronomy &#38; Astrophysics</i>, vol. 652, A70, EDP Sciences, 2021, doi:<a href=\"https://doi.org/10.1051/0004-6361/202140507\">10.1051/0004-6361/202140507</a>.","short":"J. Bodensteiner, H. Sana, C. Wang, N. Langer, L. Mahy, G. Banyard, A. de Koter, S.E. de Mink, C.J. Evans, Y.L.L. Götberg, L.R. Patrick, F.R.N. Schneider, F. Tramper, Astronomy &#38; Astrophysics 652 (2021).","ista":"Bodensteiner J, Sana H, Wang C, Langer N, Mahy L, Banyard G, de Koter A, de Mink SE, Evans CJ, Götberg YLL, Patrick LR, Schneider FRN, Tramper F. 2021. The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. Astronomy &#38; Astrophysics. 652, A70."},"type":"journal_article","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","volume":652,"year":"2021","_id":"13457","arxiv":1,"extern":"1","abstract":[{"lang":"eng","text":"Context. Observations of massive stars in open clusters younger than ∼8 Myr have shown that a majority of them are in binary systems, most of which will interact during their life. While these can be used as a proxy of the initial multiplicity properties, studying populations of massive stars older than ∼20 Myr allows us to probe the outcome of these interactions after a significant number of systems have experienced mass and angular momentum transfer and may even have merged.\r\n\r\nAims. Using multi-epoch integral-field spectroscopy, we aim to investigate the multiplicity properties of the massive-star population in the dense core of the ∼40 Myr old cluster NGC 330 in the Small Magellanic Cloud in order to search for possible imprints of stellar evolution on the multiplicity properties.\r\n\r\nMethods. We obtained six epochs of VLT/MUSE observations operated in wide-field mode with the extended wavelength setup and supported by adaptive optics. We extracted spectra and measured radial velocities for stars brighter than mF814W = 19. We identified single-lined spectroscopic binaries through significant RV variability with a peak-to-peak amplitude larger than 20 km s−1. We also identified double-lined spectroscopic binaries, and quantified the observational biases for binary detection. In particular, we took into account that binary systems with similar line strengths are difficult to detect in our data set.\r\n\r\nResults. The observed spectroscopic binary fraction among stars brighter than mF814W = 19 (approximately 5.5 M⊙ on the main sequence) is fSBobs = 13.2 ± 2.0%. Considering period and mass ratio ranges from log(P) = 0.15−3.5 (about 1.4 to 3160 d), q = 0.1−1.0, and a representative set of orbital parameter distributions, we find a bias-corrected close binary fraction of fcl = 34−7+8%. This fraction seems to decline for the fainter stars, which indicates either that the close binary fraction drops in the B-type domain, or that the period distribution becomes more heavily weighted toward longer orbital periods. We further find that both fractions vary strongly in different regions of the color-magnitude diagram, which corresponds to different evolutionary stages. This probably reveals the imprint of the binary history of different groups of stars. In particular, we find that the observed spectroscopic binary fraction of Be stars (fSBobs = 2 ± 2%) is significantly lower than that of B-type stars (fSBobs = 9 ± 2%).\r\n\r\nConclusions. We provide the first homogeneous radial velocity study of a large sample of B-type stars at a low metallicity ([Fe/H] ≲ −1.0). The overall bias-corrected close binary fraction (log(P) < 3.5 d) of the B-star population in NGC 330 is lower than the fraction reported for younger Galactic and Large Magellanic Cloud clusters in previous works. More data are needed, however, to establish whether the observed differences are caused by an age or a metallicity effect."}],"publisher":"EDP Sciences","title":"The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population","publication":"Astronomy & Astrophysics","oa_version":"Published Version","date_created":"2023-08-03T10:11:34Z"},{"day":"23","language":[{"iso":"eng"}],"month":"07","publication_status":"published","intvolume":"       916","main_file_link":[{"url":"https://arxiv.org/abs/2104.03317","open_access":"1"}],"doi":"10.3847/2041-8213/ac0b42","date_updated":"2023-08-21T11:37:48Z","article_processing_charge":"No","date_published":"2021-07-23T00:00:00Z","author":[{"full_name":"Vartanyan, David","last_name":"Vartanyan","first_name":"David"},{"full_name":"Laplace, Eva","last_name":"Laplace","first_name":"Eva"},{"last_name":"Renzo","first_name":"Mathieu","full_name":"Renzo, Mathieu"},{"first_name":"Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","last_name":"Götberg","full_name":"Götberg, Ylva Louise Linsdotter","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d"},{"last_name":"Burrows","first_name":"Adam","full_name":"Burrows, Adam"},{"last_name":"de Mink","first_name":"Selma E.","full_name":"de Mink, Selma E."}],"quality_controlled":"1","scopus_import":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"article_number":"L5","article_type":"original","external_id":{"arxiv":["2104.03317"]},"issue":"1","oa":1,"status":"public","publication_identifier":{"eissn":["2041-8213"],"issn":["2041-8205"]},"citation":{"ama":"Vartanyan D, Laplace E, Renzo M, Götberg YLL, Burrows A, de Mink SE. Binary-stripped stars as core-collapse supernovae progenitors. <i>The Astrophysical Journal Letters</i>. 2021;916(1). doi:<a href=\"https://doi.org/10.3847/2041-8213/ac0b42\">10.3847/2041-8213/ac0b42</a>","ista":"Vartanyan D, Laplace E, Renzo M, Götberg YLL, Burrows A, de Mink SE. 2021. Binary-stripped stars as core-collapse supernovae progenitors. The Astrophysical Journal Letters. 916(1), L5.","short":"D. Vartanyan, E. Laplace, M. Renzo, Y.L.L. Götberg, A. Burrows, S.E. de Mink, The Astrophysical Journal Letters 916 (2021).","mla":"Vartanyan, David, et al. “Binary-Stripped Stars as Core-Collapse Supernovae Progenitors.” <i>The Astrophysical Journal Letters</i>, vol. 916, no. 1, L5, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/2041-8213/ac0b42\">10.3847/2041-8213/ac0b42</a>.","chicago":"Vartanyan, David, Eva Laplace, Mathieu Renzo, Ylva Louise Linsdotter Götberg, Adam Burrows, and Selma E. de Mink. “Binary-Stripped Stars as Core-Collapse Supernovae Progenitors.” <i>The Astrophysical Journal Letters</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/2041-8213/ac0b42\">https://doi.org/10.3847/2041-8213/ac0b42</a>.","ieee":"D. Vartanyan, E. Laplace, M. Renzo, Y. L. L. Götberg, A. Burrows, and S. E. de Mink, “Binary-stripped stars as core-collapse supernovae progenitors,” <i>The Astrophysical Journal Letters</i>, vol. 916, no. 1. American Astronomical Society, 2021.","apa":"Vartanyan, D., Laplace, E., Renzo, M., Götberg, Y. L. L., Burrows, A., &#38; de Mink, S. E. (2021). Binary-stripped stars as core-collapse supernovae progenitors. <i>The Astrophysical Journal Letters</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/2041-8213/ac0b42\">https://doi.org/10.3847/2041-8213/ac0b42</a>"},"type":"journal_article","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","volume":916,"year":"2021","_id":"13458","arxiv":1,"extern":"1","abstract":[{"lang":"eng","text":"Most massive stars experience binary interactions in their lifetimes that can alter both the surface and core structure of the stripped star with significant effects on their ultimate fate as core-collapse supernovae. However, core-collapse supernovae simulations to date have focused almost exclusively on the evolution of single stars. We present a systematic simulation study of single and binary-stripped stars with the same initial mass as candidates for core-collapse supernovae (11–21 M⊙). Generally, we find that binary-stripped stars core tend to have a smaller compactness parameter, with a more prominent, deeper silicon/oxygen interface, and explode preferentially to the corresponding single stars of the same initial mass. Such a dichotomy of behavior between these two modes of evolution would have important implications for supernovae statistics, including the final neutron star masses, explosion energies, and nucleosynthetic yields. Binary-stripped remnants are also well poised to populate the possible mass gap between the heaviest neutron stars and the lightest black holes. Our work presents an improvement along two fronts, as we self-consistently account for the pre-collapse stellar evolution and the subsequent explosion outcome. Even so, our results emphasize the need for more detailed stellar evolutionary models to capture the sensitive nature of explosion outcome."}],"publisher":"American Astronomical Society","title":"Binary-stripped stars as core-collapse supernovae progenitors","publication":"The Astrophysical Journal Letters","oa_version":"Preprint","date_created":"2023-08-03T10:11:45Z"},{"volume":161,"type":"journal_article","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13459","year":"2021","status":"public","oa":1,"external_id":{"arxiv":["2103.13642"]},"article_type":"original","issue":"5","citation":{"ista":"Wang L, Gies DR, Peters GJ, Götberg YLL, Chojnowski SD, Lester KV, Howell SB. 2021. The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy. The Astronomical Journal. 161(5), 248.","mla":"Wang, Luqian, et al. “The Detection and Characterization of Be+sdO Binaries from HST/STIS FUV Spectroscopy.” <i>The Astronomical Journal</i>, vol. 161, no. 5, 248, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-3881/abf144\">10.3847/1538-3881/abf144</a>.","short":"L. Wang, D.R. Gies, G.J. Peters, Y.L.L. Götberg, S.D. Chojnowski, K.V. Lester, S.B. Howell, The Astronomical Journal 161 (2021).","ama":"Wang L, Gies DR, Peters GJ, et al. The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy. <i>The Astronomical Journal</i>. 2021;161(5). doi:<a href=\"https://doi.org/10.3847/1538-3881/abf144\">10.3847/1538-3881/abf144</a>","apa":"Wang, L., Gies, D. R., Peters, G. J., Götberg, Y. L. L., Chojnowski, S. D., Lester, K. V., &#38; Howell, S. B. (2021). The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy. <i>The Astronomical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-3881/abf144\">https://doi.org/10.3847/1538-3881/abf144</a>","chicago":"Wang, Luqian, Douglas R. Gies, Geraldine J. Peters, Ylva Louise Linsdotter Götberg, S. Drew Chojnowski, Kathryn V. Lester, and Steve B. Howell. “The Detection and Characterization of Be+sdO Binaries from HST/STIS FUV Spectroscopy.” <i>The Astronomical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-3881/abf144\">https://doi.org/10.3847/1538-3881/abf144</a>.","ieee":"L. Wang <i>et al.</i>, “The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy,” <i>The Astronomical Journal</i>, vol. 161, no. 5. American Astronomical Society, 2021."},"publication_identifier":{"eissn":["1538-3881"],"issn":["0004-6256"]},"title":"The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy","publication":"The Astronomical Journal","publisher":"American Astronomical Society","oa_version":"Preprint","date_created":"2023-08-03T10:11:57Z","arxiv":1,"abstract":[{"text":"The B emission-line stars are rapid rotators that were probably spun up by mass and angular momentum accretion through mass transfer in an interacting binary. Mass transfer will strip the donor star of its envelope to create a small and hot subdwarf remnant. Here we report on Hubble Space Telescope/STIS far-ultraviolet spectroscopy of a sample of Be stars that reveals the presence of the hot sdO companion through the calculation of cross-correlation functions of the observed and model spectra. We clearly detect the spectral signature of the sdO star in 10 of the 13 stars in the sample, and the spectral signals indicate that the sdO stars are hot, relatively faint, and slowly rotating as predicted by models. A comparison of their temperatures and radii with evolutionary tracks indicates that the sdO stars occupy the relatively long-lived, He-core burning stage. Only 1 of the 10 detections was a known binary prior to this investigation, which emphasizes the difficulty of finding such Be+sdO binaries through optical spectroscopy. However, these results and others indicate that many Be stars probably host hot subdwarf companions.","lang":"eng"}],"extern":"1","intvolume":"       161","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2103.13642"}],"publication_status":"published","day":"04","language":[{"iso":"eng"}],"month":"05","article_number":"248","date_published":"2021-05-04T00:00:00Z","author":[{"full_name":"Wang, Luqian","first_name":"Luqian","last_name":"Wang"},{"full_name":"Gies, Douglas R.","first_name":"Douglas R.","last_name":"Gies"},{"last_name":"Peters","first_name":"Geraldine J.","full_name":"Peters, Geraldine J."},{"id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","full_name":"Götberg, Ylva Louise Linsdotter","last_name":"Götberg","orcid":"0000-0002-6960-6911","first_name":"Ylva Louise Linsdotter"},{"full_name":"Chojnowski, S. Drew","first_name":"S. Drew","last_name":"Chojnowski"},{"full_name":"Lester, Kathryn V.","last_name":"Lester","first_name":"Kathryn V."},{"full_name":"Howell, Steve B.","last_name":"Howell","first_name":"Steve B."}],"date_updated":"2023-08-21T11:35:50Z","doi":"10.3847/1538-3881/abf144","article_processing_charge":"No","scopus_import":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"quality_controlled":"1"},{"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","type":"journal_article","volume":7,"year":"2021","_id":"13995","issue":"49","article_type":"original","external_id":{"pmid":["34860540"]},"oa":1,"status":"public","publication_identifier":{"eissn":["2375-2548"]},"citation":{"apa":"Heck, S., Baykusheva, D. R., Han, M., Ji, J.-B., Perry, C., Gong, X., &#38; Wörner, H. J. (2021). Attosecond interferometry of shape resonances in the recoil frame of CF4. <i>Science Advances</i>. American Association for the Advancement of Science. <a href=\"https://doi.org/10.1126/sciadv.abj8121\">https://doi.org/10.1126/sciadv.abj8121</a>","chicago":"Heck, Saijoscha, Denitsa Rangelova Baykusheva, Meng Han, Jia-Bao Ji, Conaill Perry, Xiaochun Gong, and Hans Jakob Wörner. “Attosecond Interferometry of Shape Resonances in the Recoil Frame of CF4.” <i>Science Advances</i>. American Association for the Advancement of Science, 2021. <a href=\"https://doi.org/10.1126/sciadv.abj8121\">https://doi.org/10.1126/sciadv.abj8121</a>.","ieee":"S. Heck <i>et al.</i>, “Attosecond interferometry of shape resonances in the recoil frame of CF4,” <i>Science Advances</i>, vol. 7, no. 49. American Association for the Advancement of Science, 2021.","ista":"Heck S, Baykusheva DR, Han M, Ji J-B, Perry C, Gong X, Wörner HJ. 2021. Attosecond interferometry of shape resonances in the recoil frame of CF4. Science Advances. 7(49), abj8121.","short":"S. Heck, D.R. Baykusheva, M. Han, J.-B. Ji, C. Perry, X. Gong, H.J. Wörner, Science Advances 7 (2021).","mla":"Heck, Saijoscha, et al. “Attosecond Interferometry of Shape Resonances in the Recoil Frame of CF4.” <i>Science Advances</i>, vol. 7, no. 49, abj8121, American Association for the Advancement of Science, 2021, doi:<a href=\"https://doi.org/10.1126/sciadv.abj8121\">10.1126/sciadv.abj8121</a>.","ama":"Heck S, Baykusheva DR, Han M, et al. Attosecond interferometry of shape resonances in the recoil frame of CF4. <i>Science Advances</i>. 2021;7(49). doi:<a href=\"https://doi.org/10.1126/sciadv.abj8121\">10.1126/sciadv.abj8121</a>"},"publisher":"American Association for the Advancement of Science","publication":"Science Advances","title":"Attosecond interferometry of shape resonances in the recoil frame of CF4","date_created":"2023-08-09T13:09:02Z","oa_version":"Published Version","extern":"1","abstract":[{"text":"Shape resonances play a central role in many areas of science, but the real-time measurement of the associated many-body dynamics remains challenging. Here, we present measurements of recoil frame angle-resolved photoionization delays in the vicinity of shape resonances of CF4. This technique provides insights into the spatiotemporal photoionization dynamics of molecular shape resonances. We find delays of up to ∼600 as in the ionization out of the highest occupied molecular orbital (HOMO) with a strong dependence on the emission direction and a pronounced asymmetry along the dissociation axis. Comparison with quantum-scattering calculations traces the asymmetries to the interference of a small subset of partial waves at low kinetic energies and, additionally, to the interference of two overlapping shape resonances in the HOMO-1 channel. Our experimental and theoretical results establish a broadly applicable approach to space- and time-resolved photoionization dynamics in the molecular frame.","lang":"eng"}],"publication_status":"published","intvolume":"         7","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1126/sciadv.abj8121"}],"day":"03","pmid":1,"month":"12","language":[{"iso":"eng"}],"article_number":"abj8121","article_processing_charge":"No","doi":"10.1126/sciadv.abj8121","date_updated":"2023-08-22T07:30:25Z","date_published":"2021-12-03T00:00:00Z","author":[{"last_name":"Heck","first_name":"Saijoscha","full_name":"Heck, Saijoscha"},{"id":"71b4d059-2a03-11ee-914d-dfa3beed6530","full_name":"Baykusheva, Denitsa Rangelova","last_name":"Baykusheva","first_name":"Denitsa Rangelova"},{"last_name":"Han","first_name":"Meng","full_name":"Han, Meng"},{"last_name":"Ji","first_name":"Jia-Bao","full_name":"Ji, Jia-Bao"},{"full_name":"Perry, Conaill","first_name":"Conaill","last_name":"Perry"},{"full_name":"Gong, Xiaochun","first_name":"Xiaochun","last_name":"Gong"},{"first_name":"Hans Jakob","last_name":"Wörner","full_name":"Wörner, Hans Jakob"}],"quality_controlled":"1","keyword":["Multidisciplinary"],"scopus_import":"1"}]