A galaxy-driven model of type Ia supernova luminosity variations

Accepted/In Press date: 11 July 2022

e-pub ahead of print date: 25 July 2022

Published date: 25 July 2022

Additional Information: Funding Information: We thank the referee Mickael Rigault for comments which significantly impro v ed this paper. P.W. acknowledges support from the Science and Technology Facilities Council (STFC) grant ST/R000506/1. MS acknowledges support from EU/FP7-ERC grant 615929. LK thanks the UKRI Future Leaders Fellowship for support through the grant MR/T01881X/1. LG acknowledges financial support from the Spanish Ministerio de Ciencia e Innovacion (MCIN), the Agencia Estatal de Investigacion (AEI) 10.13039/501100011033, and the European Social Fund (ESF) 'Investing in your future' under the 2019 Ramon y Cajal program RYC2019-027683-I and the PID2020115253GA-I00 HOSTFLOWS project, from Centro Superior de Investigaciones Cientýficas (CSIC) under the PIE project 20215AT016, and the program Unidad de Excelencia Marýa de Maeztu CEX2020001058-M. This project has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (grant agreement number 759194 USNAC). Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Te xas A&M Univ ersity, Financiadora de Estudos e Projetos, Fundaçao Carlos Chagas Filho de Amparo `a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cientýfico e Tecnologico and the Ministerio da Ciencia, Tecnologia e Inovaçao, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Surv e y. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgen ¨ossische Technische Hochschule (ETH) Z ¨urich, Fermi National Accelerator Laboratory, the University of Illinois at UrbanaChampaign, the Institut de Ci `encies de l'Espai (IEEC/CSIC), the Institut de Fýsica d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universit ¨at M ¨unchen and the associated Excellence Cluster Universe, the University of Michigan, NSF's NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford Uni versity, the Uni versity of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF's NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under Grant Numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-20160597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union's Se venth Frame work Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciencia e Tecnologia (INCT) do e-Universo (CNPq grant 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. Publisher Copyright: © 2022 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Related URLs:

• http://adsabs.harvard.edu/abs/...220705583W

Keywords: cosmology: observations, dust, extinction, galaxies: evolution, supernovae: general

Local EPrints ID: 471906

URI: http://eprints.soton.ac.uk/id/eprint/471906

DOI: doi:10.1093/mnras/stac1984

ISSN: 1365-2966

PURE UUID: 9635b6ba-3861-4558-8562-682ab586a8ec

ORCID for P. Wiseman: orcid.org/0000-0002-3073-1512

ORCID for M. Sullivan: orcid.org/0000-0001-9053-4820

Date deposited: 22 Nov 2022 17:42

Last modified: 17 Mar 2024 03:48