A revised SALT2 surface for fitting Type Ia supernova light curves
dc.contributor.author | Taylor, Georgina | |
dc.contributor.author | Lidman, Christopher | |
dc.contributor.author | Tucker, Brad | |
dc.contributor.author | Brout, D | |
dc.contributor.author | Hilton, S R | |
dc.contributor.author | Kessler, R | |
dc.date.accessioned | 2023-03-06T04:35:59Z | |
dc.date.available | 2023-03-06T04:35:59Z | |
dc.date.issued | 2021 | |
dc.date.updated | 2021-12-26T07:18:33Z | |
dc.description.abstract | We present a revised Spectral Adaptive Light Curve Template (SALT2) surface (SALT2-2021) for fitting the light curves of Type Ia supernovae (SNe Ia), which incorporates new measurements of zero-point calibration offsets and Milky Way extinction. The most notable change in the new surface occurs in the UV region. This new surface alters the distance measurements of SNe Ia, which can be used to investigate the nature of dark energy by probing the expansion history of the Universe. Using the revised SALT2 surface on public data from the first 3 yr of the Dark Energy Survey Supernova Program (combined with an external low-z SNe Ia sample) and combining with cosmic microwave background constraints, we find a change in the dark energy equation-of-state parameter, Δw = 0.015 ± 0.004. This result highlights the continued importance of controlling and reducing systematic uncertainties, particularly with the next generation of supernova analyses aiming to improve constraints on dark energy properties. | en_AU |
dc.description.sponsorship | This research was supported by an Australian Government Research Training Program (RTP) Scholarship. | en_AU |
dc.format.mimetype | application/pdf | en_AU |
dc.identifier.issn | 0035-8711 | en_AU |
dc.identifier.uri | http://hdl.handle.net/1885/286638 | |
dc.language.iso | en_AU | en_AU |
dc.provenance | https://v2.sherpa.ac.uk/id/publication/24618/..."published version can be archived in institutional repository" from SHERPA/RoMEO site as at 06/03/2023 | en_AU |
dc.publisher | Blackwell Publishing Ltd | en_AU |
dc.rights | © 2021 The authors | en_AU |
dc.source | Monthly Notices of the Royal Astronomical Society | en_AU |
dc.subject | supernovae: general | en_AU |
dc.subject | dark energy | en_AU |
dc.title | A revised SALT2 surface for fitting Type Ia supernova light curves | en_AU |
dc.type | Journal article | en_AU |
dcterms.accessRights | Open Access | en_AU |
local.bibliographicCitation.issue | 3 | en_AU |
local.bibliographicCitation.lastpage | 4122 | en_AU |
local.bibliographicCitation.startpage | 4111 | en_AU |
local.contributor.affiliation | Taylor, Georgina, College of Science, ANU | en_AU |
local.contributor.affiliation | Lidman, Christopher, College of Science, ANU | en_AU |
local.contributor.affiliation | Tucker, Brad, College of Science, ANU | en_AU |
local.contributor.affiliation | Brout, D, University of Pennsylvania | en_AU |
local.contributor.affiliation | Hilton, S R, University of Queensland | en_AU |
local.contributor.affiliation | Kessler, R, University of Chicago | en_AU |
local.contributor.authoremail | u4362859@anu.edu.au | en_AU |
local.contributor.authoruid | Taylor, Georgina, u6253153 | en_AU |
local.contributor.authoruid | Lidman, Christopher, u3712407 | en_AU |
local.contributor.authoruid | Tucker, Brad, u4362859 | en_AU |
local.description.notes | Imported from ARIES | en_AU |
local.identifier.absfor | 510103 - Cosmology and extragalactic astronomy | en_AU |
local.identifier.absfor | 510106 - High energy astrophysics and galactic cosmic rays | en_AU |
local.identifier.absseo | 280120 - Expanding knowledge in the physical sciences | en_AU |
local.identifier.ariespublication | a383154xPUB19681 | en_AU |
local.identifier.citationvolume | 504 | en_AU |
local.identifier.doi | 10.1093/mnras/stab962 | en_AU |
local.identifier.scopusID | 2-s2.0-85107875896 | |
local.identifier.uidSubmittedBy | a383154 | en_AU |
local.publisher.url | https://academic.oup.com/ | en_AU |
local.type.status | Published Version | en_AU |
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