A revised SALT2 surface for fitting Type Ia supernova light curves

dc.contributor.authorTaylor, Georgina
dc.contributor.authorLidman, Christopher
dc.contributor.authorTucker, Brad
dc.contributor.authorBrout, D
dc.contributor.authorHilton, S R
dc.contributor.authorKessler, R
dc.date.accessioned2023-03-06T04:35:59Z
dc.date.available2023-03-06T04:35:59Z
dc.date.issued2021
dc.date.updated2021-12-26T07:18:33Z
dc.description.abstractWe 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.sponsorshipThis research was supported by an Australian Government Research Training Program (RTP) Scholarship.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0035-8711en_AU
dc.identifier.urihttp://hdl.handle.net/1885/286638
dc.language.isoen_AUen_AU
dc.provenancehttps://v2.sherpa.ac.uk/id/publication/24618/..."published version can be archived in institutional repository" from SHERPA/RoMEO site as at 06/03/2023en_AU
dc.publisherBlackwell Publishing Ltden_AU
dc.rights© 2021 The authorsen_AU
dc.sourceMonthly Notices of the Royal Astronomical Societyen_AU
dc.subjectsupernovae: generalen_AU
dc.subjectdark energyen_AU
dc.titleA revised SALT2 surface for fitting Type Ia supernova light curvesen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue3en_AU
local.bibliographicCitation.lastpage4122en_AU
local.bibliographicCitation.startpage4111en_AU
local.contributor.affiliationTaylor, Georgina, College of Science, ANUen_AU
local.contributor.affiliationLidman, Christopher, College of Science, ANUen_AU
local.contributor.affiliationTucker, Brad, College of Science, ANUen_AU
local.contributor.affiliationBrout, D, University of Pennsylvaniaen_AU
local.contributor.affiliationHilton, S R, University of Queenslanden_AU
local.contributor.affiliationKessler, R, University of Chicagoen_AU
local.contributor.authoremailu4362859@anu.edu.auen_AU
local.contributor.authoruidTaylor, Georgina, u6253153en_AU
local.contributor.authoruidLidman, Christopher, u3712407en_AU
local.contributor.authoruidTucker, Brad, u4362859en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor510103 - Cosmology and extragalactic astronomyen_AU
local.identifier.absfor510106 - High energy astrophysics and galactic cosmic raysen_AU
local.identifier.absseo280120 - Expanding knowledge in the physical sciencesen_AU
local.identifier.ariespublicationa383154xPUB19681en_AU
local.identifier.citationvolume504en_AU
local.identifier.doi10.1093/mnras/stab962en_AU
local.identifier.scopusID2-s2.0-85107875896
local.identifier.uidSubmittedBya383154en_AU
local.publisher.urlhttps://academic.oup.com/en_AU
local.type.statusPublished Versionen_AU

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