A revised SALT2 surface for fitting Type Ia supernova light curves

G. Taylor*, C. Lidman, B. E. Tucker, D. Brout, S. R. Hinton, R. Kessler

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    18 Citations (Scopus)

    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.

    Original languageEnglish
    Pages (from-to)4111-4122
    Number of pages12
    JournalMonthly Notices of the Royal Astronomical Society
    Volume504
    Issue number3
    DOIs
    Publication statusPublished - 1 Jul 2021

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