A cosmology-independent calibration of Type Ia supernovae data. Issue 3 (29th June 2018)

• Record Type: Journal Article
• Authors: Hauret, C; Magain, P; Biernaux, J
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 479:Issue 3(2018)
• Page Start: 3996
• Page End: 4003
• Publication Date: 2018-06-29
• Subjects: methods: data analysis -- supernovae: general -- cosmology: miscellaneous; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/sty1715
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Recently, the common methodology used to transform Type Ia supernovae (SNe Ia) into genuine standard candles has been suffering criticism. Indeed, it assumes a particular cosmological model [namely the flat Λ cold dark matter (ΛCDM)] to calibrate the standardization corrections parameters, i.e. the dependence of the supernova peak absolute magnitude on its colour, post-maximum decline rate and host galaxy mass. As a result, this assumption could make the data compliant to the assumed cosmology and thus nullify all works previously conducted on model comparison. In this work, we verify the viability of these hypotheses by developing a cosmology-independent approach to standardize SNe Ia data from the recent JLA compilation. Our resulting corrections turn out to be very close to the ΛCDM-based corrections. Therefore, even if a ΛCDM-based calibration is questionable from a theoretical point of view, the potential compliance of SNe Ia data does not happen in practice for the JLA compilation. Previous works of model comparison based on these data do not have to be called into question. However, as this cosmology-independent standardization method has the same degree of complexity than the model-dependent one, it is worth using it in future works, especially if smaller samples are considered, such as the superluminous Type Ic supernovae.