SUPERNOVA CONSTRAINTS AND SYSTEMATIC UNCERTAINTIES FROM THE FIRST THREE YEARS OF THE SUPERNOVA LEGACY SURVEY
University of Toronto · Laboratory for Atmospheric and Space Physics · +24 more institutions
Abstract
We combine high-redshift Type Ia supernovae from the first three years of the Supernova Legacy Survey (SNLS) with other supernova (SN) samples, primarily at lower redshifts, to form a high-quality joint sample of 472 SNe (123 low-z, 93 SDSS, 242 SNLS, and 14 Hubble Space Telescope). SN data alone require cosmic acceleration at >99.999% confidence, including systematic effects. For the dark energy equation of state parameter (assumed constant out to at least z = 1.4) in a flat universe, we find w = –0.91^(+0.16)_(–0.20)(stat)^(+0.07)_(–0.14)(sys) from SNe only, consistent with a cosmological constant. Our fits include a correction for the recently discovered relationship between host-galaxy mass and SN…
Citation impact
- FWCI
- 36.76
- Percentile
- 100%
- References
- 130
Authors
36- ACA. ConleyCorresponding
University of Toronto, Laboratory for Atmospheric and Space Physics
- JGJ. Guy
Centre National de la Recherche Scientifique, Université Paris Cité, Sorbonne Université, Laboratoire de Physique Nucléaire et de Hautes Énergies
- MSM. Sullivan
University of Oxford
- NRN. Regnault
Centre National de la Recherche Scientifique, Université Paris Cité, Sorbonne Université, Laboratoire de Physique Nucléaire et de Hautes Énergies
- PAP. Astier
Centre National de la Recherche Scientifique, Université Paris Cité, Sorbonne Université, Laboratoire de Physique Nucléaire et de Hautes Énergies
Topics & keywords
- Physics
- Dark energy
- Astrophysics
- Redshift
- Luminosity
- Supernova
- Hubble's law
- Cosmological constant