Abstract
High-redshift supernovae observed with the Hubble Space Telescope (HST) are crucial for constraining any time variation of dark energy. In a forthcoming paper (Rubin et al., in prep), we will present a cosmological analysis incorporating an updated sample of these supernovae with updated photometry. We also present improved calibrations for the HST ACS and NICMOS cameras.
Original language | English |
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Pages | 245.09 |
Publication status | Published - 1 Jan 2014 |