Light-curve parameters from the SNLS (Conley+, 2011)

Details Light-curve parameters from the SNLS (Conley+, 2011) Light-curve parameters from the SNLS (Conley+, 2011)

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..21920001c&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/192/1. Originally published in: 2011ApJS..192....1C

Computer Science

Supernovae, Redshifts, Photometry

Scientific paper

SNLS combines photometry from the deep component of the CFHT-LS (Canada-France-Hawaii Telescope Legacy survey) with extensive spectroscopic follow-up from the Keck, Very Large Telescope (VLT), and Gemini telescopes to determine SN types and measure redshifts. The photometry is carried out with MegaCam, a 1deg2 imager at the prime focus of CFHT. We use the natural systems of the SNLS, HST, SDSS, Hicken et al. (2009ApJ...700..331H), and Contreras et al. (2010AJ....139..519C) samples in our analysis, which together account for ~90% of our sample.
(1 data file).

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