Carnegie supernova project-II: Extending the near-infrared hubble diagram for type ia supernovae to z ~ 0.1
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Authors
Phillips, M. M.
Contreras, C
Hsiao, E Y
Morrell, N
Burns, Christopher R
Stritzinger, M
Ashall, C.
Freedman, Wendy L
Hoeflich, P.
Persson, S E
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University of Chicago Press
Abstract
The Carnegie Supernova Project-II (CSP-II) was an NSF-funded, four-year program to obtain optical and near-infrared observations of a "Cosmology" sample of ~100 Type Ia supernovae located in the smooth Hubble flow (0.03 lesssim z lesssim 0.10). Light curves were also obtained of a "Physics" sample composed of 90 nearby Type Ia supernovae at z ≤ 0.04 selected for near-infrared spectroscopic timeseries observations. The primary emphasis of the CSP-II is to use the combination of optical and near-infrared photometry to achieve a distance precision of better than 5%. In this paper, details of the supernova sample, the observational strategy, and the characteristics of the photometric data are provided. In a companion paper, the near-infrared spectroscopy component of the project is presented.
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Publications of the Astronomical Society of the Pacific
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Restricted until
2099-12-31