Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology
  We describe the creation, content, and validation of the Dark Energy Survey
(DES) internal year-one cosmology data set, Y1A1 GOLD, in support of upcoming
cosmological analyses. The Y1A1 GOLD data set is assembled from multiple epochs
of DES imaging and consists of calibrated photometric zeropoints, object
catalogs, and ancillary data products - e.g., maps of survey depth and
observing conditions, star-galaxy classification, and photometric redshift
estimates - that are necessary for accurate cosmological analyses. The Y1A1
GOLD wide-area object catalog consists of ~137 million objects detected in
coadded images covering ~1800 deg$^2$ in the DES grizY filters. The 10{\sigma}
limiting magnitude for galaxies is g = 23.4, r = 23.2, i = 22.5, z = 21.8, and
Y = 20.1. Photometric calibration of Y1A1 GOLD was performed by combining
nightly zeropoint solutions with stellar-locus regression, and the absolute
calibration accuracy is better than 2% over the survey area. DES Y1A1 GOLD is
the largest photometric data set at the achieved depth to date, enabling
precise measurements of cosmic acceleration at z $\lesssim$ 1.
