The Pan-STARRS1 Surveys
arXiv:1612.05560
Abstract
Pan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the Steradian Survey and the Medium Deep Survey in 5 bands (). The mean 5 point source limiting sensitivities in the stacked 3 Steradian Survey in are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals () are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively. The Pan-STARRS system and the design of the PS1 surveys are described and an overview of the resulting image and catalog data products and their basic characteristics are described together with a summary of important results. The images, reduced data products, and derived data products from the Pan-STARRS1 surveys are available to the community from the Mikulski Archive for Space Telescopes (MAST) at STScI.
arXiv comment38 pages, 29 figures, 12 tables
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