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SkyMapper Southern Survey: Second data release (DR2)

Christopher A. OnkenAustralian Research Council (ARC) Centre of Excellence for All-sky Astrophysics (CAASTROChristian WolfAustralian Research Council (ARC) Centre of Excellence for All-sky Astrophysics (CAASTROMichael S. BessellResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaSeo-Won ChangAustralian Research Council (ARC) Centre of Excellence for All-sky Astrophysics (CAASTROGary S. Da CostaResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaLance C. LuvaulResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaDougal MackeyResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaBrian P. SchmidtAustralian Research Council (ARC) Centre of Excellence for All-sky Astrophysics (CAASTROLi ShaoKavli Institute for Astronomy and Astrophysics, Peking University, 5 Yiheyuan Road, Haidian District, Beijing 100871, P. R.China
2019en
ABI

Аннотация

Abstract We present the second data release (DR2) of the SkyMapper Southern Survey, a hemispheric survey carried out with the SkyMapper Telescope at Siding Spring Observatory in Australia, using six optical filters: u, v, g, r, i, z . DR2 is the first release to go beyond the $\sim\!18$ mag (10 $\sigma$ ) limit of the Shallow Survey released in the first data release (DR1), and includes portions of the sky at full survey depth that reach $>\!21$ mag in g and r filters. The DR2 photometry has a precision as measured by internal reproducibility of 1% in u and v , and 0.7% in griz . More than 21 000 $\deg^2$ have data in some filters (at either Shallow or Main Survey depth) and over 7 000 $\deg^2$ have deep Main Survey coverage in all six filters. Finally, about 18 000 $\deg^2$ have Main Survey data in i and z filters, albeit not yet at full depth. The release contains over 120 000 images, as well as catalogues with over 500 million unique astrophysical objects and nearly 5 billion individual detections. It also contains cross-matches with a range of external catalogues such as Gaia DR2, Pan-STARRS1 DR1, GALEX GUVcat, 2MASS, and AllWISE, as well as spectroscopic surveys such as 2MRS, GALAH, 6dFGS, and 2dFLenS.

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