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SkyMapper Southern Survey: First Data Release (DR1)

Christian WolfARC Centre of Excellence for All-sky Astrophysics (CAASTROChristopher A. OnkenARC Centre of Excellence for All-sky Astrophysics (CAASTROLance C. LuvaulResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaBrian P. SchmidtARC Centre of Excellence for All-sky Astrophysics (CAASTROMichael S. BessellResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaSeo-Won ChangARC Centre of Excellence for All-sky Astrophysics (CAASTROGary S. Da CostaResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaDougal MackeyResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaTony Martin-JonesResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaSimon J. MurphyResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaTim PrestonCarolus Software Ltd., 244 5th Avenue, New York, NY 10001, USAR. ScalzoARC 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. ChinaJon SmillieNational Computational Infrastructure, Australian National University, Canberra, ACT 2601, AustraliaPatrick TisserandSorbonne UniversitéMarc C. WhiteResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaFang YuanARC Centre of Excellence for All-sky Astrophysics (CAASTRO
2018en
ABI

Аннотация

Abstract We present the first data release of the SkyMapper Southern Survey, a hemispheric survey carried out with the SkyMapper Telescope at Siding Spring Observatory in Australia. Here, we present the survey strategy, data processing, catalogue construction, and database schema. The first data release dataset includes over 66 000 images from the Shallow Survey component, covering an area of 17 200 deg 2 in all six SkyMapper passbands uvgriz , while the full area covered by any passband exceeds 20 000 deg 2 . The catalogues contain over 285 million unique astrophysical objects, complete to roughly 18 mag in all bands. We compare our griz point-source photometry with Pan-STARRS1 first data release and note an RMS scatter of 2%. The internal reproducibility of SkyMapper photometry is on the order of 1%. Astrometric precision is better than 0.2 arcsec based on comparison with Gaia first data release. We describe the end-user database, through which data are presented to the world community, and provide some illustrative science queries.

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