A Gaia-PS1-SDSS (GPS1) Proper Motion Catalog Covering 3/4 of the Sky | |
Martin, Nicolas F.3,5; Waters, Christopher Z.1; Kudritzki, Rolf-Peter1; Platais, Imants7; Goldman, Bertrand3,5; Liu, Chao6; Rix, Hans-Walter3; Sesar, Branimir3; Gupta, Prashansa4; Tian, Hai-Jun2,3 | |
刊名 | ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES |
2017-09-01 | |
卷号 | 232期号:1 |
关键词 | Astrometry Catalogs Galaxy: Kinematics And Dynamics Proper Motions |
DOI | 10.3847/1538-4365/aa826a |
文献子类 | Article |
英文摘要 | We combine Gaia DR1, PS1, Sloan Digital Sky Survey (SDSS), and 2MASS astrometry to measure proper motions for 350 million sources across three-fourths of the sky down to a magnitude of m(r) similar to 20. Using positions of galaxies from PS1, we build a common reference frame for the multi-epoch PS1, single-epoch SDSS and 2MASS data, and calibrate the data in small angular patches to this frame. As the Gaia DR1 excludes resolved galaxy images, we choose a different approach to calibrate its positions to this reference frame: we exploit the fact that the proper motions of stars in these patches are linear. By simultaneously fitting the positions of stars at different epochs of-Gaia DR1, PS1, SDSS, and 2MASS-we construct an extensive catalog of proper motions dubbed GPS1. GPS1 has a characteristic systematic error of less than 0.3 mas yr(-1) and a typical precision of 1.5-2.0mas yr(-1). The proper motions have been validated using galaxies, open clusters, distant giant stars, and QSOs. In comparison with other published faint proper motion catalogs, GPS1's systematic error (<0.3 mas yr(-1)) should be nearly an order of magnitude better than that of PPMXL and UCAC4 (>2.0 mas yr(-1)). Similarly, its precision (similar to 1.5 mas yr(-1)) is a four-fold improvement relative to PPMXL and UCAC4 (similar to 6.0 mas yr(-1)). For QSOs, the precision of GPS1 is found to be worse (similar to 2.0-3.0mas yr(-1)), possibly due to their particular differential chromatic refraction. The GPS1 catalog will be released online and be available via the VizieR Service and VO Service. |
WOS关键词 | SURVEY 2MASS ; USNO-B ; STARS ; TELESCOPE ; POSITIONS |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000408442500004 |
资助机构 | National Natural Science Foundation of China (NSFC)(11503012 ; National Natural Science Foundation of China (NSFC)(11503012 ; China Scholarship Council (CSC) ; China Scholarship Council (CSC) ; Max Planck Institute for Astronomy ; Max Planck Institute for Astronomy ; European Research Council under European Union(321035) ; European Research Council under European Union(321035) ; German Research Foundation (DFG)(SFB 881) ; German Research Foundation (DFG)(SFB 881) ; National Aeronautics and Space Administration through Planetary Science Division of the NASA Science Mission Directorate(NNX08AR22G) ; National Aeronautics and Space Administration through Planetary Science Division of the NASA Science Mission Directorate(NNX08AR22G) ; National Science Foundation(AST-1238877) ; National Science Foundation(AST-1238877) ; U1331202) ; U1331202) ; National Natural Science Foundation of China (NSFC)(11503012 ; National Natural Science Foundation of China (NSFC)(11503012 ; China Scholarship Council (CSC) ; China Scholarship Council (CSC) ; Max Planck Institute for Astronomy ; Max Planck Institute for Astronomy ; European Research Council under European Union(321035) ; European Research Council under European Union(321035) ; German Research Foundation (DFG)(SFB 881) ; German Research Foundation (DFG)(SFB 881) ; National Aeronautics and Space Administration through Planetary Science Division of the NASA Science Mission Directorate(NNX08AR22G) ; National Aeronautics and Space Administration through Planetary Science Division of the NASA Science Mission Directorate(NNX08AR22G) ; National Science Foundation(AST-1238877) ; National Science Foundation(AST-1238877) ; U1331202) ; U1331202) |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/20089] |
专题 | 国家天文台_光学天文研究部 |
作者单位 | 1.Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA 2.China Three Gorges Univ, Yichang 443002, Peoples R China 3.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany 4.Indian Inst Sci Educ & Res, Dept Phys Sci, Sect 81, Sas Nagar 140306, Punjab, India 5.Univ Strasbourg, CNRS, Observ Astron Strasbourg, UMR 7550, 11 Rue Univ, F-67000 Strasbourg, France 6.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China 7.Johns Hopkins Univ, Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA |
推荐引用方式 GB/T 7714 | Martin, Nicolas F.,Waters, Christopher Z.,Kudritzki, Rolf-Peter,et al. A Gaia-PS1-SDSS (GPS1) Proper Motion Catalog Covering 3/4 of the Sky[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2017,232(1). |
APA | Martin, Nicolas F..,Waters, Christopher Z..,Kudritzki, Rolf-Peter.,Platais, Imants.,Goldman, Bertrand.,...&Tian, Hai-Jun.(2017).A Gaia-PS1-SDSS (GPS1) Proper Motion Catalog Covering 3/4 of the Sky.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,232(1). |
MLA | Martin, Nicolas F.,et al."A Gaia-PS1-SDSS (GPS1) Proper Motion Catalog Covering 3/4 of the Sky".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 232.1(2017). |
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