Three-dimensional interstellar dust reddening maps of the Galactic plane
文献类型：期刊论文
| 作者 | Chen, B. -Q.4; Huang, Y.4; Yuan, H. -B.5; Wang, C.1; Fan, D. -W.3; Xiang, M. -S.3; Zhang, H. -W.1; Tian, Z. -J.1,2; Liu, X. -W.4 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 出版日期 | 2019-03-01 |
| 卷号 | 483期号:4页码:4277-4289 |
| ISSN号 | 0035-8711 |
| 关键词 | dust, extinction ISM: structure Galaxy: structure |
| DOI | 10.1093/mnras/sty3341 |
| 英文摘要 | We present new three-dimensional (3D) interstellar dust reddening maps of the Galactic plane in three colours, E(G - K-S), E(G(BP) - G(RP)), and E(H - K-S). The maps have a spatial angular resolution of 6 arcmin and covers over 7000 deg(2) of the Galactic plane for Galactic longitude 0 degrees < l < 360 degrees and latitude vertical bar b vertical bar < 10 degrees. The maps are constructed from robust parallax estimates from the Gaia Data Release 2 (Gaia DR2) combined with the high-quality optical photometry from the Gaia DR2 and the infrared photometry from the Two Micron All Sky Survey and Wide-Field Infrared Survey Explorer survey. We estimate the colour excesses, E(G - K-S), E(G(BP) - G(RP)), and E(H - K-S), of over 56 million stars with the machine-learning algorithm Random Forest regression, using a training data set constructed from the large-scale spectroscopic surveys, Large Sky Area Multi-Object Fibre Spectroscopic Telescope, Sloan Extension for Galactic Understanding and Exploration, and Apache Point Observatory Galactic Evolution Experiment. The results reveal the large-scale dust distribution in the Galactic disc, showing a number of features consistent with the earlier studies. The Galactic dust disc is clearly warped and show complex structures possibly spatially associated with the Sagittarius, Local, and Perseus arms. We also provide the empirical extinction coefficients for the Gaia photometry that can be used to convert the colour excesses presented here to the line-of-sight extinction values in the Gaia photometric bands. |
| WOS关键词 | LAMOST SPECTROSCOPIC SURVEY ; EXTINCTION MAP ; SKY SURVEY ; 3D ; ANTICENTRE ; PARAMETERS ; PHOTOMETRY ; SELECTION ; 2MASS ; SDSS |
| 资助项目 | National Key Basic Research Program of China[2014CB845700] ; National Natural Science Foundation of China[11803029] ; National Natural Science Foundation of China[U1531244] ; National Natural Science Foundation of China[11833006] ; National Natural Science Foundation of China[U1731308] ; NSFC[11603002] ; Beijing Normal University[310232102] ; National Development and Reform Commission ; Alfred P. Sloan Foundation ; National Aeronautics and Space Administration ; National Science Foundation ; U.S. Department of Energy ; Japanese Monbukagakusho ; Max Planck Society ; University of Chicago ; Fermilab ; Institute for Advanced Study ; Japan Participation Group ; Johns Hopkins University ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy ; Max-Planck-Institute for Astrophysics ; New Mexico State University ; University of Pittsburgh ; Princeton University ; United States Naval Observatory ; University of Washington |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | OXFORD UNIV PRESS |
| WOS记录号 | WOS:000462281900001 |
| 资助机构 | National Key Basic Research Program of China ; National Key Basic Research Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; NSFC ; NSFC ; Beijing Normal University ; Beijing Normal University ; National Development and Reform Commission ; National Development and Reform Commission ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; University of Chicago ; University of Chicago ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy ; Max-Planck-Institute for Astronomy ; Max-Planck-Institute for Astrophysics ; Max-Planck-Institute for Astrophysics ; New Mexico State University ; New Mexico State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; NSFC ; NSFC ; Beijing Normal University ; Beijing Normal University ; National Development and Reform Commission ; National Development and Reform Commission ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; University of Chicago ; University of Chicago ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy ; Max-Planck-Institute for Astronomy ; Max-Planck-Institute for Astrophysics ; Max-Planck-Institute for Astrophysics ; New Mexico State University ; New Mexico State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; NSFC ; NSFC ; Beijing Normal University ; Beijing Normal University ; National Development and Reform Commission ; National Development and Reform Commission ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; University of Chicago ; University of Chicago ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy ; Max-Planck-Institute for Astronomy ; Max-Planck-Institute for Astrophysics ; Max-Planck-Institute for Astrophysics ; New Mexico State University ; New Mexico State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; National Key Basic Research Program of China ; National Key Basic Research Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; NSFC ; NSFC ; Beijing Normal University ; Beijing Normal University ; National Development and Reform Commission ; National Development and Reform Commission ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; University of Chicago ; University of Chicago ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group ; Japan Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Los Alamos National Laboratory ; Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy ; Max-Planck-Institute for Astronomy ; Max-Planck-Institute for Astrophysics ; Max-Planck-Institute for Astrophysics ; New Mexico State University ; New Mexico State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/25687]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Chen, B. -Q.; Liu, X. -W. |
| 作者单位 | 1.Peking Univ, Dept Astron, Beijing 100871, Peoples R China 2.Yunnan Univ, Dept Astron, Kunming 650091, Yunnan, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China 4.Yunnan Univ, South Western Inst Astron Res, Kunming 650091, Yunnan, Peoples R China 5.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China |
| 推荐引用方式 GB/T 7714 | Chen, B. -Q.,Huang, Y.,Yuan, H. -B.,et al. Three-dimensional interstellar dust reddening maps of the Galactic plane[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,483(4):4277-4289. |
| APA | Chen, B. -Q..,Huang, Y..,Yuan, H. -B..,Wang, C..,Fan, D. -W..,...&Liu, X. -W..(2019).Three-dimensional interstellar dust reddening maps of the Galactic plane.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,483(4),4277-4289. |
| MLA | Chen, B. -Q.,et al."Three-dimensional interstellar dust reddening maps of the Galactic plane".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 483.4(2019):4277-4289. |
入库方式： OAI收割
来源：国家天文台
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