THE LARGE SKY AREA MULTI-OBJECT FIBER SPECTROSCOPIC TELESCOPE QUASAR SURVEY: QUASAR PROPERTIES FROM THE FIRST DATA RELEASE | |
Ai, Y. L.1,2; Wu, Xue-Bing1,3; Yang, Jinyi1,3; Yang, Qian1,3; Wang, Feige1,3; Guo, Rui1,3; Zu, Wenwen4; Dong, Xiaoyi1; Zhang, Y. -X.5; Yuan, H. -L.5; Song, Y. -H.5; Wang JG(王建国)6,7; Dong XB(董小波)6,7; Yang, M.5; Wu, H.5; Shen, S. -Y.4; Shi, J. -R.5; He, B. -L.5; Lei, Y-J.5; Li, Y-B.5; Luo, A. -L.5; Zhao, Y-H.5; Zhang, H. -T.5 | |
发表期刊 | ASTRONOMICAL JOURNAL |
2016-02-01 | |
卷号 | 151期号:2 |
DOI | 10.3847/0004-6256/151/2/24 |
产权排序 | 第6完成单位 |
收录类别 | SCI |
关键词 | Catalogs Quasars: General Surveys |
摘要 | We present preliminary results of the quasar survey in the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) first data release (DR1), which includes the pilot survey and the first year of the regular survey. There are 3921 quasars reliably identified, among which 1180 are new quasars discovered in the survey. These quasars are at low to median redshifts, with a highest z of 4.83. We compile emission line measurements around the H alpha, H beta, MgII, and C IV regions for the new quasars. The continuum luminosities are inferred from SDSS photometric data with model fitting, as the spectra in DR1 are non-flux-calibrated. We also compile the virial black hole mass estimates, with flags indicating the selection methods, and broad absorption line quasars. The catalog and spectra for these quasars are also available. Of the 3921 quasars, 28% are independently selected with optical-infrared colors, indicating that the method is quite promising for the completeness of the quasar survey. LAMOST DR1 and the ongoing quasar survey will provide valuable data for studies of quasars. |
资助项目 | National Aeronautics and Space Administration ; National Key Basic Research Program of China[2014CB845700] ; National Key Basic Research Program of China[2013CB834900] ; National Key Basic Research Program of China[2015CB857000] ; NSFC[11103071] ; NSFC[11033001] ; NSFC[11033007] ; NSFC[11373008] ; NSFC[11533001] ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences[XDB09000000] ; State Key Development Program for Basic Research of China[2013CB834900] ; State Key Development Program for Basic Research of China[2015CB857000] ; National Development ; Reform Commission ; Alfred P. Sloan Foundation ; Participating Institutions ; Center for High-Performance Computing at the University of Utah |
项目资助者 | National Aeronautics and Space Administration ; National Key Basic Research Program of China[2014CB845700, 2013CB834900, 2015CB857000] ; NSFC[11103071, 11033001, 11033007, 11373008, 11533001] ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences[XDB09000000] ; State Key Development Program for Basic Research of China[2013CB834900, 2015CB857000] ; National Development ; Reform Commission ; Alfred P. Sloan Foundation ; Participating Institutions ; Center for High-Performance Computing at the University of Utah |
语种 | 英语 |
学科领域 | 天文学 ; 星系与宇宙学 ; 星系天文学 |
文章类型 | Article |
出版者 | IOP PUBLISHING LTD |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
ISSN | 0004-6256 |
URL | 查看原文 |
WOS记录号 | WOS:000371248600004 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | BLACK-HOLE MASSES ; EFFICIENT PHOTOMETRIC SELECTION ; ACTIVE GALACTIC NUCLEI ; TARGET SELECTION ; EMISSION-LINE ; CANDIDATE SELECTION ; OPTICAL VARIABILITY ; LUMINOSITY FUNCTION ; STELLAR OBJECTS ; REDSHIFT SURVEY |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/9350 |
专题 | 南方基地 中国科学院天体结构与演化重点实验室 |
通讯作者 | Ai, Y. L. |
作者单位 | 1.Department of Astronomy, School of Physics, Peking University, Beijing 100871, China 2.School of Physics and Astronomy, Sun Yat-Sen University, Guangzhou 510275, China 3.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China 4.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China 5.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences 100012, Beijing, China 6.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China 7.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China |
推荐引用方式 GB/T 7714 | Ai, Y. L.,Wu, Xue-Bing,Yang, Jinyi,et al. THE LARGE SKY AREA MULTI-OBJECT FIBER SPECTROSCOPIC TELESCOPE QUASAR SURVEY: QUASAR PROPERTIES FROM THE FIRST DATA RELEASE[J]. ASTRONOMICAL JOURNAL,2016,151(2). |
APA | Ai, Y. L..,Wu, Xue-Bing.,Yang, Jinyi.,Yang, Qian.,Wang, Feige.,...&Zhang, H. -T..(2016).THE LARGE SKY AREA MULTI-OBJECT FIBER SPECTROSCOPIC TELESCOPE QUASAR SURVEY: QUASAR PROPERTIES FROM THE FIRST DATA RELEASE.ASTRONOMICAL JOURNAL,151(2). |
MLA | Ai, Y. L.,et al."THE LARGE SKY AREA MULTI-OBJECT FIBER SPECTROSCOPIC TELESCOPE QUASAR SURVEY: QUASAR PROPERTIES FROM THE FIRST DATA RELEASE".ASTRONOMICAL JOURNAL 151.2(2016). |
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