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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
Source PublicationASTRONOMICAL JOURNAL
2016-02-01
Volume151Issue:2
DOI10.3847/0004-6256/151/2/24
Contribution Rank第6完成单位
Indexed BySCI
KeywordCatalogs Quasars: General Surveys
Abstract

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.

Funding ProjectNational 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
Funding OrganizationNational 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
Language英语
Subject Area天文学 ; 星系与宇宙学 ; 星系天文学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherIOP PUBLISHING LTD
Publication PlaceTEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-6256
URL查看原文
WOS IDWOS:000371248600004
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordBLACK-HOLE MASSES ; EFFICIENT PHOTOMETRIC SELECTION ; ACTIVE GALACTIC NUCLEI ; TARGET SELECTION ; EMISSION-LINE ; CANDIDATE SELECTION ; OPTICAL VARIABILITY ; LUMINOSITY FUNCTION ; STELLAR OBJECTS ; REDSHIFT SURVEY
Citation statistics
Cited Times:7[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9350
Collection丽江天文观测站(南方基地)
中国科学院天体结构与演化重点实验室
Corresponding AuthorAi, Y. L.
Affiliation1.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
Recommended Citation
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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