T
Teng Liu
Researcher at Max Planck Society
Publications - 60
Citations - 1981
Teng Liu is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Active galactic nucleus. The author has an hindex of 18, co-authored 60 publications receiving 1687 citations. Previous affiliations of Teng Liu include University of Science and Technology of China & University of Massachusetts Amherst.
Papers
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Journal ArticleDOI
THE CHANDRA DEEP FIELD-SOUTH SURVEY: 4 Ms SOURCE CATALOGS
Yongquan Xue,Bin Luo,W. N. Brandt,Franz E. Bauer,Franz E. Bauer,Bret D. Lehmer,Bret D. Lehmer,Patrick S. Broos,Donald P. Schneider,David M. Alexander,Marcella Brusa,Andrea Comastri,Andrew C. Fabian,Roberto Gilli,Günther Hasinger,Ann Hornschemeier,Anton M. Koekemoer,Teng Liu,Teng Liu,V. Mainieri,Maurizio Paolillo,D. A. Rafferty,Piero Rosati,Ohad Shemmer,John D. Silverman,Ian Smail,Paolo Tozzi,Cristian Vignali +27 more
TL;DR: In this article, the authors presented a source catalog for the 4Ms Chandra Deep Field-South (CDF-S) survey, which is the deepest Chandra survey to date and covers an area of 464.5 arcmin2.
Journal ArticleDOI
High-redshift AGN in the Chandra Deep Fields: the obscured fraction and space density of the sub-L * population
Fabio Vito,W. N. Brandt,Guang Yang,Roberto Gilli,B. Luo,Cristian Vignali,Cristian Vignali,Yongquan Xue,Andrea Comastri,Anton M. Koekemoer,Bret D. Lehmer,Teng Liu,Teng Liu,Maurizio Paolillo,Maurizio Paolillo,Piero Ranalli,Donald P. Schneider,Ohad Shemmer,M. Volonteri,Jun Xian Wang +19 more
TL;DR: In this paper, the authors derived the high-redshift AGN number counts down to F0.6-0.8, once incompleteness effects are taken into account, with no strong dependence on redshift or luminosity.
Journal ArticleDOI
Are x-ray emitting coronae around supermassive black holes outflowing?
TL;DR: In this article, the authors compare the intrinsic corona X-ray emission between Seyfert 1 and Compton-thin Seyfer 2 galaxies, which are viewed at different inclinations according to the unification scheme.
Journal ArticleDOI
Black Hole Growth Is Mainly Linked to Host-galaxy Stellar Mass Rather Than Star Formation Rate
Guang Yang,Chien-Ting J. Chen,Fabio Vito,W. N. Brandt,David M. Alexander,Bin Luo,Mouyuan Sun,Yongquan Xue,Franz E. Bauer,Franz E. Bauer,Anton M. Koekemoer,Bret Lehmer,Teng Liu,Donald P. Schneider,Ohad Shemmer,Jonathan R. Trump,Cristian Vignali,J. X. Wang +17 more
TL;DR: In this paper, the dependence of black-hole accretion rate (BHAR) on host-galaxy star formation rate (SFR) and stellar mass (M∗) in the CANDELS/GOODS-South field in the redshift range of 0.5≤z<2.0 was investigated.
Journal ArticleDOI
Are X-ray Emitting Coronae around Super Massive Black Holes Outflowing?
TL;DR: In this paper, the authors compare the intrinsic corona X-ray emission between Seyfert 1 and Compton-thin Seyfer 2 galaxies, which are viewed at different inclinations according to the unification scheme.