Lei Hao, Ph.D.

Affiliations:

2009-

Shanghai Astronomical Observatory

Area:

Astronomy and Astrophysics

Website:

http://sourcedb.shao.cas.cn/yw/pl/fs/201012/t20101218_3046501.html

Google:

"Lei Hao"

Bio:

Hao Lei received her Bachelor degree from University of Science and Technology of China in 1998 and her Ph.D from Princeton University in 2004. She was a postdoc in Cornell University and University of Texas at Austin from 2004 to 2008 and from 2008 to 2009, respectively. She joined the Shanghai Astronomical Observatory as a BaiRen Professor and Researcher in December of 2009. Her main research interest is the evolution of galaxies and AGNs, which involves the AGNs, Starbursts, dwarf galaxies, and high-redshift Lyman-Alpha emission-line galaxies. She is an expert on the multi-wavelength (especially optical and infrared) and statistical studies of galaxies and their black holes. She has published over 40 papers, been cited by over 3000 times, including 350 times citations on the first-author papers. She has lead or participated in various projects, including the NSFC general program, Shanghai Pujiang Talented program, and national 973 program “Astrophysics around Black Holes”. She is now leading a project of installing an IFU instrument on the 2.4m telescope (China Lijiang IFU, CHILI).
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Parents

Michael Abram Strauss	grad student	2004	Princeton
(Active galactive nuclei and metal poor galaxies in the Sloan Digital Sky Survey.)

Children

Collaborators

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Publications

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Li Z, Zhou H, Hao L, et al. (2020) Ultradense Gas at the Dusty Torus Scale in a Partially Obscured Quasar The Astrophysical Journal. 900: 47
Zhou H, Shi X, Yuan W, et al. (2019) Fast inflows as the adjacent fuel of supermassive black hole accretion disks in quasars. Nature. 573: 83-86
Pan X, Zhou H, Liu W, et al. (2019) Discovery of Metastable He I* λ10830 Mini-broad Absorption Lines and Very Narrow Paschen α Emission Lines in the ULIRG Quasar IRAS F11119+3257 The Astrophysical Journal. 883: 173
Liu C, Hao L, Wang H, et al. (2019) The Morphological Transformation and the Quenching of Galaxies The Astrophysical Journal. 878: 69
Zhang K, Hao L. (2018) A New Diagnostic Diagram of Ionization Sources for High-redshift Emission Line Galaxies The Astrophysical Journal. 856: 171
Yuan F, Argudo-Fernández M, Shen S, et al. (2018) Spatially resolved star formation and dust attenuation in Mrk 848: Comparison of the integral field spectra and the UV-to-IR SED Astronomy and Astrophysics. 613
Xie Y, Li A, Hao L. (2017) Silicate Dust in Active Galactic Nuclei Astrophysical Journal Supplement Series. 228: 6
Lin L, Lin J, Hsu C, et al. (2017) SDSS IV MaNGA: discovery of an Hα blob associated with a dry galaxy pair - ejected gas or a 'dark' galaxy candidate? The Astrophysical Journal. 837: 32
Srinivasan S, Kemper F, Zhou Y, et al. (2017) The mineralogy of newly formed dust in active galactic nuclei Planetary and Space Science. 149: 56-63
Chen YM, Shi Y, Tremonti CA, et al. (2016) The growth of the central region by acquisition of counterrotating gas in star-forming galaxies. Nature Communications. 7: 13269