Cien Shang, Ph.D.

Affiliations: 
2010 Columbia University, New York, NY 
Area:
Astronomy and Astrophysics
Google:
"Cien Shang"
Mean distance: (not calculated yet)
 

Parents

Sign in to add mentor
Zoltan Haiman grad student 2010 Columbia
 (The Large, the Deep and the Mysterious A study of galaxy clusters, supermassive black holes and their use as astrophysical probes of cosmology.)
BETA: Related publications

Publications

You can help our author matching system! If you notice any publications incorrectly attributed to this author, please sign in and mark matches as correct or incorrect.

Shang C, Oh SP. (2012) Probing gas motions in the intra-cluster medium: A mixture model approach Monthly Notices of the Royal Astronomical Society. 426: 3435-3454
Shang C, Haiman Z. (2011) Cosmology with standard sirens: The importance of the shape of the lensing magnification distribution Monthly Notices of the Royal Astronomical Society. 411: 9-22
Shang C, Bryan GL, Haiman Z. (2010) Supermassive black hole formation by direct collapse: keeping protogalactic gas H2 free in dark matter haloes with virial temperatures Tvir > rsim 104 K Monthly Notices of the Royal Astronomical Society. 402: 1249-1262
Molnar SM, Chiu IN, Umetsu K, et al. (2010) Testing strict hydrostatic equilibrium in simulated clusters of galaxies: Implications for A1689 Astrophysical Journal Letters. 724: L1-L4
Molnar SM, Umetsu K, Birkinshaw M, et al. (2010) Constraining intracluster gas models with AMiBA13 Astrophysical Journal. 723: 1272-1285
Shang C, Haiman Z, Verde L. (2009) Probing cosmology and galaxy cluster structure with the Sunyaev-Zel'dovich decrement versus X-ray temperature scaling relation Monthly Notices of the Royal Astronomical Society. 400: 1085-1104
Shang C, Scharf C. (2009) A low-redshift galaxy cluster x-ray temperature function incorporating Suzaku data Astrophysical Journal. 690: 879-890
Shang C, Crotts A, Haiman Z. (2007) Constraints on the Abundance of Highly Ionized Protocluster Regions from the Absence of Large Voids in the Lyα Forest The Astrophysical Journal. 671: 136-145
See more...