Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
Scientist
Peking University
Univ. of Chicago, USA
UNIVERSITY OF WASHINGTON.
Department of Astronomy and Astrophysics, The University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637; Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 1-87, Nankang, Taipei, Taiwan 115, ROC
Department of Astronomy and Astrophysics, The University of Chicago, Chicago, IL 60637, USA
Department of Astronomy and Astrophysics, The University of Chicago, Chicago, Illinois 60637, USA
Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637
National Astronomical Observatoires, Chinese Academy of Sciences, A20, Datun Road, Beijing 100012, People's Republic of China; Department of Astronomy and Astrophysics, The University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637; Beijing Astrophysical Center, CAS-PKU, Beijing 100871, People's Republic of China.
Astronomy and Astrophysics Center, The University of Chicago, Chicago, IL 60637, USA
Department of Astronomy and Astrophysics, The University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637; Department of Physics, National Taiwan University, 1, Roosevelt Road Section 4, Taipei, Taiwan, Republic of China; Institute of Astronomy & Astrophysics, Academia Sinica, PO Box 1-87, Nankang, Taipei, Taiwan 115, Republic of China
Beijing Observatory, People's Republic of China
Department of Physics, Peking Observatory, China
Circumnuclear Spiral Arms and Starburst Rings in Magnetized Barred Spiral Galaxies
Comparison of Halo Detection from Noisy Weak Lensing Convergence Maps with Gaussian Smoothing and MRLens Treatment
Constraints on Dark Energy Models Including Gamma Ray Bursts
Coupled galactic density-wave modes in a composite system of thin stellar and gaseous discs
Determining the Geometry and the Cosmological Parameters of the Universe through SZE Cluster Counts
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