Tracing cosmic star formation with EXIST

被引：3
|
作者：
Hartmann, DH [1 ]
Grindlay, J
Band, D
Blandford, R
Craig, W
Fishman, GJ
Gehrels, N
Harrison, F
Hong, J
Kouveliotou, C
Loeb, A
Woosley, SE
机构：
[1] Clemson Univ, Clemson, SC 29634 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA
[4] Lawrence Livermore Natl Lab, Livermore, CA USA
[5] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA
[6] Harvard Univ, CfA, Cambridge, MA 02138 USA
[7] CALTECH, Pasadena, CA 91125 USA
[8] Univ Calif Santa Cruz, Lick Observ, Santa Cruz, CA 95064 USA
来源：
NEW ASTRONOMY REVIEWS | 2004年 / 48卷 / 1-4期
关键词：
gamma-ray telescopes; supernovae; novae; bursts; black holes; stars-formation;
D O I：
10.1016/j.newar.2003.11.055
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We describe the energetic X-ray imaging survey telescope EXIST, designed to carry out a sensitive all-sky survey in the 10-600 keV band. The primary goal of EXIST is to find black holes in the local and distant universe. EXIST also traces cosmic star formation via gamma-ray bursts and gamma-ray lines from radioactivity ejected by supernovae and novae. (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码：237 / 241
页数：5
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