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

页码：237 / 241

页数：5

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