The third EGRET catalog of high-energy gamma-ray sources

被引:1644
作者
Hartman, RC
Bertsch, DL
Bloom, SD
Chen, AW
Deines-Jones, P
Esposito, JA
Fichtel, CE
Friedlander, DP
Hunter, SD
McDonald, LM
Sreekumar, P
Thompson, DJ
Jones, BB
Lin, YC
Michelson, PF
Nolan, PL
Tompkins, WF
Kanbach, G
Mayer-Hasselwander, HA
Mücke, A
Pohl, M
Reimer, O
Kniffen, DA
Schneid, EJ
von Montigny, C
Mukherjee, R
Dingus, BL
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Stanford Univ, WW Hansen Expt Phys Lab, Stanford, CA 94305 USA
[3] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[4] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[5] Hampden Sydney Coll, Dept Phys, Hampden Sydney, VA 23943 USA
[6] Northrup Grumman Corp, Bethpage, NY 11714 USA
[7] Landessternwarte Heidelberg, D-69117 Heidelberg, Germany
[8] Columbia Univ Barnard Coll, New York, NY 10027 USA
[9] Columbia Univ, Dept Phys, New York, NY 10027 USA
关键词
catalogs; galaxies : active; gamma rays : observations; pulsars : general; Sun : flares;
D O I
10.1086/313231
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The third catalog of high-energy gamma-ray sources detected by the EGRET telescope on the Compton Gamma Ray Observatory includes data from 1991 April 22 to 1995 October 3 (cycles 1, 2, 3, and 4 of the mission). In addition to including more data than the second EGRET catalog and its supplement, this catalog uses completely reprocessed data (to correct a number of mostly minimal errors and problems). The 271 sources (E > 100 MeV) in the catalog include the single 1991 solar flare bright enough to be detected as a source, the Large Magellanic Cloud, five pulsars, one probable radio galaxy detection (Cen A), and 66 high-confidence identifications of blazars (BL Lac objects, flat-spectrum radio quasars, or unidentified hat-spectrum radio sources). In addition, 27 lower confidence potential blazar identifications are noted. Finally, the catalog contains 170 sources not yet identified firmly with known objects, although potential identifications have been suggested for a number of those. A figure is presented that gives approximate upper limits for gamma-ray sources at any point in the sky, as well as information about sources listed in the second catalog and its supplement, that do not appear in this catalog.
引用
收藏
页码:79 / 202
页数:124
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