The Crab total gamma-ray emission as seen by CGRO

被引：0
作者：
Much, R
Harmon, BA
Nolan, P
Strickman, MS
Bennett, K
Buccheri, R
Diehl, R
Fierro, JM
Fishman, GJ
Grabelsky, DA
Grove, JE
Hermsen, W
Johnson, WN
Jung, GV
Kinzer, RL
Kroeger, RA
Kuiper, L
Kurfess, JD
Lichti, GG
Matz, SM
McConnell, M
Paciesas, WS
Purcell, WR
Ryan, J
Schonfelder, V
Steinle, H
Strong, A
Thompson, DJ
Ulmer, MP
Varendorff, M
Wilson, CA
Wilson, RB
机构：
[1] MAX PLANCK INST EXTRATERR PHYS,D-85740 GARCHING,GERMANY
[2] SRON,NL-3584 CA UTRECHT,NETHERLANDS
[3] UNIV NEW HAMPSHIRE,CTR SPACE SCI,DURHAM,NH 03857
[4] CNR,IFCAI,I-90139 PALERMO,ITALY
[5] USN,RES LAB,WASHINGTON,DC 20375
[6] NORTHWESTERN UNIV,DEPT PHYS & ASTRON,EVANSTON,IL 60208
[7] UNIV SPACE RES ASSOCIATES,WASHINGTON,DC 20375
[8] STANFORD UNIV,HANSEN EXPT PHYS LAB,STANFORD,CA 94305
[9] NASA,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771
[10] NASA,GEORGE C MARSHALL SPACE FLIGHT CTR ES84,HUNTSVILLE,AL 35812
[11] UNIV ALABAMA,DEPT PHYS,HUNTSVILLE,AL 35899
来源：
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1996年 / 120卷 / 04期
关键词：
gamma rays; observations; ISM; Crab nebula;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Compton Gamma-Ray Observatory has completed 4 years of observations comprising a full-sky survey and several deep pointings. The Crab is one of the strongest perma- nent sources in the CGRO energy range (20 keV to 10 GeV). Its total (pulsed and unpulsed) emission is often used as a calibration standard. We present the results of an analysis of data from all four CGRO instruments obtained during contemporaneous Crab observations made during Phase I, II and III between 1991 and 1994. Emphasis is given to the cross-calibration of the four CGRO instruments.
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收藏
页码：C703 / C706
页数：4
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