THE 2 HIGH-LATITUDE COS-B GAMMA-RAY SOURCES OBSERVED BY SAS-2 IN THE GREATER-THAN 100 MEV ENERGY-RANGE

被引：0
|
作者：
YU, KN
机构：
[1] Department of Applied Science, City Polytechnic of Hong Kong, Kowloon, Kowloon Tong
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1991年 / 181卷 / 02期
关键词：
D O I：
10.1007/BF00639093
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The two sources with high galactic latitudes detected by the COS-B detector, namely 3C273 and 2CG 010-31, have been studied with the SAS-2 data by using the cross-correlation function method. It has been found that both of them have a corresponding gamma-ray peak in the SAS-2 correlated flux. The flux values derived are in good agreement with previous results. These indicate that it is consistently appropriate to apply the cross-correlation function method to the SAS-2 data and that fruitful results are available from the analysis of the SAS-2 data.
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页码：261 / 266
页数：6
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