Observations of the flux of very-high-energy gamma rays from the blazar 3C 66A

被引：18
|
作者：
Stepanyan, AA [1 ]
Neshpor, YI [1 ]
Andreeva, NA [1 ]
Kalekin, OR [1 ]
Zhogolev, NA [1 ]
Fomin, VP [1 ]
Shitov, VG [1 ]
机构：
[1] Crimean Astrophys Observ, UA-334413 Nauchnyi, Crimea, Ukraine
来源：
ASTRONOMY REPORTS | 2002年 / 46卷 / 08期
关键词：
Radiation; Optical Radiation;
D O I：
10.1134/1.1502223
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Measurements of the flux of very-high-energy (> 1 TeV) gamma rays from the blazar 3C 66A obtained over four years are presented. The mean flux over the four-year period was (2.8 +/- 0.4) x 10(-11) cm(-2) s(-1). There is a correlation between the season-averaged flux of very-high-energy gamma rays and the observed optical radiation. (C) 2002 MAIK "Nauka/Interperiodica".
引用
收藏
页码：634 / 638
页数：5
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