TeV gamma-ray observations of Markarian 421 using TACTIC during 2009-10

被引:14
作者
Chandra, P. [1 ]
Rannot, R. C. [1 ]
Yadav, K. K. [1 ]
Tickoo, A. K. [1 ]
Singh, K. K. [1 ]
Chanchalani, K. [1 ]
Kothari, M. [1 ]
Agarwal, N. K. [1 ]
Goyal, A. [1 ]
Goyal, H. C. [1 ]
Kotwal, S. [1 ]
Kumar, N. [1 ]
Marandi, P. [1 ]
Venugopal, K. [1 ]
Bhat, C. K. [1 ]
Bhatt, N. [1 ]
Bhattacharya, S. [1 ]
Borwankar, C. [1 ]
Chouhan, N. [1 ]
Dhar, V. K. [1 ]
Kaul, S. R. [1 ]
Koul, S. K. [1 ]
Koul, M. K. [1 ]
Koul, R. [1 ]
Mitra, A. K. [1 ]
Sahayanathan, S. [1 ]
Sharma, M. [1 ]
机构
[1] Bhabha Atom Res Ctr, Astrophys Sci Div, Bombay 400085, Maharashtra, India
关键词
BL-LAC OBJECTS; CRAB-NEBULA; MULTIWAVELENGTH OBSERVATIONS; ENERGY-SPECTRUM; IMAGING CAMERA; EMISSION; MKN-421; RADIATION; SYSTEM; FLARE;
D O I
10.1088/0954-3899/39/4/045201
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
We have observed the blazar Markarian 421 with the TACTIC gamma-ray telescope at Mt. Abu, India, from 22 November 2009 to 16 May 2010 for 265 h. Detailed analysis of the data so recorded revealed the presence of a TeV gamma-ray signal with a statistical significance of 12.12 sigma at E-gamma >= 1 TeV. We have estimated the time-averaged differential energy spectrum of the source in the energy range 1.0-16.44 TeV. The spectrum fits well with the power-law function of the form (dF/dE = f(0)E(-Gamma)) with f(0) = (1.39 +/- 0.239) x 10(-11) cm(-2) s(-1) TeV-1 and Gamma = 2.31 +/- 0.14.
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页数:13
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