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Very high energy γ-ray observations of Mrk 501 using the TACTIC imaging γ-ray telescope during 2005 06

Godambe, S. V. (author)
Bhabha Atomic Research Centre, India
Rannot, R. C. (author)
Bhabha Atomic Research Centre, India
Chandra, P. (author)
Bhabha Atomic Research Centre, India
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Yadav, K. K. (author)
Bhabha Atomic Research Centre, India
Tickoo, A. K. (author)
Bhabha Atomic Research Centre, India
Venugopal, K. (author)
Bhabha Atomic Research Centre, India
Bhatt, N. (author)
Bhabha Atomic Research Centre, India
Bhattacharyya, S. (author)
Bhabha Atomic Research Centre, India
Chanchalani, K. (author)
Bhabha Atomic Research Centre, India
Dhar, V. K. (author)
Bhabha Atomic Research Centre, India
Goyal, H. C. (author)
Bhabha Atomic Research Centre, India
Kaul, R. K. (author)
Bhabha Atomic Research Centre, India
Kothari, M. (author)
Bhabha Atomic Research Centre, India
Kotwal, S. (author)
Bhabha Atomic Research Centre, India
Koul, M. K. (author)
Bhabha Atomic Research Centre, India
Koul, R. (author)
Bhabha Atomic Research Centre, India
Sahaynathan, B. S. (author)
Bhabha Atomic Research Centre, India
Sharma, M. (author)
Bhabha Atomic Research Centre, India
Thoudam, Satyendra (author)
Bhabha Atomic Research Centre, India
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 (creator_code:org_t)
2008-04-29
2008
English.
In: Journal of Physics G. - : IOP Publishing. - 0954-3899 .- 1361-6471. ; 35:6
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • In this paper we report on the Markarian 501 results obtained during our TeV γ-ray observations from 11 March to 12 May 2005 and 28 February to 7 May 2006 for 112.5 h with the TACTIC γ-ray telescope. During 2005 observations for 45.7 h, the source was found to be in a low state and we have placed an upper limit of 4.62 × 10−12 photons cm−2 s−1 at 3σ level on the integrated TeV γ-ray flux above 1 TeV from the source direction. However, during 2006 observations for 66.8 h, detailed data analysis revealed the presence of a TeV γ-ray signal from the source with a statistical significance of 7.5σ above Eγ≥ 1 TeV. The time-averaged differential energy spectrum of the source in the energy range 1–11 TeV is found to match well with the power-law function of the form (dΦ/dE = f0E−Γ) with f0 = (1.66 ± 0.52) × 10−11 cm−2 s−1 TeV−1 and Γ = 2.80 ± 0.27.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

Physics
Fysik

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