- icrc2007@icrc2007.unam.mx
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Contribution Oral (WITHDRAWN)
Speakers
- Dr. R. C. RANNOT
Primary authors
- Dr. R. C. RANNOT (BARC)
- Mr. S.V GODAMBE (BARC)
Co-authors
- Mr. P. CHNANDRA (BARC)
- Mr. K. YADAV (BARC)
- Dr. A.K. TICKOO (BARC)
- Mr. K. VENUGOPAL (BARC)
- Mr. N. BHATT (BARC)
- S. BHATTACHARYA (BARC)
- K. CHANCHALANI (BARC)
- V.K DHAR (BARC)
- H.C GOYAL (BARC)
- Dr. R.K. KAUL (BARC)
- M.K. KOTHARI (BARC)
- S. KOTWAL (BARC)
- M.K. KOUL (BARC)
- R. KOUL (BARC)
- S. SAHAYNATHAN (BARC)
- M. SHARMA (BARC)
- S. THOUDAM (BARC)
Abstract content
We have observed the BL Lac object Mrk 501, during the period Feb. 2006 - May 2006 for a total on- source duration of 65 hours using the TACTIC gamma-ray telescope at Mt. Abu Rajasthan India. During these observations the telescope was used in a tracking mode of its operation in order to collect maximum possible data on the source. Detailed analysis of 65 hours of data shows the presence of a significant TeV gamma-ray signal from the source direction with a statistical significance of ~ 8.3 σ above system threshold energy of 1.5 TeV . We have estimated the differential source spectrum in the energy range 1.5 - 11 TeV which fits well with the power law function of the form fo x E-γ, γ = 2.83 ± 0.1 and fo = (2.74 ±0.19) x 10-11 photons /sec cm² TeV. Details of data analysis and results so obtained would be presented at the conference.