Abstract
The TACTIC γ-ray telescope has observed Mrk 421 on 66 clear nights from December 07, 2005 to April 30, 2006, totalling ∼202 h of on-source observations. Here, we report the detection of flaring activity from the source at ≥1 TeV energy and the time-averaged differential γ-ray spectrum in the energy range 1-11 TeV for the data taken between December 27, 2005 and February 07, 2006 when the source was in a relatively higher state as compared to the rest of the observation period. Analysis of this data spell, comprising ∼97 h reveals the presence of a ∼12.0σ γ-ray signal with daily flux of >1 Crab unit on several days. A pure power law spectrum with exponent -3.11 ± 0.11 as well as a power law spectrum with an exponential cutoff (Γ = -2.51 ± 0.26 and E0 = (4.7 ± 2.1) TeV) are found to provide reasonable fits to the inferred differential spectrum within statistical uncertainties. We believe that the TeV light curve presented here, for nearly 5 months of extensive coverage, as well as the spectral information at γ-ray energies of >5 TeV provide a useful input for other groups working in the field of γ-ray astronomy.
| Original language | British English |
|---|---|
| Pages (from-to) | 447-454 |
| Number of pages | 8 |
| Journal | Astroparticle Physics |
| Volume | 27 |
| Issue number | 5 |
| DOIs | |
| State | Published - Jun 2007 |
Keywords
- Energy spectrum
- Light curve
- Mrk 421
- Observations
- TeV γ-rays
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