Study of short term enhanced TeV $\gamma$- ray emission from Mrk 421 observed with TACTIC on December 28, 2014
K K Singh, K K Yadav, K Chanchalani, P Chandra, B Ghosal, A K Tickoo,, R C Rannot, P Marandi, N K Agarwal, M Kothari, K K Gour, H C Goyal, A Goyal,, N Kumar, C Borwankar, S R Kaul, V K Dhar, M K Koul, R Koul, K Venugopal, C K, Bhat, N Chouhan

TL;DR
This paper reports the detection of a short-term TeV gamma-ray flare from Mrk 421 using TACTIC, analyzing multi-wavelength data to understand the emission mechanisms during high activity states.
Contribution
First detailed TeV gamma-ray observation of Mrk 421 on December 28, 2014, with multi-wavelength analysis to study rapid variability and emission mechanisms.
Findings
Detected TeV gamma-ray flare with 5.17 sigma significance
Observed a variability timescale of ~0.72 days
TeV emission was more prominent than lower energy bands during the flare
Abstract
In this work, we report on the detection of enhanced TeV gamma- ray emission from the high synchrotron-peaked blazar Mrk 421 with the TACTIC telescope on the night of December 28, 2014 (MJD 57019). We use data from the TACTIC observations of Mrk 421 for one week during December 25-31, 2014 (MJD 57016-57022) in this study. The TACTIC observation on December 28, 2014 (MJD 57019) alone results in the detection of 86+-17 gamma- ray like events from Mrk 421 with a statistical significance of 5.17sigma in a livetime of ~ 2.2 hours above an energy threshold of 0.85 TeV. The high statistics (higher than three Crab Units) of TeV photons enables us to study the very high energy (VHE) gamma- ray emission from the source at shorter timescales. A minimum variability timescale of ~ 0.72 days is obtained for the TeV gamma- ray emission from Mrk 421 during the above flaring activity of the source. We…
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