Study of short term enhanced TeV $\gamma$- ray emission from Mrk 421 observed with TACTIC on December 28, 2014
| Autor: | N. K. Agarwal, B. Ghosal, M. K. Koul, K. K. Gour, K. K. Singh, K. Venugopal, C. Borwankar, P. Marandi, C.K. Bhat, Naveen Kumar, M. Kothari, R. Koul, R. C. Rannot, P. Chandra, H. C. Goyal, A. Goyal, K. Chanchalani, A. K. Tickoo, V. K. Dhar, S. R. Kaul, K. K. Yadav, N. Chouhan |
|---|---|
| Jazyk: | angličtina |
| Rok vydání: | 2018 |
| Předmět: |
Physics
Spectral index Photon 010308 nuclear & particles physics Astrophysics::High Energy Astrophysical Phenomena Flux Astronomy and Astrophysics Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics 01 natural sciences Synchrotron Galaxy law.invention Telescope law Observatory 0103 physical sciences Blazar Astrophysics - High Energy Astrophysical Phenomena 010303 astronomy & astrophysics Astrophysics::Galaxy Astrophysics |
| Popis: | 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 have also analyzed the contemporaneous data from Fermi-LAT to study the high energy (HE) gamma- ray emission during the high activity state of the source. The HE gamma- ray emission is observed to be increasing after the TeV flaring activity detected with the TACTIC. We also use other near simultaneous archival data available from the Swift-BAT in hard X-rays and from SPOL at Steward Observatory in optical V and R bands to characterize the multi-wavelength emission of Mrk 421 during the high activity state observed at TeV energies. The TeV gamma- ray emission observed on December 28, 2014 (MJD 57019) is found to be more prominant than the emissions in lower energy bands during the same period. The TeV gamma- ray observation of Mrk 421 in high activity state with the TACTIC telescope is also used to understand the physical mechanism for blazar emission under the frame work of the leptonic single zone synchrotron self Compton process. Comment: 21 pages, 5 figures, Accepted for publication in Astroparticle Physics |
| Databáze: | OpenAIRE |
| Externí odkaz: |
|