Long-term multi-wavelength study of temporal and spectral properties of 3C 279

• Published in: Astroparticle physics 2022-06, Vol.139, p.102687, Article 102687
• Main Authors: Tolamatti, A., Ghosal, B., Singh, K.K., Bhattacharyya, S., Bhatt, N., Yadav, K.K., Chandra, P., Das, M.P., Tickoo, A.K., Rannot, R.C., Kothari, M., Gaur, K.K., Goyal, A., Kumar, N., Marandi, P., Agarwal, N.K., Godambe, S., Mankuzhiyil, N., Sarkar, D., Sharma, M., Chouhan, N., Borwankar, C., Dhar, V.K., Koul, M.K., Venugopal, K., Kotwal, S.V., Godiyal, S.
• Format: Article
• Language: English
• Subjects: 3C 279; Data analysis-Gamma-rays; Flat Spectrum Radio Quasars; Galaxies; Individual
• ISSN: 0927-6505; 1873-2852
• DOI: 10.1016/j.astropartphys.2022.102687

We present a long-term multi-wavelength study of the flat spectrum radio quasar 3C 279 using near simultaneous observations available from July 01, 2012 and June 31, 2018 (MJD 56109-58301). The data set includes measurements from the TACTIC, Fermi-LAT, Swift-XRT, Swift-UVOT, SMARTS, Steward-SPOL, and OVRO. The TACTIC telescope has monitored the source 3C 279 for ∼ 70 h between 2013 and 2018 in the energy range of > 0.85 TeV and yields null result. We have analysed the Fermi-LAT data to obtain the 5-day binned light curve in the energy range 0.1–300 GeV. One low and six high emission states are identified in the Fermi-LAT light curve. The high emission states are modelled with an exponential rise and decay time profile using 1-day averaged flux points and have been characterized as the asymmetric flares. The spectral analysis of near simultaneous X-ray and γ-ray data from the Swift-XRT and Fermi-LAT respectively indicates harder when brighter trend during the high activity states. The time averaged broadband spectral energy distributions corresponding to the seven states are successfully reproduced under the framework of a simple one zone leptonic emission model with IR photons originating from the dusty torus as the dominant target for the inverse Compton scattering by the relativistic electrons. Results obtained from the broadband modelling suggest that the non-thermal emission region in the jet is above the broadline region. This is also supported by the average value of seed factor estimated using the derived model parameters. A positive correlation between the bulk Lorentz factor of the emission zone and average γ-ray flux measurements for each state indicates that an increase in the bulk Lorentz factor can be the dominant cause for the observed flares from 3C 279. We also discuss the implications of the obtained model parameters in detail to understand the long-term behaviour of the source.