Detection of periodicity in the gamma-ray light curve of the BL Lac 4FGL J2202.7+4216

Author:

Banerjee Anuvab1ORCID,Sharma Ajay1ORCID,Mandal Avijit1ORCID,Das Avik Kumar2ORCID,Bhatta Gopal3ORCID,Bose Debanjan4ORCID

Affiliation:

1. S. N. Bose National Centre for Basic Sciences , Block JD, Sector III, Salt Lake, Kolkata 700106, West Bengal, India

2. Department of Physical Sciences, Indian Institute of Science Education and Research Mohali , Knowledge City, Sector 81, SAS Nagar 140306, Punjab, India

3. Institute of Nuclear Physics, Polish Academy of Sciences , PL-31342 Kraków, Poland

4. School of Astrophysics, Presidency University , 86/1 College Street, Kolkata 700073, West Bengal, India

Abstract

ABSTRACT In this study, we carry out a comprehensive variability analysis of the BL Lac object 4FGL J2202.7+4216 detected by the Fermi-LAT, over a period of more than 3 yr, from 2019 April 27 to 2022 August 09. We detect the presence of quasi-periodic fluctuations with a period of ∼100 d with a confidence level exceeding 4σ. We also tentatively detect two other quasi-periodic fluctuations with a period of ∼75 and ∼50 d, which persist over the entire duration of observation. This is the first time such a variability feature pertaining to this source is being reported. We propose that the observed quasi-periodic oscillations may be related to the precession of the blazar jet with a high Lorentz factor or to the motion of a plasma blob through the helical structure of the jet. The harmonicity among the detected periodicities suggests the global p-mode oscillations of the thick disc to be a plausible mechanism as well. For a decisive conclusion on the physical origin of such fluctuation, further multiwavelength complementary observations, especially very long baseline interferometric observations, would be required.

Funder

DST

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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