Probable low-frequency quasi-periodic oscillations in blazars from the ZTF survey

Author:

Banerjee Anuvab1,Negi Vibhore23ORCID,Joshi Ravi45ORCID,Kumar Nagendra6ORCID,Wiita Paul J7,Chand Hum8,Rawat Nikita23ORCID,Wu Xue-Bing59,Ho Luis C59

Affiliation:

1. S.N. Bose National Centre for Basic Sciences , Block JD, Sector 3, Salt Lake, Kolkata 700106 , India

2. Aryabhatta Research Institute of Observational Sciences (ARIES) , Manora Peak, Nainital 263002 , India

3. Department of Physics, Deen Dayal Upadhyaya Gorakhpur University , Gorakhpur 273009 , India

4. Indian Institute of Astrophysics , Koramangla, Bangalore 560034 , India

5. Kavli Institute for Astronomy and Astrophysics, Peking University , Beijing 100871 , China

6. No. 1006, Santosh M’house, 9th Cross, Divanarapalya, Bangalore 560054 , India

7. Department of Physics, The College of New Jersey , 2000 Pennington Rd., Ewing, NJ 08628-0718 , USA

8. Department of Physics and Astronomical Sciences, Central University of Himachal Pradesh , Dharamshala 176215 , India

9. Department of Astronomy, School of Physics, Peking University , Beijing 100871 , China

Abstract

ABSTRACT We investigate the possible presence of quasi-periodic oscillation (QPO) signals in 2103 blazars from the Zwicky Transient Facility (ZTF) time-domain survey. We detect a low-frequency QPO signal in five blazars observed over these 3.8-yr-long optical r-band ZTF light curves. These periods range from 144 to 196 d detected at ≳4σ significance levels in both the Lomb–Scargle periodogram and weighted wavelet Z-transform analyses. We find consistent results using the phase dispersion minimization technique. A similar peak is detected in the g-band light curves at a slightly lower significance of 3σ. Such nearly periodic signals on these time-scales in optical wavebands most likely originate from a precessing jet with high Lorentz factor, closely aligned to the observer’s line of sight or the movement of plasma blobs along a helical structure in the jet.

Funder

National Science Foundation of China

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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