Detection of Quasiperiodic Oscillations in the Blazar PKS 0735+178 with TESS
Shubham Kishore, Alok C. Gupta, Paul J. Wiita, Sandeep K. Mondal, M. Vivek
astro-ph.HE
Submitted: 2026-07-08
Comments: Accepted for publication in MNRAS, 10 pages, 7 figures, 1 table
License: http://creativecommons.org/publicdomain/zero/1.0/
The gist: We report here the detection of signatures of a quasiperiodic oscillation (QPO) and a short flare in the optical light curve of the blazar PKS 0735+178, observed in two sectors, 71 and 72, spanning
Terminology
Abstract
We report here the detection of signatures of a quasiperiodic oscillation (QPO) and a short flare in the optical light curve of the blazar PKS 0735+178, observed in two sectors, 71 and 72, spanning around 49 days with the Transiting Exoplanet Survey Satellite. The modest flare in sector 71 lasted 4.3 days and appears as a combination of two sub-flares. In sector 72, a transient QPO with a period 11.2 hours is detected at local and global significance levels of 4.11 sigma and 3.06 sigma, respectively. We used weighted wavelet z transform, Lomb-Scargle periodogram, and phase dispersion minimization analysis techniques to look for and confirm the QPO feature. We also performed a segment-wise statistical inspection of these light curves and discuss here possible mechanisms that could explain the observed flux behavior.
Sources
- Fermi Large Area Telescope Fourth Source Catalog Data Release 4 (4FGL-DR4)
- The Bayesian Block Algorithm
- Black-Hole Mass Measurements
- Fermipy: An open-source Python package for analysis of Fermi-LAT Data
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