| Name: | Avik Das |
| Affiliation: | Indian Institute of Science Education and Research Mohali |
| Conference ID : | ASI2024_158 |
| Title : | The Detection of Possible Transient Quasiperiodic Oscillations in the γ-Ray Light Curve of PKS 0244-470 and 4C+38.41 |
| Authors : | Avik Kumar Das, Raj Prince, Alok C. Gupta, Pankaj Kushwaha |
| Authors Affiliation: | 1 Department of Physical Sciences, Indian Institute of Science Education and Research Mohali, Knowledge City, Sector 81, SAS Nagar, Punjab 140306, India
2 Center for Theoretical Physics, Polish Academy of Sciences, Al.Lotnikow 32/46, 02-668, Warsaw, Poland
3 Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital 263001, India
4 Department of Physical Sciences, Indian Institute of Science Education and Research Mohali, Knowledge City, Sector 81, SAS Nagar, Punjab 140306, India |
| Mode of Presentation: | Poster |
| Abstract Category : | High Energy Phenomena, Fundamental Physics and Astronomy |
| Abstract : | Blazars are the most luminous and variable subclass of active galactic nuclei (AGN). Gamma-ray flux variation of blazars are generally stochastic in nature. However, several light curves of blazars show either transient or persistent (relative) quasiperiodic behavior. The continuous monitoring capability of Fermi-LAT has enabled the exploration of quasiperiodic oscillations (QPOs) in the gamma-ray light curve of blazars that has given a new perspective to probe these sources over a wide range of timescales. In this work, we report the presence of transient QPOs in the long-term gamma-ray light curve of blazars PKS 0244-470 and 4C +38.41. We first identified different flux states using the Bayesian block algorithm and then explored the possible transient QPOs in the segments of each flux phase where the flux level changes over fairly regular intervals. Combining this with the source’s intrinsic variance, we identified two flux phases for PKS 0244-470: one activity (AP-1) and one quiescent phase (QP-1). For 4C+38.41, we similarly identified four activity (AP-1, AP-2,
AP-3, and AP-4) and two quiescent (QP-1 and QP-2) phases. The AP-1 phase of PKS 0244-470 shows QPO of ∼225 days persisting for eight cycles (∼4.1σ). In 4C+38.41, AP-1 and AP-2 phases show QPO-like behavior of ~110 days and ~60 days, respectively, persisting for five cycles. In AP-3, we identified three subphases, and all
show a ~7 day scale possible recurrent rise with five complete cycles, while in QP-1, we could identify two subphases (Q1 and Q2). The Q1 phase shows a period of ~104 days with six complete cycles. The Q2 phase also
shows QPO but with only ~3.7 cycles. We discuss the possible origin and argue that the current-driven kink instability and curved jet model seem to be the most likely causes for shorter and longer QPOs. |
