| dc.contributor.author | Banerjee, Anuvab | |
| dc.contributor.author | Negi, Vibhore | |
| dc.contributor.author | Joshi, Ravi | |
| dc.contributor.author | Kumar, Nagendra | |
| dc.contributor.author | Wiita, Paul J. | |
| dc.contributor.author | Chand, Hum | |
| dc.contributor.author | Rawat, Nikita | |
| dc.contributor.author | Wu, Xue-Bing | |
| dc.contributor.author | Ho, Luis C. | |
| dc.date.accessioned | 2024-02-05T10:50:13Z | |
| dc.date.available | 2024-02-05T10:50:13Z | |
| dc.date.issued | 2023-12 | |
| dc.identifier.uri | https://doi.org/10.1093/mnras/stad3056 | |
| dc.identifier.uri | http://localhost:8080/xmlui/handle/123456789/1421 | |
| dc.description.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. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Monthly Notices of the Royal Astronomical Society | en_US |
| dc.relation.ispartofseries | 2055;mn526-5172 | |
| dc.subject | galaxies: active | en_US |
| dc.subject | galaxies: jets | en_US |
| dc.subject | quasars: general | en_US |
| dc.title | Probable low-frequency quasi-periodic oscillations in blazars from the ZTF survey | en_US |
| dc.type | Article | en_US |