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 |