Abstract:
We explore the potential of the ongoing Zwicky Transient Facility (ZTF) survey for studying intranight optical variability
(INOV) of active galactic nuclei (AGNs), in particular for picking rare events of large INOV amplitudes, whose detection may
require extensive temporal coverage. For this, we have used the available high cadence subsets of the ZTF data base to build a
well-defined large sample of 53 blazars and another sample of 132 radio-quiet quasars (RQQs), matched to the blazar sample in
the redshift−magnitude plane. High-cadence ZTF monitoring of these two matched samples is available, respectively, for 156
and 418 intranight sessions. Median durations for both sets of sessions are 3.7 h. The two classes of powerful AGNs monitored
in these sessions represent opposite extremes of jet activity. The present analysis of their ZTF light curves has revealed some
strong INOV events that, although not exceptionally rare for blazars, are indeed so for RQQs, and their possible nature is briefly
discussed.
