Probing jet-induced optical variability across timescales in radio-loud NLSy1 galaxies

Abstract

We investigate optical variability across multiple timescales in a sample of radio-loud narrow-line Seyfert~1 (RL-NLSy1) galaxies, including ${\hat{I}}^3$-ray detected, ${\hat{I}}^3$-ray undetected, and non-jetted systems along with a comparison set of highly polarised core-dominated quasars (HPQs). Using Zwicky Transient Facility light curves, we measure fractional variability ($F_{\mathrm{var}}$) and rest-frame structure functions (SFs) to test whether short-term jet-linked variability is reflected in long-term behaviour. ${\hat{I}}^3$-ray detected RL-NLSy1s and HPQs show steeply rising SFs, revealing strong long-term coherence despite modest $F_{\mathrm{var}}$, consistent with Doppler-boosted synchrotron emission from relativistic jets. Non-jetted RL-NLSy1s exhibit the highest $F_{\mathrm{var}}$ but plateauing SFs, indicative of stochastic, disc-driven fluctuations lacking long-term coherence. ${\hat{I}}^3$-ray undetected RL-NLSy1s show the lowest $F_{\mathrm{var}}$ and nearly flat SFs, consistent with weak or absent jet activity across all timescales. Colour-magnitude trends show that jet-dominated sources exhibit redder-when-brighter behaviour, whereas disc-dominated systems exhibit bluer-when-brighter trends. These results show that SF-derived temporal coherence, rather than variability amplitude alone, is a promising diagnostic of jet dominance and orientation, offering a framework for interpreting AGN variability in forthcoming time-domain surveys.

7 pages, 3 Figures; Accepted for publication in MNRAS