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

TL;DR

This study analyzes optical variability in radio-loud NLSy1 galaxies across different timescales, revealing that long-term coherence in variability is linked to jet activity and orientation, aiding interpretation of AGN behavior.

Contribution

It demonstrates that structure function-derived temporal coherence effectively indicates jet dominance and orientation in AGN, advancing variability diagnostics.

Findings

Gamma-ray detected RL-NLSy1s and HPQs show strong long-term coherence.

Non-jetted RL-NLSy1s exhibit stochastic, disc-driven variability.

Jet-dominated sources display redder-when-brighter trends.

Abstract

We investigate optical variability across multiple timescales in a sample of radio-loud narrow-line Seyfert~1 (RL-NLSy1) galaxies, including $\gamma$-ray detected, $\gamma$-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 ($F_{\rm var}$) and rest-frame structure functions (SFs) to test whether short-term jet-linked variability is reflected in long-term behaviour. $\gamma$-ray detected RL-NLSy1s and HPQs show steeply rising SFs, revealing strong long-term coherence despite modest $F_{\rm var}$, consistent with Doppler-boosted synchrotron emission from relativistic jets. Non-jetted RL-NLSy1s exhibit the highest $F_{\rm var}$ but plateauing SFs, indicative of stochastic, disc-driven fluctuations lacking long-term coherence. $\gamma$-ray undetected RL-NLSy1s show the lowest $F_{\rm var}$ 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.