A Short-timescale Negative Optical Continuum Lag in SDSS J083717.88+191647

TL;DR

This study reports a unique negative optical continuum lag in an AGN, SDSS J083717.88+191647, revealing complex variability possibly caused by dust obscuration, challenging traditional accretion disk models.

Contribution

It presents the first clear phase-dependent negative lag in an AGN, supported by multi-phase observations and a dust-cloud obscuration explanation.

Findings

Detected a negative inter-band lag of about -1.6 days during the declining phase.

Observed opposite lag signs during stabilizing and declining phases.

Proposed dust obscuration as a cause for lag reversal in AGN variability.

Abstract

Continuum reverberation mapping (RM) is a powerful technique for constraining the accretion disk structure in active galactic nuclei (AGNs). In typical cases, the shorter-wavelength emission is used as the reference, and a positive time lag is observed since the inner, hotter regions of the accretion disk respond earlier than the cooler outer regions at longer wavelengths. However, we detect a short-timescale negative inter-band lag in SDSS~J083717.88+191647 using RM techniques, where the \textit{g}-band lags behind the \textit{r}-band emission. The light curves from the Zwicky Transient Facility reveal two distinct phases, a stabilizing and a declining phase, in which the time lags show opposite signs. Using \texttt{JAVELIN} with the $g$-band as the reference, we obtain time lags of $3.68^{+1.94}_{-2.78}$~days during the stabilizing phase and $-1.60^{+0.69}_{-0.54}$~days during the declining phase. Although negative continuum lags have been reported in a few previous studies, the present case is distinguished by its clear phase dependence and the accompanying color evolution. We attribute the observed lag reversal to a moving dust-cloud obscuration scenario, in which the cloud crossing the line of sight preferentially obscures emission from the outer longer-wavelength regions of the disk, causing the $r$-band to decline earlier than the $g$-band and thus producing the observed negative inter-band lag. Our results indicate that AGN variability may be more complex than previously thought. Future high-cadence, multi-band observations will be essential to test this dust-obscuration model and to further explore the interplay between the accretion disk emission and dust in AGNs.