AGN Continuum Reverberation Mapping Based on Zwicky Transient Facility Light Curves
arXiv:2207.06432 · doi:10.3847/1538-4357/ac96ec
Abstract
We perform a systematic survey of active galactic nucleus (AGN) continuum lags using 3 day cadence -band light curves from the Zwicky Transient Facility. We select a sample of 94 type 1 AGN at with significant and consistent inter-band lags based on the interpolated cross-correlation function method and the Bayesian method JAVELIN. Within the framework of the lamp-post reprocessing model, our findings are: 1) The continuum emission (CE) sizes inferred from the data are larger than the disk sizes predicted by the standard thin disk model; 2) For a subset of the sample, the CE size exceeds the theoretical limit of the self-gravity radius (12 lt-days) for geometrically thin disks; 3) The CE size scales with continuum luminosity as with a scatter of 0.2 dex, analogous to the well-known radius-luminosity relation of broad H. These findings suggest a significant contribution of diffuse continuum emission from the broad-line region (BLR) to AGN continuum lags. We find that the relation can be explained by a photoionization model that assumes 23% of the total flux comes from the diffuse BLR emission. In addition, the ratio of the CE size and model-predicted disk size anti-correlates with the continuum luminosity, indicative of a potential non-disk BLR lag contribution evolving with luminosity. Finally, a robust positive correlation between CE size and black hole mass is detected.
arXiv comment26 pages, 12 figures, 4 tables. Accepted by ApJ
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