Unveiling Accretion-Disk Reverberation Beneath BLR Contamination with TILDE

@misc{jung2026unveiling,
  title = {{Unveiling Accretion-Disk Reverberation Beneath BLR Contamination with TILDE}},
  author = {Sungho Jung and Jong-Hak Woo},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.29173},
  eprint = {2610.29173},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.29173},
  note = {CC BY 4.0},
}

TY  - UNPB
TI  - Unveiling Accretion-Disk Reverberation Beneath BLR Contamination with TILDE
AU  - Sungho Jung
AU  - Jong-Hak Woo
PY  - 2026
DA  - 2026/10/21
PB  - arXiv
DO  - 10.48550/arxiv.2610.29173
UR  - https://arxiv.org/abs/2610.29173
AB  - We present a Bayesian framework, Two-stage Inference for Light curve DEcomposition (TILDE), for mapping the accretion disk and the broad line region (BLR) from active galactic nuclei (AGN) multi-band light curves. By inferring delayed BLR contamination from the underlying disk variability, TILDE provides the delay measurements of the disk as well as the BLR. We validate TILDE using synthetic data, finding that TILDE recovers the known time delays of the disk and BLR. By applying TILDE to the Seoul National University AGN Monitoring Project sample, we find that the inferred BLR light curves match the observed Hβ emission light curves, providing consistent BLR lags compared to the reported Hβ lags. Using the lag spectrum, effectively corrected for the BLR contamination, we find that the disk size is broadly consistent with the standard thin-disk model, suggesting that BLR contamination can significantly bias the disk size derived from the cross-correlation analysis of the broad-band photometry. These results demonstrate that the new inference method is a powerful tool for determining both disk and BLR sizes from broad-band photometry in the era of time-domain surveys.
ER  -