Colin J. Burke
Optical Variability of the Dwarf AGN NGC 4395 from the Transiting Exoplanet Survey Satellite
Burke, Colin J.; Shen, Yue; Chen, Yu-Ching; Scaringi, Simone; Faucher-Giguere, Claude-Andre; Liu, Xin; Yang, Qian
Authors
Yue Shen
Yu-Ching Chen
Dr Simone Scaringi simone.scaringi@durham.ac.uk
Associate Professor
Claude-Andre Faucher-Giguere
Xin Liu
Qian Yang
Abstract
We present optical light curves from the Transiting Exoplanet Survey Satellite (TESS) for the archetypical dwarf active galactic nucleus (AGN) in the nearby galaxy NGC 4395 hosting a ~105 M⊙ supermassive black hole (SMBH). Significant variability is detected on timescales from weeks to hours before reaching the background noise level. The ~month-long, 30 minute-cadence, high-precision TESS light curve can be well fit by a simple damped random walk (DRW) model, with the damping timescale τDRW constrained to be ${2.3}_{-0.7}^{+1.8}$ days (1σ). NGC 4395 lies almost exactly on the extrapolation of the ${\tau }_{\mathrm{DRW}}-{M}_{\mathrm{BH}}$ relation measured for AGNs with BH masses that are more than three orders of magnitude larger. The optical variability periodogram can be well fit by a broken power law with the high-frequency slope (−1.88 ± 0.15) and the characteristic timescale (${\tau }_{\mathrm{br}}\equiv 1/(2\pi {f}_{\mathrm{br}})={1.4}_{-0.5}^{+1.9}$ days) consistent with the DRW model within 1σ. This work demonstrates the power of TESS light curves in identifying low-mass accreting SMBHs with optical variability, and a potential global ${\tau }_{\mathrm{DRW}}-{M}_{\mathrm{BH}}$ relation that can be used to estimate SMBH masses with optical variability measurements.
Citation
Burke, C. J., Shen, Y., Chen, Y.-C., Scaringi, S., Faucher-Giguere, C.-A., Liu, X., & Yang, Q. (2020). Optical Variability of the Dwarf AGN NGC 4395 from the Transiting Exoplanet Survey Satellite. Astrophysical Journal, 899(2), https://doi.org/10.3847/1538-4357/aba3ce
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 4, 2020 |
Online Publication Date | Aug 24, 2020 |
Publication Date | 2020 |
Deposit Date | Dec 31, 2020 |
Publicly Available Date | Aug 24, 2021 |
Journal | Astrophysical Journal |
Print ISSN | 0004-637X |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 899 |
Issue | 2 |
DOI | https://doi.org/10.3847/1538-4357/aba3ce |
Public URL | https://durham-repository.worktribe.com/output/1283138 |
Files
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