2024RNAAS...8..253C

Query : 2024RNAAS...8..253C

2024RNAAS...8..253C - Research Notes of the AAS, 8, 253 (2024/October-0)

Frequency-resolved Lag Predictions of the Corona-heated Accretion-disk Reprocessing Model Agree Well with the UV/Optical Reverberation Mapping of Mrk 817.

CHEN J., SUN M. and ZHOU S.

Abstract (from CDS):

The frequency-resolved time lags of UV/optical reverberation mappings of active galactic nuclei (AGNs) can uniquely probe the accretion physics around supermassive black holes. In previous work, we made frequency-resolved lag predictions for Mrk 817, the AGN STORM II target, based on the Corona-Heated Accretion-disk Reprocessing model. Recently, the frequency-resolved time lags of Mrk 817 have been reported. Here we show that the reported time lags are fully consistent with our earlier theoretical predictions.

Abstract Copyright: © 2024. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Active galactic nuclei - Supermassive black holes

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 Mrk 335 Sy1 00 06 19.5372339024 +20 12 10.617404076   14.19 13.85     ~ 1344 0
2 ESO 113-45 Sy1 01 23 45.7631533440 -58 48 20.808928944   14.08 13.83 13.34   ~ 965 0
3 NGC 5548 Sy1 14 17 59.5400291832 +25 08 12.603122268   14.35 13.73     ~ 2895 0
4 Z 296-15 Sy1 14 36 22.0820611632 +58 47 39.394934844   14.19 13.79     ~ 592 0

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