Radial-dependent Responsivity of Broad-line Regions in Active Galactic Nuclei: Observational Consequences for Reverberation Mapping and Black Hole Mass Measurements

The reverberation mapping (RM) technique has seen wide applications in probing geometry and kinematics of broad-line regions (BLRs) and measuring masses of supermassive black holes (SMBHs) in active galactic nuclei. However, key quantities in RM analysis such as emissivity, responsivity, transfer fu...

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Main Authors: Yan-Rong Li, Jian-Min Wang
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ad9fee
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author Yan-Rong Li
Jian-Min Wang
author_facet Yan-Rong Li
Jian-Min Wang
author_sort Yan-Rong Li
collection DOAJ
description The reverberation mapping (RM) technique has seen wide applications in probing geometry and kinematics of broad-line regions (BLRs) and measuring masses of supermassive black holes (SMBHs) in active galactic nuclei. However, key quantities in RM analysis such as emissivity, responsivity, transfer functions, and mean and rms spectra are fragmentally defined in the literature and largely lack a unified formulation. Here we establish a rigorous framework for BLR RM and include a locally dependent responsivity according to photoionization calculations. The mean and rms spectra are analytically expressed with emissivity- and responsivity-weighted transfer functions, respectively. We demonstrate that the rms spectrum is proportional to the responsivity-weighted transfer function only when the continuum variation timescale is much longer than the typical extension in time delay of the BLR; otherwise, biases arise in the obtained rms line widths. The long-standing phenomenon pertaining to the different shapes between the mean and rms spectra can be explained by a radial-increasing responsivity of BLRs. The debate on the choice of emission-line widths for SMBH mass measurements is explored, and the virial factors are suggested to also depend on the luminosity states, in addition to the geometry and kinematics of BLRs.
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spelling doaj-art-c168e5ca4b9a414f89e8a34a3c3288372025-08-20T03:09:28ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01979212610.3847/1538-4357/ad9feeRadial-dependent Responsivity of Broad-line Regions in Active Galactic Nuclei: Observational Consequences for Reverberation Mapping and Black Hole Mass MeasurementsYan-Rong Li0https://orcid.org/0000-0001-5841-9179Jian-Min Wang1https://orcid.org/0000-0001-9449-9268Key Laboratory for Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, People’s Republic of China ; liyanrong@mail.ihep.ac.cn, wangjm@mail.ihep.ac.cnKey Laboratory for Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, People’s Republic of China ; liyanrong@mail.ihep.ac.cn, wangjm@mail.ihep.ac.cn; School of Astronomy and Space Sciences, University of Chinese Academy of Sciences , Beijing 100049, People’s Republic of China; National Astronomical Observatory of China , 20A Datun Road, Beijing 100020, People’s Republic of ChinaThe reverberation mapping (RM) technique has seen wide applications in probing geometry and kinematics of broad-line regions (BLRs) and measuring masses of supermassive black holes (SMBHs) in active galactic nuclei. However, key quantities in RM analysis such as emissivity, responsivity, transfer functions, and mean and rms spectra are fragmentally defined in the literature and largely lack a unified formulation. Here we establish a rigorous framework for BLR RM and include a locally dependent responsivity according to photoionization calculations. The mean and rms spectra are analytically expressed with emissivity- and responsivity-weighted transfer functions, respectively. We demonstrate that the rms spectrum is proportional to the responsivity-weighted transfer function only when the continuum variation timescale is much longer than the typical extension in time delay of the BLR; otherwise, biases arise in the obtained rms line widths. The long-standing phenomenon pertaining to the different shapes between the mean and rms spectra can be explained by a radial-increasing responsivity of BLRs. The debate on the choice of emission-line widths for SMBH mass measurements is explored, and the virial factors are suggested to also depend on the luminosity states, in addition to the geometry and kinematics of BLRs.https://doi.org/10.3847/1538-4357/ad9feeReverberation mappingSupermassive black holesActive galactic nuclei
spellingShingle Yan-Rong Li
Jian-Min Wang
Radial-dependent Responsivity of Broad-line Regions in Active Galactic Nuclei: Observational Consequences for Reverberation Mapping and Black Hole Mass Measurements
The Astrophysical Journal
Reverberation mapping
Supermassive black holes
Active galactic nuclei
title Radial-dependent Responsivity of Broad-line Regions in Active Galactic Nuclei: Observational Consequences for Reverberation Mapping and Black Hole Mass Measurements
title_full Radial-dependent Responsivity of Broad-line Regions in Active Galactic Nuclei: Observational Consequences for Reverberation Mapping and Black Hole Mass Measurements
title_fullStr Radial-dependent Responsivity of Broad-line Regions in Active Galactic Nuclei: Observational Consequences for Reverberation Mapping and Black Hole Mass Measurements
title_full_unstemmed Radial-dependent Responsivity of Broad-line Regions in Active Galactic Nuclei: Observational Consequences for Reverberation Mapping and Black Hole Mass Measurements
title_short Radial-dependent Responsivity of Broad-line Regions in Active Galactic Nuclei: Observational Consequences for Reverberation Mapping and Black Hole Mass Measurements
title_sort radial dependent responsivity of broad line regions in active galactic nuclei observational consequences for reverberation mapping and black hole mass measurements
topic Reverberation mapping
Supermassive black holes
Active galactic nuclei
url https://doi.org/10.3847/1538-4357/ad9fee
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AT jianminwang radialdependentresponsivityofbroadlineregionsinactivegalacticnucleiobservationalconsequencesforreverberationmappingandblackholemassmeasurements