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Improving calibration of the MBH-σ* relation for AGN with the BRAVE program

Improving calibration of the MBH-σ* relation for AGN with the BRAVE program
Improving calibration of the MBH-σ* relation for AGN with the BRAVE program
The MBH - σ* relation for AGN, which relates the mass of the central supermassive black hole (MBH) to the bulge stellar velocity dispersion (σ*) of the host galaxy, is a powerful tool for studying the evolution of structure across cosmic time. Accurate calibration of this relation is essential, and much effort has been put into improving MBH determinations with this in mind. However calibration remains difficult because many nearby AGN with secure MBH determinations are hosted by late-type galaxies, with significant kinematic substructure such as bars, disks and rings. Kinematic substructure is known to contaminate and bias σ* determinations from long-slit and single aperture spectroscopy, ultimately limiting the utility of the MBH - σ* relation, and hampering efforts to investigate morphological dependencies. Integral-field spectroscopy (IFS) can be used to map the two dimensional kinematics, providing a method for measuring σ* absent some of the biases inherent in other methods, and giving a more complete picture of the spatial variations in the dynamics. We present the first set of results from the BRAVE program, the long-term goal of which is to use IFS to more accurately determine σ* for the calibrating sample of reverberation-mapped AGN. We present IFS kinematic maps for the sample of galaxies we have so far observed, which show clearly how spatial variation can impact σ* determinations from long-slit spectroscopy. We present a new fit to the MBH - σ* relation for the sample of 16 reverberation-mapped AGN for which we currently have σ* determinations from IFS, as well as a new determination of the virial scaling factor, f, for use with reverberation-mapping.
2041-8205
Batiste, Merida
4fadf88b-cbf1-4f37-b1db-d4387b24c501
Bentz, Misty C.
23985c11-6a62-4679-a66e-88e71b14da5b
Manne-Nicholas, Emily
75ee64d0-5b7f-4e89-a9c9-c3f69d7c0250
Raimundo, Sandra I.
e409d9d3-17e8-4049-ad29-43ada60b24e2
Onken, Christopher A.
0915cd93-3ee5-4f45-90ba-af671d66e02c
Vestergaard, Marianne
3d2377bc-0c0a-4198-9439-e7e9ac344b4e
Bershady, Matthew A.
558c593a-e59e-4650-9ed5-f776c1b2a3b2
Batiste, Merida
4fadf88b-cbf1-4f37-b1db-d4387b24c501
Bentz, Misty C.
23985c11-6a62-4679-a66e-88e71b14da5b
Manne-Nicholas, Emily
75ee64d0-5b7f-4e89-a9c9-c3f69d7c0250
Raimundo, Sandra I.
e409d9d3-17e8-4049-ad29-43ada60b24e2
Onken, Christopher A.
0915cd93-3ee5-4f45-90ba-af671d66e02c
Vestergaard, Marianne
3d2377bc-0c0a-4198-9439-e7e9ac344b4e
Bershady, Matthew A.
558c593a-e59e-4650-9ed5-f776c1b2a3b2

Batiste, Merida, Bentz, Misty C., Manne-Nicholas, Emily, Raimundo, Sandra I., Onken, Christopher A., Vestergaard, Marianne and Bershady, Matthew A. (2017) Improving calibration of the MBH-σ* relation for AGN with the BRAVE program. The Astrophysical Journal Letters, Meeting 229.

Record type: Meeting abstract

Abstract

The MBH - σ* relation for AGN, which relates the mass of the central supermassive black hole (MBH) to the bulge stellar velocity dispersion (σ*) of the host galaxy, is a powerful tool for studying the evolution of structure across cosmic time. Accurate calibration of this relation is essential, and much effort has been put into improving MBH determinations with this in mind. However calibration remains difficult because many nearby AGN with secure MBH determinations are hosted by late-type galaxies, with significant kinematic substructure such as bars, disks and rings. Kinematic substructure is known to contaminate and bias σ* determinations from long-slit and single aperture spectroscopy, ultimately limiting the utility of the MBH - σ* relation, and hampering efforts to investigate morphological dependencies. Integral-field spectroscopy (IFS) can be used to map the two dimensional kinematics, providing a method for measuring σ* absent some of the biases inherent in other methods, and giving a more complete picture of the spatial variations in the dynamics. We present the first set of results from the BRAVE program, the long-term goal of which is to use IFS to more accurately determine σ* for the calibrating sample of reverberation-mapped AGN. We present IFS kinematic maps for the sample of galaxies we have so far observed, which show clearly how spatial variation can impact σ* determinations from long-slit spectroscopy. We present a new fit to the MBH - σ* relation for the sample of 16 reverberation-mapped AGN for which we currently have σ* determinations from IFS, as well as a new determination of the virial scaling factor, f, for use with reverberation-mapping.

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Published date: 1 January 2017

Identifiers

Local EPrints ID: 504429
URI: http://eprints.soton.ac.uk/id/eprint/504429
ISSN: 2041-8205
PURE UUID: e6a506bb-f704-4a37-b2ec-d64fccf0c3b4
ORCID for Sandra I. Raimundo: ORCID iD orcid.org/0000-0002-6248-398X

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Date deposited: 09 Sep 2025 17:20
Last modified: 10 Sep 2025 10:27

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Contributors

Author: Merida Batiste
Author: Misty C. Bentz
Author: Emily Manne-Nicholas
Author: Christopher A. Onken
Author: Marianne Vestergaard
Author: Matthew A. Bershady

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