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.
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
1 January 2017
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
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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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