Self-consistent Bulge/Disk/Halo Galaxy Dynamical Modeling Using Integral Field Kinematics
We introduce a method for modeling disk galaxies designed to take full advantage of data from integral field spectroscopy (IFS). The method fits equilibrium models to simultaneously reproduce the surface brightness, rotation, and velocity dispersion profiles of a galaxy. The models are fully self-co...
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2017
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Online Access: | https://espace.library.uq.edu.au/view/UQ:702276/UQ702276_OA.pdf https://espace.library.uq.edu.au/view/UQ:702276 |
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ftunivqespace:oai:espace.library.uq.edu.au:UQ:702276 2023-05-15T18:11:52+02:00 Self-consistent Bulge/Disk/Halo Galaxy Dynamical Modeling Using Integral Field Kinematics Taranu, D. S. Obreschkow, D. Dubinski, J. J. Fogarty, L. M. R. van de Sande, J. Catinella, B. Cortese, L. Moffett, A. Robotham, A. S. G. Allen, J. T. Bland-Hawthorn, J. Bryant, J. J. Colless, M. Croom, S. M. D'Eugenio, F. Davies, R. L. Drinkwater, M. J. Driver, S. P. Goodwin, M. Konstantopoulos, I. S. Lawrence, J. S. Lopez-Sanchez, A. R. Lorente, N. P. F. Medling, A. M. Mould, J. R. Owers, M. S. Power, C. Richards, S. N. Tonini, C. 2017-11-20 https://espace.library.uq.edu.au/view/UQ:702276/UQ702276_OA.pdf https://espace.library.uq.edu.au/view/UQ:702276 eng eng Institute of Physics Publishing doi:10.3847/1538-4357/aa9221 issn:0004-637X issn:1538-4357 orcid:0000-0003-4867-0022 CE110001020 Not set FT120100660 ST/K00106X/1 ST/N000919/1 Bulge-Disc Decomposition Fundamental Plane Elliptic Galaxies Sauron Project Halo Models Sky Survey Stellar Systems Profile Images 1912 Space and Planetary Science 3103 Astronomy and Astrophysics Journal Article 2017 ftunivqespace https://doi.org/10.3847/1538-4357/aa9221 2020-12-22T13:19:57Z We introduce a method for modeling disk galaxies designed to take full advantage of data from integral field spectroscopy (IFS). The method fits equilibrium models to simultaneously reproduce the surface brightness, rotation, and velocity dispersion profiles of a galaxy. The models are fully self-consistent 6D distribution functions for a galaxy with a Srsic profile stellar bulge, exponential disk, and parametric dark-matter halo, generated by an updated version of GalactICS. By creating realistic flux-weighted maps of the kinematic moments (flux, mean velocity, and dispersion), we simultaneously fit photometric and spectroscopic data using both maximumlikelihood and Bayesian (MCMC) techniques. We apply the method to a GAMA spiral galaxy (G79635) with kinematics from the SAMI Galaxy Survey and deep g- and r-band photometry from the VST-KiDS survey, comparing parameter constraints with those from traditional 2D bulge-disk decomposition. Our method returns broadly consistent results for shared parameters while constraining the mass-to-light ratios of stellar components and reproducing the H I-inferred circular velocity well beyond the limits of the SAMI data. Although the method is tailored for fitting integral field kinematic data, it can use other dynamical constraints like central fiber dispersions and H I circular velocities, and is well-suited for modeling galaxies with a combination of deep imaging and H I and/or optical spectra (resolved or otherwise). Our implementation (MagRite) is computationally efficient and can generate well-resolved models and kinematic maps in under a minute on modern processors. Article in Journal/Newspaper sami The University of Queensland: UQ eSpace The Astrophysical Journal 850 1 70 |
institution |
Open Polar |
collection |
The University of Queensland: UQ eSpace |
op_collection_id |
ftunivqespace |
language |
English |
topic |
Bulge-Disc Decomposition Fundamental Plane Elliptic Galaxies Sauron Project Halo Models Sky Survey Stellar Systems Profile Images 1912 Space and Planetary Science 3103 Astronomy and Astrophysics |
spellingShingle |
Bulge-Disc Decomposition Fundamental Plane Elliptic Galaxies Sauron Project Halo Models Sky Survey Stellar Systems Profile Images 1912 Space and Planetary Science 3103 Astronomy and Astrophysics Taranu, D. S. Obreschkow, D. Dubinski, J. J. Fogarty, L. M. R. van de Sande, J. Catinella, B. Cortese, L. Moffett, A. Robotham, A. S. G. Allen, J. T. Bland-Hawthorn, J. Bryant, J. J. Colless, M. Croom, S. M. D'Eugenio, F. Davies, R. L. Drinkwater, M. J. Driver, S. P. Goodwin, M. Konstantopoulos, I. S. Lawrence, J. S. Lopez-Sanchez, A. R. Lorente, N. P. F. Medling, A. M. Mould, J. R. Owers, M. S. Power, C. Richards, S. N. Tonini, C. Self-consistent Bulge/Disk/Halo Galaxy Dynamical Modeling Using Integral Field Kinematics |
topic_facet |
Bulge-Disc Decomposition Fundamental Plane Elliptic Galaxies Sauron Project Halo Models Sky Survey Stellar Systems Profile Images 1912 Space and Planetary Science 3103 Astronomy and Astrophysics |
description |
We introduce a method for modeling disk galaxies designed to take full advantage of data from integral field spectroscopy (IFS). The method fits equilibrium models to simultaneously reproduce the surface brightness, rotation, and velocity dispersion profiles of a galaxy. The models are fully self-consistent 6D distribution functions for a galaxy with a Srsic profile stellar bulge, exponential disk, and parametric dark-matter halo, generated by an updated version of GalactICS. By creating realistic flux-weighted maps of the kinematic moments (flux, mean velocity, and dispersion), we simultaneously fit photometric and spectroscopic data using both maximumlikelihood and Bayesian (MCMC) techniques. We apply the method to a GAMA spiral galaxy (G79635) with kinematics from the SAMI Galaxy Survey and deep g- and r-band photometry from the VST-KiDS survey, comparing parameter constraints with those from traditional 2D bulge-disk decomposition. Our method returns broadly consistent results for shared parameters while constraining the mass-to-light ratios of stellar components and reproducing the H I-inferred circular velocity well beyond the limits of the SAMI data. Although the method is tailored for fitting integral field kinematic data, it can use other dynamical constraints like central fiber dispersions and H I circular velocities, and is well-suited for modeling galaxies with a combination of deep imaging and H I and/or optical spectra (resolved or otherwise). Our implementation (MagRite) is computationally efficient and can generate well-resolved models and kinematic maps in under a minute on modern processors. |
format |
Article in Journal/Newspaper |
author |
Taranu, D. S. Obreschkow, D. Dubinski, J. J. Fogarty, L. M. R. van de Sande, J. Catinella, B. Cortese, L. Moffett, A. Robotham, A. S. G. Allen, J. T. Bland-Hawthorn, J. Bryant, J. J. Colless, M. Croom, S. M. D'Eugenio, F. Davies, R. L. Drinkwater, M. J. Driver, S. P. Goodwin, M. Konstantopoulos, I. S. Lawrence, J. S. Lopez-Sanchez, A. R. Lorente, N. P. F. Medling, A. M. Mould, J. R. Owers, M. S. Power, C. Richards, S. N. Tonini, C. |
author_facet |
Taranu, D. S. Obreschkow, D. Dubinski, J. J. Fogarty, L. M. R. van de Sande, J. Catinella, B. Cortese, L. Moffett, A. Robotham, A. S. G. Allen, J. T. Bland-Hawthorn, J. Bryant, J. J. Colless, M. Croom, S. M. D'Eugenio, F. Davies, R. L. Drinkwater, M. J. Driver, S. P. Goodwin, M. Konstantopoulos, I. S. Lawrence, J. S. Lopez-Sanchez, A. R. Lorente, N. P. F. Medling, A. M. Mould, J. R. Owers, M. S. Power, C. Richards, S. N. Tonini, C. |
author_sort |
Taranu, D. S. |
title |
Self-consistent Bulge/Disk/Halo Galaxy Dynamical Modeling Using Integral Field Kinematics |
title_short |
Self-consistent Bulge/Disk/Halo Galaxy Dynamical Modeling Using Integral Field Kinematics |
title_full |
Self-consistent Bulge/Disk/Halo Galaxy Dynamical Modeling Using Integral Field Kinematics |
title_fullStr |
Self-consistent Bulge/Disk/Halo Galaxy Dynamical Modeling Using Integral Field Kinematics |
title_full_unstemmed |
Self-consistent Bulge/Disk/Halo Galaxy Dynamical Modeling Using Integral Field Kinematics |
title_sort |
self-consistent bulge/disk/halo galaxy dynamical modeling using integral field kinematics |
publisher |
Institute of Physics Publishing |
publishDate |
2017 |
url |
https://espace.library.uq.edu.au/view/UQ:702276/UQ702276_OA.pdf https://espace.library.uq.edu.au/view/UQ:702276 |
genre |
sami |
genre_facet |
sami |
op_relation |
doi:10.3847/1538-4357/aa9221 issn:0004-637X issn:1538-4357 orcid:0000-0003-4867-0022 CE110001020 Not set FT120100660 ST/K00106X/1 ST/N000919/1 |
op_doi |
https://doi.org/10.3847/1538-4357/aa9221 |
container_title |
The Astrophysical Journal |
container_volume |
850 |
container_issue |
1 |
container_start_page |
70 |
_version_ |
1766184475556839424 |