Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies ...

We present a framework to build realistic mock spectroscopic observations for state-of-the-art hydrodynamical simulations, using high spectral resolution stellar population models and full radiative transfer treatment with SKIRT. As a first application we generate stellar continuum mock observations...

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Main Authors: Acevedo, Daniela Barrientos, van der Wel, Arjen, Baes, Maarten, Grand, Robert J. J, Kapoor, Anand Utsav, Camps, Peter, de Graaff, Anna, Straatman, Caroline M. S., Bezanson, Rachel
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Published: arXiv 2023
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Online Access:https://dx.doi.org/10.48550/arxiv.2306.08040
https://arxiv.org/abs/2306.08040
id ftdatacite:10.48550/arxiv.2306.08040
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spelling ftdatacite:10.48550/arxiv.2306.08040 2023-10-01T03:59:15+02:00 Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies ... Acevedo, Daniela Barrientos van der Wel, Arjen Baes, Maarten Grand, Robert J. J Kapoor, Anand Utsav Camps, Peter de Graaff, Anna Straatman, Caroline M. S. Bezanson, Rachel 2023 https://dx.doi.org/10.48550/arxiv.2306.08040 https://arxiv.org/abs/2306.08040 unknown arXiv https://dx.doi.org/10.1093/mnras/stad1771 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics of Galaxies astro-ph.GA FOS Physical sciences ScholarlyArticle Article article-journal Text 2023 ftdatacite https://doi.org/10.48550/arxiv.2306.0804010.1093/mnras/stad1771 2023-09-04T12:52:50Z We present a framework to build realistic mock spectroscopic observations for state-of-the-art hydrodynamical simulations, using high spectral resolution stellar population models and full radiative transfer treatment with SKIRT. As a first application we generate stellar continuum mock observations for the Auriga cosmological zoom simulations emulating integral-field observations from the SAMI Galaxy survey. We perform spectral fitting on our synthetic cubes and compute the resulting rotation velocity ($V_{\rm{rot}}$) and velocity dispersion within 1$R_{\text{e}}$ ($σ_{\text{e}}$) for a sub-set of the Auriga sample. We find that the kinematics produced by Auriga are in good agreement with the observations from the SAMI Galaxy survey after taking into account the effects of dust and the systematics produced by the observation limitations. We also explore the effects of seeing convolution, inclination, and attenuation on the line-of-sight velocity distribution. For highly inclined galaxies, these effects can ... : 17 pages, 11 figures. Accepted for publication in MNRAS ... Text sami DataCite Metadata Store (German National Library of Science and Technology)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics of Galaxies astro-ph.GA
FOS Physical sciences
spellingShingle Astrophysics of Galaxies astro-ph.GA
FOS Physical sciences
Acevedo, Daniela Barrientos
van der Wel, Arjen
Baes, Maarten
Grand, Robert J. J
Kapoor, Anand Utsav
Camps, Peter
de Graaff, Anna
Straatman, Caroline M. S.
Bezanson, Rachel
Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies ...
topic_facet Astrophysics of Galaxies astro-ph.GA
FOS Physical sciences
description We present a framework to build realistic mock spectroscopic observations for state-of-the-art hydrodynamical simulations, using high spectral resolution stellar population models and full radiative transfer treatment with SKIRT. As a first application we generate stellar continuum mock observations for the Auriga cosmological zoom simulations emulating integral-field observations from the SAMI Galaxy survey. We perform spectral fitting on our synthetic cubes and compute the resulting rotation velocity ($V_{\rm{rot}}$) and velocity dispersion within 1$R_{\text{e}}$ ($σ_{\text{e}}$) for a sub-set of the Auriga sample. We find that the kinematics produced by Auriga are in good agreement with the observations from the SAMI Galaxy survey after taking into account the effects of dust and the systematics produced by the observation limitations. We also explore the effects of seeing convolution, inclination, and attenuation on the line-of-sight velocity distribution. For highly inclined galaxies, these effects can ... : 17 pages, 11 figures. Accepted for publication in MNRAS ...
format Text
author Acevedo, Daniela Barrientos
van der Wel, Arjen
Baes, Maarten
Grand, Robert J. J
Kapoor, Anand Utsav
Camps, Peter
de Graaff, Anna
Straatman, Caroline M. S.
Bezanson, Rachel
author_facet Acevedo, Daniela Barrientos
van der Wel, Arjen
Baes, Maarten
Grand, Robert J. J
Kapoor, Anand Utsav
Camps, Peter
de Graaff, Anna
Straatman, Caroline M. S.
Bezanson, Rachel
author_sort Acevedo, Daniela Barrientos
title Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies ...
title_short Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies ...
title_full Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies ...
title_fullStr Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies ...
title_full_unstemmed Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies ...
title_sort spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies ...
publisher arXiv
publishDate 2023
url https://dx.doi.org/10.48550/arxiv.2306.08040
https://arxiv.org/abs/2306.08040
genre sami
genre_facet sami
op_relation https://dx.doi.org/10.1093/mnras/stad1771
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.2306.0804010.1093/mnras/stad1771
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