Comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations
Cosmological hydrodynamical simulations are rich tools to understand the role and impact of galaxy environment and mergers, and gas dynamics and stellar kinematics in galaxy formation and evolution. However, these simulations require some level of calibration to observations. In this talk, I will co...
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ftdatacite:10.5281/zenodo.2635205 2023-05-15T18:12:08+02:00 Comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations van de Sande, Jesse None 2019 https://dx.doi.org/10.5281/zenodo.2635205 https://zenodo.org/record/2635205 unknown Zenodo https://zenodo.org/communities/esoaus2019 https://dx.doi.org/10.5281/zenodo.2635204 https://zenodo.org/communities/esoaus2019 Open Access Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 info:eu-repo/semantics/openAccess CC-BY Text Presentation article-journal ScholarlyArticle 2019 ftdatacite https://doi.org/10.5281/zenodo.2635205 https://doi.org/10.5281/zenodo.2635204 2021-11-05T12:55:41Z Cosmological hydrodynamical simulations are rich tools to understand the role and impact of galaxy environment and mergers, and gas dynamics and stellar kinematics in galaxy formation and evolution. However, these simulations require some level of calibration to observations. In this talk, I will compare predictions at z=0 from the Eagle, Hydrangea, Horizon-AGN, and Magneticum simulations with IFS data from the SAMI Galaxy Survey, ATLAS-3D, CALIFA and MASSIVE surveys. The main goal of our work is to simultaneously compare structural, dynamical, and stellar population measurements, in order to identify key areas of success and tension. I will show that our comparison between simulations and observational data has highlighted several areas for improvement, such as the need for improved modelling resulting in a better vertical disk structure. Yet these results that I will present, will demonstrate the vast improvement of cosmological simulations in recent years. Conference Object sami DataCite Metadata Store (German National Library of Science and Technology) |
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Cosmological hydrodynamical simulations are rich tools to understand the role and impact of galaxy environment and mergers, and gas dynamics and stellar kinematics in galaxy formation and evolution. However, these simulations require some level of calibration to observations. In this talk, I will compare predictions at z=0 from the Eagle, Hydrangea, Horizon-AGN, and Magneticum simulations with IFS data from the SAMI Galaxy Survey, ATLAS-3D, CALIFA and MASSIVE surveys. The main goal of our work is to simultaneously compare structural, dynamical, and stellar population measurements, in order to identify key areas of success and tension. I will show that our comparison between simulations and observational data has highlighted several areas for improvement, such as the need for improved modelling resulting in a better vertical disk structure. Yet these results that I will present, will demonstrate the vast improvement of cosmological simulations in recent years. |
format |
Conference Object |
author |
van de Sande, Jesse None |
spellingShingle |
van de Sande, Jesse None Comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations |
author_facet |
van de Sande, Jesse None |
author_sort |
van de Sande, Jesse |
title |
Comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations |
title_short |
Comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations |
title_full |
Comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations |
title_fullStr |
Comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations |
title_full_unstemmed |
Comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations |
title_sort |
comparing 3d spectroscopic observations with galaxies from cosmological hydrodynamical simulations |
publisher |
Zenodo |
publishDate |
2019 |
url |
https://dx.doi.org/10.5281/zenodo.2635205 https://zenodo.org/record/2635205 |
genre |
sami |
genre_facet |
sami |
op_relation |
https://zenodo.org/communities/esoaus2019 https://dx.doi.org/10.5281/zenodo.2635204 https://zenodo.org/communities/esoaus2019 |
op_rights |
Open Access Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 info:eu-repo/semantics/openAccess |
op_rightsnorm |
CC-BY |
op_doi |
https://doi.org/10.5281/zenodo.2635205 https://doi.org/10.5281/zenodo.2635204 |
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1766184693102804992 |