Published June 8, 2023 | Version v1
Dataset Open

Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of the simulated galaxies of the Auriga project

  • 1. Ghent University
  • 1. Ghent University
  • 2. Liverpool John Moores University
  • 3. Max Planck Institute fur Astronomie
  • 4. University of Pittsburgh

Description

We present realistic mock spectroscopic observations for state-of-the-art hydrodynamical simulations, using high spectral resolution stellar population models (FSPS) and full radiative transfer treatment with SKIRT. The dataset contains IFS-like spectroscopy of the stellar continuum for 10 (of the 30) galaxies in the Auriga Project at z=0. One galaxy at z=0.8 (Au 6) and another at z=3 (Au 29).

Notes

Visit www.auriga.ugent.be for further information. This project received funding from the European Research Council (ERC) under the European Union's Horizon 2020 Framework Programme, grant agreement no. 683184 (Consolidator Grant LEGA-C). D.B, M.B and A.U.K acknowledge the financial support of the Flemish Fund for Scientific Research (FWO-Vlaanderen), research projects G039216N and G030319N. R.G acknowledges financial support from the Spanish Ministry of Science and Innovation (MICINN) through the Spanish State Research Agency, under the Severo Ochoa Program 2020-2023 (CEX2019-000920-S) and an STFC Ernest Rutherford Fellowship (ST/W003643/1).

Files

Au1-z0.zip

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Additional details

Funding

European Commission
LEGA-C – The Physics of Galaxies 7 Gyr Ago 683184