Synthetic galaxy images and spectra from the Illustris simulation
@article{Torrey2015SyntheticGI, title={Synthetic galaxy images and spectra from the Illustris simulation}, author={Paul Torrey and Gregory F. Snyder and Mark Vogelsberger and Christopher C. Hayward and Shy Genel and Debora Sijacki and Volker Springel and Lars Hernquist and Dylan Nelson and Mariska Kriek and Annalisa Pillepich and Laura V. Sales and Cameron McBride}, journal={Monthly Notices of the Royal Astronomical Society}, year={2015}, volume={447}, pages={2753-2771} }
We present our methods for generating a catalogue of 7000 synthetic images and 40 000 integrated spectra of redshift z = 0 galaxies from the Illustris simulation. The mock data products are produced by using stellar population synthesis models to assign spectral energy distributions (SED) to each star particle in the galaxies. The resulting synthetic images and integrated SEDs therefore properly reflect the spatial distribution, stellar metallicity distribution, and star formation history of…
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References
SHOWING 1-10 OF 135 REFERENCES
Recovering stellar population properties and redshifts from broadband photometry of simulated galaxies: Lessons for SED modeling
- Physics
- 2009
We present a detailed analysis of our ability to determine stellar masses, ages, reddening, and extinction values, and star formation rates (SFRs) of high-redshift galaxies by modeling broadband…
Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
- Physics
- 2014
We present an overview of galaxy evolution across cosmic time in the Illustris Simulation. Illustris is an N-body/hydrodynamical simulation that evolves 2*1820^3 resolution elements in a (106.5Mpc)^3…
SIMULATED GALAXY INTERACTIONS AS PROBES OF MERGER SPECTRAL ENERGY DISTRIBUTIONS
- Physics
- 2014
We present the first systematic comparison of ultraviolet-millimeter spectral energy distributions (SEDs) of observed and simulated interacting galaxies. Our sample is drawn from the Spitzer…
High-resolution panchromatic spectral models of galaxies including photoionization and dust
- Physics
- 2009
An updated version of the dust radiation-transfer code SUNRISE, including models for star-forming regions and a self-consistent calculation of the spatially dependent dust and PAH emission, is…
How well can we really estimate the stellar masses of galaxies from broad-band photometry?
- Physics
- 2013
The estimated stellar masses of galaxies are widely used to characterize how the galaxy population evolves over cosmic time. If stellar masses can be estimated in a robust manner, free from any bias,…
A model for cosmological simulations of galaxy formation physics: multi-epoch validation
- Physics
- 2014
We present a multi-epoch analysis of the galaxy populations formed within the cosmological hydrodynamical simulations presented in Vogelsberger et al. (2013). These simulations explore the…
Confronting theoretical models with the observed evolution of the galaxy population out to z= 4
- Physics
- 2011
We construct lightcones for the semi-analytic galaxy formation simulation of Guo et al. (2011) and make mock catalogues for comparison with deep high-redshift surveys. Photometric properties are…
The Propagation of Uncertainties in Stellar Population Synthesis Modeling. II. The Challenge of Comparing Galaxy Evolution Models to Observations
- Physics
- 2010
Models for the formation and evolution of galaxies readily predict physical properties such as star formation rates, metal-enrichment histories, and, increasingly, gas and dust content of synthetic…
Stellar population synthesis at the resolution of 2003
- Physics
- 2003
We present a new model for computing the spectral evolution of stellar populations at ages between 1 x 10 5 and 2 x 10 1 0 yr at a resolution of 3 A across the whole wavelength range from 3200 to…
Modeling the Pan-Spectral Energy Distribution of Starburst Galaxies. IV. The Controlling Parameters of the Starburst SED
- Physics
- 2008
We combine the stellar spectral synthesis code Starburst99, the nebular modeling code MAPPINGS III and a one-dimensional dynamical evolution model of H II regions around massive clusters of young…