On the recovery of galaxy properties from SED fitting solutions
arXiv:1411.7029 · doi:10.1086/679742
Abstract
We explore the ability of four different inverse population synthesis codes to recover the physical properties of galaxies from their spectra by SED fitting. Three codes, DynBaS, TGASPEX, and GASPEX, have been implemented by the authors and are described in detail in the paper. STARLIGHT, the fourth code, is publicly available. DynBaS selects dynamically a different spectral basis to expand the spectrum of each target galaxy; TGASPEX uses an unconstrained age basis, whereas GASPEX and STARLIGHT use for all fits a fixed spectral basis selected a priori by the code developers. Variable and unconstrained basis reflect the peculiarities of the fitted spectrum and allow for simple and robust solutions to the problem of extracting galaxy parameters from spectral fits. We assemble a Synthetic Spectral Atlas of Galaxies (SSAG), comprising 100,000 galaxy spectra corresponding to an equal number of star formation histories based on the recipe of Chen et al. (2012). We select a subset of 120 galaxies from SSAG with a colour distribution similar to that of local galaxies in the seventh data release (DR7) of the Sloan Digital Sky Survey (SDSS) and produce 30 random noise realisations for each of these spectra. For each spectrum we recover the mass, mean age, metallicity, internal dust extinction, and velocity dispersion characterizing the dominant stellar population in the problem galaxy. All methods produce almost perfect fits to the target spectrum, but the recovered physical parameters can differ significantly. Our tests provide a quantitative measure of the accuracy and precision with which these parameters are recovered by each method. From a statistical point of view all methods yield similar precisions, whereas DynBaS produces solutions with minimal systematic biases in the distributions of residuals for all of these parameters.
Minor typos fixed. Accepted for publication at PASP. Synthetic Spectral Atlas of Galaxies (SSAG) available at http://www.astro.ljmu.ac.uk/~asticabr/SSAG.html
References in corpus (4)
- A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
- Recovering galaxy star formation and metallicity histories from spectra using VESPA
- Biases and Uncertainties in Physical Parameter Estimates of Lyman Break Galaxies from Broad-band Photometry
- Constraining globular cluster formation through studies of young massive clusters - II. A Single Stellar Population Young Massive Cluster in NGC 34
Cited by in corpus (14)
- The miniJPAS survey: Identification and characterization of galaxy populations with the J-PAS photometric system
- Simultaneous Constraints on the Star Formation History and Nucleosynthesis of Sculptor dSph
- The miniJPAS survey: The role of group environment in quenching the star formation
- Being WISE II: Reducing the Influence of Star Formation History on the Mass-to-Light Ratio of Quiescent Galaxies
- WEAVE-StePS. A stellar population survey using WEAVE at WHT
- The miniJPAS survey: Identification and characterization of the emission line galaxies down to in the AEGIS field
- Removing biases in resolved stellar mass-maps of galaxy disks through successive Bayesian marginalization
- DIGS: Deep Inference of Galaxy Spectra with Neural Posterior Estimation
- J-PLUS: Detecting and studying extragalactic globular clusters -- the case of NGC 1023
- How the spectral energy distribution and galaxy morphology constrain each other, with application to morphological selection using galaxy colours
- Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
- Central Concentration of Asymmetric Features in Post-starburst Galaxies at
- Empirically-Driven Multiwavelength K-corrections At Low Redshift
- J-PAS: A Neural Network Approach to Single Stellar Population Characterization