Stellar mass estimates in early-type galaxies: procedures, uncertainties and models dependence

Abstract

The aim of the present paper is to quantify the dependence of the estimates of luminosities and stellar mass of early-type galaxies on the different models and model parameters which can be used to analyze the observational data. The paper is organized in two parts. The first one analyzes the dependence of the M/L ratios and of the k-corrections in different bands on model parameters (IMF, metallicity, star formation history, age), assuming some among the most popular spectrophotometric codes usually adopted to study the evolutionary status of galaxies [...]. The second part of our work is dedicated to quantify the reliability and systematics affecting the mass and luminosity estimates obtained by means of the best fitting technique applied to the photometric SEDs of early-type galaxies at $1<z<2$. To this end, we apply the best fitting technique to some mock catalogs built on the basis of a wide set of models of early-type galaxies. We then compare the luminosity and the stellar mass estimated from the SED fitting with the true known input values. The goodness of the mass estimate is found to be dependent on the mass estimator adopted to derive it, but masses cannot anyhow be retrieved better than within a factor 2-3, depending on the quality of the available photometric data and/or on the distance of the galaxies since more distant galaxies are fainter on average and thus affected by larger photometric errors. Finally, we present a new empirical mass estimator based on the K band apparent magnitude and on the observed (V-K) colour. We show that the reliability of the stellar mass content derived with this new estimator for early-type galaxies and its stability are even higher than those achievable with the best classic estimators, with the not negligible advantage that it does not need any multi-wavelength data fitting.

Accepted for publication in MNRAS

References in corpus (42)

• Stellar population synthesis at the resolution of 2003
• Galactic Stellar and Substellar Initial Mass Function
• On the variation of the Initial Mass Function
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• Evolutionary population synthesis: models, analysis of the ingredients and application to high-z galaxies
• The epochs of early-type galaxy formation as a function of environment
• The size distribution of galaxies in the Sloan Digital Sky Survey
• Passively Evolving Early-type Galaxies at 1.4<z<2.5 in the Hubble Ultra Deep Field
• Towards an understanding of the rapid decline of the cosmic star formation rate
• The Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies
• The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5<=IAB<=24, and the redshift distribution over 0< z <=5
• Evolution of asymptotic giant branch stars I. Updated synthetic TP-AGB models and their basic calibration
• Stellar Population Diagnostics of Elliptical Galaxy Formation
• The Recent and Continuing Assembly of Field Ellipticals by Red Mergers
• Evidence for TP-AGB stars in high redshift galaxies, and their effect on deriving stellar population parameters
• The Great Observatories Origins Deep Survey. VLT/FORS2 Spectroscopy in the GOODS-South Field: Part III
• The GOODS-MUSIC sample: a multicolour catalog of near-IR selected galaxies in the GOODS-South field
• GMASS Ultradeep Spectroscopy of Galaxies at 1.4<z<2. II. Superdense passive galaxies: how did they form and evolve ?
• Dry Mergers in GEMS: The Dynamical Evolution of Massive Early-Type Galaxies
• Multiple minor mergers: formation of elliptical galaxies and constraints for the growth of spiral disks
• The Assembly History of Field Spheroidals: Evolution of Mass-to-light Ratios and Signatures of Recent Star Formation
• The K20 survey. VII. The spectroscopic catalogue: spectral properties and evolution of the galaxy population
• A grid of synthetic ionizing spectra for very hot compact stars from NLTE model atmospheres
• The Great Observatories Origins Deep Survey
• Evolved Galaxies at z > 1.5 from the Gemini Deep Deep Survey: The Formation Epoch of Massive Stellar Systems
• Mass-to-Light Ratios of Field Early-Type Galaxies at z~1 from Ultra-Deep Spectroscopy: Evidence for Mass-dependent Evolution
• The Color-Magnitude Relation in CL 1358+62 at z=0.33: Evidence for Significant Evolution in the S0 Population
• The Vimos VLT Deep Survey: Stellar mass segregation and large-scale galaxy environment in the redshift range 0.2<z<1.4
• A critical investigation on the discrepancy between the observational and theoretical Red Giant luminosity function "Bump"
• The evolution of early-type galaxies at z~1 from the K20 survey
• Exploring Cluster Ellipticals as Cosmological Standard Rods
• The population of early-type galaxies at 1<z<2 - New clues on their formation and evolution
• The Fundamental Plane of Field Early Type Galaxies at z=1
• The density of very massive evolved galaxies to z~1.7
• The Munich Near-Infrared Cluster Survey - I. Field selection, object extraction, and photometry
• Galactic Globular Clusters as a test for Very Low-Mass stellar models
• Comparing Dynamical and Photometric Mass Estimates of Low- and High-Redshift Galaxies: Random and Systematic Uncertainties
• Comparing dynamical and photometric-stellar masses of early-type galaxies at z ~ 1
• The effect of diffusion on the Red Giant luminosity function 'bump'
• Dating the stellar population in massive early-type galaxies at $z\sim$1.5
• Massive z ~ 1.3 evolved galaxies revealed
• Kinematic and chemical evolution of early-type galaxies

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