Star formation and dust obscuration at z~2: galaxies at the dawn of downsizing

Abstract

We present first results of a study aimed to constrain the star formation rate and dust content of galaxies at z~2. We use a sample of BzK-selected star-forming galaxies, drawn from the COSMOS survey, to perform a stacking analysis of their 1.4 GHz radio continuum as a function of different stellar population properties, after removing AGN contaminants from the sample. Dust unbiased star formation rates are derived from radio fluxes assuming the local radio-IR correlation. The main results of this work are: i) specific star formation rates are constant over about 1 dex in stellar mass and up to the highest stellar mass probed; ii) the dust attenuation is a strong function of galaxy stellar mass with more massive galaxies being more obscured than lower mass objects; iii) a single value of the UV extinction applied to all galaxies would lead to grossly underestimate the SFR in massive galaxies; iv) correcting the observed UV luminosities for dust attenuation based on the Calzetti recipe provide results in very good agreement with the radio derived ones; v) the mean specific star formation rate of our sample steadily decreases by a factor of ~4 with decreasing redshift from z=2.3 to 1.4 and a factor of ~40 down the local Universe. These empirical SFRs would cause galaxies to dramatically overgrow in mass if maintained all the way to low redshifts, we suggest that this does not happen because star formation is progressively quenched, likely starting from the most massive galaxies.

5 pages, 5 figures. Accepted for publication in Astrophysical Journal Letters

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• Extinction in the Large Magellanic Cloud Bar around NGC1854, NGC1856, and NGC1858
• The Shape of the Cosmic X-ray Background: Nuclear Starburst Discs and the Redshift Evolution of AGN Obscuration
• UV slope of z$\sim$3 bright ($L>L^{\ast }$) Lyman-break galaxies in the COSMOS field
• Constraints on the galaxy "main sequence" at z>5: the stellar mass of HDF850.1
• Effect of the environment on star formation activity and stellar mass for star-forming galaxies in the COSMOS field
• Lyman break and UV-selected galaxies at $z\sim 1$ I. Stellar populations from ALHAMBRA survey
• Physical Models for the Clustering of Obscured and Unobscured Quasars
• Morphology and structure of BzK-selected galaxies at z~2 in the CANDELS-COSMOS field
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• What size halos do local LIRGs live in?
• Star formation history of $0.1\le \text{z}\le 1.5$ mass-selected galaxies in the ELAIS-N1 Field
• F-VIPGI: a new adapted version of VIPGI for FORS2 spectroscopy. Application to a sample of 16 X-ray selected galaxy clusters at 0.6 < z < 1.2
• Merging galaxies in isolated environments I. Multiband photometry, classification, stellar masses, and star formation rates
• The MOSDEF Survey: Probing Resolved Stellar Populations at $z\sim 2$ Using a New Bayesian-defined Morphology Metric Called Patchiness
• Detailed study of the Bootes field using 300-500 MHz uGMRT observations: Source Properties and radio--infrared correlations
• SHAPE. I. A SOM-SED hybrid approach for efficient galaxy parameter estimation leveraging JWST
• A phenomenological approach to the evolution of galaxies
• Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
• Physical properties of distant red galaxies in the COSMOS/UltraVISTA field
• The ViSta method for stacking in the Fourier domain and its application to the dusty star-forming galaxies in the ALMA Science Archive
• Radio studies of galaxy formation: Dense Gas History of the Universe