Naslov
Star Formation and Dust Obscuration at z ≈ 2 : Galaxies at the Dawn of Downsizing

Autori
Pannella, M. ; Carilli, C. L. ; Daddi, E. ; McCracken, H.J. ; Owen, F. N. ; Renzini, A. ; Strazzullo, V. ; Civano, F. ; Koekemoer, A.M. ; Schinnerer, E. ; Scoville, N. ; Smolčić, Vernesa ; Taniguchi, Y. ; Aussel, H. ; Kneib, J.P. ; Ilbert, O. ; Mellier, Y. ; Salvato, M. ; Thompson, D. ; Willott, C.J.

Izvornik
The Astrophysical journal (0004-637X) 698 (2009), 2; 116-120

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
galaxies: evolution; galaxies: fundamental parameters; galaxies: ISM; galaxies: luminosity function; mass function; galaxies: statistics; surveys

Sažetak
We present first results of a study aimed to constrain the star formation rate (SFR) and dust content of galaxies at z ≈ 2. We use a sample of BzK-selected star-forming galaxies, drawn from the Cosmic Evolution Survey, to perform a stacking analysis of their 1.4 GHz radio continuum as a function of different stellar population properties, after cleaning the sample from contamination by active galactic nuclei. Dust unbiased SFRs are derived from radio fluxes assuming the local radio-IR correlation. The main results of this work are: (1) specific star formation rate (SSFR)s are constant over about 1 dex in stellar mass and up to the highest stellar mass probed, (2) the dust attenuation is a strong function of galaxy stellar mass with more massive galaxies being more obscured than lower mass objects, (3) a single value of the UV extinction applied to all galaxies would lead to a gross underestimate of the SFR in massive galaxies, (4) correcting the observed UV luminosities for dust attenuation based on the Calzetti recipe provides results in very good agreement with the radio derived ones, (5) the mean SSFR 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.

Izvorni jezik
Engleski

Znanstvena područja
Fizika

POVEZANOST RADA