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19992009
most citedThe Kormendy relation of massive elliptical galaxies at z~1.5. Evidence for size evolution ?

151 citations · 257 across the 7 of their papers we have counts for

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Showing 2004Show all

8 papers · 1 filter

astro-ph2004

The stellar mass function of galaxies to z ~ 5 in the Fors Deep and GOODS-S fields

N. Drory, M. Salvato, A. Gabasch +4

We present a measurement of the evolution of the stellar mass function (MF) of galaxies and the evolution of the total stellar mass density at 0<z<5. We use deep multicolor data in…

astro-ph2004

Specific Star Formation Rates to Redshift 1.5

A. E. Bauer, N. Drory, G. J. Hill +1

We present a study to determine how star formation contributes to galaxy growth since z=1.5 over five decades in galaxy stellar mass. We investigate the specific star formation rat…

astro-ph2004

The density of very massive evolved galaxies to z~1.7

P. Saracco, M. Longhetti, P. Severgnini +8

We spectroscopically identified 7 massive evolved galaxies with magnitudes 17.8<K<18.4 at 1.3<z<1.7 over an area of ~160 arcmin^2 of the MUNICS survey. Their rest-frame K-band abso…

astro-ph2004

The connection between star formation and stellar mass: Specific star formation rates to redshift one

Georg Feulner, Yuliana Goranova, Niv Drory +2

We investigate the contribution of star formation to the growth of stellar mass in galaxies over the redshift range 0.5 < z < 1.1 by studying the redshift evolution of the specific…

astro-ph2004

Looking for obscured QSOs in the X-ray emitting ERO population

P. Severgnini, R. Della Ceca, V. Braito +8

We present XMM-Newton data centered on one of the MUNICS Near Infrared Cluster Survey fields (S2F1) and we discuss the X-ray properties of the 6 X-ray emitting EROs found. For one…

astro-ph2004

The star formation rate history in the FORS Deep and GOODS South Fields

A. Gabasch, M. Salvato, R. P. Saglia +8

We measure the star formation rate (SFR) as a function of redshift z up to z \~4.5, based on B, I and (I+B) selected galaxy catalogues from the FORS Deep Field (FDF) and the K-sele…