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The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3
A. Durkalec, O. Le Fèvre, S. de la Torre +45
The relation between the galaxy stellar mass M_star and the dark matter halo mass M_h gives important information on the efficiency in forming stars and assembling stellar mass in…
The VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5<z<5.5 and the colour selection of high redshift galaxies
R. Thomas, O. Le Fèvre, V. Le Brun P. Cassata +43
(arXiv abridged abstract) The observed UV rest-frame spectra of distant galaxies are the result of their intrinsic emission combined with absorption along the line of sight produce…
The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
A. Durkalec, O. Le Fèvre, A. Pollo +45
We investigate the evolution of galaxy clustering for galaxies in the redshift range 2.0<<5.0 using the VIMOS Ultra Deep Survey (VUDS). We present the projected (real-space) two…
The evolving SFR-M_star relation and sSFR since z~5 from the VUDS spectroscopic survey
L. A. M. Tasca, O. Le Fevre, N. P. Hathi +44
We study the evolution of the star formation rate (SFR) - stellar mass (M_star) relation and specific star formation rate (sSFR) of star forming galaxies (SFGs) since a redshift z~…
Probing the galaxy-halo connection in UltraVISTA to
H. J. McCracken, M. Wolk, S. Colombi +10
We use percent-level precision photometric redshifts in the UltraVISTA-DR1 near-infrared survey to investigate the changing relationship be- tween galaxy stellar mass and the dark…
The galaxy luminosity function at z ~ 6 and evidence for rapid evolution in the bright end from z ~ 7 to 5
R. A . A. Bowler, J. S. Dunlop, R. J. McLure +8
We present the results of a search for bright (-22.7 < M_UV < -20.5) Lyman-break galaxies at z ~ 6 within a total of 1.65 square degrees of imaging in the UltraVISTA/COSMOS and UKI…