activity
20072024
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 5.4k across the 51 of their papers we have counts for

collaborators
Showing 2014Show all

19 papers · 1 filter

astro-ph.GA201425 cited

The evolution of the cluster optical galaxy luminosity function between z=0.4 and 0.9 in the DAFT/FADA survey

Nicolas Martinet, Florence Durret, Loic Guennou +8

We compute optical galaxy luminosity functions (GLFs) in the B, V, R, and I rest-frame bands for one of the largest medium-to-high-redshift (0.4 < z < 0.9) cluster samples to date…

astro-ph.CO201432 cited

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…

astro-ph.CO201475 cited

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…

astro-ph.GA201432 cited

The Next Generation Virgo Cluster Survey. XV. The photometric redshift estimation for background sources

A. Raichoor, S. Mei, T. Erben +28

The Next Generation Virgo Cluster Survey is an optical imaging survey covering 104 deg^2 centered on the Virgo cluster. Currently, the complete survey area has been observed in the…

astro-ph.GA2014164 cited

Are Dusty Galaxies Blue? Insights on UV Attenuation from Dust-Selected Galaxies

C. M. Casey, N. Z. Scoville, D. B. Sanders +12

Galaxies' rest-frame ultraviolet (UV) properties are often used to directly infer the degree to which dust obscuration affects the measurement of star formation rates. While much r…

astro-ph.GA20144 cited

Evolution of the specific Star Formation Rate Function at z<1.4 - Dissecting the mass-SFR plane in COSMOS and GOODS

O. Ilbert, S. Arnouts, E. Le Floc'h +21

The relation between the stellar mass and the star formation rate characterizes how the instantaneous star formation is determined by the galaxy past star formation history and by…