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The rest-frame optical (900nm) galaxy luminosity function at z~4-7: abundance matching points to limited evolution in the Mstar/Mhalo ratio at z>4
Mauro Stefanon, Rychard J. Bouwens, Ivo Labbé +4
We present the first determination of the galaxy luminosity function (LF) at z~4, 5, 6 and 7 in the rest-frame optical at lambda_rest~900 nm (z' band). The rest-frame optical light…
Evidence for strong evolution in galaxy environmental quenching efficiency between z = 1.6 and z = 0.9
Julie B. Nantais, Adam Muzzin, Remco F. J. van der Burg +7
We analyse the evolution of environmental quenching efficiency, the fraction of quenched cluster galaxies that would be star-forming if they were in the field, as a function of red…
The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z=3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
Nicholas S. Martis, Danilo Marchesini, Gabriel B. Brammer +7
Using the UltraVISTA DR1 and 3D-HST catalogs, we construct a stellar-mass-complete sample, unique for its combination of surveyed volume and depth, to study the evolution of the fr…
Stellar mass function of cluster galaxies at z 1.5: evidence for reduced quenching efficiency at high redshift
Julie B. Nantais, Remco F. J. van der Burg, Chris Lidman +7
We present the stellar mass functions (SMFs) of passive and star-forming galaxies with a limiting mass of 10 M in four spectroscopically confirmed Spitzer Adapta…
Ultra-deep Ks-band Imaging of the Hubble Frontier Fields
Gabriel B. Brammer, Danilo Marchesini, Ivo Labbé +16
We present an overview of the "KIFF" project, which provides ultra-deep Ks-band imaging of all six of the Hubble Frontier Fields clusters Abell 2744, MACS-0416, Abell S1063, Abell…
A spectroscopic follow-up program of very massive galaxies at 3<z<4: confirmation of spectroscopic redshifts, and a high fraction of powerful AGN
Z. Cemile Marsan, Danilo Marchesini, Gabriel B. Brammer +5
We present the analysis and results of a spectroscopic follow-up program of a mass-selected sample of six galaxies at 3 < z < 4 using data from Keck-NIRSPEC and VLT-Xshooter. We co…