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6 papers · 2 filters
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…
Cluster and field elliptical galaxies at z~1.3. The marginal role of the environment and the relevance of the galaxy central regions
P. Saracco, A. Gargiulo, F. Ciocca +1
We compared the properties of 56 elliptical galaxies selected from three clusters at with those of field galaxies in the GOODS-S (~30), COSMOS (~180) and CANDELS (~220)…
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…
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…
The evolution in the stellar mass of Brightest Cluster Galaxies over the past 10 billion years
Sabine Bellstedt, Chris Lidman, Adam Muzzin +14
Using a sample of 98 galaxy clusters recently imaged in the near infra-red with the ESO NTT, WIYN and WHT telescopes, supplemented with 33 clusters from the ESO archive, we measure…