464 citations · 2k across the 12 of their papers we have counts for
10 papers · 1 filter
Structure and star formation in galaxies out to z=3: evidence for surface density dependent evolution and upsizing
Marijn Franx, Pieter G. van Dokkum, Natascha M. Foerster Schreiber +3
We present an analysis of galaxies in the CDF-South. We find a tight relation to z=3 between color and size at a given mass, with red galaxies being small, and blue galaxies being…
FIREWORKS U38-to-24 micron photometry of the GOODS-CDFS: multi-wavelength catalog and total IR properties of distant Ks-selected galaxies
Stijn Wuyts, Ivo Labbe, Natascha M. Forster Schreiber +4
We present a Ks-selected catalog, dubbed FIREWORKS, for the Chandra Deep Field South (CDFS) containing photometry in U_38, B_435, B, V, V_606, R, i_775, I, z_850, J, H, Ks, [3.6 um…
A Near-Infrared Spectroscopic Survey of K-selected Galaxies at z~2.3: Redshifts and Implications for Broadband Photometric Studies
Mariska Kriek, Pieter G. van Dokkum, Marijn Franx +10
Using the Gemini Near-InfraRed Spectrograph (GNIRS), we have completed a near-infrared spectroscopic survey for K-bright galaxies at z~2.3, selected from the MUSYC survey. We deriv…
The Evolution of the Field and Cluster Morphology-Density Relation for Mass-Selected Samples of Galaxies
A. van der Wel, B. P. Holden, M. Franx +7
The Sloan Digital Sky Survey (SDSS) and photometric/spectroscopic surveys in the GOODS-South field (the Chandra Deep Field-South, CDFS) are used to construct volume-limited, stella…
The rest-frame optical luminosity functions of galaxies at 2<z<3.5
Danilo Marchesini, Pieter van Dokkum, Ryan Quadri +7
We present the rest-frame optical (B, V, and R band) luminosity functions (LFs) of galaxies at 2<z<3.5, measured from a K-selected sample constructed from the deep NIR MUSYC, the u…
What do we learn from IRAC observations of galaxies at 2 < z < 3.5?
Stijn Wuyts, Ivo Labbe, Marijn Franx +9
We analyze very deep HST, VLT and Spitzer photometry of galaxies at 2<z<3.5 in the Hubble Deep Field South. The sample is selected from the deepest public K-band imaging currently…