Despite their relative sparseness, during the recent years it has become more and more
clear that extragalactic radio sources (both AGN and star-forming galaxies) constitute an …

We present the results of a systematic search for candidate quiescent galaxies in the distant
universe in 11 JWST fields with publicly available observations collected during the first 3 …

The study of galaxy evolution hinges on our ability to interpret multiwavelength galaxy
observations in terms of their physical properties. To do this, we rely on spectral energy …

We present the ultraviolet luminosity function and an estimate of the cosmic star formation
rate density at 8< z< 13 derived from deep NIRCam observations taken in parallel with the …

We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …

We measure the stellar mass function (SMF) and stellar mass density of galaxies in the
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …

ABSTRACT The 3D-HST and CANDELS programs have provided WFC3 and ACS
spectroscopy and photometry over≈ 900 arcmin 2 in five fields: AEGIS, COSMOS, GOODS …

We present measurements of the stellar mass functions (SMFs) of star-forming and
quiescent galaxies to z= 4 using a sample of 95,675 K s-selected galaxies in the …

In this paper we present the MOSFIRE Deep Evolution Field (MOSDEF) survey. The
MOSDEF survey aims to obtain moderate-resolution (R= 3000-3650) rest-frame optical …

We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …