Since more than 70 years ago, the colours of galaxies derived from flux measurements at
different wavelengths have been used to estimate their cosmological distances. Such …

Fitting the spectral energy distributions (SEDs) of galaxies is an almost universally used
technique that has matured significantly in the last decade. Model predictions and fitting …

We report ultra-deep, medium-resolution spectroscopic observations for four quiescent
galaxies with log at. These data were obtained with JWST NIRSpec as part of the Early …

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 …

We describe the creation, content, and validation of the Dark Energy Survey (DES) internal
year-one cosmology data set, Y1A1 GOLD, in support of upcoming cosmological analyses …

We present redshift distribution estimates of galaxies selected from the fourth data release of
the Kilo-Degree Survey over an area of∼ 1000 deg 2 (KiDS-1000). These redshift …

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 …

Photometric redshifts are a key component of many science objectives in the Hyper Suprime-
Cam Subaru Strategic Program (HSC-SSP). In this paper, we describe and compare the …

We present a combined tomographic weak gravitational lensing analysis of the Kilo Degree
Survey (KV450) and the Dark Energy Survey (DES-Y1). We homogenize the analysis of …

Abstract We present the Canada–France–Hawaii Telescope Lensing Survey (CFHTLenS)
that accurately determines a weak gravitational lensing signal from the full 154 deg2 of deep …