Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

ABSTRACT We present Bayesian Analysis of Galaxies for Physical Inference and Parameter
EStimation, or bagpipes, a new python tool that can be used to rapidly generate complex …

We present reduced data and data products from the 3D-HST survey, a 248-orbit HST
Treasury program. The survey obtained WFC3 G141 grism spectroscopy in four of the five …

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 the KMOS 3D survey, a new integral field survey of over 600 galaxies at 0.7< z<
2.7 using KMOS at the Very Large Telescope. The KMOS 3D survey utilizes synergies with …

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 the wide field slitless spectroscopy mode of the NIRISS instrument on the James
Webb Space Telescope. This mode employs two orthogonal low-resolution (resolving …

We investigate the stellar populations for a sample of 24 quiescent galaxies at 1.5< z< 2.5
using deep rest-frame optical spectra obtained with Keck MOSFIRE. By fitting templates …

Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and
Quiescent Galaxies - IOPscience This site uses cookies. By continuing to use this site you …

We present the first photometric redshift distribution for a large sample of 870 μm
submillimeter galaxies (SMGs) with robust identifications based on observations with ALMA …