The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …

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 …

Using observations from the MOSFIRE Deep Evolution Field survey, we investigate the
physical conditions of star-forming regions in z∼ 2.3 galaxies, specifically the electron …

We present the" SINS/zC-SINF AO survey" of 35 star-forming galaxies, the largest sample
with deep adaptive optics (AO)–assisted near-infrared integral field spectroscopy at z∼ 2 …

We present a census of ionized gas outflows in 599 normal galaxies at redshift 0.6< z< 2.7,
mostly based on integral field spectroscopy of Hα,[N ii], and [S ii] line emission. The sample …

We present results on the z∼ 2.3 mass–metallicity relation (MZR) using early observations
from the MOSFIRE Deep Evolution Field survey. We use an initial sample of 87 star-forming …

We present results on the excitation properties of z∼ 2.3 galaxies using early observations
from the MOSFIRE Deep Evolution Field (MOSDEF) Survey. With its coverage of the full …

In this paper, we follow up on our previous detection of nuclear ionized outflows in the most
massive (log (M*/M☉)⩾ 10.9) z∼ 1–3 star-forming galaxies by increasing the sample size …

We derive 2D dust attenuation maps at∼ 1 kpc resolution from the UV continuum for 10
galaxies on the z∼ 2 star-forming main sequence (SFMS). Comparison with IR data shows …

The nature of dust in distant galaxies is not well understood, and until recently few direct
dust measurements have been possible. We investigate dust in distant star-forming galaxies …