The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

We investigate how star formation quenching proceeds within central and satellite galaxies
using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a …

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 high-resolution (0 farcs 16) 870 μm Atacama Large Millimeter/submillimeter
Array (ALMA) imaging of 16 luminous (${L} _ {\mathrm {IR}}\sim 4\times {10}^{12}\,{L} …

Dusty star-forming galaxies at high redshift (1< z< 3) represent the most intense star-forming
regions in the universe. Key aspects to these processes are the gas heating and cooling …

The Evolution and Origin of Ionized Gas Velocity Dispersion from z ∼ 2.6 to z ∼ 0.6 with
KMOS3D - IOPscience This site uses cookies. By continuing to use this site you agree to our …

We examine the scalings of galactic outflows with halo mass across a suite of 20 high-
resolution cosmological zoom galaxy simulations covering halo masses in the range …

We present an analysis of star formation and quenching in the SDSS-IV MaNGA-DR15,
utilizing over 5 million spaxels from∼ 3500 local galaxies. We estimate star formation rate …

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 …