Star-forming galaxies at cosmic noon

NM Förster Schreiber, S Wuyts - Annual Review of Astronomy …, 2020 - annualreviews.org
Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

High-redshift star formation in the Atacama large millimetre/submillimetre array era

JA Hodge, E da Cunha - Royal Society Open Science, 2020 - royalsocietypublishing.org
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 …

An atlas of color-selected quiescent galaxies at z> 3 in public JWST fields

F Valentino, G Brammer, KML Gould… - The Astrophysical …, 2023 - iopscience.iop.org
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 …

An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies

U Dudzevičiūtė, I Smail, AM Swinbank… - Monthly Notices of …, 2020 - academic.oup.com
We analyse the physical properties of a large, homogeneously selected sample of ALMA-
located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across …

A dynamically cold disk galaxy in the early Universe

F Rizzo, S Vegetti, D Powell, F Fraternali, JP McKean… - Nature, 2020 - nature.com
The extreme astrophysical processes and conditions that characterize the early Universe
are expected to result in young galaxies that are dynamically different from those observed …

3D-HST+ CANDELS: the evolution of the galaxy size–mass distribution since z= 3

A van der Wel, M Franx, PG Van Dokkum… - The Astrophysical …, 2014 - iopscience.iop.org
Spectroscopic+ photometric redshifts, stellar mass estimates, and rest-frame colors from the
3D-HST survey are combined with structural parameter measurements from CANDELS …

Introducing the Illustris project: the evolution of galaxy populations across cosmic time

S Genel, M Vogelsberger, V Springel… - Monthly Notices of …, 2014 - academic.oup.com
We present an overview of galaxy evolution across cosmic time in the Illustris simulation.
Illustris is an N-body/hydrodynamical simulation that evolves 2× 18203 resolution elements …

ISM Masses and the Star formation Law at Z= 1 to 6: ALMA Observations of Dust Continuum in 145 Galaxies in the COSMOS Survey Field

N Scoville, K Sheth, H Aussel, PV Bout… - The Astrophysical …, 2016 - iopscience.iop.org
ISM MASSES AND THE STAR FORMATION LAW AT Z = 1 TO 6: ALMA OBSERVATIONS
OF DUST CONTINUUM IN 145 GALAXIES IN THE COSMOS SURVEY FIELD - IOPscience …

Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors

F Valentino, M Tanaka, I Davidzon, S Toft… - The Astrophysical …, 2020 - iopscience.iop.org
We report two secure (= z 3.775, 4.012) and one tentative (z≈ 3.767) spectroscopic
confirmations of massive and quiescent galaxies through K-band observations with …

MOSFIRE spectroscopy of quiescent galaxies at 1.5< z< 2.5. II. Star formation histories and galaxy quenching

S Belli, AB Newman, RS Ellis - The Astrophysical Journal, 2019 - iopscience.iop.org
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 …