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 …

Dusty star-forming galaxies at high redshift

CM Casey, D Narayanan, A Cooray - Physics Reports, 2014 - Elsevier
Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

The assembly of Milky-Way-like galaxies since z∼ 2.5

PG Van Dokkum, J Leja, EJ Nelson… - The Astrophysical …, 2013 - iopscience.iop.org
Galaxies with the mass of the Milky Way dominate the stellar mass density of the universe
but it is uncertain how and when they were assembled. Here we study progenitors of these …

Star formation relations and CO spectral line energy distributions across the J-ladder and redshift

TR Greve, I Leonidaki, EM Xilouris, A Weiß… - The Astrophysical …, 2014 - iopscience.iop.org
ABSTRACT We present FIR [50–300 μm]− CO luminosity relations (ie, $\log L_ {\rm
FIR}=\alpha\log L^{\prime} _ {\rm CO}+\beta $) for the full CO rotational ladder from J= 1–0 …

MusE GAs FLOw and Wind (MEGAFLOW) VIII. Discovery of a Mgii emission halo probed by a quasar sightline

J Zabl, NF Bouché, L Wisotzki, J Schaye… - Monthly Notices of …, 2021 - academic.oup.com
Using deep () VLT/MUSE data from the MEGAFLOW survey, we report the first detection of
extended emission from a galaxy's halo that is probed by a quasar sightline. The emission …

PHIBSS2: survey design and z= 0.5–0.8 results-Molecular gas reservoirs during the winding-down of star formation

J Freundlich, F Combes, LJ Tacconi, R Genzel… - Astronomy & …, 2019 - aanda.org
Following the success of the Plateau de Bure high-z Blue Sequence Survey (PHIBSS), we
present the PHIBSS2 legacy program, a survey of the molecular gas properties of star …

Giant clumps in simulated high-z Galaxies: properties, evolution and dependence on feedback

N Mandelker, A Dekel, D Ceverino… - Monthly Notices of …, 2017 - academic.oup.com
We study the evolution and properties of giant clumps in high-z disc galaxies using adaptive
mesh refinement cosmological simulations at redshifts z∼ 6–1. Our sample consists of 34 …

The population of giant clumps in simulated high-z galaxies: in situ and ex situ migration and survival

N Mandelker, A Dekel, D Ceverino… - Monthly Notices of …, 2014 - academic.oup.com
We study the properties of giant clumps and their radial gradients in high-z disc galaxies
using AMR cosmological simulations. Our sample consists of 770 snapshots in the redshift …

The ALMA-ALPINE [CII] survey: Kennicutt-Schmidt relation in four massive main-sequence galaxies at z∼ 4.5

M Béthermin, C Accard, C Guillaume… - Astronomy & …, 2023 - aanda.org
Aims. The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR)
surface density (Σ gas− Σ SFR) is essential to understand star formation processes in …

What FIREs up star formation: the emergence of the Kennicutt–Schmidt law from feedback

ME Orr, CC Hayward, PF Hopkins… - Monthly Notices of …, 2018 - academic.oup.com
We present an analysis of the global and spatially resolved Kennicutt–Schmidt (KS) star
formation relation in the FIRE (Feedback In Realistic Environments) suite of cosmological …