Cool gas in high-redshift galaxies

CL Carilli, F Walter - Annual Review of Astronomy and …, 2013 - annualreviews.org
Over the past decade, observations of the cool interstellar medium (ISM) in distant galaxies
via molecular and atomic fine structure line (FSL) emission have gone from a curious look …

What drives the growth of black holes?

DM Alexander, RC Hickox - New Astronomy Reviews, 2012 - Elsevier
Massive black holes (BHs) are at once exotic and yet ubiquitous, residing at the centers of
massive galaxies in the local Universe. Recent years have seen remarkable advances in …

The Herschel view of the dominant mode of galaxy growth from z= 4 to the present day

C Schreiber, M Pannella, D Elbaz, M Béthermin… - Astronomy & …, 2015 - aanda.org
We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …

The merger rate of galaxies in the Illustris simulation: a comparison with observations and semi-empirical models

V Rodriguez-Gomez, S Genel… - Monthly Notices of …, 2015 - academic.oup.com
We have constructed merger trees for galaxies in the Illustris simulation by directly tracking
the baryonic content of subhaloes. These merger trees are used to calculate the galaxy …

THE KMOS3D SURVEY: DESIGN, FIRST RESULTS, AND THE EVOLUTION OF GALAXY KINEMATICS FROM 0.7⩽ z⩽ 2.7

E Wisnioski, NMF Schreiber, S Wuyts… - The Astrophysical …, 2015 - iopscience.iop.org
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 …

Galaxy Zoo DECaLS: Detailed visual morphology measurements from volunteers and deep learning for 314 000 galaxies

M Walmsley, C Lintott, T Géron, S Kruk… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT We present Galaxy Zoo DECaLS: detailed visual morphological classifications
for Dark Energy Camera Legacy Survey images of galaxies within the SDSS DR8 footprint …

The two phases of galaxy formation

L Oser, JP Ostriker, T Naab… - The Astrophysical …, 2010 - iopscience.iop.org
Cosmological simulations of galaxy formation appear to show a" two-phase" character with a
rapid early phase at z≳ 2 during which" in situ" stars are formed within the galaxy from …

The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars

V Rodriguez-Gomez, A Pillepich… - Monthly Notices of …, 2016 - academic.oup.com
We use the Illustris simulation to study the relative contributions of in situ star formation and
stellar accretion to the build-up of galaxies over an unprecedentedly wide range of masses …

The JWST Hubble sequence: The rest-frame optical evolution of galaxy structure at 1.5< z< 6.5

L Ferreira, CJ Conselice, E Sazonova… - The Astrophysical …, 2023 - iopscience.iop.org
We present results on the morphological and structural evolution of a total of 3956 galaxies
observed with JWST at 1.5< z< 6.5 in the JWST CEERS observations that overlap with the …

New constraints on the evolution of the stellar-to-dark matter connection: a combined analysis of galaxy–galaxy lensing, clustering, and stellar mass functions from z …

A Leauthaud, J Tinker, K Bundy… - The Astrophysical …, 2011 - iopscience.iop.org
Using data from the COSMOS survey, we perform the first joint analysis of galaxy–galaxy
weak lensing, galaxy spatial clustering, and galaxy number densities. Carefully accounting …