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 …
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …
The SCUBA-2 Cosmology Legacy Survey: 850μm maps, catalogues and number counts
We present a catalogue of∼ 3,000 submillimetre sources detected (≥ 3.5 σ) at 850μm
over∼ 5 deg2 surveyed as part of the James Clerk Maxwell Telescope (JCMT) SCUBA-2 …
over∼ 5 deg2 surveyed as part of the James Clerk Maxwell Telescope (JCMT) SCUBA-2 …
Map** Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies
CM Casey, JA Zavala, SM Manning… - The Astrophysical …, 2021 - iopscience.iop.org
We present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …
The dust content of galaxies from z = 0 to z = 9
G Pop**, RS Somerville… - Monthly Notices of the …, 2017 - academic.oup.com
We study the dust content of galaxies from z= 0 to z= 9 in semi-analytic models of galaxy
formation that include new recipes to track the production and destruction of dust. We …
formation that include new recipes to track the production and destruction of dust. We …
A massive core for a cluster of galaxies at a redshift of 4.3
Massive galaxy clusters have been found that date to times as early as three billion years
after the Big Bang, containing stars that formed at even earlier epochs,–. The high-redshift …
after the Big Bang, containing stars that formed at even earlier epochs,–. The high-redshift …
The brightest galaxies in the dark ages: galaxies' dust continuum emission during the reionization era
CM Casey, JA Zavala, J Spilker… - The Astrophysical …, 2018 - iopscience.iop.org
Though half of cosmic starlight is absorbed by dust and reradiated at long wavelengths (3
μm–3 mm), constraints on the infrared through the millimeter galaxy luminosity function (or …
μm–3 mm), constraints on the infrared through the millimeter galaxy luminosity function (or …
Reproducing submillimetre galaxy number counts with cosmological hydrodynamic simulations
Matching the number counts of high-z submillimetre-selected galaxies (SMGs) has been a
long-standing problem for galaxy formation models. In this paper, we use 3D dust radiative …
long-standing problem for galaxy formation models. In this paper, we use 3D dust radiative …
Characterization of Scuba-2 450 μm and 850 μm selected galaxies in the COSMOS field
We present deep 450 μm and 850 μm observations of a large, uniformly covered 394
arcmin2 area in the Cosmic Evolution Survey (COSMOS) field obtained with the Scuba-2 …
arcmin2 area in the Cosmic Evolution Survey (COSMOS) field obtained with the Scuba-2 …
The ALPINE-ALMA [CII] survey: Data processing, catalogs, and statistical source properties
The Atacama Large Millimeter Array (ALMA) Large Program to INvestigate [CII] at Early
times (ALPINE) targets the [CII] 158 μm line and the far-infrared continuum in 118 …
times (ALPINE) targets the [CII] 158 μm line and the far-infrared continuum in 118 …
An ALMA survey of submillimeter galaxies in the extended Chandra deep field south: near-infrared morphologies and stellar sizes
ABSTRACT We analyze Hubble Space Telescope WFC3/H 160-band observations of a
sample of 48 Atacama Large Millimeter/submillimeter Array detected submillimeter galaxies …
sample of 48 Atacama Large Millimeter/submillimeter Array detected submillimeter galaxies …