Line-intensity mapping: theory review with a focus on star-formation lines
Line-intensity mapping (LIM) is an emerging approach to survey the Universe, using
relatively low-aperture instruments to scan large portions of the sky and collect the total …
relatively low-aperture instruments to scan large portions of the sky and collect the total …
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 …
Normal, dust-obscured galaxies in the epoch of reionization
Y Fudamoto, PA Oesch, S Schouws, M Stefanon… - Nature, 2021 - nature.com
Over the past decades, rest-frame ultraviolet (UV) observations have provided large
samples of UV luminous galaxies at redshift (z) greater than 6 (refs.,–), during the so-called …
samples of UV luminous galaxies at redshift (z) greater than 6 (refs.,–), during the so-called …
Reionization era bright emission line survey: selection and characterization of luminous interstellar medium reservoirs in the z> 6.5 Universe
RJ Bouwens, R Smit, S Schouws… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …
Large Program (LP) that is identifying and performing a first characterization of many of the …
A survey of high-z galaxies: serra simulations
We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
The ALMA REBELS Survey: cosmic dust temperature evolution out to z ∼ 7
L Sommovigo, A Ferrara, A Pallottini… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT ALMA observations have revealed the presence of dust in the first generations
of galaxies in the Universe. However, the dust temperature T d remains mostly …
of galaxies in the Universe. However, the dust temperature T d remains mostly …
The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at z ≈ 7
We analyse FIR dust continuum measurements for 14 galaxies (redshift z≈ 7) in the ALMA
Reionization Era Bright Emission Line Survey (REBELS) Large Program to derive their …
Reionization Era Bright Emission Line Survey (REBELS) Large Program to derive their …
Tracing the total molecular gas in galaxies:[CII] and the CO-dark gas
SC Madden, D Cormier, S Hony, V Lebouteiller… - Astronomy & …, 2020 - aanda.org
Context. Molecular gas is a necessary fuel for star formation. The CO (1− 0) transition is
often used to deduce the total molecular hydrogen but is challenging to detect in low …
often used to deduce the total molecular hydrogen but is challenging to detect in low …
The Gas and Stellar Content of a Metal-poor Galaxy at z= 8.496 as Revealed by JWST and ALMA
KE Heintz, C Giménez-Arteaga… - The Astrophysical …, 2023 - iopscience.iop.org
We present a joint analysis of the galaxy S04590 at z= 8.496 based on NIRSpec, NIRCam,
and NIRISS observations obtained as part of the Early Release Observations program of the …
and NIRISS observations obtained as part of the Early Release Observations program of the …
Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XIII. Large-scale feedback and star formation in a low-luminosity quasar at z= 7.07 on the local …
Abstract We present Atacama Large Millimeter/submillimeter Array [C ii] 158 μm line and
underlying far-infrared (FIR) continuum emission observations (0 farcs 70× 0 farcs 56 …
underlying far-infrared (FIR) continuum emission observations (0 farcs 70× 0 farcs 56 …