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 …
Dusty star-forming galaxies at high redshift
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 …
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …
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 …
A dusty compact object bridging galaxies and quasars at cosmic dawn
Understanding how super-massive black holes form and grow in the early Universe has
become a major challenge, since it was discovered that luminous quasars existed only 700 …
become a major challenge, since it was discovered that luminous quasars existed only 700 …
Kiloparsec-scale ALMA Imaging of [C II] and Dust Continuum Emission of 27 Quasar Host Galaxies at z∼ 6
BP Venemans, F Walter, M Neeleman… - The Astrophysical …, 2020 - iopscience.iop.org
We present a study of the [C ii] 158 μm line and underlying far-infrared (FIR) continuum
emission of 27 quasar host galaxies at z∼ 6, traced by the Atacama Large Millimeter …
emission of 27 quasar host galaxies at z∼ 6, traced by the Atacama Large Millimeter …
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 …
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …
An ALMA [C II] Survey of 27 Quasars at z> 5.94
R Decarli, F Walter, BP Venemans… - The Astrophysical …, 2018 - iopscience.iop.org
An ALMA [C ii] Survey of 27 Quasars at z > 5.94 - IOPscience Skip to content IOP Science
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home Accessibility Help Search Journals Journals list Browse more than 100 science journal …
Physical Properties of 15 Quasars at z≳ 6.5
C Mazzucchelli, E Bañados… - The Astrophysical …, 2017 - iopscience.iop.org
Physical Properties of 15 Quasars at z ≳ 6.5 - IOPscience This site uses cookies. By continuing
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Galaxies at redshifts 5 to 6 with systematically low dust content and high [C ii] emission
The rest-frame ultraviolet properties of galaxies during the first three billion years of cosmic
time (redshift z> 4) indicate a rapid evolution in the dust obscuration of such galaxies,,. This …
time (redshift z> 4) indicate a rapid evolution in the dust obscuration of such galaxies,,. This …
The [C ii] emission as a molecular gas mass tracer in galaxies at low and high redshifts
We present ALMA Band 9 observations of the [C ii] 158 m emission for a sample of 10 main-
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …