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 cosmic baryon and metal cycles
C Péroux, JC Howk - Annual Review of Astronomy and …, 2020 - annualreviews.org
Characterizing the relationship between stars, gas, and metals in galaxies is a critical
component of understanding the cosmic baryon cycle. We compile contemporary censuses …
component of understanding the cosmic baryon cycle. We compile contemporary censuses …
The ALPINE-ALMA [CII] survey-The nature, luminosity function, and star formation history of dusty galaxies up to z≃ 6
C Gruppioni, M Béthermin, F Loiacono… - Astronomy & …, 2020 - aanda.org
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …
The muse hubble ultra deep field survey-i. survey description, data reduction, and source detection
R Bacon, S Conseil, D Mary, J Brinchmann… - Astronomy & …, 2017 - aanda.org
We present the MUSE Hubble Ultra Deep Survey, a mosaic of nine MUSE fields covering
90% of the entire HUDF region with a 10-h deep exposure time, plus a deeper 31-h …
90% of the entire HUDF region with a 10-h deep exposure time, plus a deeper 31-h …
Evolution of interstellar medium, star formation, and accretion at high redshift
N Scoville, N Lee, PV Bout, T Diaz-Santos… - The Astrophysical …, 2017 - iopscience.iop.org
Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift - IOPscience
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This site uses cookies. By continuing to use this site you agree to our use of cookies. To find …
The evolution of the baryons associated with galaxies averaged over cosmic time and space
F Walter, C Carilli, M Neeleman, R Decarli… - The Astrophysical …, 2020 - iopscience.iop.org
We combine the recent determination of the evolution of the cosmic density of molecular gas
(H 2) using deep, volumetric surveys, with previous estimates of the cosmic density of stellar …
(H 2) using deep, volumetric surveys, with previous estimates of the cosmic density of stellar …
Shark: introducing an open source, free, and flexible semi-analytic model of galaxy formation
CP Lagos, RJ Tobar, ASG Robotham… - Monthly Notices of …, 2018 - academic.oup.com
We present a new, open source, free, semi-analytic model (SAM) of galaxy formation, Shark,
designed to be highly flexible and modular, allowing easy exploration of different physical …
designed to be highly flexible and modular, allowing easy exploration of different physical …
Dust, CO, and [C i]: cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time
L Dunne, SJ Maddox, PP Papadopoulos… - Monthly Notices of …, 2022 - academic.oup.com
We present a self-consistent cross-calibration of the three main molecular gas mass tracers
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …
FIREbox: simulating galaxies at high dynamic range in a cosmological volume
R Feldmann, E Quataert… - Monthly Notices of …, 2023 - academic.oup.com
We introduce a suite of cosmological volume simulations to study the evolution of galaxies
as part of the Feedback in Realistic Environments project. FIREbox, the principal simulation …
as part of the Feedback in Realistic Environments project. FIREbox, the principal simulation …
The alma spectroscopic survey in the hubble ultra deep field: co excitation and atomic carbon in star-forming galaxies at z= 1–3
LA Boogaard, P van der Werf, A Weiss… - The Astrophysical …, 2020 - iopscience.iop.org
We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas
mass-selected sample of 22 star-forming galaxies at z= 0.46–3.60, observed as part of the …
mass-selected sample of 22 star-forming galaxies at z= 0.46–3.60, observed as part of the …