The evolution of the star-forming interstellar medium across cosmic time

LJ Tacconi, R Genzel, A Sternberg - Annual Review of …, 2020 - annualreviews.org
Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

[HTML][HTML] From clusters to proto-clusters: the infrared perspective on environmental galaxy evolution

S Alberts, A Noble - Universe, 2022 - mdpi.com
Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

PHIBSS: unified scaling relations of gas depletion time and molecular gas fractions

LJ Tacconi, R Genzel, A Saintonge… - The Astrophysical …, 2018 - iopscience.iop.org
This paper provides an update of our previous scaling relations between galaxy-integrated
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …

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 …

The [C ii] emission as a molecular gas mass tracer in galaxies at low and high redshifts

A Zanella, E Daddi, G Magdis… - Monthly Notices of …, 2018 - academic.oup.com
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 …

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 …

The ALMA spectroscopic survey in the hubble ultra deep field: multiband constraints on line-luminosity functions and the cosmic density of molecular gas

R Decarli, M Aravena, L Boogaard… - The Astrophysical …, 2020 - iopscience.iop.org
We present a CO and atomic fine-structure line-luminosity function analysis using the ALMA
Spectroscopic Survey (ASPECS) in the Hubble Ultra Deep Field. ASPECS consists of two …

ALMA spectroscopic survey in the Hubble Ultra Deep Field: survey description

F Walter, R Decarli, M Aravena, C Carilli… - The Astrophysical …, 2016 - iopscience.iop.org
We present the rationale for and the observational description of ASPECS: the ALMA
SPECtroscopic Survey in the Hubble Ultra-Deep Field (UDF), the cosmological deep field …

COLDz: shape of the CO luminosity function at high redshift and the cold gas history of the universe

DA Riechers, R Pavesi, CE Sharon… - The Astrophysical …, 2019 - iopscience.iop.org
We report the first detailed measurement of the shape of the CO luminosity function at high
redshift, based on> 320 hr of the NSF's Karl G. Jansky Very Large Array (VLA) observations …

The ALMA spectroscopic survey in the HUDF: CO luminosity functions and the molecular gas content of galaxies through cosmic history

R Decarli, F Walter, J Gónzalez-López… - The Astrophysical …, 2019 - iopscience.iop.org
We use the results from the ALMA large program ASPECS, the spectroscopic survey in the
Hubble Ultra Deep Field (HUDF), to constrain CO luminosity functions of galaxies and the …