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COLDz:
COLDz: Deep 34 GHz continuum observations and free-free emission in high-redshift star-forming galaxies
MusE GAs FLOw and wind (MEGAFLOW) VII
Dust, gas, and metal content in star-forming galaxies at z ~ 3.3 revealed with ALMA and near-IR spectroscopy
The infrared-radio correlation of star-forming galaxies is strongly M*-dependent but nearly redshift-invariant since z ~ 4
The ALMA Spectroscopic Survey in the HUDF
MusE GAs FLOw and Wind (MEGAFLOW) VII: a NOEMA pilot program to probe molecular gas in galaxies with measured circumgalactic gas flows
The ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO excitation and atomic carbon in star-forming galaxies at z = 1-3
The ALMA spectroscopic survey large program: the infrared excess of z = 1.5-10 UV-selected galaxies and the implied high-redshift star formation history
The ALMA spectroscopic survey in the Hubble Ultra Deep Field: multiband constraints on line-luminosity functions and the cosmic density of molecular gas
The ALMA spectroscopic survey in the Hubble Ultra Deep Field: constraining the molecular content at log(M*/M) 9.5 with CO stacking of MUSE-detected z >1.5 galaxies
The evolution of the baryons associated with galaxies averaged over cosmic time and space
The ALMA spectroscopic survey in the Hubble Ultra Deep Field: the nature of the faintest dusty star-forming galaxies
The ALMA spectroscopic survey in the HUDF: deep 1.2 mm continuum number counts
COLDz: a high space density of massive dusty starburst galaxies ~1 billion years after the Big Bang
The ALMA spectroscopic survey in the HUDF: the cosmic dust and gas mass densities in galaxies up to z ~ 3
Deceptively cold dust in the massive starburst galaxy GN20 at z ~ 4
The ALMA Spectroscopic Survey in the HUDF: the Molecular Gas Content of Galaxies and Tensions with IllustrisTNG and the Santa Cruz SAM
The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
The ALMA Spectroscopic Survey in the HUDF: CO Luminosity Functions and the Molecular Gas Content of Galaxies through Cosmic History

Pages