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The MUSE-Faint survey
The MUSE-Faint survey
MusE GAs FLOw and Wind (MEGAFLOW) IX. The impact of gas flows on the relations between the mass, star formation rate, and metallicity of galaxies
Bipolar outflows out to 10 kpc for massive galaxies at redshift z ≈ 1
Scaling relations of z ~ 0.25-1.5 galaxies in various environments from the morpho-kinematics analysis of the MAGIC sample
Significant dust-obscured star formation in luminous Lyman-break galaxies at z ~ 7-8
MusE GAs FLOw and wind (MEGAFLOW) VII
The Tully-Fisher relation in dense groups at z~0.7 in the MAGIC survey
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
Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra
The ALMA spectroscopic survey in the HUDF: deep 1.2 mm continuum number counts
VLA-ALMA spectroscopic survey in the hubble ultra deep field (VLASPECS): total cold gas masses and CO line ratios for z = 2-3 main-sequence galaxies
The ALMA spectroscopic survey in the HUDF: the cosmic dust and gas mass densities in galaxies up to z ~ 3
The ALMA spectroscopic survey in the HUDF: a model to explain observed 1.1 and 0.85 mm dust continuum number counts

Pages