Leiden University Scholarly Publications

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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 MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly emitters at z > 3
The nature of CR7 revealed with MUSE: a young starburst powering extended Ly emission at z = 6.6
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
Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emitters
Nature and physical properties of gas-mass selected galaxies using integral field spectroscopy
A comparison of the stellar, CO, and dust-continuum emission from three star-forming HUDF galaxies at z ~ 2