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- 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
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- Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
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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
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- The ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO excitation and atomic carbon in star-forming galaxies at z = 1-3
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- 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
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- The ALMA spectroscopic survey in the Hubble Ultra Deep Field: multiband constraints on line-luminosity functions and the cosmic density of molecular gas
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- 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