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The MUSE-Faint survey
The MUSE-Faint survey
Scaling relations of z ~ 0.25-1.5 galaxies in various environments from the morpho-kinematics analysis of the MAGIC sample
The MUSE eXtremely deep field: first panoramic view of an Mg II emitting intragroup medium
Significant dust-obscured star formation in luminous Lyman-break galaxies at z ~ 7-8
Deciphering stellar metallicities in the early Universe
The MUSE Hubble Ultra Deep Field survey XVI
Cold gas in distant galaxies
MusE GAs FLOw and wind (MEGAFLOW) VII
Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
Exploring He II λ1640 emission line properties at z ~ 2-4 (Corrigendum)
The MUSE-Wide survey
The MUSE Extremely Deep Field
The Tully-Fisher relation in dense groups at z~0.7 in the MAGIC survey
Measuring the average molecular gas content of star-forming galaxies at z = 3-4
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
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