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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
The MUSE-Faint survey. I. Spectroscopic evidence for a star cluster in Eridanus 2 and constraints on MACHOs as a constituent of dark matter
A comparison of the stellar, CO, and dust-continuum emission from three star-forming HUDF galaxies at z ~ 2
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
The Atacama Large Millimeter/submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field: CO Emission Lines and 3 mm Continuum Sources
Resolved UV and [C II] Structures of Luminous Galaxies within the Epoch of Reionization
The mean Hα EW and Lyman-continuum photon production efficiency for faint z ≈ 4-5 galaxies
The MUSE-Wide Survey: survey description and first data release
Exploring He II lambda 1640 emission line properties at z similar to 2-4
The MUSE-Wide Survey: A determination of the Lyman α emitter luminosity function at 3 < z < 6
The mean H alpha EW and Lyman- continuum photon production efficiency for faint z approximate to 4-5 galaxies
The evolution of the cosmic molecular gas density
The MUSE Hubble Ultra Deep Field Survey. XI. Constraining the low-mass end of the stellar mass - star formation rate relation at z < 1
MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with MUV~-15
The MUSE Hubble Ultra Deep Field Survey. IV. Global properties of C III] emitters
The MUSE Hubble Ultra Deep Field Survey. III. Testing photometric redshifts to 30th magnitude
The MUSE Hubble Ultra Deep Field Survey. VII. Fe II* emission in star-forming galaxies
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