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JWST/NIRSpec measurements of extremely low metallicities in high equivalent width Lyα emitters
Updated measurements of [O III] 88micron, [C II] 158micron, and dust continuum emission from a z = 7.2 galaxy
Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep
The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly emitters at z > 3
Large population of ALMA galaxies at z > 6 with very high [O III] 88 m to [C II] 158 m flux ratios: evidence of extremely high ionization parameter or PDR deficit?
The MUSE Hubble Ultra Deep Field Survey. XIV. Evolution of the Ly α emitter fraction from z = 3 to z = 6
Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emitters
The MUSE Hubble Ultra Deep Field Survey. XIII. Spatially resolved spectral properties of Lyman haloes around star-forming galaxies at z > 3
Recovering the systemic redshift of galaxies from their Lyman alpha line profile
MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with MUV~-15
The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
The MUSE Hubble Ultra Deep Field Survey. X. Lyα equivalent widths at 2.9 < z < 6.6
The MUSE Hubble Ultra Deep Field Survey. VIII. Extended Lyman-α haloes around high-z star-forming galaxies
MUSE deep-fields: the Ly alpha luminosity function in the Hubble Deep Field-South at 2.91 < z < 6.64
The MUSE Hubble Ultra Deep Field Survey. VI. The faint-end of the Ly alpha luminosity function at 2.91 < z < 6.64 and implications for reionisation
A promoter-level mammalian expression atlas