_id,doi,title
11488,10.1051/0004-6361/202142302,"The MUSE eXtremely Deep Field: Individual detections of Ly<i>α</i> haloes around rest-frame UV-selected galaxies at <i>z</i> ≃ 2.9–4.4"
11497,10.1051/0004-6361/202141900,Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep
11585,10.1038/s41550-021-01415-y,Differences in galaxy colours are not just about the mass
11504,10.1051/0004-6361/201937339,The MUSE Hubble Ultra Deep field survey: XIII. Spatially resolved spectral properties of Lyman α haloes around star-forming galaxies at z > 3
11499,10.1051/0004-6361/201834565,"Exploring He II λ1640 emission line properties at z ∼2−4"
11507,10.1051/0004-6361/201833075,Predicting Lyα escape fractions with a simple observable: Lyα in emission as an empirically calibrated star formation rate indicator
11518,10.3847/1538-4357/aa9931,ALMA reveals metals yet no dust within multiple components in CR7