_id,doi,title
14852,10.1093/mnras/stad3853,"Linking UV spectral properties of MUSE Ly α emitters at <i>z</i> ≳ 3 to Lyman continuum escape"
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"
11490,10.1051/0004-6361/202142187,Deciphering stellar metallicities in the early universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
11497,10.1051/0004-6361/202141900,Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep
11509,10.3847/1538-4357/ac3509,"EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M∗= 10⁴-10⁵⊙ and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae"
11510,10.3847/1538-4357/ac4419,"The LEGA-C of nature and nurture in stellar populations at z ∼ 0.6–1.0: Dn4000 and Hδ reveal different assembly histories for quiescent galaxies in different environments"
11511,10.3847/1538-4357/ac350b,On the variation in stellar α-enhancements of star-forming galaxies in the EAGLE simulation
11521,10.1093/mnras/stac801,"(Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background"
11498,10.1051/0004-6361/202140876,Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
11500,10.1051/0004-6361/202039887,The MUSE Extremely Deep Field: The cosmic web in emission at high redshift
11512,10.3847/1538-4357/ac01d7,"Measuring the average molecular gas content of star-forming galaxies at z = 3–4"
11522,10.1093/mnras/stab2762,Lyman-α transmission properties of the intergalactic medium in the CoDaII simulation
11523,10.1093/mnras/stab1304,The X-SHOOTER Lyman α survey at z = 2 (XLS-z2) I: What makes a galaxy a Lyman α emitter?
11524,10.1093/mnras/stab1218,"The evolution of the UV luminosity and stellar mass functions of Lyman-α emitters from z ∼ 2 to z ∼ 6"
11525,10.1093/mnras/stab796,Constraining the cosmic UV background at z > 3 with MUSE Lyman-α emission observations
11526,10.1093/mnras/staa3277,Revealing the impact of quasar luminosity on giant Lyα nebulae
11585,10.1038/s41550-021-01415-y,Differences in galaxy colours are not just about the mass
11501,10.1051/0004-6361/202038133,The MUSE Hubble Ultra Deep Field Survey: XV. The mean rest-UV spectra of Lyα emitters at z > 3
11503,10.1051/0004-6361/201937340,The MUSE Hubble Ultra Deep Field Survey: XIV. Evolution of the Lyα emitter fraction from z = 3 to z = 6
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