DOI,IST REx ID,Research Group,Title of publication
10.1093/mnras/stad3853,14852,"GradSch,JoMa","Linking UV spectral properties of MUSE Ly α emitters at <i>z</i> ≳ 3 to Lyman continuum escape"
10.1051/0004-6361/202142302,11488,,"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"
10.1051/0004-6361/202142187,11490,,Deciphering stellar metallicities in the early universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
10.1051/0004-6361/202141900,11497,,Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep
10.3847/1538-4357/ac3509,11509,,"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"
10.3847/1538-4357/ac4419,11510,,"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"
10.3847/1538-4357/ac350b,11511,,On the variation in stellar α-enhancements of star-forming galaxies in the EAGLE simulation
10.1093/mnras/stac801,11521,,"(Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background"
10.1051/0004-6361/202140876,11498,,Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at 1.5 < z < 6.4
10.1051/0004-6361/202039887,11500,,The MUSE Extremely Deep Field: The cosmic web in emission at high redshift
10.3847/1538-4357/ac01d7,11512,,"Measuring the average molecular gas content of star-forming galaxies at z = 3–4"
10.1093/mnras/stab2762,11522,,Lyman-α transmission properties of the intergalactic medium in the CoDaII simulation
10.1093/mnras/stab1304,11523,,The X-SHOOTER Lyman α survey at z = 2 (XLS-z2) I: What makes a galaxy a Lyman α emitter?
10.1093/mnras/stab1218,11524,,"The evolution of the UV luminosity and stellar mass functions of Lyman-α emitters from z ∼ 2 to z ∼ 6"
10.1093/mnras/stab796,11525,,Constraining the cosmic UV background at z > 3 with MUSE Lyman-α emission observations
10.1093/mnras/staa3277,11526,,Revealing the impact of quasar luminosity on giant Lyα nebulae
10.1038/s41550-021-01415-y,11585,,Differences in galaxy colours are not just about the mass
10.1051/0004-6361/202038133,11501,,The MUSE Hubble Ultra Deep Field Survey: XV. The mean rest-UV spectra of Lyα emitters at z > 3
10.1051/0004-6361/201937340,11503,,The MUSE Hubble Ultra Deep Field Survey: XIV. Evolution of the Lyα emitter fraction from z = 3 to z = 6
10.1051/0004-6361/201937339,11504,,The MUSE Hubble Ultra Deep field survey: XIII. Spatially resolved spectral properties of Lyman α haloes around star-forming galaxies at z > 3