_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"
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
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?
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
11533,10.1093/mnras/staa093,"The evolution of rest-frame UV properties, Ly α EWs, and the SFR–stellar mass relation at z ∼ 2–6 for SC4K LAEs"
11586,10.1017/s1743921319009451,Unveiling the most luminous Lyman-α emitters in the epoch of reionisation
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
11540,10.1093/mnras/stz030,"The origin of scatter in the star formation rate–stellar mass relation"
11508,10.1051/0004-6361/201833528,Confirmation of double peaked Lyα emission at z = 6.593: Witnessing a galaxy directly contributing to the reionisation of the universe
11555,10.1093/mnras/sty1088,"Kiloparsec-scale gaseous clumps and star formation at z = 5–7"
11558,10.1093/mnras/sty378,"Slicing COSMOS with SC4K: The evolution of typical Ly α emitters and the Ly α escape fraction from z ∼ 2 to 6"
11584,10.1093/mnrasl/sly093,"Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate, and α-enhancement"
11518,10.3847/1538-4357/aa9931,ALMA reveals metals yet no dust within multiple components in CR7
11565,10.1093/mnras/stw2884,"The origin of scatter in the stellar mass–halo mass relation of central galaxies in the EAGLE simulation"
11575,10.1093/mnras/stw717,The Fundamental Plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
11580,10.1093/mnras/stv1076,"CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O III] + Hβ and [O II] luminosity functions at z = 0.8, 1.4 and 2.2 "