_id,doi,title
11521,10.1093/mnras/stac801,"(Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background"
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?
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
11529,10.1093/mnras/staa2550,"The nature of CR7 revealed with MUSE: A young starburst powering extended Ly α emission at z = 6.6"
11534,10.1093/mnras/stz3554,Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionized bubble at z = 6.53 
11505,10.1051/0004-6361/201834471,"Faint end of the z ∼ 3–7 luminosity function of Lyman-alpha emitters behind lensing clusters observed with MUSE"
11541,10.1093/mnras/sty2779,"On the nature and physical conditions of the luminous Ly α emitter CR7 and its rest-frame UV components"
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
11518,10.3847/1538-4357/aa9931,ALMA reveals metals yet no dust within multiple components in CR7
11564,10.1093/mnras/stw2973,"The production and escape of Lyman-Continuum radiation from star-forming galaxies at z ∼ 2 and their redshift evolution"
11572,10.1093/mnras/stx2061,"Spectroscopic properties of luminous Ly α emitters at z ≈ 6–7 and comparison to the Lyman-break population"
11574,10.1093/mnras/stw2076,"The Lyα luminosity function at z= 5.7–6.6 and the steep drop of the faint end: Implications for reionization"
11519,10.1088/0004-637X/808/2/139,Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation
11583,10.1093/mnras/stu392,A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys