_id,doi,title
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
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?
11531,10.1093/mnras/staa622,Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-α emitters
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
11541,10.1093/mnras/sty2779,"On the nature and physical conditions of the luminous Ly α emitter CR7 and its rest-frame UV components"
11555,10.1093/mnras/sty1088,"Kiloparsec-scale gaseous clumps and star formation at z = 5–7"
11557,10.1093/mnras/sty782,"The nature of luminous Ly α emitters at z ∼ 2–3: Maximal dust-poor starbursts and highly ionizing AGN"
11518,10.3847/1538-4357/aa9931,ALMA reveals metals yet no dust within multiple components in CR7
11575,10.1093/mnras/stw717,The Fundamental Plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
11578,10.1093/mnras/stw322,The CALYMHA survey: Lyα escape fraction and its dependence on galaxy properties at z = 2.23