DOI,IST REx ID,Research Group,Title of publication
10.1051/0004-6361/202557633,22265,JoMa,Euclid Quick Data Release (Q1): XII. Quenching precedes bulge formation in dense environments but follows it in the field
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"
10.1051/0004-6361/202141900,11497,,Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep
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"
10.1051/0004-6361/202038133,11501,,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
10.1093/mnras/staa2550,11529,,"The nature of CR7 revealed with MUSE: A young starburst powering extended Ly α emission at z = 6.6"
10.1093/mnras/staa622,11531,,Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-α emitters
10.1093/mnras/staa093,11533,,"The evolution of rest-frame UV properties, Ly α EWs, and the SFR–stellar mass relation at z ∼ 2–6 for SC4K LAEs"
10.1093/mnras/stz3554,11534,,Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionized bubble at z = 6.53 
10.1093/mnras/staa476,11539,,"The X-ray and radio activity of typical and luminous Ly α emitters from z ∼ 2 to z ∼ 6: Evidence for a diverse, evolving population"
10.1017/s1743921319009451,11586,,Unveiling the most luminous Lyman-α emitters in the epoch of reionisation
10.1051/0004-6361/201834565,11499,,"Exploring He II λ1640 emission line properties at z ∼2−4"
10.1051/0004-6361/201833075,11507,,Predicting Lyα escape fractions with a simple observable: Lyα in emission as an empirically calibrated star formation rate indicator
10.1093/mnras/stz2149,11535,,"The clustering of typical Ly α emitters from z ∼ 2.5–6: Host halo masses depend on Ly α and UV luminosities"
10.1093/mnras/stz030,11540,,"The origin of scatter in the star formation rate–stellar mass relation"
10.1093/mnras/sty2779,11541,,"On the nature and physical conditions of the luminous Ly α emitter CR7 and its rest-frame UV components"
10.1093/mnras/sty925,11549,,"The clustering of H β + [O III] and [O II] emitters since z ∼ 5: Dependencies with line luminosity and stellar mass"
10.1093/mnras/sty1088,11555,,"Kiloparsec-scale gaseous clumps and star formation at z = 5–7"