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"
10.1093/mnras/stad1977,14104,,"Observational predictions for Thorne–Żytkow objects"
10.1093/mnras/stac2598,13452,,"The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities"
10.1093/mnras/stac2598,14098,,"The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at solar, LMC, and SMC metallicities"
10.1093/mnras/stac801,11521,,"(Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background"
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
10.1093/mnras/staa549,13465,,Sensitivity of the lower edge of the pair-instability black hole mass gap to the treatment of time-dependent convection
10.1093/mnras/staa1347,11528,,MUSEQuBES: Calibrating the redshifts of Lyα emitters using stacked circumgalactic medium absorption profiles
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/staa1269,11530,,"Probing the AGN unification model at redshift z ∼ 3 with MUSE observations of giant Lyα nebulae"
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"
10.1093/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"