_id,doi,title
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"
11539,10.1093/mnras/staa476,"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"
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
11535,10.1093/mnras/stz2149,"The clustering of typical Ly α emitters from z ∼ 2.5–6: Host halo masses depend on Ly α and UV luminosities"
11540,10.1093/mnras/stz030,"The origin of scatter in the star formation rate–stellar mass relation"
11549,10.1093/mnras/sty925,"The clustering of H β + [O III] and [O II] emitters since z ∼ 5: Dependencies with line luminosity and stellar mass"
11584,10.1093/mnrasl/sly093,"Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate, and α-enhancement"
11561,10.1093/mnras/stx1569,"Boötes-HiZELS: An optical to near-infrared survey of emission-line galaxies at z = 0.4–4.7"
11566,10.1093/mnras/stx1712,"A 1.4 deg2 blind survey for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature, morphologies and equivalent widths "