DOI,IST REx ID,Title of publication
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/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"
10.1051/0004-6361/201834565,11499,"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/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/mnrasl/sly093,11584,"Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate, and α-enhancement"
10.1093/mnras/stx1569,11561,"Boötes-HiZELS: An optical to near-infrared survey of emission-line galaxies at z = 0.4–4.7"
10.1093/mnras/stx1712,11566,"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 "