DOI,IST REx ID,Title of publication
10.1093/mnras/stx3134,17632,On the rate of black hole binary mergers in galactic nuclei due to dynamical hardening
10.1093/mnras/stx2524,17633,Interactions between multiple supermassive black holes in galactic nuclei: A solution to the final parsec problem
10.1093/mnras/stx167,17668,Beyond Jcrit: A critical curve for suppression of H2-cooling in protogalaxies
10.1093/mnras/stx909,17696,What is the maximum mass of a Population III galaxy?
10.1093/mnras/stx1130,17698,On the orbital evolution of supermassive black hole binaries with circumbinary accretion discs
10.1093/mnras/stw2076,11574,"The Lyα luminosity function at z= 5.7–6.6 and the steep drop of the faint end: Implications for reionization"
10.1093/mnras/stw717,11575,The Fundamental Plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
10.1093/mnras/stw022,11576,"The most luminous H α emitters at z ∼ 0.8–2.23 from HiZELS: Evolution of AGN and star-forming galaxies"
10.1093/mnras/stw322,11578,The CALYMHA survey: Lyα escape fraction and its dependence on galaxy properties at z = 2.23
10.1093/mnras/stw3292,15242,Using galaxy formation simulations to optimize LIGO follow-up observations
10.1093/mnras/stw3210,17621,Lyα emission-line reconstruction for high-z QSOs
10.1093/mnras/stw2260,17656,"Assisted inspirals of stellar mass black holes embedded in AGN discs: Solving the ‘final au problem’"
10.1093/mnras/stw792,17658,A transition in circumbinary accretion discs at a binary mass ratio of 1:25
10.1093/mnras/stw1431,17659,Gravitational wave background from Population III binary black holes consistent with cosmic reionization
10.1093/mnras/stw1838,17672,A population of short-period variable quasars from PTF as supermassive black hole binary candidates
10.1093/mnras/stw1652,17693,Hyper-Eddington mass accretion on to a black hole with super-Eddington luminosity
10.1093/mnras/stw3351,17699,Are we witnessing the epoch of reionization at z=7.1 from the spectrum of J1120+0641?
10.1093/mnras/stw1241,17700,Intermediate-mass black holes from Population III remnants in the first galactic nuclei
10.1093/mnras/stw836,17709,Hyper-Eddington accretion flows on to massive black holes
10.1093/mnras/stv1795,11579,The brightest Lyα emitter: Pop III or black hole?