DOI,IST REx ID,Title of publication
10.1093/mnras/stad686,17551,Cosmological constraints from HSC survey first-year data using deep learning
10.1093/mnras/stad3641,17557,"Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings"
10.1093/mnras/stad1926,17602,Black hole binary formation in AGN discs: from isolation to merger
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/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/stac2740,15206,Testing general relativity using quasi-periodic oscillations from X-ray black holes: XTE J1550-564 and GRO J1655-40
10.1093/mnras/stac1571,15208,Probing magnetar emission mechanisms with X-ray spectropolarimetry
10.1093/mnras/stac1363,15209,Slow convection and fast rotation in crystallization-driven white dwarf dynamos
10.1093/mnras/stac458,15212,The cooling of massive white dwarfs from <i>Gaia</i> EDR3
10.1093/mnras/stac161,17562,Simultaneously constraining cosmology and baryonic physics via deep learning from weak lensing
10.1093/mnras/stac3715,17571,How long do high redshift massive black hole seeds remain outliers in black hole versus host galaxy relations?
10.1093/mnras/stac3664,17580,The X-ray view of optically selected dual AGN
10.1093/mnras/stac3191,17588,Radiative feedback on supermassive star formation: the massive end of the population III initial mass function
10.1093/mnras/stac3592,17599,Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
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