DOI,IST REx ID,Title of publication
10.1093/mnrasl/slad016,17611,Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios
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/mnrasl/slw071,17654,"Formation of massive Population III galaxies through photoionization feedback: A possible explanation for CR 7"
10.1093/mnrasl/slv111,17622,Multiple periods in the variability of the supermassive black hole binary candidate quasar PG1302-102?
10.1093/mnrasl/slu184,17625,Binary black hole accretion during inspiral and merger
10.1093/mnrasl/slu063,17643,A no-go theorem for direct collapse black holes without a strong ultraviolet background
10.1093/mnrasl/slu160,17644,Characteristic signatures in the thermal emission from accreting binary black holes
10.1093/mnrasl/slu075,17682,Lyman edges in supermassive black hole binaries
10.1093/mnrasl/slu136,17692,Stars as resonant absorbers of gravitational waves
10.1093/mnrasl/slt093,17631,Focusing on warm dark matter with lensed high-redshift galaxies
10.1111/j.1745-3933.2012.01298.x,17636,Feedback from the infrared background in the early universe