Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios
S. Komossa, D. Grupe, A. Kraus, M.A. Gurwell, Z. Haiman, F.K. Liu, A. Tchekhovskoy, L.C. Gallo, M. Berton, R. Blandford, J.L. Gómez, A.G. Gonzalez, Monthly Notices of the Royal Astronomical Society: Letters 522 (2023) L84–L88.

Formation of massive Population III galaxies through photoionization feedback: A possible explanation for CR 7
E. Visbal, Z. Haiman, G.L. Bryan, Monthly Notices of the Royal Astronomical Society: Letters 460 (2016) L59–L63.

Multiple periods in the variability of the supermassive black hole binary candidate quasar -102?
M. Charisi, I. Bartos, Z. Haiman, A.M. Price-Whelan, S. Márka, Monthly Notices of the Royal Astronomical Society: Letters 454 (2015) L21–L25.

Binary black hole accretion during inspiral and merger
B.D. Farris, P. Duffell, A.I. MacFadyen, Z. Haiman, Monthly Notices of the Royal Astronomical Society: Letters 447 (2014) L80–L84.

A no-go theorem for direct collapse black holes without a strong ultraviolet background
E. Visbal, Z. Haiman, G.L. Bryan, Monthly Notices of the Royal Astronomical Society: Letters 442 (2014) L100–L104.

Characteristic signatures in the thermal emission from accreting binary black holes
B.D. Farris, P. Duffell, A.I. MacFadyen, Z. Haiman, Monthly Notices of the Royal Astronomical Society: Letters 446 (2014) L36–L40.

Lyman edges in supermassive black hole binaries
A. Generozov, Z. Haiman, Monthly Notices of the Royal Astronomical Society: Letters 443 (2014) L64–L68.

Stars as resonant absorbers of gravitational waves
B. McKernan, K.E.S. Ford, B. Kocsis, Z. Haiman, Monthly Notices of the Royal Astronomical Society: Letters 445 (2014) L74–L78.

Focusing on warm dark matter with lensed high-redshift galaxies
F. Pacucci, A. Mesinger, Z. Haiman, Monthly Notices of the Royal Astronomical Society: Letters 435 (2013) L53–L57.

Feedback from the infrared background in the early universe
J. Wolcott-Green, Z. Haiman, Monthly Notices of the Royal Astronomical Society: Letters 425 (2012) L51–L55.