Zoltán Haiman

A post-starburst pathway for the formation of massive galaxies and black holes at z > 6

The Santa Barbara Binary−disk Code Comparison

Eccentric Minidisks in Accreting Binaries

Astrophysics with the Laser Interferometer Space Antenna

Detection of stellar light from quasar host galaxies at redshifts above 6

A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z = 6.61 Quasar

A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of z > 6.5 Quasars Using JWST

Disappearing thermal X-ray emission as a tell-tale signature of merging massive black hole binaries

The effect of mission duration on LISA science objectives

Multiband light curves from eccentric accreting supermassive black hole binaries

How Binaries Accrete: Hydrodynamic Simulations with Passive Tracer Particles

Tidal Disruption on Stellar-mass Black Holes in Active Galactic Nuclei

Unveiling the gravitational universe at μ-Hz frequencies

Equilibrium Eccentricity of Accreting Binaries

High angular resolution gravitational wave astronomy

Evolution of gas disc–embedded intermediate mass ratio inspirals in the<i>LISA</i>band

Titans of the early Universe: The Prato statement on the origin of the first supermassive black holes

Probing gas disc physics with LISA: simulations of an intermediate mass ratio inspiral in an accretion disc

The late inspiral of supermassive black hole binaries with circumbinary gas discs in the LISA band

Testing the Binary Hypothesis: Pulsar Timing Constraints on Supermassive Black Hole Binary Candidates

Self-consistent semi-analytic models of the first stars

On the rate of black hole binary mergers in galactic nuclei due to dynamical hardening

On the orbital evolution of supermassive black hole binaries with circumbinary accretion discs

Rapid formation of massive black holes in close proximity to embryonic protogalaxies

Interactions between multiple supermassive black holes in galactic nuclei: a solution to the final parsec problem

Probing stellar binary black hole formation in galactic nuclei via the imprint of their center of mass acceleration on their gravitational wave signal

Electromagnetic chirp of a compact binary black hole: A phase template for the gravitational wave inspiral

Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers

Validity of the Born approximation for beyond Gaussian weak lensing observables

Beyond <i>J</i> _crit : a critical curve for suppression of H ₂ –cooling in protogalaxies