Area of research
Astronomy and Astrophysics · Oceanography
Research interest
Research interests include Pulsars and Gravitational Waves Research, Gamma-ray bursts and supernovae, Astrophysical Phenomena and Observations, and Cosmology and Gravitation Theories.
Compact binary coalescence sensitivity estimates with injection campaigns during the LIGO-Virgo-KAGRA Collaborations’ fourth observing run
Gravity Spy: lessons learned and a path forward
A Population of Short-duration Gamma-Ray Bursts with Dwarf Host Galaxies
POSYDON: A General-purpose Population Synthesis Code with Detailed Binary-evolution Simulations
Observational Evidence for Cosmological Coupling of Black Holes and its Implications for an Astrophysical Source of Dark Energy
Things That Might Go Bump in the Night: Assessing Structure in the Binary Black Hole Mass Spectrum
Data quality up to the third observing run of advanced LIGO: Gravity Spy glitch classifications
A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z ≲ 2
What You Don’t Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses
The Missing Link between Black Holes in High-mass X-Ray Binaries and Gravitational-wave Sources: Observational Selection Effects
Modeling Dense Star Clusters in the Milky Way and beyond with the Cluster Monte Carlo Code
Short GRB Host Galaxies. II. A Legacy Sample of Redshifts, Stellar Population Properties, and Implications for Their Neutron Star Merger Origins
Stochastic gravitational-wave background as a tool for investigating multi-channel astrophysical and primordial black-hole mergers
Suspicious Siblings: The Distribution of Mass and Spin across Component Black Holes in Isolated Binary Evolution
Observational Inference on the Delay Time Distribution of Short Gamma-Ray Bursts
The <i>χ</i><sub>eff</sub> − <i>z</i> correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
Black Hole–Black Hole Total Merger Mass and the Origin of LIGO/Virgo Sources
Avoiding a Cluster Catastrophe: Retention Efficiency and the Binary Black Hole Mass Spectrum
Intermediate-mass Black Holes on the Run from Young Star Clusters
One Channel to Rule Them All? Constraining the Origins of Binary Black Holes Using Multiple Formation Pathways
Archive ouverte UNIGE (University of Geneva) 2021cited by 259position: first
The impact of mass-transfer physics on the observable properties of field binary black hole populations
Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts
The missing link in gravitational-wave astronomy
Classifying the unknown: Discovering novel gravitational-wave detector glitches using similarity learning
Post-Newtonian dynamics in dense star clusters: Formation, masses, and merger rates of highly-eccentric black hole binaries
Gravity Spy: integrating advanced LIGO detector characterization, machine learning, and citizen science