9 citations · 10 across the 8 of their papers we have counts for
10 papers
Toward a complete understanding of the properties of GW190521
Aasim Jan, Sophia Nicolella, Aaron Zimmerman +4
Interpreting GW190521 remains challenging due to its exceptionally high total mass and correspondingly small number of observable gravitational-wave cycles, which gives rise to deg…
Scaling RIFT 1: Extending RIFT to third-generation gravitational-wave analyses
R. O'Shaughnessy, A. Jan, J. Lange +1
Interpretation of compact binary signals observed by third-generation gravitational-wave detectors is complicated by their high signal-to-noise ratios, often reaching hundreds to t…
Impact of eccentricity and higher-modes on neutron star-black hole parameter estimation
Snehal Tibrewal, Aasim Jan, Aaron Zimmerman +1
Detections of gravitational waves from neutron star-black hole systems provide avenues for studying extreme matter, constraining binary formation channels, and testing the nature o…
Measuring Eccentricity and Addressing Waveform Systematics in GW231123
Aasim Jan, Sophia Nicolella, Deirdre Shoemaker +1
The gravitational-wave event GW231123_135430 is the heaviest binary black hole system observed by the LIGO--Virgo--KAGRA Collaboration to date, with the initial analysis indicating…
GW200105: A detailed study of eccentricity in the neutron star-black hole binary
Aasim Jan, Bing-Jyun Tsao, Richard O'Shaughnessy +2
GW200105_162426 is the first neutron star-black hole merger to be confidently confirmed through either gravitational-wave or electromagnetic observations. Although initially analyz…
Adapting a novel framework for rapid inference of massive black hole binaries for LISA
Aasim Jan, Richard O'Shaughnessy, Deirdre Shoemaker +1
The Laser Interferometer Space Antenna (LISA) is designed to detect a variety of gravitational-wave events, including mergers of massive black hole binaries, stellar-mass black hol…
Waveform systematics in gravitational-wave inference of signals from binary neutron star merger models incorporating higher order modes information
A. B. Yelikar, R. O' Shaughnessy, J. Lange +1
Accurate information from gravitational wave signals from coalescing binary neutron stars provides essential input to downstream interpretations, including inference of the neutron…
Accuracy limitations of existing numerical relativity waveforms on the data analysis of current and future ground-based detectors
Aasim Jan, Deborah Ferguson, Jacob Lange +2
As gravitational wave detectors improve in sensitivity, signal-to-noise ratios of compact binary coalescences will dramatically increase, reaching values in the hundreds and potent…
Mayawaves: Python Library for Interacting with the Einstein Toolkit and the MAYA Catalog
Deborah Ferguson, Surendra Anne, Miguel Gracia-Linares +9
Numerical relativity simulations are crucial for studying black holes and have been instrumental in the detection of gravitational waves by the LVK. However, these simulations prod…
Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
Deborah Ferguson, Evelyn Allsup, Surendra Anne +14
Numerical relativity waveforms are a critical resource in the quest to deepen our understanding of the dynamics of, and gravitational waves emitted from, merging binary systems. We…