Showing 1–20 of 160 results
/ Date/ Name
Mar 30, 2021Brought to Light II: Revealing the Origins of Cloaked Spiral Features in Cluster Passive Dwarf GalaxiesJul 6, 2022Unexpected dancing partners: Tracing the coherence between the spin and motion of dark matter halosAug 16, 2023BCG alignment with the Locations of Cluster Members and the Large Scale Structure out to 10 R$_{200}$Jul 14, 2015Fast Simulation of Gaussian-Mode Scattering for Precision InterferometryDec 3, 2017The optimal search for an astrophysical gravitational-wave backgroundJan 5, 2024Precision constraints on the neutron star equation of state with third-generation gravitational-wave observatoriesFeb 25, 2011Surviving infant mortality in the hierarchical merging scenarioOct 2, 2012Infant mortality in the hierarchical merging scenario: Dependency on gas expulsion timescalesApr 23, 2022Orbital dynamics and extreme scattering event properties from long-term scintillation observations of PSR J1603-7202May 16, 2013Rapidly evaluating the compact binary likelihood function via interpolationAug 13, 2020A scalable random forest regressor for combining neutron-star equation of state measurements: A case study with GW170817 and GW190425Apr 5, 2019Parallelized Inference for Gravitational-Wave AstronomyNov 7, 2021Measuring the properties of active galactic nuclei disks with gravitational wavesOct 9, 2020Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform modelOct 13, 2016The Preferential Tidal Stripping of Dark Matter versus Stars in GalaxiesNov 12, 2012The impact of galaxy harassment on the globular cluster systems of early-type cluster dwarf galaxiesMar 14, 2019Accelerated detection of the binary neutron star gravitational-wave backgroundMay 10, 2021High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipolesJul 26, 2021A follow-up on intermediate-mass black hole candidates in the second LIGO-Virgo observing run with the Bayes Coherence RatioSep 8, 2015The Sensitivity of Harassment to Orbit: Mass Loss from Early-Type Dwarfs in Galaxy Clusters