Constraints on Line-of-Sight Acceleration from O1-O4
Labani Roy, Alexander H. Nitz
astro-ph.HE, gr-qc
Submitted: 2026-06-24
Comments: 14 pages including references, 15 figures, data release at URL - https://github.com/labani-01/LOS-acceleration_LIGO-pe
Code: https://github.com/labani-01/LOS-acceleration_LIGO-pe
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Advanced LIGO
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- 4-OGC: Catalog of gravitational waves from compact-binary mergers
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
- GWTC-5.0: An Introduction to Version 5.0 of the Gravitational-Wave Transient Catalog
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- Observation of gravitational waves from two neutron star-black hole coalescences
- GWTC-4.0: Population Properties of Merging Compact Binaries
- Binary black hole mergers: formation and populations
- First constraints on compact binary environments from LIGO-Virgo data
- Dynamics of stellar black holes in young star clusters with different metallicities - II. Black hole-black hole binaries
- Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO
- The Cosmic Evolution of Binary Black Holes in Young, Globular and Nuclear Star Clusters: Rates, Masses, Spins and Mixing Fractions
- Formation channels of single and binary stellar-mass black holes
- Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
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