Detailed comparison of LIGO and Virgo Inspiral Pipelines in Preparation for a Joint Search
arXiv:gr-qc/0701027 · doi:10.1088/0264-9381/25/4/045001
Abstract
Presented in this paper is a detailed and direct comparison of the LIGO and Virgo binary neutron star detection pipelines. In order to test the search programs, numerous inspiral signals were added to 24 hours of simulated detector data. The efficiencies of the different pipelines were tested, and found to be comparable. Parameter estimation routines were also tested. We demonstrate that there are definite benefits to be had if LIGO and Virgo conduct a joint coincident analysis; these advantages include increased detection efficiency and the providing of source sky location information.
LIGO-Virgo Working Group. Submitted to Physical Review D
Cited by in corpus (7)
- Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run
- Relativistic Simulations of Black Hole-Neutron Star Mergers: Effects of black-hole spin
- Importance of cooling in triggering the collapse of hypermassive neutron stars
- Degeneracies in Sky Localisation Determination from a Spinning Coalescing Binary through Gravitational Wave Observations: a Markov-Chain Monte-Carlo Analysis for two Detectors
- Head-on collisions of binary white dwarf--neutron stars: Simulations in full general relativity
- Evolution of near-extremal-spin black holes using the moving puncture technique
- A comparison of methods for gravitational wave burst searches from LIGO and Virgo