First joint observation by the underground gravitational-wave detector, KAGRA, with GEO600
arXiv:2203.01270 · doi:10.1093/ptep/ptac073
Abstract
We report the results of the first joint observation of the KAGRA detector with GEO600. KAGRA is a cryogenic and underground gravitational-wave detector consisting of a laser interferometer with three-kilometer arms, and located in Kamioka, Gifu, Japan. GEO600 is a British--German laser interferometer with 600 m arms, and located near Hannover, Germany. GEO600 and KAGRA performed a joint observing run from April 7 to 20, 2020. We present the results of the joint analysis of the GEO--KAGRA data for transient gravitational-wave signals, including the coalescence of neutron-star binaries and generic unmodeled transients. We also perform dedicated searches for binary coalescence signals and generic transients associated with gamma-ray burst events observed during the joint run. No gravitational-wave events were identified. We evaluate the minimum detectable amplitude for various types of transient signals and the spacetime volume for which the network is sensitive to binary neutron-star coalescences. We also place lower limits on the distances to the gamma-ray bursts analysed based on the non-detection of an associated gravitational-wave signal for several signal models, including binary coalescences. These analyses demonstrate the feasibility and utility of KAGRA as a member of the global gravitational-wave detector network.
Matches with published version
References in corpus (26)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
- An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
- Inspiral, merger and ring-down of equal-mass black-hole binaries
- First measurement of the Hubble constant from a dark standard siren using the Dark Energy Survey galaxies and the LIGO/Virgo binary-black-hole merger GW170814
- Black Hole-Neutron Star Mergers: Disk Mass Predictions
- Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
- The Masses and Spins of Neutron Stars and Stellar-Mass Black Holes
- Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run
- GRB afterglow plateaus and Gravitational Waves: multi-messenger signature of a millisecond magnetar?
- Very high efficiency photospheric emission in long duration gamma-ray bursts
- Fragmentation of Collapsar Disks and the Production of Gravitational Waves
- All-sky search for short gravitational-wave bursts in the first Advanced LIGO run
- A bright gamma-ray flare interpreted as a giant magnetar flare in NGC 253
- Precursors in Swift Gamma Ray Bursts with redshift
- All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run
- Rapid Spectral Variability of a Giant Flare from a Magnetar in NGC 253
- GRB Precursors in the Fallback Collapsar Scenario
- Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing run
- Prospects for joint gravitational-wave and electromagnetic observations of neutron-star--black-hole coalescing binaries
- Improved methods for detecting gravitational waves associated with short gamma-ray bursts
- On the origin of short GRBs with Extended Emission and long GRBs without associated SN
- Search for transient gravitational waves in coincidence with short duration radio transients during 2007-2013