The status of KAGRA underground cryogenic gravitational wave telescope
arXiv:1710.04823 · doi:10.1088/1742-6596/1342/1/012014
Abstract
KAGRA is a 3-km interferometric gravitational wave telescope located in the Kamioka mine in Japan. It is the first km-class gravitational wave telescope constructed underground to reduce seismic noise, and the first km-class telescope to use cryogenic cooling of test masses to reduce thermal noise. The construction of the infrastructure to house the interferometer in the tunnel, and the initial phase operation of the interferometer with a simple 3-km Michelson configuration have been completed. The first cryogenic operation is expected in 2018, and the observing runs with a full interferometer are expected in 2020s. The basic interferometer configuration and the current status of KAGRA are described.
arXiv comment7 pages, 2 figures. Proceedings for XV International Conference on Topics in Astroparticle and Underground Physics (TAUP2017), Sudbury, July 24-28, 2017
References in corpus (6)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Sensitivity Studies for Third-Generation Gravitational Wave Observatories
- Interferometer design of the KAGRA gravitational wave detector
- Detector configuration of KAGRA - the Japanese cryogenic gravitational-wave detector
- Evaluation of heat extraction through sapphire fibers for the GW observatory KAGRA
Cited by in corpus (8)
- Parameter estimation with gravitational waves
- Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky
- Stochastic gravitational wave background: methods and Implications
- Polarization distortions of lensed gravitational waves
- Gravitational wave forms, polarizations, response functions and energy losses of triple systems in Einstein-Aether theory
- Gravitational Wave Astronomy: Delivering on the Promises
- J-GEM optical and near-infrared follow-up of gravitational wave events during LIGO's and Virgo's third observing run
- Status of the Advanced Virgo gravitational-wave detector