The LIGO interferometers are operating as gravitational wave observatories, with a noise level near an order of magnitude of the goal and the first scientific data recently taken. This data has been analyzed for four different categories of gravitational wave sources; millisecond bursts, inspiralling binary neutron stars, periodic waves from a known pulsar, and stochastic background. Research and development is also underway for the next generation LIGO detector, Advanced LIGO
Construction activities at the LIGO Observatories near Hanford, Washington and Livingston, Louisiana...
The Laser Interferometer Gravitational Wave Observatory (LIGO) has been directly detecting gravitati...
The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km...
The LIGO interferometers are operating as gravitational wave observatories, with a noise level near ...
The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study g...
The LIGO (Laser Interferometer Gravitational-Wave Observatory) project is designed to open a new fie...
For 17 days in August and September 2002, the LIGO and GEO interferometer gravitational wave detecto...
The first generation of ground-based interferometric gravitational wave detectors, LIGO, GEO and Vir...
We report on a search for gravitational-wave bursts in data from the three LIGO interferometric dete...
On April 1st, 2019, the Advanced Laser Interferometer Gravitational-Wave Observatory (aLIGO), joined...
The LIGO Project is a joint effort between the California Institute of Technology and the Massachuse...
The characterization of the Advanced LIGO detectors in the second and third observing runs has incre...
In gravitational-wave detection, special emphasis is put onto searches that focus on cosmic events d...
We present the analysis of between 50 and 100 h of coincident interferometric strain data used to se...
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravi...
Construction activities at the LIGO Observatories near Hanford, Washington and Livingston, Louisiana...
The Laser Interferometer Gravitational Wave Observatory (LIGO) has been directly detecting gravitati...
The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km...
The LIGO interferometers are operating as gravitational wave observatories, with a noise level near ...
The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study g...
The LIGO (Laser Interferometer Gravitational-Wave Observatory) project is designed to open a new fie...
For 17 days in August and September 2002, the LIGO and GEO interferometer gravitational wave detecto...
The first generation of ground-based interferometric gravitational wave detectors, LIGO, GEO and Vir...
We report on a search for gravitational-wave bursts in data from the three LIGO interferometric dete...
On April 1st, 2019, the Advanced Laser Interferometer Gravitational-Wave Observatory (aLIGO), joined...
The LIGO Project is a joint effort between the California Institute of Technology and the Massachuse...
The characterization of the Advanced LIGO detectors in the second and third observing runs has incre...
In gravitational-wave detection, special emphasis is put onto searches that focus on cosmic events d...
We present the analysis of between 50 and 100 h of coincident interferometric strain data used to se...
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravi...
Construction activities at the LIGO Observatories near Hanford, Washington and Livingston, Louisiana...
The Laser Interferometer Gravitational Wave Observatory (LIGO) has been directly detecting gravitati...
The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km...