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
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
On April 1st, 2019, the Advanced Laser Interferometer Gravitational-Wave Observatory (aLIGO), joined...
The LIGO interferometers are operating as gravitational wave observatories, with a noise level near ...
For 17 days in August and September 2002, the LIGO and GEO interferometer gravitational wave detecto...
The LIGO (Laser Interferometer Gravitational-Wave Observatory) project is designed to open a new fie...
The first generation of ground-based interferometric gravitational wave detectors, LIGO, GEO and Vir...
The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study g...
The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km...
The characterization of the Advanced LIGO detectors in the second and third observing runs has incre...
The Advanced LIGO detectors have recently completed their second observation run successfully. The r...
I will review the most recent and interesting results from gravitational-wave detection experiments,...
The LIGO Project is a joint effort between the California Institute of Technology and the Massachuse...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
On April 1st, 2019, the Advanced Laser Interferometer Gravitational-Wave Observatory (aLIGO), joined...
The LIGO interferometers are operating as gravitational wave observatories, with a noise level near ...
For 17 days in August and September 2002, the LIGO and GEO interferometer gravitational wave detecto...
The LIGO (Laser Interferometer Gravitational-Wave Observatory) project is designed to open a new fie...
The first generation of ground-based interferometric gravitational wave detectors, LIGO, GEO and Vir...
The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study g...
The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km...
The characterization of the Advanced LIGO detectors in the second and third observing runs has incre...
The Advanced LIGO detectors have recently completed their second observation run successfully. The r...
I will review the most recent and interesting results from gravitational-wave detection experiments,...
The LIGO Project is a joint effort between the California Institute of Technology and the Massachuse...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
On April 1st, 2019, the Advanced Laser Interferometer Gravitational-Wave Observatory (aLIGO), joined...