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LIGO: The Laser Interferometer Gravitational-Wave Observatory
The LIGO Scientific Collaboration, B. Abbott
The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study gravitational waves of astrophysical origin. Direct detection of gravitational wa…
Higher signal harmonics, LISA's angular resolution, and dark energy
K. G. Arun, Bala R. Iyer, B. S. Sathyaprakash +2
It is generally believed that the angular resolution of the Laser Interferometer Space Antenna (LISA) for binary supermassive black holes (SMBH) will not be good enough to identify…
Searching for Gravitational Waves from Binary Inspirals with LIGO
Duncan A. Brown, Stanislav Babak, Patrick R. Brady +9
We describe the current status of the search for gravitational waves from inspiralling compact binary systems in LIGO data. We review the result from the first scientific run of LI…
Higher harmonics increase LISA's mass reach for supermassive black holes
K. G. Arun, Bala R. Iyer, B. S. Sathyaprakash +1
Current expectations on the signal to noise ratios and masses of supermassive black holes which the Laser Interferometer Space Antenna (LISA) can observe are based on using in matc…
Upper limits on gravitational wave emission from 78 radio pulsars
The LIGO Scientific Collaboration, B. Abbott, M. Kramer +1
We present upper limits on the gravitational wave emission from 78 radio pulsars based on data from the third and fourth science runs of the LIGO and GEO600 gravitational wave dete…