Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave detectors will offer a unique opportunity for multi-messenger astronomy. Prompt detection alerts for the astronomical community might make it possible to observe the onset of electromagnetic emission from CBC. We demonstrate a computationally practical filtering strategy that could produce early-warning triggers before gravitational radiation from the final merger has arrived at the detectors. © 2012. The American Astronomical Society. All rights reserved.
The question “what is the observable electromagnetic (EM) signature of a compact binary merger? ” is...
International audienceWe describe a stream-based analysis pipeline to detect gravitational waves fro...
We present an improved search for binary compact-object mergers using a network of ground-based grav...
Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave de...
Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave de...
Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave de...
Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave de...
Gravitational-wave observations became commonplace in Advanced LIGO-Virgo's recently concluded third...
International audienceNext-generation gravitational-wave detectors will provide unprecedented sensit...
Binary neutron stars (BNSs) will spend ≅10–15 minutes in the band of Advanced Laser Interferometer G...
International audienceGravitational-wave observations became commonplace in Advanced LIGO-Virgo’s re...
We describe a stream-based analysis pipeline to detect gravitational waves from the merger of binary...
Reviews sources of gravitational radiation that are likely to be detected by gravitational wave dete...
Among the most promising sources of gravitational waves for ground‐based detectors are the signals e...
Binary neutron stars (BNSs) will spend ;10–15 minutes in the band of Advanced Laser Interferometer G...
The question “what is the observable electromagnetic (EM) signature of a compact binary merger? ” is...
International audienceWe describe a stream-based analysis pipeline to detect gravitational waves fro...
We present an improved search for binary compact-object mergers using a network of ground-based grav...
Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave de...
Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave de...
Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave de...
Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave de...
Gravitational-wave observations became commonplace in Advanced LIGO-Virgo's recently concluded third...
International audienceNext-generation gravitational-wave detectors will provide unprecedented sensit...
Binary neutron stars (BNSs) will spend ≅10–15 minutes in the band of Advanced Laser Interferometer G...
International audienceGravitational-wave observations became commonplace in Advanced LIGO-Virgo’s re...
We describe a stream-based analysis pipeline to detect gravitational waves from the merger of binary...
Reviews sources of gravitational radiation that are likely to be detected by gravitational wave dete...
Among the most promising sources of gravitational waves for ground‐based detectors are the signals e...
Binary neutron stars (BNSs) will spend ;10–15 minutes in the band of Advanced Laser Interferometer G...
The question “what is the observable electromagnetic (EM) signature of a compact binary merger? ” is...
International audienceWe describe a stream-based analysis pipeline to detect gravitational waves fro...
We present an improved search for binary compact-object mergers using a network of ground-based grav...