Abstract
We present the results of a search for long-duration gravitational wave transients in the data of the LIGO Hanford and LIGO Livingston second generation detectors between September 2015 and January 2016, with a total observational time of 49 d. The search targets gravitational wave transients of 10-500 s duration in a frequency band of 24-2048 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. No significant events were observed. As a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also show that the search is sensitive to sources in the Galaxy emitting at least similar to 10-8 M(circle dot)c(2) in gravitational waves.
Original language | English |
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Article number | 065009 |
Number of pages | 25 |
Journal | Classical and Quantum Gravity |
Volume | 35 |
Issue number | 6 |
DOIs | |
Publication status | Published - 22 Mar 2018 |
Externally published | Yes |
Keywords
- LIGO-Virgo
- gravitational waves
- long duration transient
- UPPER LIMITS
- BLACK-HOLE
- SIGNALS
- RADIATION
- NEUTRINO
- MODEL