LIGO Document P070113-x0
- All three LIGO gravitational wave detectors have reached their design sensitivities. A sky-averaged detection range (SNR > 8) of more than 15 Mpc for gravitational waves emitted from inspiral binary neutron stars with masses of 1.4 M has been achieved with the two 4 km instruments. The fifth LIGO science run started in November 2005 and ended in September 2007. A full year of triple coincidence data has been acquired. The duty cycle of a single instrument was between 66% and 79%. Results from previous science runs are presented.
Rev P070113-B-D:
- Full document number: LIGO-P070113-B-D
- Author(s): Daniel Sigg
- Document date: 2007-12-14
- Document received date: 2007-12-18
- Document entry date: 2007-12-18
Rev P070113-A-D:
- Full document number: LIGO-P070113-A-D
- Author(s): Daniel Sigg
- Document date: 2007-12-14
- Document received date: 2007-12-18
- Document entry date: 2007-12-18
Rev P070113-00-D:
- Full document number: LIGO-P070113-00-D
- Author(s): Daniel Sigg
- Document date: 2007-10-10
- Document received date: 2007-10-12
- Document entry date: 2007-10-12
- Published in Class Quant Grav vol. 25 pg. 114041 (8pp).
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