Researchers have made enhancements to LIGO's lasers, electronics, and optics and have increased the observatory's sensitivity by 10 to 25 per cent.
The detectors will now be able to tune in to gravitational waves - and the extreme events from which they arise - that emanate from farther out in the universe, scientists said.
On September 14 last year, the Laser Interferometer Gravitational-wave Observatory (LIGO)'s detectors detected gravitational waves for the first time, just two days after it was restarted as Advanced LIGO - an upgraded version of LIGO's two large interferometers, placed 3,000 kilometres apart from each other.
Three months later, on December 26, the detectors picked up another signal, which scientists decoded as a second gravitational wave, rippling out from yet another black hole merger, slightly farther out in the universe, 1.4 billion light years away.
With LIGO's latest upgrades, researchers are hoping to detect more frequent signals of gravitational waves, arising from colliding black holes and other extreme cosmic phenomena.
One of the LIGO's two large interferometers is located in Washington, and the other 3,000 kilometres away in Lousiana.
For the Washington detector the corresponding sensitivity range is pretty much on par with what it was during the first run and is about 15 per cent lower than these figures, said Fritschel.
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