The two US-based underground detectors are known as the Laser Interferometer Gravitational-wave Observatory, or LIGO for short.
One is located in Hanford, Washington; the other 1,800 miles (3,000 kilometers) away in Livingston, Louisiana.
Construction began in 1999, and observations were taken from 2001 to 2007.
Then they underwent a major upgrade to make them 10 times more powerful.
The advanced LIGO detectors became fully operational for the first time in September 2015.
More From This Section
In this case of this discovery, made on September 14, 2015, the detector in Louisiana first picked up the signal of a gravitational wave, originating 1.3 billion years ago in the southern sky.
The detector in Washington picked up the same signal 7.1 milliseconds later, allowing scientists to confirm the finding was real and not just a glitch.
The ultra-sophisticated tools work by using huge laser interferometers -- each about 2.5 miles (four kilometers) long -- which are buried beneath the ground to allow the most precise measurements.
The L-shaped instruments track gravitational waves using the physics of laser light and space.
Rather, they sense the vibrations in space, an advantage which allows them to uncover the properties of black holes.
"As a gravitational wave propagates through space it stretches space-time," said David Shoemaker, leader of the Advanced LIGO project at the Massachusetts Institute of Technology (MIT).
The detector, in short, "is just a big device for changing strain in space into an electrical signal."
One way to imagine the curvature of space and time is to imagine a ball falling on a trampoline.
The trampoline bows downward first, stretching the fabric vertically and shortening the sides.
The instrument acts like a transducer, changing that strain into changes in light -- and then into an electronic signal so scientists can digitize it and analyze it.
The LIGO detectors contain two very long arms that contain optical instruments for bending light, and are positioned like the letter L.