Black holes are a result of Einstein's general relativity equations and were initially believed to be purely theoretical.
The advent of the Event Horizon Telescope provided the first direct image of a black hole, confirming their existence.
Reverberation mapping and light echoes allow researchers to study black holes by analyzing the echoes of light bouncing off gas flows around them.
Black holes can be identified by the energy and arrival time of photons emitted by gas flows surrounding them.
Stellar-mass black holes, such as Cygnus X-1, are some of the brightest objects in the universe.