This method uses a network of pulsars that are monitored over a long period of time. Any change in the timing of the pulsars is caused by the passage of gravitational waves through the space between the pulsars and the observation point.
This method uses a network of pulsars that are monitored over a long period of time. Any change in the timing of the pulsars is caused by the passage of gravitational waves through the space between the pulsars and the observation point.