NANOGrav recently made headlines by observing the stochastic gravitational waves background produced by the combination of many supermassive black hole binaries. Will a Pulsar Timing Array successfully pinpoint and resolve a specific supermassive black hole binary as a point source of gravitational waves before the year 2030.

This question will be resolved with a "YES" if a Pulsar Timing Arrays colaboration  announces the successful identification of a point source of gravitational waves with a significance  exceeding 3σ by the year 2030. Otherwise, it will be resolved as "NO."