Summary
OJ 287 hosts a binary system of two supermassive black holes with a twelve‑year orbital period.
The blazar emits relativistic jets directed toward Earth, causing rapid variations across the electromagnetic spectrum.
More than one hundred scientists from 48 institutions across 18 nations contributed data from dozens of ground‑based and space telescopes.
Findings improve understanding of black‑hole dynamics, jet emission mechanisms, and multimessenger astronomy.