About J0534+2200
J0534+2200 is an anomaly pulsar. It spins once every 33.392 ms, has a dispersion measure of 56.77 pc cm⁻³ and carries a surface magnetic field around 3.79×10^12 G.
The remains of a supernova that Chinese and Japanese astronomers recorded exploding in 1054 AD, bright enough to be visible in daylight for three weeks.