SDSS J120136.02+300305.5

X-ray fluxes in the galaxy were first detected in June 2010 with a flux 56 times higher than an upper limit from ROSAT, corresponding to L_X ~ 3 × 10⁴⁴ erg s⁻¹.^[3] It had the rough optical spectrum of quiescent galaxy. All in all, the flux evolved in fair consistency with the normal t^−5/3 model, something that would be normal for returning stellar debris, before fading by a factor of roughly 300 after 300 days.^[3] However, the source was incredibly volatile, becoming invisible between 27–48 days after discovery. It may have matched a Bremsstrahlung or double-power-law model and usually softens as time passes.