BOKS 45906 was identified as having colors consistent with other CVs in a pre-launch survey of the Kepler spacecraft’s field of view, and was also seen to go through an outburst period, increasing in brightness by a factor of ~25 for five days. Ramsay et al. were looking to study CVs in the Kepler field, so they included it as one of their targets for further monitoring during the Kepler mission. In the end, they were able to use three years of Kepler data, as well as observations from the Isaac Newton Telescope, Swift, and the Hale 200″ Telescope, to learn more.