The continuous light curve during 1997 April 2–17, spliced from the SAAO 0.75 m, the CTIO 0.9 m, the CBA-Awanui 0.25 m, and the Stubbings 0.32 m telescopes. Easily apparent is a quasi-regular variation of ~1.1 mag amplitude and 23 hr period ; we interpret this as the “normal eruption” cycle of a helium dwarf nova. (Figure 4 from Patterson, J., et al. 2000, PASP, 112, 625.)