NSV04838 According to CVNET messages, NSV04838 is most likely an SU UMa-type dwarf nova presently in superoutburst. cf. message by Jochen Pietz: The lightcurve data from 2005-06-08/09 shows clear 0.25mag humps. ( http://home.arcor.de/j.pietz/#nsv4838 ) Tonny Vanmunster has reported a period of 0.0697(4) d.