GSC 09075-02022 , the SIMBAD biblio

We performed time-series observations of a dwarf nova V344 Pav during the outburst on 2004 August. The object showed superhumps, which establish that the object is a new SU UMa-type dwarf nova. We calculate the superhump period to be 0.079607(82) d In conjunction with the reported supercycle of V344 Pav, the relatively long superhump period indicates that it is one of ordinary SU UMa stars.