V2051 Oph superoutburst The data kindly provided by Gordon Garradd (cf. vsnet-obs 22039) indicates the current outburst of V2051 Oph is indeed a superoutburst. The superhump structures up to amplitude 0.4 mag are visibile around eclipse phases 0.5-0.6 in July 29 (so please continues observations outside eclipses!). The single eclipse caught on July 28 is highly asymmetric, indicating the superhump light source was just asymmetrically eclipsed. The present observation thus confirms the SU UMa-type signature of this system, independently discovered by S. Kiyota and L. T. Jensen on the 1998 May outburst occasion. cf. http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/v2051oph.html Regards, Taichi Kato