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SDSSp J173008.38+624754.7 superoutburst confirmed
We performed time-series photometry of this object on February 20.
The light curve cleary shows two superhumps with the amplitude of 0.3mag,
which indicates the current bright outburst is a genuine superoutbust.
Our period analysis yields a superhump period of 0.0728(10) d,
slightly shorter than that reported during the last superoutburst
(0.079294(34) d, [vsnet-campaign-dn 1790]), however the baseline
is currently too short, of course.
Regards,
Makoto Uemura
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
