CR Boo: superoutburst confirmed
The Kyoto team detected superhumps in the light curve on March
8 and 9. The period was calculated to be 0.01727(1) d, 1.4% longer
than the orbital period. This provides evidence for the superoutburst
nature of the current outburst, and short supercycle of about two
weeks still continues. The object is fading 0.1mag/d.
Regards,
Makoto Uemura

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