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During 2006 November an outburst of the dwarf nova AW Sge was observed usingCCD photometry. This revealed 0.25 magnitude superhumps confirming it to be asuperoutburst, possibly only the second confirmed such outburst of this star.The superhumps were observed for 4 days and had a stable period Psh =0.0745(2)d, a value which is consistent with Psh measured during the 2000superoutburst.

Photometry of the dwarf nova AW Sagittae during the 2006 November superoutburst