2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/129691During 2006 November an outburst of the dwarf nova AW Sge was observed using CCD photometry. This revealed 0.25 magnitude superhumps confirming it to be a superoutburst, 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 2000 superoutburst.10 pages, 9 figures. Accepted for publication in the Journal of the British Astronomical AssociationAstrophysicstext