Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 3(352), p. 1056-1060
DOI: 10.1111/j.1365-2966.2004.08000.x
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We present high-speed photometry of the Sloan Digital Sky Survey cataclysmic variable SDSS J013701.06 - 091234.9 in quiescence and during its 2003 December superoutburst. The orbital modulation at 79.71 +/- 0.01 min is double-humped; the superhump period is 81.702 +/- 0.007 min. Towards the end of the outburst late superhumps with a period of 81.29 +/- 0.01 min were observed. We argue that this is a system of very low mass transfer rate, and that it probably has a long outburst interval.