DH Aql: superhump period The VSNET collaboration team now has ~8400 CCD observations obtained during the current superoutburst of DH Aql. We have performed a preliminary period analysis using these data sets, and calculated a superhump period to be 0.080029 +/- 0.000008 d. Our results furthermore show a gradual decreasing of superhump period during July 29 - August 1. We have the tonight run on DH Aql now. The object is still bright and the superoutburst is still ongoing. CCD time-series observations are encouraged. Regards, Makoto Uemura on behalf of VSNET collaboration team