Dear colleagues, The CBA campaign on CP Dra is progressing well, with additional contributions coming from CBA East (Dave Skillman) and Nicolas Copernicus Observatory (Rudolf Novak). The complete data set very well shows the transition from initial superhumps at the start of the CP Dra outburst, (amplitude of about 0.22 mag), to full-developed common superhumps with a peak-to-peak amplitude of 0.34 mag. The profile of the superhumps is stable over the entire period, and the same seems to hold for the superhump period, which - using the PDM method - yields a value of 0.08473 +- 0.00006 d. We are now observing the fading part of the outburst. This is a rather interesting phase and we urge observers to continue monitoring the outburst till the object completely fades from visibility. With kind regards, Tonny Vanmunster - CBA Belgium Brian Martin - CBA Alberta David Skillman - CBA East Denis Buczynski - UK Rudolf Novak - Czech Republic