RX J0459.7+1926 revised superhumps period Dear Colleagues, We have updated the superhump light curve of RX J0459.7+1926. New data are from Gordon Garradd and Kyoto team. http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/j0459.html The analysis of the entire observations has yielded an updated superhump period of 0.07060 d, perfectly consistent with the value in vsnet-alert 4149. The Kyoto team (Makoto Uemura and Taichi Kato) is presently observing this star. The sky is ideal. The star is still bright on the monitor and evidently superhumping. Regards, Gianluca Masi, Alessia Cassetti, Patrick Schmeer, Rudolf Novak, Gordon Garradd, Lew Cook, Taichi Kato, Makoto Uemura On behalf of the VSNET RX J0459.7+1926 team