XTE J1118+480: possible growth of superhumps Dear Colleagues, Thanks to all contributed to the (quasi-)simultaneous spectroscopic and photometic runs of XTE J1118+480, we have able to detect a remarkable change in the light modulation, which now shows steeper rise and slower decline, characterstic to SU UMa-type superhumps. The finding is consistent with that reported by Lew Cook in [vsnet-alert 4733]. The hump amplitude has now grown to 0.07 mag. The best period determined from 5397 observations between Apr. 21 and May 3 is 0.1704(3), which is slightly shorter than the initially determined period (cf. 0.17078(4) d by Uemura et al. 2000). The preliminary O-C analysis also suggests the existence of period shortening. Altough the present uncertainty of the period, mainly due to the short baseline, would make the conclusion still preliminary, the detectable change in periodicity and the variation profile strongly suggest that superhumps in black-hole transients are now indeed developing (eg. Bailyn 1992, ApJ 391, 298; Mineshige et al. 1992, PASJ 44, L15; O'Donoghue and Charles 1996, MNRAS 282, 191 etc.). The result of more detailed analysis, with continuously incoming and updated data, will be presented later by Uemura-san. We strongly encourage all observers to continue observing this target. We are planning to have a collaborative multiwavelength campaign in the coming week, which will be soon announced. Please keep up your excellent works on this remarkable target! We are very looking forward to receiving any data for further analysis [when submitting data to us, please send them to both addresses uemura@kusastro.kyoto-u.ac.jp (optical campaign coordinator) and tkato@kusastro.kyoto-u.ac.jp (on behalf of the VSNET managing team) or directly to vsnet-campaign@kusastro.kyoto-u.ac.jp]. Regards, Makoto Uemura, Taichi Kato, Katsura Matsumoto, Lew Cook, Rudolf Novak, Biran Martin, Arto Oksanen, Marko Moilanen, Yasuo Sano, Denis Buczynski, Gianluca Masi, Alessia Cassetti, Masami Honkawa and Osaka Kyoiku University team, Kesao Takamizawa, Katsumi Haseda, Gunma Astronomical Observatory team on behalf of the VSNET Collaboration team