UV Per, a well-known SU UMa-type dwarf nova, is undergoing an outburst as inidicated by the following observations posted to vsnet-obs. 1996 Mar 13.824 UT, [14.1 (E. Broens, 0.35-m refl., seq: AAVSO); Mar 14.836 UT, 11.9 (E. Broens); Mar 14.882 UT, 12.1 (T. Vanmunster, 0.35-m refl., seq: AAVSO); (from CVC 86, by Tonny Vanmunster) We have made some more information on UV Per available on the VSNET Home Page (http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/, "Whats's new" menu). Corresponding GIF files are also available by ftp (ftp.kusastro.kyoto-u.ac.jp, under /pub/vsnet/DNe/UV_Per). The present Web page of UV Per contains: * The 1989 superoutburst with a prominent "reflare" (VSOLJ data) * Visual observations of superhumps in 1989 (VSOLJ data) * Normal outburst in 1996 March (VSNET data) * The 1992 superoutburst, CCD photometry: presistent superhumps and prominent QPOs during the rapid decline, data taken at Ouda Station * finding charts * photoelectric sequence by Brian Skiff Regards, Taichi Kato