ASCA - VSNET multiwavelength campaign on XTE J1118+480: optical high-speed photometry > Anyone who will have a simultaneous run on this object will > be welcomed into this campaign. [...] The light curve has shown short-time > fluctuation, so a shorter exposure time (a few second) is better for > photometry, which means photomultiplier tube has advantage. Those who make CCD time-resolved photometry would be advised to use the following comparison star, which lies 5' east to the variable. GSC 3451.1612 11h 18m 40s.73 (J2000.0) +48o 03' 25".7 The star has much advantage in the brightness and the color (V=10.96, B-V=0.52). This star is also a Tycho/Tycho-2 star. For more UBVRI sequence information . see vsnet-chat 2778,2779,2783 http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02778.html http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02779.html http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-chat/msg02783.html and the updated Henden and Bruce sequence: http://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/sumner/j1118.seq Regards, Taichi Kato