> BZ Cam varied from 12.9 to 13.2, far either from the last value > 13.9 observed by T.Watanabe or from the value 14.13+-0.03 expected > from continuation of the linear decline. > Thus we conclude that the star is bright again, with an incline > much faster (<60 days) than the decline from the same magnitude > (~250 days assuming linear decrease). I have some observation data after the date 51551 as follows. UT JD-2400000 Mag. 2000/1/7 15:00 51551.125 13.9 2000/2/4 15:34 51579.149 13.7 2000/2/9 14:47 51584.116 13.5 2000/2/11 15:31 51586.147 13.4 2000/2/16 13:49 51591.076 13.4 2000/2/16 13:50 51591.076 13.4 2000/2/27 10:26 51601.935 13.3 2000/3/2 12:26 51606.018 12.8 2000/3/8 15:26 51612.143 12.6 tonight The brightening is announced in vsnet-alart 4162: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/alert4000/msg00162.html Rrecent data are mentioned in vsnet-recent 54702, too: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/recent54000/msg00702.html The increasing speed is 1.1mag/33days = 30 days/mag (from 13.7 to 12.6, assuming linear increase). Regards, Tsutomu Watanabe (VSOLJ) JCC00212@nifty.ne.jp