HadV82 = WR104 T. Watanabe-san has provided the following finding chart (with preliminary magnitudes). http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-j/jpg00010.jpg An analysis is Haseda-san's data has yielded a possible period of 388 d, but this requires further confirmation. Phase-folded light curves near the rotation period of 220 d show much scatter. Regards, Taichi Kato