BZ Cam slightly fainter The VY Scl-type cataclysmic variable, BZ Cam, is reported to have slightly faded. Further observations are encouraged. See Watanabe (2000) VSOLJ Variable Star Bulletin 37, 1, (2001) 38, 1; Kato and Uemura (2001) IBVS 5077; Greiner et al. (2001) A&A 376, 1031; for the 1999-2000 fading and variations during the fading. YYYYMMDD(UT) mag observer 20030209.785 125 (Gary Poyner) 20030213.792 125 (Gary Poyner) 20030217.792 125 (Gary Poyner) 20030218.774 126 (Gary Poyner) 20030222.860 125 (Gary Poyner) 20030225.837 127 (Pavol A. Dubovsky) 20030226.738 132 (Pavol A. Dubovsky) 20030226.840 130 (Pavol A. Dubovsky) 20030226.940 130 (Pavol A. Dubovsky) 20030227.812 129 (Pavol A. Dubovsky) 20030228.978 125 (Gary Poyner) 20030301.947 124 (Gary Poyner) 20030302.851 125 (Gary Poyner) 20030305.832 130 (Pavol A. Dubovsky) 20030306.858 130 (Pavol A. Dubovsky) 20030307.598 127 (Hiroshi Itoh) 20030307.812 129 (Pavol A. Dubovsky) 20030307.957 125 (Gary Poyner) 20030309.964 125 (Gary Poyner) 20030314.887 124 (Gary Poyner) 20030315.885 128 (Gary Poyner) 20030316.894 127 (Gary Poyner) 20030318.881 128 (Gary Poyner) 20030319.885 131 (Gary Poyner) 20030321.894 129 (Gary Poyner)
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