True amplitude of WZ Sge? Looking at the current outburst, I am wondering about the reality of the 7.0 mag maximum documented in the literature. This was the point which I had a discussion with Dr. Nogami, who made a compilation of dwarf nova parameters. The maxima of the past two outbursts of WZ Sge have been around 8.0 or even fainter (averaging "early superhumps"). Could the 7.0 magnitude have been a result of different sensitivity of photographic plates and different comparison stars? Regards, Taichi Kato
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