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[vsnet-alert 5828] Re: New Haseda variable (HadV82) = WR104



Re: New Haseda variable (HadV82) = WR104

   Katsumi Haseda reports that <12.8p observations merely represent the
GSC limit.  The object was caught at much fainter magnitudes.
Could someone obtain images to extend the sequence?

Regards,
Taichi Kato

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