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[vsnet-history 593] UV Per (Poyner)

Date: Mon, 28 Apr 2003 20:10:40 +0900 (JST)
To: vsnet-history@ooruri.kusastro.kyoto-u.ac.jp
From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
Subject: [vsnet-history 593] UV Per (Poyner)
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Date: Fri, 2 Apr 93 21:46 GMT
From: GP@STARLINK.SPACE-RESEARCH.BIRMINGHAM.AC.UK
Subject: UV Per

Further observation of UV Per....
Apr 02.833UT  13.0 mag
Their is large discrepancies between AAVSO and BAA sequences.  The 
above observation was reduced using BAA sequence.  When using AAVSO,
the magnitude reduces to 12.2
Regards,
Gary Poyner

PS  SN 1993J
Apr 02.843 UT  11.3 mag

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