[vsnet-obs 19571] MISAO Project observation report

[Seiichi Yoshida <seiichi@muraoka.info.waseda.ac.jp>]

Dear colleagues,

I am Seiichi Yoshida, working on the MISAO Project. Here I report the
magnitude data of variables stars and some other objects. The
magnitude are estimated automatically by the PIXY system from CCD
images taken by KenIchi Kadota, Ageo City, Japan. 

Some of the data are blending magnitude. I put a word "blending" after 
observers code "Mis" for such data.

The magnitude data are also available at the MISAO Project Home Page:

  http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/misao/

The report contains magnitude data of STM objects. They are candidates 
of errors in the GSC compiled by Minoru Sato. The report also contains 
magnitude data of MisE.GSC and MisE.UA1 objects. They are errors in
the GSC/USNO-A1.0, too. The list of these objects are available at the 
MISAO Project Home Page.

Best regards,

--
Seiichi Yoshida
Muraoka Lab., Waseda University, Japan
seiichi@muraoka.info.waseda.ac.jp
http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html

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