[vsnet-obs 20386] 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 MISAO new variable stars. The
magnitude are estimated automatically by the PIXY system from CCD
images taken by KenIchi Kadota, Ageo City, Japan. 

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

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

MisV0001 990404.77060 141C Mis
MisV0001 990408.76785 140C Mis
MisV0001 990408.76929 139C Mis
MisV0001 990429.68597 162C Mis
MisV0001 990429.68708 161C Mis
MisV0002 990429.49424 133C Mis
MisV0002 990429.50557 133C Mis
MisV0003 990408.76785 125C Mis
MisV0003 990429.68597 130C Mis
MisV0003 990429.68708 128C Mis
MisV0004 990408.76785 132C Mis
MisV0004 990429.68597 138C Mis
MisV0004 990429.68708 139C Mis

MisV0001 has suddenly faded out after its peak on Apr. 8. In Arne's
image (cf. vsnet-chat 1822), MisV0001 is as faint as 17.5 (V mag).
So it should be faded out rapidly between Apr. 8 and 22.

MisV0002, a possible eclipse binary, is in normal phase.

MisV0003 turned to be fading. 

MisV0004 keeps fading out. Now it is faintest since the discovery.

Best regards,

--
Seiichi Yoshida
seiichi@muraoka.info.waseda.ac.jp
http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html

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