[vsnet-newvar 575] New variable star MisV1001

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1001).

MisV1001
  R.A.  18h58m50s.39
  Decl. +17o42'09".1  (2000.0)
  Mag.  12.8C-14.0C
  Type  ?
= USNO-A2.0_1050.12446737  18 58 50.389  +17 42 09.09  14.6R  18.8B

  http://vsnet.aerith.net/misao/data/MisV/MisV1001.gif

MisV1001 19990429.70773 134C Mis image="KenIchi Kadota"
MisV1001 19990429.70817 134C Mis image="KenIchi Kadota"
MisV1001 19990429.70912 133C Mis image="KenIchi Kadota"
MisV1001 19990429.70956 134C Mis image="KenIchi Kadota"
MisV1001 19990604.66662 128C Mis image="KenIchi Kadota"
MisV1001 19990604.67439 129C Mis image="KenIchi Kadota"
MisV1001 19990604.67752 128C Mis image="KenIchi Kadota"
MisV1001 19990707.66919 139C Mis image="KenIchi Kadota"
MisV1001 19990707.66968 140C Mis image="KenIchi Kadota"
MisV1001 19990923.46762 139C Mis image="KenIchi Kadota"
MisV1001 19990923.46823 138C Mis image="KenIchi Kadota"
MisV1001 19990923.46889 136C Mis image="KenIchi Kadota"
MisV1001 20000525.64116 139C Mis image="Nobuo Ohkura"
MisV1001 20000525.64300 140C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1001.

It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from images taken by Ohkura comparing with
images taken by Kadota. Kadota and Yoshida judged it as a real
variable star.

The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".

Please see the URL below for the MISAO Project and the PIXY system.

  http://vsnet.aerith.net/misao/

--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/

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