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[vsnet-newvar 898] New variable star MisV1103

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1103).

MisV1103
  R.A.  20h02m07s.29
  Decl. +36o19'28".8  (2000.0)
  Mag.  13.1-13.6C
  Type  SR?
= USNO-A2.0 1200.14235773  20h02m07s.721 +36o19'29".90  Mag(R):15.7  Mag(B):17.3

  http://vsnet.aerith.net/misao/data/MisV/MisV1103.gif

MisV1103 19990430.69374 13.16C Mis KAF-1600 - KenIchi_Kadota
MisV1103 19990430.69417 13.06C Mis KAF-1600 - KenIchi_Kadota
MisV1103 19990707.67965 13.33C Mis KAF-1600 - KenIchi_Kadota
MisV1103 19990707.68009 13.44C Mis KAF-1600 - KenIchi_Kadota
MisV1103 19990801.61065 13.46C Mis KAF-1600 - KenIchi_Kadota
MisV1103 19990801.61109 13.57C Mis KAF-1600 - KenIchi_Kadota
MisV1103 19990803.65726 13.54C Mis KAF-1600 - KenIchi_Kadota
MisV1103 19990803.65770 13.44C Mis KAF-1600 - KenIchi_Kadota
MisV1103 19990831.63196 13.54C Mis KAF-1600 - KenIchi_Kadota
MisV1103 19990831.63242 13.52C Mis KAF-1600 - KenIchi_Kadota
MisV1103 20000920.43821 13.12C Mis KAF-1600 - Nobuo_Ohkura
MisV1103 20000920.44007 13.11C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1103.

It was picked up by Seiichi Yoshida from the candidates of new
variable stars detected by the PIXY system 2 from images taken by
Nobuo Ohkura comparing with images taken by KenIchi Kadota, and
confirmed by KenIchi Kadota. 

The identification is researched by Taichi Kato (Kyoto University),
John Greaves (the United Kingdom), and Seiichi Yoshida.

The magnitude are measured automatically by the PIXY system 2.

About the MISAO Project and the PIXY system 2:
  http://vsnet.aerith.net/misao/

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

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