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[vsnet-newvar 887] New variable star MisV1092

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1092).

MisV1092
  R.A.  19h58m21s.55
  Decl. +35o48'20".4  (2000.0)
  Mag.  13.3-13.8C
  Type  SR?
= USNO-A2.0 1200.14005102  19h58m21s.549 +35o48'20".00  Mag(R):16.8  Mag(B):20.2
= 2MASS 195821.532 +354819.81 (2000.0)  8.679  7.444  6.907

  http://vsnet.aerith.net/misao/data/MisV/MisV1092.gif

MisV1092 19990430.69374 13.60C Mis KAF-1600 - KenIchi_Kadota
MisV1092 19990430.69417 13.61C Mis KAF-1600 - KenIchi_Kadota
MisV1092 19990707.67965 13.34C Mis KAF-1600 - KenIchi_Kadota
MisV1092 19990707.68009 13.27C Mis KAF-1600 - KenIchi_Kadota
MisV1092 19990801.61065 13.54C Mis KAF-1600 - KenIchi_Kadota
MisV1092 19990801.61109 13.64C Mis KAF-1600 - KenIchi_Kadota
MisV1092 19990803.65726 13.72C Mis KAF-1600 - KenIchi_Kadota
MisV1092 19990803.65770 13.71C Mis KAF-1600 - KenIchi_Kadota
MisV1092 19990831.63196 13.83C Mis KAF-1600 - KenIchi_Kadota
MisV1092 19990831.63242 13.84C Mis KAF-1600 - KenIchi_Kadota
MisV1092 20000920.43636 13.48C Mis KAF-1600 - Nobuo_Ohkura
MisV1092 20000920.43821 13.41C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1092.

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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