[vsnet-newvar 894] New variable star MisV1099

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1099).

MisV1099
  R.A.  20h03m33s.39
  Decl. +35o55'46".9  (2000.0)
  Mag.  12.5-13.1C
  Type  SR?
= USNO-A2.0 1200.14314510  20h03m33s.291 +35o55'46".87  Mag(R):14.9  Mag(B):18.4
= 2MASS 200333.305 +355546.75 (2000.0)  8.646  7.434  6.973

  http://vsnet.aerith.net/misao/data/MisV/MisV1099.gif

MisV1099 19990430.69374 12.74C Mis KAF-1600 - KenIchi_Kadota
MisV1099 19990430.69417 12.75C Mis KAF-1600 - KenIchi_Kadota
MisV1099 19990801.61065 13.13C Mis KAF-1600 - KenIchi_Kadota
MisV1099 19990801.61109 13.12C Mis KAF-1600 - KenIchi_Kadota
MisV1099 19990803.65726 13.10C Mis KAF-1600 - KenIchi_Kadota
MisV1099 19990803.65770 13.13C Mis KAF-1600 - KenIchi_Kadota
MisV1099 19990831.63196 12.97C Mis KAF-1600 - KenIchi_Kadota
MisV1099 19990831.63242 12.96C Mis KAF-1600 - KenIchi_Kadota
MisV1099 20000920.43821 12.46C Mis KAF-1600 - Nobuo_Ohkura
MisV1099 20000920.44007 12.52C Mis KAF-1600 - Nobuo_Ohkura
MisV1099 20000920.44193 12.58C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1099.

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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