[vsnet-newvar 892] New variable star MisV1097

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1097).

MisV1097
  R.A.  01h15m28s.73
  Decl. +41o19'59".3  (2000.0)
  Mag.  12.4-13.2C
  Type  S
= GSC 2808-00139  01h15m28s.75 +41o19'59".1  Error:0.2"  Mag:12.41  MagError:0.40  Band:6  Class:0  Plate:02RY  Flag:F  Epoch:04 AUG 1984
= USNO-A2.0 1275.00747331  01h15m28s.736 +41o19'59".40  Mag(R):12.5  Mag(B):13.1

  http://vsnet.aerith.net/misao/data/MisV/MisV1097.gif

MisV1097 20000906.66479 12.79C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000906.66664 12.86C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000917.65230 13.08C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000917.65415 13.13C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000919.65115 12.38C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000919.65300 12.47C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000920.64627 12.52C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000920.64813 12.62C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000920.64998 12.70C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000924.64858 12.75C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000924.65044 12.73C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000924.65230 12.79C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000926.62969 12.41C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20000926.63154 12.48C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20001010.62218 13.06C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20001010.62403 13.19C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20001011.62285 12.68C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20001011.62472 12.59C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20001011.62657 12.58C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20001030.57082 12.89C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20001106.53748 12.65C Mis KAF-1600 - Nobuo_Ohkura
MisV1097 20001106.53933 12.79C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, MISAO Project, discovered a new variable star
MisV1097.

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, 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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