[vsnet-newvar 900] New variable star MisV1105

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1105).

MisV1105
  R.A.  20h14m38s.61
  Decl. +41o56'14".3  (2000.0)
  Mag.  13.4-14.2C
  Type  SR?
= GSC 3159-01247  20h14m38s.55 +41o56'14".6  Error:0.2"  Mag:13.93  MagError:0.38  Band:1  Class:3  Plate:003S  Flag:F  Epoch:03 SEP 1983
= USNO-A2.0 1275.13699980  20h14m38s.575 +41o56'14".67  Mag(R):14.4  Mag(B):14.6

  http://vsnet.aerith.net/misao/data/MisV/MisV1105.gif

MisV1105 19990803.68972 13.42C Mis KAF-1600 - KenIchi_Kadota
MisV1105 19990803.69016 13.64C Mis KAF-1600 - KenIchi_Kadota
MisV1105 19991121.42156 14.12C Mis KAF-1600 - KenIchi_Kadota
MisV1105 19991121.42201 14.22C Mis KAF-1600 - KenIchi_Kadota
MisV1105 20000907.47131 13.70C Mis KAF-1600 - Nobuo_Ohkura
MisV1105 20000907.47318 13.70C Mis KAF-1600 - Nobuo_Ohkura
MisV1105 20000926.43291 13.67C Mis KAF-1600 - Nobuo_Ohkura
MisV1105 20000926.43476 13.63C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1105.

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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