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[vsnet-newvar 853] New variable star MisV1074

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1074).

MisV1074
  R.A.  20h08m31s.32
  Decl. +48o41'50".2  (2000.0)
  Mag.  11.1-11.8C
  Type  SR:
= GSC 03563-00179  20h08m31s.29 +48o41'49".0  Error:0.2"  Mag:13.23  MagError:0.40  Band:1  Class:3  Plate:00TD  Flag:F  Epoch:14 JUN 1983
= USNO-A2.0 1350.11708375  20h08m31s.311 +48o41'49".46  Mag(R):11.4  Mag(B):14.0
= IRAS 20070+4833  20h08m31s.9 +48o41'51"  Ellipse:36x5"  P.A.:62  Flux(12):0.4072  Flux(25):0.2278  Flux(60):<0.7777  Flux(100):<8.016  Var:61%

  http://vsnet.aerith.net/misao/data/MisV/MisV1074.gif

MisV1074 19990803.69709 11.74C Mis KAF-1600 - KenIchi_Kadota
MisV1074 19990803.69754 11.77C Mis KAF-1600 - KenIchi_Kadota
MisV1074 19991121.43031 11.27C Mis KAF-1600 - KenIchi_Kadota
MisV1074 19991121.43073 11.32C Mis KAF-1600 - KenIchi_Kadota
MisV1074 20001011.41382 11.09C Mis KAF-1600 - Nobuo_Ohkura
MisV1074 20001011.41566 11.13C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1074.

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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