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[vsnet-newvar 601] New variable star MisV1010

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1010).

MisV1010
  R.A.  21h02m18s.95
  Decl. +38o54'04".6  (2000.0)
  Mag.  11.1C-12.6C
  Type  SR:
= USNO-A2.0_1275.14544959  21 02 18.945  +38 54 04.59  13.3R  15.8B
= IRAS 21003+3841  R.A.=21 02 16.96  Decl.=+38 53 50.8  (29 x 8", p.a.=63)  flux(12)=1.42  flux(25)=0.47  flux(60)=<0.80  flux(100)=<10.45  78% variable
= 2MASS 210218.902 +385403.91 (2000.0)  7.333  6.331  5.707

  http://vsnet.aerith.net/misao/data/MisV/MisV1010.gif

MisV1010 19990501.74888 111C Mis image="KenIchi Kadota"
MisV1010 19990501.74932 111C Mis image="KenIchi Kadota"
MisV1010 19990707.70274 118C Mis image="KenIchi Kadota"
MisV1010 19990707.70319 120C Mis image="KenIchi Kadota"
MisV1010 19990817.73130 126C Mis image="KenIchi Kadota"
MisV1010 20000726.56966 115C Mis image="Nobuo Ohkura"
MisV1010 20000726.57152 115C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1010.

It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from images taken by Ohkura comparing with
images taken by Kadota. Kadota and Yoshida judged it as a real
variable star.

The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".

The identification with the 2MASS data is by Taichi Kato.

Please see the URL below for the MISAO Project and the PIXY system.

  http://vsnet.aerith.net/misao/

--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/

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