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[vsnet-newvar 2082] New variable star MisV1203



Dear colleagues,

New variable star discovery by the MISAO Project (MisV1203).

MisV1203
  R.A.  23h01m49s.83
  Decl. +59o19'02".2  (2000.0)
  Mag.  11.3-12.2C
  Type  SR:
= USNO-A2.0 1425.14473832  23h01m49s.822 +59o19'02".20  Mag(R):14.1  Mag(B):18.3
= IRAS 22597+5902  23h01m50s.0 +59o19'02"  Ellipse:11x4"  P.A.:19  Flux(12):2.822  Flux(25):1.596  Flux(60):<4.976  Flux(100):<66.44  Var:3%
= MSX5C G109.3490-00.6332  23h01m50s.21 +59o19'00".8  InScanError:1.8"  CrossScanError:1.2"  Flux(A):2.9612  Flux(C):3.4869  Flux(D):2.7380  Flux(E):4.1378

  http://vsnet.aerith.net/misao/data/MisV/MisV1203.gif

MisV1203 20000830.59291 12.06C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20000830.59476 12.06C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20000830.59661 12.08C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20000831.56560 12.04C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20000831.56745 12.05C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20000831.56932 11.92C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20001013.51369 11.47C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20001013.51554 11.47C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20001013.51741 11.50C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20001013.51926 11.55C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20010917.57300 11.33C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20010917.57485 11.41C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20010917.57670 11.36C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20010917.57855 11.36C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20011002.53184 11.54C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20011002.53381 11.53C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20011002.53578 11.70C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20011002.53774 11.60C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20011031.47444 11.63C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20011031.47641 11.67C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20011031.47839 11.60C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20011031.48036 11.61C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1203 20011120.42391 12.17C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20011120.42589 12.13C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20011120.42786 12.16C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1203 20011120.42983 12.23C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
Ken-ichi Kadota, MISAO Project, discovered a new variable star
MisV1203.

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 Ken-ichi Kadota. 

The identification is researched by Taichi Kato (Kyoto University),
John Greaves, 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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