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[vsnet-newvar 1549] New variable star MisV1175
- Date: Tue, 3 Sep 2002 23:00:06 -0500
- To: dubois@simbad.u-strasbg.fr, gerard@simbad.u-strasbg.fr, samus@sai.msu.ru, vsnet-newvar@kusastro.kyoto-u.ac.jp
- From: Seiichi Yoshida <comet@aerith.net>
- Subject: [vsnet-newvar 1549] New variable star MisV1175
- Delivered-To: vsnet-newvar@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
Dear colleagues,
# I have sent this mail on Sept. 1, however, it seems to be lost. So I
send this again.
New variable star discovery by the MISAO Project (MisV1175).
MisV1175
R.A. 20h21m02s.24
Decl. +44o17'43".7 (2000.0)
Mag. 13.1-14.1C
Type SR?
= IRAS 20193+4408 20h21m02s.5 +44o17'45" Ellipse:41x7" P.A.:65 Flux(12):0.5720 Flux(25):<0.4590 Flux(60):<4.675 Flux(100):<234.1
= MSX5C G081.3528+04.3415 20h21m02s.09 +44o17'42".7 InScanError:2.7" CrossScanError:2.4" Flux(A):0.82042
= 2MASS 202102.176 +441743.79 (2000.0) 7.761 6.348 5.598
http://vsnet.aerith.net/misao/data/MisV/MisV1175.gif
MisV1175 20000803.52979 13.16C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1175 20000803.53166 13.13C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1175 20000905.46668 13.32C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1175 20000905.46853 13.38C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1175 20011015.39953 13.95C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1175 20011015.40149 14.07C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, MISAO Project, discovered a new variable star
MisV1175.
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/
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp