Home Page Updated on December 16, 2020
MisV1027
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| R.A. | 20h14m25s.10 | |
| Decl. | +47o55'26".0 | (2000.0) |
| Mag. | 10.2-11.6C | |
| Type | SR? |
= GSC3563.2178 20 14 25.59 +47 55 23.0 13.04
= IRAS 20128+4746 R.A.=20 14 25.61 Decl.=+47 55 27.9 (21 x 4", p.a.
=59) flux(12)=3.54 flux(25)=1.39 flux(60)=<1.36 flux(100)=<10.94
20% variable
= 2MASS 201425.004 +475526.21 (2000.0) 6.135 5.077 4.501
Digitized Sky Survey GIF image (15 x 15 arcmin)
NSVS Light Curve (NSVS 5769580)
Discovery Information
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and Ken-ichi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1027.
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.
MisV1027 is a pair of double stars.
The identification with GSC3563.2178 is by Taichi Kato and John Greaves.
The identification with the 2MASS data is by Taichi Kato.
Light Curve
10.1 +--------------------------------------------------------+
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11.7 +--------------------------------------------------------+
2451488 2451844
1999 Nov. 5 2000 Oct. 26
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Nov. 21.42921 | 10.2 | C | Ken-ichi Kadota |
| 1999 Nov. 21.42965 | 10.2 | C | Ken-ichi Kadota |
| 2000 Aug. 15.47177 | 11.5 | C | Nobuo Ohkura |
| 2000 Aug. 15.47362 | 11.6 | C | Nobuo Ohkura |
| 2000 Oct. 10.41706 | 10.5 | C | Nobuo Ohkura |
| 2000 Oct. 10.41892 | 10.6 | C | Nobuo Ohkura |