Home Page Updated on December 16, 2020
MisV0842
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| R.A. | 18h00m06s.06 | |
| Decl. | -29o28'47".8 | (2000.0) |
| Mag. | 11.7-[14.0C |
= USNO-A2.0_0600.29900330 18 00 06.401 -29 28 51.46 12.7R 16.5B = IRAS 17568-2928 R.A.=18 00 05.40 Decl.=-29 28 52.6 (38 x 6", p.a. =92) flux(12)=1.32 flux(25)=<2.09 flux(60)=<7.52 flux(100)=<102. 30
Digitized Sky Survey GIF image (15 x 15 arcmin)
Discovery Information
It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ken-ichi Kadota, Ageo City, Saitama, Japan, then confirmed by Seiichi Yoshida.
V998 Sgr is 2.9 arcmin from MisV0842, that was detected as a 14.1 mag star. MisV0842 is thus a new variable star. MisV0090 is also 1.1 arcmin from MisV0842, which is another variable star.
Light Curve
11.6 +--------------------------------------------------------+
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14.1 +--------------------------------------------------------+
2451437 2451607
1999 Sept. 15 2000 Mar. 3
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Sept. 23.43545 | 11.9 | C | Ken-ichi Kadota |
| 1999 Sept. 23.43589 | 11.7 | C | Ken-ichi Kadota |
| 2000 Feb. 24.83931 | [14.0 | C | Ken-ichi Kadota |
| 2000 Feb. 24.83986 | [14.0 | C | Ken-ichi Kadota |