Home Page Updated on December 16, 2020
MisV0800
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| R.A. | 18h02m23s.18 | |
| Decl. | -29o45'24".6 | (2000.0) |
| Mag. | 13.3-[14.4C | |
| Type | SR: |
= USNO-A2.0_0600.30091491 18 02 23.272 -29 45 21.53 12.6R 15.1B
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.
V1337 Sgr, V4102 Sgr, V4103 Sgr and V4104 Sgr are within 2.3 arcmin from MisV0800. They are short-period variable stars fainter than 16 mag. Therefore, MisV0800 is probably another new variable star.
Light Curve
13.2 +--------------------------------------------------------+
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14.5 +--------------------------------------------------------+
2451269 2451453
1999 Mar. 31 1999 Oct. 1
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Apr. 8.75917 | 13.3 | C | Ken-ichi Kadota |
| 1999 May 20.68331 | 14.1 | C | Ken-ichi Kadota |
| 1999 Sept. 23.43589 | [14.4 | C | Ken-ichi Kadota |