Home Page Updated on December 16, 2020
MisV0857
|
R.A. | 17h57m59s.52 | |
Decl. | -28o25'42".3 | (2000.0) |
Mag. | 11.9-13.8C | |
Type | SR? |
Digitized Sky Survey GIF image (15 x 15 arcmin)
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.
MisV0858 is 36 arcsec from MisV0857.
11.8 +--------------------------------------------------------+ | * | | * | | * | | | | | | | | | | | | | | | | | | | | | | | | | | * | | * * | | | | | | * | | * | 13.9 +--------------------------------------------------------+ 2451261 2451615 1999 Mar. 23 2000 Mar. 11
Date | Mag | Filter | Observer |
---|---|---|---|
1999 Apr. 8.75742 | 13.4 | C | Ken-ichi Kadota |
1999 Apr. 8.75797 | 13.3 | C | Ken-ichi Kadota |
1999 Apr. 30.74247 | 13.4 | C | Ken-ichi Kadota |
1999 Sept. 23.43274 | 13.7 | C | Ken-ichi Kadota |
1999 Sept. 23.43324 | 13.8 | C | Ken-ichi Kadota |
2000 Feb. 24.83672 | 12.0 | C | Ken-ichi Kadota |
2000 Feb. 24.83728 | 11.9 | C | Ken-ichi Kadota |
2000 Feb. 24.83799 | 12.0 | C | Ken-ichi Kadota |
2000 Feb. 24.83854 | 12.1 | C | Ken-ichi Kadota |