Home Page Updated on March 15, 2018
MisV0569
|
R.A. | 16h57m00s.70 | |
Decl. | -20o35'37".8 | (2000.0) |
Mag. | 12.2-14.3C |
= USNO-A2.0_0675.17133649 16 57 00.695 -20 35 37.84 15.6R 15.8B
Digitized Sky Survey GIF image (15 x 15 arcmin)
NSVS Light Curve (NSVS 19258236)
NSVS Light Curve (NSVS 16445170)
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.
Taichi Kato pointed out that MisV0569 is about 3 arcmin from WSV79, one of the new variable stars discovered by Wakuda. However, only approximate position is reported for WSV79 and the identification with MisV0569 is uncertain.
12.1 +--------------------------------------------------------+ | * | | * | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | * | | * | 14.4 +--------------------------------------------------------+ 2451278 2451397 1999 Apr. 9 1999 Aug. 6
Date | Mag | Filter | Observer |
---|---|---|---|
1999 Apr. 14.71407 | 12.2 | C | Ken-ichi Kadota |
1999 Apr. 14.71463 | 12.3 | C | Ken-ichi Kadota |
1999 Aug. 1.51620 | 14.3 | C | Ken-ichi Kadota |
1999 Aug. 1.51757 | 14.2 | C | Ken-ichi Kadota |