Home Page Updated on December 16, 2020
MisV1282
|
| R.A. | 01h57m03s.52 | |
| Decl. | +66o08'11".2 | (2000.0) |
| Mag. | 12.4-13.1C | |
| Type | M | |
| Period | 170 | |
| Epoch | 2451370 |
= USNO-A2.0 1500.01975966 01h57m03s.519 +66o08'10".78 Mag(R):14.9 M
ag(B):19.5
= MSX5C G129.5095+04.1063 01h57m03s.38 +66o08'11".4 InScanError:2.7"
CrossScanError:2.5" Flux(A):0.24692
Digitized Sky Survey GIF image (15 x 15 arcmin)
NSVS Light Curve (NSVS 1817864)
Discovery Information
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and John Greaves, the United Kingdom, discovered a new variable star MisV1282.
It was picked up by Seiichi Yoshida from the candidates of new variable stars detected by the PIXY system 2 from images taken by Nobuo Ohkura. John Greaves researched the NSVS data and confirmed the variation.
http://skydot.lanl.gov/nsvs/star.php?num=1817864&mask=32020
Special Notes
John Greaves researched the NSVS data and found that it is a Mira type variable with a period of 170 days.
Light Curve
Light curve by the Northern Sky Variability Survey (NSVS) created using SkyDOT.
SkyDOT is operated by the University of California for the National Nuclear Security Administration of the US Department of Energy.
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 2001 Sept. 19.67233 | 12.4 | C | Nobuo Ohkura |
| 2001 Sept. 19.67418 | 12.4 | C | Nobuo Ohkura |
| 2001 Sept. 19.67604 | 12.4 | C | Nobuo Ohkura |
| 2001 Sept. 19.67789 | 12.5 | C | Nobuo Ohkura |
| 2001 Sept. 22.69456 | 12.6 | C | Nobuo Ohkura |
| 2001 Sept. 22.69641 | 12.6 | C | Nobuo Ohkura |
| 2001 Nov. 10.56609 | 13.0 | C | Nobuo Ohkura |
| 2001 Nov. 10.56806 | 13.0 | C | Nobuo Ohkura |
| 2001 Nov. 10.57002 | 13.0 | C | Nobuo Ohkura |
| 2001 Nov. 10.57200 | 13.0 | C | Nobuo Ohkura |
| 2001 Nov. 10.57397 | 13.0 | C | Nobuo Ohkura |
| 2001 Nov. 14.56562 | 13.1 | C | Nobuo Ohkura |