Variabilty of the GSC
1874:399 in Auriga was discovered in 2004by J. Robertson (Arkansas Tech
University)
The following
observation have been performed at the request of J. Robertson.
Coordinates (2000.0)
RA 5h 48m 04s
DE 28o
30'48"
Observation dates
JD 2453 706 (2005-12-01)
JD 2453 716 (2005-12-11)
JD 2453 733 (2005-12-28)
JD 2453 741 (2006-01-05)
JD 2453 742 (2006-01-06)
JD 2453 759 (2006-01-23)
JD 2453 760 (2006-01-24)
Observation instruments
Meade 8"LX200GPS
f/10 telescope
SBIG ST-7xMEI CCD
camera
Unfiltered exposures
Phase diagram
Orbital period
An orbital period of 0.250833d ± 0.000046 (6h 1m 12s ± 4s) has been calculated using ANOVA method of Peranso program (www.peranso.com).
Time of minimum
Based on observation
of 2006 01 24
Used method : Kwee-van
Woerden as implemented in Peranso.
Time heliocentric
correction has been applied on dataset.
JD = 2453760.335794
+/- 0.000219d (+/-19sec)
References:
New Eclipsing Contact Binary System in Auriga,
Austin, S., Robertson, J, Justice, C., Campbell, T., Hoskins, J.,
American Astronomical Society, Vol. 204, pp 510., (2004)
An Eclipsing Near Contact Short Period Binary in the Field of FS Auriga
Robertson, J., Austin, S., Campbell, T., Hoskins, J., International Bulletin of Variable Stars # 5536, (2004)
R.T. McKenzie and
others
http://www.aas.org/publications/baas/v37n2/aas206/292.htm