CQ Serpentis / CQ Ser
Light curve and phase diagram of the EB type eclipsing binary CQ Serpentis / CQ Ser.
Constructed from 174 unfiltered images taken with the Cluster Camera of the Bradford Robotic Telescope between 2010 July 12 and 2015 October 29. The results have not been transformed.
CQ Ser is in the same field as my object star W Serpentis and the exposures have not been optimised for CQ Ser.
The best fit period to my data, 0.760061d, compares with the GCVS period of 0.760076d and the AAVSO VSX period of 0.76005957d. [Data correct @ 2015 December 15]
Constructed from 174 unfiltered images taken with the Cluster Camera of the Bradford Robotic Telescope between 2010 July 12 and 2015 October 29. The results have not been transformed.
CQ Ser is in the same field as my object star W Serpentis and the exposures have not been optimised for CQ Ser.
The best fit period to my data, 0.760061d, compares with the GCVS period of 0.760076d and the AAVSO VSX period of 0.76005957d. [Data correct @ 2015 December 15]
[This page updated 2015 December 15]