V367 Cygni / V367 Cyg
Light curve and phase diagram of the EB (EB/GS/SD) type eclipsing binary V367 Cygni / V367 Cyg. Constructed from photometry of 220 images taken with the Bradford Robotic Telescope Cluster Camera between 6 June 2010 and 28 December 2015. Images were unfiltered and results have not been transformed.
The best fit period to this data, 18.598077d compares to 18.59773 d (GCVS and AAVSO VSX) and 18.59778 d (Kreiner). (Accessed 2 October 2017)
The apparent variation in the magnitude range for each year's worth of data is thought to be an artefact of the camera and its annual servicing rather than of the star itself, although this is inconclusive from this data alone.
The apparent variation in the magnitude range for each year's worth of data is thought to be an artefact of the camera and its annual servicing rather than of the star itself, although this is inconclusive from this data alone.
[This page updated 2 October 2017]