Studying the nature of CXOU J204734.8+300105

We propose a 20 ks observation of the source CXOU J204734.8+300105 at the centreof FOV during XMMNewton AO16 cycle. With Chandra observation, this source wasproposed as a Polar having orbital period of virgul6097 sec and showing clear eclipse(Israel et al. 2016). In XMMNewton observation of the Cygnus Loop, for whichthis source is at the edge does not show the same characteristics and instead itshows modulations at shorter period of 237 sec and having lower luminosity. Boththese observations show different results. We would like to have a 20 ksobservation of this source which may give a much more insight to the sourcewhich will help to establish its true nature and able to study its variability.We will perform detailed timing and spectral analysis of this source. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]