V2731 OPH IS AN INTERMEDIATE POLAR WITH A COMPLEX X-RAY SPECTRUM INCLUDING A HOT (KT~100 EV) BLACKBODY COMPONENT ACCORDING TO A PREVIOUS SHORT XMM-NEWTON OBSERVATION INDICATIVE OF A LOCALLY SUPER-EDDINGTON ACCRETION RATE. HOWEVER IT IS POSSIBLE THAT THE TEMPERATURE MEASUREMENT WAS INCORRECT BECAUSE V2731 OPH IS OVERABUNDANT IN NITROGEN WHICH WENT UNNOTICED IN THE PREVIOUS ANALYSIS DUE TO THE LACK OF HIGH S/N RGS SPECTRUM.