Enlarging the population of non-thermal X-ray pulsars

Using a theoretical model for the pulsed nonthermal emission above 1 keV andextending until the gammaray domain, we have fitted all known spectra ofgammaray pulsars and obtained estimates for their flux levels in Xrays. Wehave chosen several objects for which their estimate exceeds 3e13 erg/cm2 s at10 keV. Based on the success of the model when contrasted with pulsars for whichXray and gammaray measurements exist, we propose to observe these candidatesto enlarge the sample of nonthermal Xray detected pulsars, which till nowcontains only a handful members. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]