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The Large Area Telescope onboard Fermi has discovered more than two hundred gamma-ray 
pulsars. But only eight have pulsations detected also at hard X-ray energies. Enlarging the 
X-ray-detected gamma-ray pulsars is essential to understand what are the control parameters behind 
the observed phenomenology. Using a theoretical model we recently developed, we have fitted all known 
spectra of gamma-ray pulsars and obtained estimates for their flux levels in X-rays. Based on the success 
of the model, we could enlarge the sample of non-thermal X-ray detected pulsars.
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