Abstract
We have analyzed the COMPTEL/CGRO data using a direct demodulation method. The position of the γ-ray source Crab was accurately found and the Crab and the quasar PKS 0528+134 were completely resolved in the 10–30 MeV range. Our analysis of phase-resolved data of Geminga shows Geminga still has emission in the 10–30 MeV range, and the emission is concentrated in the first peak in the light curve. The results show that application of the direct demodulation method to Compton Telescope data is entirely feasible.
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