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doi: 10.1063/1.1419479
We present the status of ongoing modelling of the populations of the EGRET point sources. To analyze the two-dimenstional distribution, we wrote Monte Carlo simulations to produce model populations. We compared models containing an isotropic component and one or two galactic components to the EGRET catalog; preliminary results indicate that while one galactic component produces a spatial distribution consistent with the EGRET sources, the resulting flux distributions are inconsistent. Simultaneous comparison of spatial and flux distributions will allow physical models to be constrained.
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