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Population studies of the gamma-ray sources

Authors: Sandro Mereghetti; M. Tavani; A. Pellizzoni; A. W. Chen; S. Vercellone;

Population studies of the gamma-ray sources

Abstract

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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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
1
Average
Average
Average
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