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arXiv · astro-ph/9910301

The Implications of Galaxy Formation Models for the TeV Observations of Current Detectors

L. M. Boone·J. S. Bullock·J. R. Primack·D. A. Williams
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Abstract

This paper represents a step toward constraining galaxy formation models via TeV gamm a ray observations. We use semi-analytic models of galaxy formation to predict a spectral distribution for the intergalactic infrared photon field, which in turn yields information about the absorption of TeV gamma rays from extra-galactic sources. By making predictions for integral flux observations at >200 GeV for several known EGRE T sources, we directly compare our models with current observational upper limits obtained by Whipple. In addition, our predictions may offer a guide to the observing programs for the current population of TeV gamma ray observatories.

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L. M. Boone, J. S. Bullock, J. R. Primack, D. A. Williams. 1999-10-16. The Implications of Galaxy Formation Models for the TeV Observations of Current Detectors. https://doi.org/10.1063/1.1291351

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