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GRIPS Poster - Santa Fe 2007
The primary goal of GRIPS is to revolutionise our understanding of the early universe using GRBs. We propose a new generation γ-ray observatory capable of unprecedented spectroscopy over a wide range of energies (200keV-50MeV) and polarimetry (100-1000keV). Secondary goals achievable by this mission include direct measurements of supernovae interiors through γ-rays from radioactivity, nuclear astrophysics with massive stars and novae, and studies of particle acceleration near compact stars, interstellar shocks and clusters of galaxies.
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