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A Clash of Clusters Provides New Clue to Dark Matter
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PoGOLite Experiment
PoGO is the light-weight Polarized Gamma-ray Observer (PoGOLite) experiment to measure the polarization of soft gamma rays in the 25 keV-100 keV energy range. Polarized
gamma rays are expected from a wide variety of sources including
rotation-powered pulsars, accreting black holes and neutron stars, and
jet-dominated active galaxies. PoGO-Lite Experiment has been supported in US, Sweden, Japan, and France.
For further information please visit the project home page.
For further information please visit the project home page.
MASS: Lance Simms