Journal
EXPERIMENTAL ASTRONOMY
Volume 20, Issue 1-3, Pages 41-47Publisher
SPRINGER
DOI: 10.1007/s10686-006-9041-6
Keywords
X-rays; background radiation; AGN
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We will briefly discuss the importance of sensitive X-ray observations above a few tens of keV for a better understanding of the physical mechanisms associated to the Supermassive Black Hole primary emission in both radio quiet and radio loud AGN and to the cosmological evolution of the most obscured sources.
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