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• W2952808506 abstract "We discuss the contribution of the blazar population to the extragalactic background radiation across the electromagnetic (e.m.) spectrum with particular reference to the microwave, hard-X-ray and γ-ray bands. Our estimates are based on a recently derived blazar radio LogN-LogS that was built by combining several radio and multi-frequency surveys. We show that blazar emission integrated over cosmic time gives rise to a considerable broad-band non-thermal cosmic background that dominates the extragalactic brightness in the high-energy part of the e.m. spectrum. We also estimate the number of blazars that are expected to be detected by future planned or hypothetical missions operating in the X-ray and γ-ray energy bands." @default.
• W2952808506 created "2019-06-27" @default.
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• W2952808506 date "2006-01-01" @default.
• W2952808506 modified "2023-09-23" @default.
• W2952808506 title "Non-thermal cosmic backgrounds and prospects for future high-energy observations of blazars" @default.
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• W2952808506 doi "https://doi.org/10.1007/978-1-4020-5304-7_4" @default.
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