Cosmic Star Formation Rate From Gamma-Ray Attenuation
classification
🌌 astro-ph
keywords
attenuationcosmicformationratestarambientcomputegalaxies
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We compute the attenuation of gamma-rays from remote quasars due to interactions with ambient low-energy photons produced by stars in galaxies and show that the next-generation gamma ray telescopes can probe the cosmic star formation rate at high redshifts.
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