Cosmic Star Formation Rate From Gamma-Ray Attenuation

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dc.creatorKneiske, T. M.
dc.creatorMannheim, K.
dc.date1999-12-21
dc.date.accessioned2026-07-07T02:35:08Z
dc.date.available2026-07-07T02:35:08Z
dc.descriptionWe 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.
dc.description4 pages, 7 figures, to appear in Proc. of 33rd ESLAB Symp. (ESA SP-445, 2000)
dc.identifierhttps://arxiv.org/abs/astro-ph/9912450
dc.identifierhttp://arxiv.org/abs/astro-ph/9912450
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15507
dc.subjectAstrophysics
dc.titleCosmic Star Formation Rate From Gamma-Ray Attenuation
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