Probing The Extragalactic Background With GLAST

Details Probing The Extragalactic Background With GLAST Probing The Extragalactic Background With GLAST

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..921...24h&link_type=abstract

THE FIRST GLAST SYMPOSIUM. AIP Conference Proceedings, Volume 921, pp. 24-25 (2007).

Mathematics

Logic

5

Background Radiations, Gamma-Ray Sources, Gamma-Ray Bursts, Active And Peculiar Galaxies And Related Systems

Scientific paper

The extragalactic radiation background across a wide wavelengths range from the radio- to the high-energy regime is in part truly diffuse and in part composed of emission from unresolved populations of sources. The cosmic history of light, recorded in the background spectrum, can be probed via γγ-pair creation absorption in high-energy spectra of sources at cosmological distances. GLAST will measure many blazar- and gamma-ray burst spectra and thus provide a significant source sample for studies of the metagalactic radiation field as a function of look-back time.

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