GLAST prospects for Swift-era afterglows

L. J. Gou, P. Mészáros

Research output: Contribution to journalArticlepeer-review

20 Scopus citations

Abstract

We calculate the GeV spectra of gamma-ray burst afterglows produced by inverse Compton scattering of these objects' sub-MeV emission. We improve on earlier treatments by using refined afterglow parameters and new model developments motivated by recent Swift observations. We present time-dependent GeV spectra for standard, constantparameter models, as well as for models with energy injection and with time-varying parameters, for a range of burst parameters. We evaluate the limiting redshift to which such afterglows can be detected by the GLAST Large Area Telescope, as well as by AGILE.

Original languageEnglish (US)
Pages (from-to)392-399
Number of pages8
JournalAstrophysical Journal
Volume668
Issue number1 I
DOIs
StatePublished - 2007

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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