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TeV gamma rays from 3C 279 - A possible probe of origin and intergalactic infrared radiation fields

Stecker, F. W., de Jager, O. C., Salamon, M. H.·1992·The Astrophysical Journal

Abstract

The γ-ray spectrum of 3C 279 during 1991 June exhibited a near perfect power law between 50 MeV and over 5 GeV with a differential spectral index of -(2.02 +/- 0.07). If extrapolated, the γ-ray spectrum of 3C 279 should be easily detectable with first generation air Cerenkov detectors operating above ~ 0.3 TeV, provided there is no intergalactic absorption. However, by using model-dependent lower and upper limits for the extragalactic infrared background radiation field, we predict a sharp cutoff of the 3C 279 spectrum between ~0.1 and ~1 TeV. The sensitivity of present air Cerenkov detectors is good enough to measure such a cutoff, which would provide the first opportunity to obtain a measurement of, or at least a severe constraint on the extragalactic background infrared radiation field.

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Metadata

Authors
Stecker, F. W., de Jager, O. C., & Salamon, M. H.
Venue
The Astrophysical Journal
Published
1992-05
Volume
390
Pages
L49
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2160991424
Cited by
433
References
0
FWCI
8.66
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: TeV gamma rays from 3C 279 - A possible probe of origin and intergalactic infrared radiation fields. https://app.cochat.ai/papers/10.1086/186369
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Stecker, F. W., de Jager, O. C., & Salamon, M. H. (1992). TeV gamma rays from 3C 279 - A possible probe of origin and intergalactic infrared radiation fields. The Astrophysical Journal. https://doi.org/10.1086/186369

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