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Gamma Ray Astronomy With IceCube
Astrophysics · Submitted 13 May 2003
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We demonstrate that the South Pole kilometer-scale neutrino observatory IceCube can detect multi-TeV gamma rays continuously over a large fraction of the southern sky.
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The abstract, sentence by sentence
We demonstrate that the South Pole kilometer-scale neutrino observatory IceCube can detect multi-TeV gamma rays continuously over a large fraction of the southern sky. While not as sensitive as pointing atmospheric Cerenkov telescopes, IceCube can roughly match the sensitivity of Milagro. Also, IceCube is complementary to Milagro because it will observe, without interruption, a relatively poorly studied fraction of the southern sky. The information which IceCube must record to function as a gamma ray observatory is only the directions and possibly energies of down-going muons.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We demonstrate that the South Pole kilometer-scale neutrino observatory IceCube can detect multi-TeV gamma rays continuously over a large fraction of the southern sky. | result 0.58 | 0.89 | 0.87 | asserted 1.00 |
| s1 | While not as sensitive as pointing atmospheric Cerenkov telescopes, IceCube can roughly match the sensitivity of Milagro. | limitation 0.59 | 0.62 | 0.09 | asserted 0.84 |
| s2 | Also, IceCube is complementary to Milagro because it will observe, without interruption, a relatively poorly studied fraction of the southern sky. | interpretation 0.92 | 0.28 | 0.12 | asserted 0.93 |
| s3 | The information which IceCube must record to function as a gamma ray observatory is only the directions and possibly energies of down-going muons. | method 0.97 | 0.41 | 0.07 | asserted 0.89 |
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The paper
Original abstract
We demonstrate that the South Pole kilometer-scale neutrino observatory IceCube can detect multi-TeV gamma rays continuously over a large fraction of the southern sky. While not as sensitive as pointing atmospheric Cerenkov telescopes, IceCube can roughly match the sensitivity of Milagro. Also, IceCube is complementary to Milagro because it will observe, without interruption, a relatively poorly studied fraction of the southern sky. The information which IceCube must record to function as a gamma ray observatory is only the directions and possibly energies of down-going muons.
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How the literature uses it
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Papers citing it
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The possibility of using muon detectors in general, and IceCube in particular, as a gamma-ray telescope has been extensively studied [ref] and has been exploited to put limits on the TeV emission of a soft gamma-ray-repeater [ref] .
Gamma-ray Astronomy with Muons: Sensitivity of IceCube to PeVatrons in the Southern Sky · Introduction and Summary of Results · 0.90
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