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Spectrum of the Isotropic Diffuse Gamma-Ray Emission Derived from First-Year Fermi Large Area Telescope Data

pmid: 20366411
arXiv: 1002.3603 , http://arxiv.org/abs/1002.3603
handle: 11368/2938461 , 11577/2439880 , 11390/878740 , 11568/195311 , 11589/6187 , 11391/172955 , 11587/516272 , 11586/118112
pmid: 20366411
arXiv: 1002.3603 , http://arxiv.org/abs/1002.3603
handle: 11368/2938461 , 11577/2439880 , 11390/878740 , 11568/195311 , 11589/6187 , 11391/172955 , 11587/516272 , 11586/118112
Spectrum of the Isotropic Diffuse Gamma-Ray Emission Derived from First-Year Fermi Large Area Telescope Data
We report on the first Fermi Large Area Telescope (LAT) measurements of the so-called "extra-galactic" diffuse gamma-ray emission (EGB). This component of the diffuse gamma-ray emission is generally considered to have an isotropic or nearly isotropic distribution on the sky with diverse contributions discussed in the literature. The derivation of the EGB is based on detailed modelling of the bright foreground diffuse Galactic gamma-ray emission (DGE), the detected LAT sources and the solar gamma-ray emission. We find the spectrum of the EGB is consistent with a power law with differential spectral index g = 2.41+/-0.05 and intensity, I(> 100 MeV) = (1.03+/-0.17) 10^-5 cm^-2 s^-1 sr^-1, where the error is systematics dominated. Our EGB spectrum is featureless, less intense, and softer than that derived from EGRET data.
4 figures, 1 table, supplementary material, accepted by Physical Review Letters
- University System of Ohio United States
- Goddard Space Flight Center United States
- Ames Research Center United States
- Purdue University West Lafayette United States
- CEA LETI France
Cosmology and Nongalactic Astrophysics (astro-ph.CO), 95.85.Pw, 95.85.Pw, 96.50.sb, 98.70.Sa, 宇宙理学, FOS: Physical sciences, [ PHYS.ASTR.CO ] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 98.70.Sa, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 宇宙科学研究, gamma-ray, Cosmic rays, 96.50.sb, High Energy Astrophysical Phenomena (astro-ph.HE), 資料請求非対応, energy spectra and interactions, 520, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR.CO] Physics/Astrophysics/Cosmology and Extra-Galactic Astrophysics, Composition, Astrophysics - Cosmology and Nongalactic Astrophysics
Cosmology and Nongalactic Astrophysics (astro-ph.CO), 95.85.Pw, 95.85.Pw, 96.50.sb, 98.70.Sa, 宇宙理学, FOS: Physical sciences, [ PHYS.ASTR.CO ] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 98.70.Sa, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 宇宙科学研究, gamma-ray, Cosmic rays, 96.50.sb, High Energy Astrophysical Phenomena (astro-ph.HE), 資料請求非対応, energy spectra and interactions, 520, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR.CO] Physics/Astrophysics/Cosmology and Extra-Galactic Astrophysics, Composition, Astrophysics - Cosmology and Nongalactic Astrophysics
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