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Digging the Cosmic Infrared Background out of the lobes of a radio galaxy

Abstract:
We describe a new, independent method for breaking the deadlock of measuring the cosmologically very important Cosmic Infrared Background. Our method measures the energy density of the Cosmic Infrared Background at the location of radio galaxies by using Fermi Gamma-ray and multiwavelength observations of their radio lobes. We present an application of our method for the well-studied radio galaxy Fornax A, showing that Fermi observations will provide us with a direct, model independent measurement of the Cosmic Infrared Background. © 2009 American Institute of Physics.
Publication status:
Published

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Publisher copy:
10.1063/1.3076749

Authors



Host title:
HIGH ENERGY GAMMA-RAY ASTRONOMY
Volume:
1085
Pages:
616-619
Publication date:
2009-01-01
DOI:
EISSN:
1551-7616
ISSN:
0094-243X
ISBN:
9780735406162


Keywords:
Pubs id:
pubs:490
UUID:
uuid:54dc0d4e-21e2-4471-be00-4ecc58bd777c
Local pid:
pubs:490
Source identifiers:
490
Deposit date:
2012-12-19

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