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Ultra deep AKARI observations of Abell 2218: resolving the 15 μm extragalactic background light

Hopwood, R.; Serjeant, S.; Negrello, M.; Pearson, C.; Egami, E.; Im, M.; Kneib, J.-P.; Ko, J.; Lee, H. M.; Lee, M. G.; Matsuhara, H.; Nakagawa, T.; Smail, I. and Takagi, T. (2010). Ultra deep AKARI observations of Abell 2218: resolving the 15 μm extragalactic background light. Astrophysical Journal Letters, 716(1) L45-L50.

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We present extragalactic number counts and a lower limit estimate for the cosmic infrared background (CIRB) at 15 μm from AKARI ultra deep mapping of the gravitational lensing cluster Abell 2218. These data are the deepest taken by any facility at this wavelength and uniquely sample the normal galaxy population. We have de-blended our sources, to resolve photometric confusion, and de-lensed our photometry to probe beyond AKARI's blank-field sensitivity. We estimate a de-blended 5σ sensitivity of 28.7 μJy. The resulting 15 μm galaxy number counts are a factor of 3 fainter than previous results, extending to a depth of ~ 0.01 mJy and providing a stronger lower limit constraint on the CIRB at 15 μm of 1.9 ± 0.5 nW m–2 sr–1.

Item Type: Article
Copyright Holders: 2010 The American Astronomical Society
ISSN: 2041-8213
Keywords: galactic clusters; galactic evolution; infrared: galaxies
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 25181
Depositing User: Astrid Peterkin
Date Deposited: 14 Dec 2010 12:21
Last Modified: 20 May 2017 17:49
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