Matute, I.; La Franca, F.; Pozzi, F.; Gruppioni, C.; Lari, C.; Zamorani, G.; Alexander, D.M.; Danese, L.; Oliver, S.; Serjeant, S. and Rowan-Robinson, M.
|DOI (Digital Object Identifier) Link:||https://doi.org/10.1046/j.1365-8711.2002.05488.x|
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We present the 15-mum luminosity function of type 1 active galactic nuclei (AGN1; quasi-stellar object+Seyfert 1) . Our sample of 21 high-redshift sources is selected from the Preliminary Analysis catalogue in the S1 field of the European Large Area ISO Survey (ELAIS). To study the cosmological evolution of the AGN1 luminosity function, our sample has been combined with a local sample of 41 sources observed by IRAS . We find that the luminosity function of AGN1 at 15mum is fairly well represented by a double-power-law-function. There is evidence for significant cosmological evolution consistent with a pure luminosity evolution (PLE) model L (z )~(1+z ) k L , with k L =3.0-3.3. The value of k L depends on the existence or non-existence of an evolution cut-off at redshift ~2, and on the adopted cosmology. From the luminosity function and its evolution we estimate a contribution of AGN1 to the cosmic infrared background (CIRB) of nuI nu ~6×10-11 Wm-2 sr-1 at 15mum. This corresponds to ~2-3 per cent of the total observed CIRB at this wavelength. Under the usual assumptions of unified models for AGN, the expected contribution of the whole AGN population to the CIRB at 15mum is 10-15 per cent.
|Item Type:||Journal Article|
|Extra Information:||Some of the symbols may not have transferred correctly into this bibliographic record and/or abstract.|
|Keywords:||surveys; galaxies; cosmology; observations; infrared|
|Academic Unit/Department:||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)|
|Depositing User:||Users 13 not found.|
|Date Deposited:||31 Oct 2006|
|Last Modified:||04 Oct 2016 09:55|
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