Negrello, M.; Serjeant, S. and Pearson, C.
Due to copyright restrictions, this file is not available for public download
Click here to request a copy from the OU Author.
|Google Scholar:||Look up in Google Scholar|
We investigate the photometric redshift accuracy achievable from infrared data alone in AKARI Deep Surveys. We exploit both real data and detailed simulations to conclude that the passage of redshifted policyclic aromatic hydrocarbon (PAH) and silicate features into the 8–24 μm window cover by AKARI can successfully be used to constrain redshift to an accuracy better than ~10 per cent at z<2, provided that emission from AGN (if any) is not dominant in the infrared. At higher redshifts, the rest-frame 1.6 μm feature associated to evolved stars can be used as a less accurate redshift estimator.
|Item Type:||Book Chapter|
|Copyright Holders:||2009 by Astronomical Society of the Pacific|
|Extra Information:||AKARI, a light to illuminiate the misty universe.
Proceedings of a conference held at Fukutake Hall, The University of Tokyo, Tokyo, Japan 16–19 February 2009
|Academic Unit/Department:||Science > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Astrid Peterkin|
|Date Deposited:||06 Jan 2011 10:24|
|Last Modified:||15 Jan 2016 21:39|
|Share this page:|