The Open UniversitySkip to content

The AKARI extragalactic Large Area Survey towards the North Ecliptic Pole

Takagi, T.; Ohyama, Y.; Matsuhara, H.; Wada, T.; Oyabu, S.; Goto, T.; Hanami, H.; Pearson, C. P.; Serjeant, S.; Negrello, M.; White, G. J.; Lee, H. M.; Im, M. and Malkan, M. (2010). The AKARI extragalactic Large Area Survey towards the North Ecliptic Pole. In: Hunting for the Dark: The Hidden Side of Galaxy Formation, 19-23 Oct 2009, Malta, pp. 47–50.

DOI (Digital Object Identifier) Link:
Google Scholar: Look up in Google Scholar


Large area surveys in the infrared wavelengths have revealed a significant evolution of the star formation activity of the universe in the past. Extragalactic surveys we have conduced with AKARI towards the north ecliptic pole (NEP) are unique, in terms of a comprehensive wavelength coverage from 2 to 24 µm using all 9 photometric bands of the IRC. This includes new wavelength windows for extragalactic surveys, such as 18 µm. We demonstrate that this IRC all-band photometry is capable of tracing a steep rise in the flux at the blue side of the polycyclic aromatic hydrocarbon (PAH) 6.2 µm emission feature of infrared luminous galaxies at z<1. Starburst-dominated ULIRGs are identified using IRC all-band photometry. The PAH-to-total IR luminosity ratio of these starburst ULIRGs is systematically higher than that of local ULIRGs. The nature of ULIRGs could be different from local ones even at z~1.

Item Type: Conference or Workshop Item
Copyright Holders: 2010 American Institute of Physics
Extra Information: Published in AIP Conf. Proc. Volume 1240, Issue 1
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Research Group: Space
Item ID: 25182
Depositing User: Astrid Peterkin
Date Deposited: 13 Jan 2011 12:26
Last Modified: 07 Dec 2018 09:44
Share this page:


Altmetrics from Altmetric

Citations from Dimensions

Actions (login may be required)

Policies | Disclaimer

© The Open University   contact the OU