Takagi, T.; Matsuhara, H.; Matsuura, S.; Wada, T.; Oyabu, S.; Hanami, H.; Goto, T.; Ohyama, Y.; Shirahata, M.; Pearson, C. P.; Lee, H. M.; Im, M.; Serjeant, S.; White, G. and Nakagawa, T.
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Using AKARI, the first Japanese satellite dedicated to infrared astronomy, we conducted multi-band large-area surveys around the ecliptic poles. The north ecliptic pole (NEP) is the best region for AKARI which has a sunsynchronous orbit that allows it conduct legacy surveys with all AKARI bands, i.e. nine bands in 2 – 24 μm and 4 bands in 65 – 160 μm. We prove that this survey, which has such unprecedented infrared wavelength coverage, is certainly unique and useful to search out new galaxy populations such as ”PAH-luminous” galaxies.
|Item Type:||Conference Item|
|Copyright Holders:||2008 by Astronomical Society of the Pacific|
|Extra Information:||Panoramic Views of Galaxy Formation and Evolution
Volume: 399 Year: 2008
Edited by Tadayuki Kodama, Toru Yamada, Kentaro Aoki
|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:||Tracy Bartlett|
|Date Deposited:||16 Dec 2010 09:49|
|Last Modified:||07 Aug 2016 19:54|
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