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Mid-infrared all-sky survey with AKARI/IRC

Authors :
Takao Nakagawa
Satoshi Takita
Itsuki Sakon
Carlos Alfageme
Hideaki Fujiwara
Issei Yamamura
Jeonghyun Pyo
Hidenori Watarai
Shinki Oyabu
C. Stephenson
Hiroshi Shibai
Munetaka Ueno
Takashi Onaka
Woojung Kim
Naofumi Fujishiro
Fumihiko Usui
Pedro García-Lario
Kazunori Uemizu
Yoshifusa Ita
Hiroshi Murakami
Takehiko Wada
Toshio Matsumoto
Daisuke Ishihara
Sunao Hasegawa
Toshihiko Tanabe
Hirokazu Kataza
C. Yamauchi
Hideo Matsuhara
Martin Cohen
Alberto Salama
Youichi Ohyama
Source :
Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter.
Publication Year :
2008
Publisher :
SPIE, 2008.

Abstract

AKARI is the first Japanese astronomical infrared satellite mission orbiting around the Earth in a sun-synchronous polar orbit at the altitude of 700 km. One of the major observation programs of the AKARI is an all-sky survey in the mid- to far-infrared spectral regions with 6 photometric bands. The mid-infrared part of the AKARI All-Sky Survey was carried out with the Infrared Camera (IRC) at the 9 and 18 µm bands with the sensitivity of about 50 and 120 mJy (5σ per scan), respectively. The spatial resolution is about 9.4" at both bands. AKARI mid-infrared (MIR) all-sky survey substantially improves the MIR dataset of the IRAS survey of two decades ago and provides a significant database for studies of various fields of astronomy ranging from star-formation and debris disk systems to cosmology. This paper describes the current status of the data reduction and the characteristics of the AKARI MIR all-sky survey data.

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter
Accession number :
edsair.doi...........635ec093189235ad0f41220c650754c3
Full Text :
https://doi.org/10.1117/12.788737