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Doi, Y.; Etxaluze Azkonaga, M.; White, G. J.; Figueredo, E.; Chinone, Y.; Hattori, M.; Nakagawa, T.; Yamauchi, C. and Shibai, H.
(2009).
URL: http://astrosociety.org/astroshop/index.php?p=prod...
Abstract
We discuss the capability of AKARI in recovering diffuse far-infrared emission, and examine the achieved reliability. Critical issues in making images of diffuse emission are the transient response and long-term stability of the far-infrared detectors. Quantitative evaluation of these characteristics are the key to achieving sensitivity comparable to or better than that for point sources (< 20–95 MJy sr-1). We describe current activity and progress toward the production of high quality images of the diffuse far-infrared emission using the AKARI all-sky survey data.