Proc. IAU volume 12, issue S333, P162-165 2017 DOI: 10.1017/s1743921317011541 View full text
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L. V. Tóth, Y. Doi, S. Pinter, T. Kovács, S. Zahorecz, Z. Bagoly, L. G. Balázs, I. Horvath, I. I. Racz, T. Onishi

Abstract: AbstractWe estimate the column density of the Galactic foreground interstellar medium (GFISM) in the direction of extragalactic sources. All-sky AKARI FIS infrared sky survey data might be used to trace the GFISM with a resolution of 2 arcminutes. The AKARI based GFISM hydrogen column density estimates are compared with similar quantities based on HI 21cm measurements of various resolution and of Planck results. High spatial resolution observations of the GFISM may be important recalculating the physical param…

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