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The structure of the ISM in the Zone of Avoidance by high-resolution multi-wavelength observations
Tóth, L. V.; Doi, Y.; Pinter, S.; Kovács, T.; Zahorecz, S.; Bagoly, Z.; Balázs, L. G.; Horvath, I.; Racz, I. I.; Onishi, T.
AA(Eötvös University, Budapest, ; MTA CSFK Konkoly Observatory, Budapest), AB(Department of Earth Science and Astronomy, The University of Tokyo, 3-8-1 Komaba, Meguro-ku, Tokyo 153-8902, Japan), AC(Eötvös University, Budapest), AD(Eötvös University, Budapest), AE(Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai, Osaka 599-8531, Japan; Chile Observatory, NAOJ, NINS, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan), AF(Eötvös University, Budapest), AG(Eötvös University, Budapest; MTA CSFK Konkoly Observatory, Budapest), AH(National University of Public Service, Budapest), AI(Eötvös University, Budapest; MTA CSFK Konkoly Observatory, Budapest), AJ(Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai, Osaka 599-8531, Japan)
Peering towards Cosmic Dawn, Proceedings of the International Astronomical Union, IAU Symposium, Volume 333, pp. 162-165
Publication Date:
ISM: structure, infrared: ISM, gamma-ray burst: general, GRB110213A
Abstract Copyright:
(c) 2018: Copyright © International Astronomical Union 2018
Bibliographic Code:


We 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 parameters of gamma-ray burst (GRB) host galaxies using the updated foreground parameters.
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