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FOREGROUND OF GAMMA-RAY BURSTS (GRBS) FROM AKARI FIS DATA
L. Viktor Toth,YASUO DOI,SAROLTA ZAHORECZ,Marton Agas,LAJOS G. BALAZS,Adrienn Forro,Istvan I. Racz 한국천문학회 2017 天文學論叢 Vol.32 No.1
A significant number of the parameters of a gamma-ray burst (GRB) and its host galaxy are calculated from the afterglow. There are various methods obtaining extinction values for the necessary correction for galactic foreground. These are: galaxy counts, from HI 21 cm surveys, from spectroscopic measurements and colors of nearby Galactic stars, or using extinction maps calculated from infrared surveys towards the GRB. We demonstrate that \textit{AKARI} Far-Infrared Surveyor sky surface brightness maps are useful uncovering the fine structure of the galactic foreground of GRBs. Galactic cirrus structures of a number of GRBs are calculated with a 2 arcminute resolution, and the results are compared to that of other methods.