We carry out a systematic study of Galactic supernova remnants (SNRs) using the AKARI Far Infrared Surveyor (FIS) survey data. The AKARI Infrared Astronomical Satellite observed the whole sky using the four FIS bands covering 50 to 180 microns with ~1 arcmin resolution. The all-sky coverage with high-spatial resolution provides an unprecedented opportunity to study diffuse, extended far-infrared (FIR) sources such as SNRs. We have searched for FIR counterparts to all 274 known Galactic SNRs, and investigate their FIR properties of identified SNRs. We report preliminary results of the study.

ABSTRACT
1. INTRODUCTION
2. PRELIMINARY RESULTS
    2.1. Detection Rate of FIR SNRs
    2.2. FIR Bright SNR
REFERENCES

• IL-GYO JEONG(Department of Physics and Astronomy, Seoul National University)
• BON-CHUL KOO(Department of Physics and Astronomy, Seoul National University)
• HO-GYU LEE(Department of Astronomy, Graduate School of Science, The University of Tokyo)