AKARI has 4 imaging bands in the far-infrared (FIR) and 9 imaging bands that cover the near-infrared (NIR) to mid-infrared (MIR) contiguously. The FIR bands probe the thermal emission from sub-micron dust grains, while the MIR bands observe emission from stochastically-heated very small grains and the unidentified infrared (UIR) band emissions from carbonaceous materials that contain aromatic and aliphatic bonds. The multi-band characteristics of the AKARI instruments are quite efficient to study the spectral energy distribution of the interstellar medium, which always shows multi-component nature, as well as its variations in the various environments. AKARI also has spectroscopic capabilities. In particular, one of the onboard instruments, Infrared Camera (IRC), can obtain a continuous spectrum from 2.5 to 13 μm with the same slit. This allows us to make a comparative study of the UIR bands in the diffuse emission from the 3.3 to 11.3 μm for the first time. The IRC explores high-sensitivity spectroscopy in the NIR, which enables the study of interstellar ices and the UIR band emission at 3.3 − 3.5 μm in various objects. Particularly, the UIR bands in this spectral range contain unique information on the aromatic and aliphatic bonds in the band carriers. This presentation reviews the results of AKARI observations of the interstellar medium with an emphasis on the observations of the NIR spectroscopy.

ABSTRACT
1. INTRODUCTION
2. IRC NEAR-INFRARED SPECTROSCOPY
    2.1. SPECTRUM OF THE GALACTIC PLANE
    2.2. DEUTERATED PAH FEATURES
3. WARM DEBRIS DISKS
4. SUMMARY
REFERENCES

• TAKASHI ONAKA(Department of Astronomy, Graduate School of Science, The University of Tokyo)