AKARI performed about 10,000 spectroscopic observations with the Infrared Camera (IRC) during its mission phase. These IRC observations provide unique spectroscopic data at near- and mid-infrared wavelengths for studies of the next few decades because of its high sensitivity and unique wavelength coverage. In this paper, we present the current status of the activity for improving the IRC spectroscopic data reduction process, including the toolkit and related data packages, and also discuss the goal of this project.

ABSTRACT
1. INTRODUCTION
2. ISSUES CONCERNING THE REDUCTION TOOLKIT
3. CONCLUDING REMARKS
REFERENCES

• Fumihiko Usui(Department of Astronomy, Graduate School of Science, The University of Tokyo)
• Takashi Onaka(Department of Astronomy, Graduate School of Science, The University of Tokyo)
• AKARI/IRC team(Department of Astronomy, Graduate School of Science, The University of Tokyo)