We have been working on data processing and calibration of AKARI/IRC images from pointed observations. As of September 2014, a data package for each pointing only contains raw data and quick- look data, so that users have to process them using the toolkit by themselves. We plan to change this situation and to provide science-ready data sets, which are easy-to-use for non-AKARI experts. For Phase 1&2, we have updated dark and at calibrations, and also the toolkit itself to produce images more reliable and easier to use. A new data package includes fully calibrated images with WCS information. We released it for about 4000 pointings at the end of March 2015.

ABSTRACT
1. DATA PROCESSING & ARCHIVE
2. NEW FEATURES OF THE TOOLKIT
    2.1. Neighbor Dark
    2.2. NEW MIR-S FLAT
    2.3. Hot Pixel Masking
    2.4. Shift Value Statistics
    2.5. WCS Registration
    2.6. Flux Calibration
3. REMAINING ISSUES
    3.1. Memory Effect
    3.2. Earthshine Light
REFERENCES

• Fumi Egusa(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency/Chile Observatory, National Astronomical Observatory of Japan)
• AKARI/IRC team(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency/Chile Observatory, National Astronomical Observatory of Japan)