1. INTRODUCTION

2. OBSERVATIONS

3. DATA REDUCTION
3.1. AKARI Reduction Facility (ARF)
3.2. Extraction of spectra
3.3. Flux and wavelength calibration
3.4. Error propagation

4. OBSERVATIONAL RESULTS
4.1. Object classification
4.2. Baseline fitting

5. SPECTRAL ANALYSIS AND DISCUSSION
5.1. H2O
5.2. CO
5.3. CO2

6. ASTROCHEMICAL IMPLICATIONS

7. CONCLUSIONS