2 THE SYDNEY-AAO MULTI-OBJECT INTEGRAL-FIELD SPECTROGRAPH (SAMI)

3 BASIC DATA PROCESSING

4 FLUX CALIBRATION AND TELLURIC ABSORPTION CORRECTION
4.1 Extracting total stellar spectra
4.2 Primary flux calibration
4.3 Telluric absorption correction
4.4 Absolute flux calibration

5 RESAMPLING TO A CARTESIAN GRID
5.1 Weight cubes
5.2 Dither frame alignment
5.3 Simple summation combination
5.4 Outlier rejection
5.5 Confirming variance propagation accuracy
5.6 Neglecting covariance
5.7 Tracking covariance

6 OPTIMAL DITHER STRATEGY

7 RECOVERING RESOLUTION VIA REDUCED DRIZZLE DROP-SIZE
7.1 Model data for drizzle resampling
7.2 Recovered PSF width
7.3 Survey data image quality
7.4 Flux scaling

8 CONCLUSION