1. INTRODUCTION

2. SCIENCE REQUIREMENTS
2.1. Requirements on the Sample
2.2. Requirements on Data Quality

3. HARDWARE

4. SAMPLE DESIGN

5. DESIGN AND EXECUTION OF THE OBSERVATIONS
5.1. Observing Strategy
5.2. Plate Completeness Thresholds
5.3. Field Planning
5.4. Plate Design
5.5. Observing preparation and procedure
5.6. Dithered observations with guider offset
5.7. Quicklook Verification of Data Quality
5.8. Data Reduction

6. SIGNAL-TO-NOISE ACCUMULATION SPEED AND SURVEY PROGRESS
6.1. S/N as a function of fiber magnitude
6.2. Exposure S/N Dependence on Airmass and Galactic Extinction
6.3. S/N prediction and expected survey speed
6.4. Final S/N Distribution and Projection
6.5. Projection for the Number of Galaxies

7. DATA QUALITY ASSESSMENT
7.1. Example Spectra from Data Cube
7.2. Resulting PSF on the Focal Plane from seeing and guiding
7.3. Sampling Uniformity from the Actual Dithers
7.4. Spectral Resolution
7.5. Quality of Sky Subtraction
7.6. Quality of Flux Calibration

8. VERIFICATION OF THE SCIENCE REQUIREMENTS
8.1. Star Formation Rate Surface Density
8.2. Gas Metallicity Gradient
8.3. Stellar Population Gradients
8.4. Specific Angular Momentum
8.5. Enclosed Gravitating Mass and Dark Matter Fraction

9. SUMMARY