1. INTRODUCTION

2. THE DATA SET
2.1. Photometric and Spectroscopic Observations – And I, II, and III
2.2. Data Reduction
2.3. Radial Velocity Measurements
2.4. Radial Velocity Uncertainties
2.5. Radial Velocity Measurements for And VII, X, and XIV

3. ESTABLISHING MEMBER STARS IN EACH DSPH

4. MEAN VELOCITIES, INTRINSIC VELOCITY DISPERSIONS, AND M/L RATIOS
4.1. More Accurate Masses and Mass Profiles of M31's dSphs

5. CHEMICAL ABUNDANCES
5.1. Photometric Metallicity Determination
5.2. Spectroscopic Metallicity Determination
5.3. Abundance Distributions

6. GLOBAL PROPERTIES: COMPARING MILKY WAY AND M31 DSPHS
6.1. An Inventory of the Milky Way and M31 dSphs
6.2. Chemical Abundance Trends
6.3. Physical Sizes
6.4. Dark Matter Masses
6.5. The Bigger Picture: The Milky Way vs M31

7. CONCLUSIONS