1. Introduction

2. Description of the Sample - Observations - Data reduction

3. Kernel smoothing method
3.1. Averaging the discrete velocity field with the adaptive kernel smoothing technique
3.2. Fitting a rotation model

4. Systemic velocity subtraction

5. Point symmetry analysis of the sample
5.1. Testing the significance of the deviations from point-symmetry

6. The halo kinematics of ETGs
6.2. Kinematic parameters
6.3. Velocity dispersion profiles
6.4. Triaxiality

7. Results per family
7.1. Slow rotators
7.2. Fast rotators
7.3. Summary

8. Discussion
8.1. Halo rotation versus central rotation
8.2. Fast rotators with disks embedded in slowly rotating halos
8.3. Signatures of triaxial halos in the kinematics
8.4. Signatures of triaxial halos in extended photometry
8.5. Comparison with the results of the ATLAS 3D survey
8.6. Kinematic transition radius
8.7. The diverse halo formation histories

9. Summary and conclusions