1. Introduction
2. Observations and data reduction
2.1. Sample
2.2. Overview of observations and data reduction
2.3. Antlia B
2.4. Leo T
2.5. Hydra II
2.6. Grus 1
3. Methods
3.1. CJAM
3.2. GravSphere
4. Results
4.1. Parameter estimation
4.2. Profile recovery
4.3. Model comparison
4.4. Tidal stripping
4.5. Galaxy–halo scaling relations
5. Discussion
5.1. Comparison to previous results
5.2. Reliability of inferred parameters
5.3. Reliability of the dynamical analysis
6. Conclusions