1. Introduction  
2. The Sample  
3. Observations and Data Reduction  
3.1. GHASP Instrumental Setup  
3.2. Comparison With Other Integral Field Spectrographs  
3.3. Data Reduction  
3.4. Flux Calibration and Hα Profiles  
4. Data Analysis  
4.1. Kinematical Models and Rotation Curves  
4.2. Kinematical Projection Parameters  
5. Discussion: Dynamical Masses  
5.2. The Optical and NIR Tully-Fisher Relation  
5.3. Stellar and Baryonic Tully-Fisher Relations  
5.4. Baryonic versus Dynamical Masses  
5.5. Baryonic and Dynamical Mass Main Sequences  
6. Conclusions