1. Introduction  
2. Data  
2.1. MUSE-Wide  
2.2. MUSE-Deep  
2.3. MUSE Extremely Deep  
2.4. LAE subsamples  
3. Methods  
3.1. K-estimator  
3.2. Error estimation  
3.3. Halo occupation distribution modeling  
4. Results from HOD modeling  
5. Discussion  
5.1. Clustering dependence on Ly α luminosity  
5.2. Comparison to Herrero Alonso et al. (2021)  
5.3. Comparison to the literature  
5.4. Satellite fraction  
5.5. Implications  
6. Conclusions