2 SIMULATIONS AND ARTIFICIAL SPECTRA
2.1 The code and input physics
2.2 Generating spectra with specexbin
2.3 Line of sight selection

3 COMPARISON TO COS-HALOS OBSERVABLES

4 COMPARING THE CGM IN WIND MODELS
4.1 Halo Mass-Stellar Mass Relationship
4.2 Baryonic Fractions within Halos
4.3 The dynamical state

5 SUMMARY