diff --git a/examples/parameter_example.yml b/examples/parameter_example.yml
index 28f3d25e291ce5ca9dd3cd4b97eb01874734e15b..26a85f4bc2b40a9bfe21b3c7eaa5b25520e1e1be 100644
--- a/examples/parameter_example.yml
+++ b/examples/parameter_example.yml
@@ -339,10 +339,33 @@ EAGLEStarFormation:
 
 # EAGLE feedback model
 EAGLEFeedback:
-  filename:                     /cosma5/data/Eagle/BG_Tables/YieldTables/       # Filepath where yield tables are stored
-  imf_model:                    Chabrier                                        # IMF model (choice of Chabrier or PowerLaw)
-  continuous_heating_switch:    0                                               # Switch between continuous heating (1) and stochastic heating (0) 
-  SNIa_timescale_Gyr:           2.0                                             # Timescale governing how many SNIa produced
-  SNIa_efficiency:              2.e-3                                           # Factor governing how efficiency of SNIa production
-  SNII_wind_delay_Gyr:          0.03                                            # Delay to production of SNII winds after star's birth 
-  SNe_heating_temperature_K:    3.16228e7                                       # Temperature to heat gas particles to when distributing SNe energy stochastically
+  use_SNe_feedback:                 1               # Global switch for SNe thermal feedback.
+  use_AGB_enrichment:               1               # Global switch for enrichement from AGB stars.
+  use_SNII_enrichment:              1               # Global switch for enrichement from SNII stars.
+  use_SNIa_enrichment:              1               # Global switch for enrichement from SNIa stars.
+  filename:                         ./yieldtables/  # Path to the directory containing the EAGLE yield tables.
+  IMF_min_mass_Msun:                0.1             # Minimal stellar mass considered for the Chabrier IMF in solar masses.
+  IMF_max_mass_Msun:              100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
+  SNII_min_mass_Msun:               6.0             # Minimal mass considered for SNII feedback (not SNII enrichment!) in solar masses.
+  SNII_max_mass_Msun:             100.0             # Maximal mass considered for SNII feedback (not SNII enrichment!) in solar masses.
+  SNII_wind_delay_Gyr:              0.03            # Time in Gyr between a star's birth and the SNII thermal feedback event.
+  SNII_delta_T_K:                   3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.
+  SNII_Energy_erg:                  1.0e51          # Energy of one SNII explosion in ergs.
+  SNII_Energy_fraction_min:         3.0             # Maximal fraction of energy applied in a SNII feedback event.
+  SNII_Energy_fraction_max:         0.3             # Minimal fraction of energy applied in a SNII feedback event.
+  SNII_Energy_fraction_Z_0:         0.0012663729    # Pivot point for the metallicity dependance of the SNII energy fraction (metal mass fraction).
+  SNII_Energy_fraction_n_0_H_p_cm3: 0.67            # Pivot point for the birth density dependance of the SNII energy fraction in cm^-3.
+  SNII_Energy_fraction_n_Z:         0.8686          # Power-law for the metallicity dependance of the SNII energy fraction.
+  SNII_Energy_fraction_n_n:         0.8686          # Power-law for the birth density dependance of the SNII energy fraction.
+  SNIa_max_mass_Msun:              8.0              # Maximal mass considered for SNIa feedback and enrichment in solar masses.
+  SNIa_timescale_Gyr:              2.0              # Time-scale of the exponential decay of the SNIa rates in Gyr.
+  SNIa_efficiency_p_Msun:          0.002            # Normalisation of the SNIa rates in inverse solar masses.
+  SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.
+  SNII_yield_factor_Helium:         1.0             # (Optional) Correction factor to apply to the Helium yield from the SNII channel.
+  SNII_yield_factor_Carbon:         0.5             # (Optional) Correction factor to apply to the Carbon yield from the SNII channel.
+  SNII_yield_factor_Nitrogen:       1.0             # (Optional) Correction factor to apply to the Nitrogen yield from the SNII channel.
+  SNII_yield_factor_Oxygen:         1.0             # (Optional) Correction factor to apply to the Oxygen yield from the SNII channel.
+  SNII_yield_factor_Neon:           1.0             # (Optional) Correction factor to apply to the Neon yield from the SNII channel.
+  SNII_yield_factor_Magnesium:      2.0             # (Optional) Correction factor to apply to the Magnesium yield from the SNII channel.
+  SNII_yield_factor_Silicon:        1.0             # (Optional) Correction factor to apply to the Silicon yield from the SNII channel.
+  SNII_yield_factor_Iron:           0.5             # (Optional) Correction factor to apply to the Iron yield from the SNII channel.