Updated all the examples to use the new EAGLE default: power-law of slope -1.

examples/EAGLE_ICs/EAGLE_12/eagle_12.yml

@@ -153,9 +153,9 @@ EAGLEFeedback:
   SNII_energy_fraction_n_0_H_p_cm3: 1.4588          # 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.
+  SNIa_DTD:                         PowerLaw        # Functional form of the SNIa delay time distribution.
+  SNIa_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun).
+  SNIa_DTD_power_law_norm_p_Msun:   0.0012          # Normalization of the SNIa delay time distribution (in Msun^-1).
   SNIa_energy_erg:                 1.0e51           # Energy of one SNIa explosion in ergs.
   AGB_ejecta_velocity_km_p_s:      10.0             # Velocity of the AGB ejectas in km/s.
   SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.

examples/EAGLE_ICs/EAGLE_25/eagle_25.yml

@@ -154,9 +154,9 @@ EAGLEFeedback:
   SNII_energy_fraction_n_0_H_p_cm3: 1.4588          # 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.
+  SNIa_DTD:                         PowerLaw        # Functional form of the SNIa delay time distribution.
+  SNIa_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun).
+  SNIa_DTD_power_law_norm_p_Msun:   0.0012          # Normalization of the SNIa delay time distribution (in Msun^-1).
   SNIa_energy_erg:                 1.0e51           # Energy of one SNIa explosion in ergs.
   AGB_ejecta_velocity_km_p_s:      10.0             # Velocity of the AGB ejectas in km/s.
   SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.

examples/EAGLE_ICs/EAGLE_50/eagle_50.yml

@@ -154,9 +154,9 @@ EAGLEFeedback:
   SNII_energy_fraction_n_0_H_p_cm3: 1.4588          # 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.
+  SNIa_DTD:                         PowerLaw        # Functional form of the SNIa delay time distribution.
+  SNIa_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun).
+  SNIa_DTD_power_law_norm_p_Msun:   0.0012          # Normalization of the SNIa delay time distribution (in Msun^-1).
   SNIa_energy_erg:                 1.0e51           # Energy of one SNIa explosion in ergs.
   AGB_ejecta_velocity_km_p_s:      10.0             # Velocity of the AGB ejectas in km/s.
   SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.

examples/EAGLE_low_z/EAGLE_12/eagle_12.yml

@@ -150,12 +150,9 @@ EAGLEFeedback:
   SNII_energy_fraction_n_0_H_p_cm3: 1.4588          # 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_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~< 8 Msun).
-  SNIa_DTD:                        PowerLaw         # Functional form of the SNIa delay time distribution.
-  SNIa_DTD_power_law_norm_p_Msun:  0.0012           # Normalization of the SNIa delay time distribution (in Msun^-1).
-  SNIa_DTD_exp_norm_p_Msun:        0.002            # Normalization of the SNIa delay time distribution (in Msun^-1).	
-  SNIa_DTD_exp_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.
+  SNIa_DTD:                         PowerLaw        # Functional form of the SNIa delay time distribution.
+  SNIa_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun).
+  SNIa_DTD_power_law_norm_p_Msun:   0.0012          # Normalization of the SNIa delay time distribution (in Msun^-1).
   SNIa_energy_erg:                 1.0e51           # Energy of one SNIa explosion in ergs.
   AGB_ejecta_velocity_km_p_s:      10.0             # Velocity of the AGB ejectas in km/s.
   SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.

examples/EAGLE_low_z/EAGLE_25/eagle_25.yml

@@ -158,9 +158,9 @@ EAGLEFeedback:
   SNII_energy_fraction_n_0_H_p_cm3: 1.4588          # 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.
+  SNIa_DTD:                         PowerLaw        # Functional form of the SNIa delay time distribution.
+  SNIa_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun).
+  SNIa_DTD_power_law_norm_p_Msun:   0.0012          # Normalization of the SNIa delay time distribution (in Msun^-1).
   SNIa_energy_erg:                 1.0e51           # Energy of one SNIa explosion in ergs.
   AGB_ejecta_velocity_km_p_s:      10.0             # Velocity of the AGB ejectas in km/s.
   SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.

examples/EAGLE_low_z/EAGLE_50/eagle_50.yml

@@ -149,9 +149,9 @@ EAGLEFeedback:
   SNII_energy_fraction_n_0_H_p_cm3: 1.4588          # 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.
+  SNIa_DTD:                         PowerLaw        # Functional form of the SNIa delay time distribution.
+  SNIa_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun).
+  SNIa_DTD_power_law_norm_p_Msun:   0.0012          # Normalization of the SNIa delay time distribution (in Msun^-1).
   SNIa_energy_erg:                 1.0e51           # Energy of one SNIa explosion in ergs.
   AGB_ejecta_velocity_km_p_s:      10.0             # Velocity of the AGB ejectas in km/s.
   SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.

examples/EAGLE_low_z/EAGLE_6/eagle_6.yml

@@ -159,9 +159,9 @@ EAGLEFeedback:
   SNII_energy_fraction_n_0_H_p_cm3: 1.4588          # 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.
+  SNIa_DTD:                         PowerLaw        # Functional form of the SNIa delay time distribution.
+  SNIa_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun).
+  SNIa_DTD_power_law_norm_p_Msun:   0.0012          # Normalization of the SNIa delay time distribution (in Msun^-1).
   SNIa_energy_erg:                 1.0e51           # Energy of one SNIa explosion in ergs.
   AGB_ejecta_velocity_km_p_s:      10.0             # Velocity of the AGB ejectas in km/s.
   SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.

examples/IsolatedGalaxy/IsolatedGalaxy_feedback/isolated_galaxy.yml

@@ -134,9 +134,9 @@ EAGLEFeedback:
   SNII_energy_fraction_n_0_H_p_cm3: 1.4588          # 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.
+  SNIa_DTD:                         PowerLaw        # Functional form of the SNIa delay time distribution.
+  SNIa_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun).
+  SNIa_DTD_power_law_norm_p_Msun:   0.0012          # Normalization of the SNIa delay time distribution (in Msun^-1).
   SNIa_energy_erg:                 1.0e51           # Energy of one SNIa explosion in ergs.
   AGB_ejecta_velocity_km_p_s:      10.0             # Velocity of the AGB ejectas in km/s.
   SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.

examples/parameter_example.yml

@@ -404,9 +404,11 @@ EAGLEFeedback:
   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.
+  SNIa_DTD:                         PowerLaw        # Functional form of the SNIa delay time distribution Two choices: 'PowerLaw' or 'Exponential'.
+  SNIa_DTD_delay_Gyr:               0.04            # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun).
+  SNIa_DTD_power_law_norm_p_Msun:   0.0012          # Normalization of the SNIa delay time distribution in the power-law DTD case (in Msun^-1).
+  SNIa_DTD_exp_norm_p_Msun:         0.002           # Normalization of the SNIa delay time distribution in the exponential DTD case (in Msun^-1).
+  SNIa_DTD_exp_timescale_Gyr:       2.0             # Time-scale of the SNIa delay time distribution in the exponential DTD case (in Gyr).
   SNIa_energy_erg:                 1.0e51           # Energy of one SNIa explosion in ergs.
   AGB_ejecta_velocity_km_p_s:      10.0             # Velocity of the AGB ejectas in km/s.
   SNII_yield_factor_Hydrogen:       1.0             # (Optional) Correction factor to apply to the Hydrogen yield from the SNII channel.