From 9ecc583701c314bf3fdceb9855905bc4e7eb070e Mon Sep 17 00:00:00 2001 From: Matthieu Schaller <schaller@strw.leidenuniv.nl> Date: Thu, 31 Oct 2019 18:02:43 +0100 Subject: [PATCH] Updated all the examples to use the new EAGLE default: power-law of slope -1. --- examples/EAGLE_ICs/EAGLE_12/eagle_12.yml | 6 +++--- examples/EAGLE_ICs/EAGLE_25/eagle_25.yml | 6 +++--- examples/EAGLE_ICs/EAGLE_50/eagle_50.yml | 6 +++--- examples/EAGLE_low_z/EAGLE_12/eagle_12.yml | 9 +++------ examples/EAGLE_low_z/EAGLE_25/eagle_25.yml | 6 +++--- examples/EAGLE_low_z/EAGLE_50/eagle_50.yml | 6 +++--- examples/EAGLE_low_z/EAGLE_6/eagle_6.yml | 6 +++--- .../IsolatedGalaxy_feedback/isolated_galaxy.yml | 6 +++--- examples/parameter_example.yml | 8 +++++--- 9 files changed, 29 insertions(+), 30 deletions(-) diff --git a/examples/EAGLE_ICs/EAGLE_12/eagle_12.yml b/examples/EAGLE_ICs/EAGLE_12/eagle_12.yml index cf4d711c5c..a6964ea303 100644 --- a/examples/EAGLE_ICs/EAGLE_12/eagle_12.yml +++ b/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. diff --git a/examples/EAGLE_ICs/EAGLE_25/eagle_25.yml b/examples/EAGLE_ICs/EAGLE_25/eagle_25.yml index ddd0470c2a..21bf89b94a 100644 --- a/examples/EAGLE_ICs/EAGLE_25/eagle_25.yml +++ b/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. diff --git a/examples/EAGLE_ICs/EAGLE_50/eagle_50.yml b/examples/EAGLE_ICs/EAGLE_50/eagle_50.yml index c12e8b33b4..7e935e4db6 100644 --- a/examples/EAGLE_ICs/EAGLE_50/eagle_50.yml +++ b/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. diff --git a/examples/EAGLE_low_z/EAGLE_12/eagle_12.yml b/examples/EAGLE_low_z/EAGLE_12/eagle_12.yml index 957ff91343..c5757b6d70 100644 --- a/examples/EAGLE_low_z/EAGLE_12/eagle_12.yml +++ b/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. diff --git a/examples/EAGLE_low_z/EAGLE_25/eagle_25.yml b/examples/EAGLE_low_z/EAGLE_25/eagle_25.yml index 4c47bd4ef8..547b769878 100644 --- a/examples/EAGLE_low_z/EAGLE_25/eagle_25.yml +++ b/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. diff --git a/examples/EAGLE_low_z/EAGLE_50/eagle_50.yml b/examples/EAGLE_low_z/EAGLE_50/eagle_50.yml index 8cdc90dc0a..1473010fb5 100644 --- a/examples/EAGLE_low_z/EAGLE_50/eagle_50.yml +++ b/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. diff --git a/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml b/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml index bf56b800c5..e07ad47d0c 100644 --- a/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml +++ b/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. diff --git a/examples/IsolatedGalaxy/IsolatedGalaxy_feedback/isolated_galaxy.yml b/examples/IsolatedGalaxy/IsolatedGalaxy_feedback/isolated_galaxy.yml index 365412195b..91e1f30c54 100644 --- a/examples/IsolatedGalaxy/IsolatedGalaxy_feedback/isolated_galaxy.yml +++ b/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. diff --git a/examples/parameter_example.yml b/examples/parameter_example.yml index b23c0a58b2..7119605b19 100644 --- a/examples/parameter_example.yml +++ b/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. -- GitLab