Modified the default maximal Eddington fraction in all the EAGLE example to...

Modified the default maximal Eddington fraction in all the EAGLE example to 150% to reflect the mistake from the original EAGLE runs where the fraction was set to 100% / h.

examples/EAGLE_ICs/EAGLE_12/eagle_12.yml

@@ -164,7 +164,7 @@ EAGLEFeedback:
 # EAGLE AGN model
 EAGLEAGN:
   subgrid_seed_mass_Msun:           1.5e5      # Black hole subgrid mass at creation time in solar masses.
-  max_eddington_fraction:           1.         # Maximal allowed accretion rate in units of the Eddington rate.
+  max_eddington_fraction:           1.5        # Maximal allowed accretion rate in units of the Eddington rate.
   viscous_alpha:                    1e6        # Normalisation constant of the Bondi viscuous time-scale accretion reduction term
   radiative_efficiency:             0.1        # Fraction of the accreted mass that gets radiated.
   coupling_efficiency:              0.15       # Fraction of the radiated energy that couples to the gas in feedback events.

examples/EAGLE_ICs/EAGLE_25/eagle_25.yml

@@ -165,7 +165,7 @@ EAGLEFeedback:
 # EAGLE AGN model
 EAGLEAGN:
   subgrid_seed_mass_Msun:           1.5e5      # Black hole subgrid mass at creation time in solar masses.
-  max_eddington_fraction:           1.         # Maximal allowed accretion rate in units of the Eddington rate.
+  max_eddington_fraction:           1.5        # Maximal allowed accretion rate in units of the Eddington rate.
   viscous_alpha:                    1e6        # Normalisation constant of the Bondi viscuous time-scale accretion reduction term
   radiative_efficiency:             0.1        # Fraction of the accreted mass that gets radiated.
   coupling_efficiency:              0.15       # Fraction of the radiated energy that couples to the gas in feedback events.

examples/EAGLE_ICs/EAGLE_50/eagle_50.yml

@@ -165,7 +165,7 @@ EAGLEFeedback:
 # EAGLE AGN model
 EAGLEAGN:
   subgrid_seed_mass_Msun:           1.5e5      # Black hole subgrid mass at creation time in solar masses.
-  max_eddington_fraction:           1.         # Maximal allowed accretion rate in units of the Eddington rate.
+  max_eddington_fraction:           1.5        # Maximal allowed accretion rate in units of the Eddington rate.
   viscous_alpha:                    1e6        # Normalisation constant of the Bondi viscuous time-scale accretion reduction term
   radiative_efficiency:             0.1        # Fraction of the accreted mass that gets radiated.
   coupling_efficiency:              0.15       # Fraction of the radiated energy that couples to the gas in feedback events.

examples/EAGLE_low_z/EAGLE_12/eagle_12.yml

@@ -156,7 +156,7 @@ EAGLEFeedback:
 # EAGLE AGN model
 EAGLEAGN:
   subgrid_seed_mass_Msun:           1.5e5      # Black hole subgrid mass at creation time in solar masses.
-  max_eddington_fraction:           1.         # Maximal allowed accretion rate in units of the Eddington rate.
+  max_eddington_fraction:           1.5        # Maximal allowed accretion rate in units of the Eddington rate.
   viscous_alpha:                    1e6        # Normalisation constant of the Bondi viscuous time-scale accretion reduction term
   radiative_efficiency:             0.1        # Fraction of the accreted mass that gets radiated.
   coupling_efficiency:              0.15       # Fraction of the radiated energy that couples to the gas in feedback events.

examples/EAGLE_low_z/EAGLE_25/eagle_25.yml

@@ -163,7 +163,7 @@ EAGLEFeedback:
 # EAGLE AGN model
 EAGLEAGN:
   subgrid_seed_mass_Msun:           1.5e5      # Black hole subgrid mass at creation time in solar masses.
-  max_eddington_fraction:           1.         # Maximal allowed accretion rate in units of the Eddington rate.
+  max_eddington_fraction:           1.5        # Maximal allowed accretion rate in units of the Eddington rate.
   viscous_alpha:                    1e6        # Normalisation constant of the Bondi viscuous time-scale accretion reduction term
   radiative_efficiency:             0.1        # Fraction of the accreted mass that gets radiated.
   coupling_efficiency:              0.15       # Fraction of the radiated energy that couples to the gas in feedback events.

examples/EAGLE_low_z/EAGLE_50/eagle_50.yml

@@ -155,7 +155,7 @@ EAGLEFeedback:
 # EAGLE AGN model
 EAGLEAGN:
   subgrid_seed_mass_Msun:           1.5e5      # Black hole subgrid mass at creation time in solar masses.
-  max_eddington_fraction:           1.         # Maximal allowed accretion rate in units of the Eddington rate.
+  max_eddington_fraction:           1.5        # Maximal allowed accretion rate in units of the Eddington rate.
   viscous_alpha:                    1e6        # Normalisation constant of the Bondi viscuous time-scale accretion reduction term
   radiative_efficiency:             0.1        # Fraction of the accreted mass that gets radiated.
   coupling_efficiency:              0.15       # Fraction of the radiated energy that couples to the gas in feedback events.

examples/EAGLE_low_z/EAGLE_6/eagle_6.yml

@@ -165,7 +165,7 @@ EAGLEFeedback:
 # EAGLE AGN model
 EAGLEAGN:
   subgrid_seed_mass_Msun:           1.5e5      # Black hole subgrid mass at creation time in solar masses.
-  max_eddington_fraction:           1.         # Maximal allowed accretion rate in units of the Eddington rate.
+  max_eddington_fraction:           1.5        # Maximal allowed accretion rate in units of the Eddington rate.
   viscous_alpha:                    1e6        # Normalisation constant of the Bondi viscuous time-scale accretion reduction term
   radiative_efficiency:             0.1        # Fraction of the accreted mass that gets radiated.
   coupling_efficiency:              0.15       # Fraction of the radiated energy that couples to the gas in feedback events.

examples/SubgridTests/BlackHoleSwallowing/swallowing.yml

@@ -86,6 +86,7 @@ EAGLECooling:
 EAGLEAGN:
   subgrid_seed_mass_Msun:           1.5e5      # Black hole subgrid mass at creation time in solar masses.
   max_eddington_fraction:           1.         # Maximal allowed accretion rate in units of the Eddington rate.
+  viscous_alpha:                    1e6        # Normalisation constant of the Bondi viscuous time-scale accretion reduction term.
   radiative_efficiency:             0.1        # Fraction of the accreted mass that gets radiated.
   coupling_efficiency:              0.15       # Fraction of the radiated energy that couples to the gas in feedback events.
   AGN_delta_T_K:                    3.16228e8  # Change in temperature to apply to the gas particle in an AGN feedback event in Kelvin.

examples/SubgridTests/BlackHoleSwallowing/swallowing_mpi.yml

@@ -86,6 +86,7 @@ EAGLECooling:
 EAGLEAGN:
   subgrid_seed_mass_Msun:           1.5e5      # Black hole subgrid mass at creation time in solar masses.
   max_eddington_fraction:           1.         # Maximal allowed accretion rate in units of the Eddington rate.
+  viscous_alpha:                    1e6        # Normalisation constant of the Bondi viscuous time-scale accretion reduction term
   radiative_efficiency:             0.1        # Fraction of the accreted mass that gets radiated.
   coupling_efficiency:              0.15       # Fraction of the radiated energy that couples to the gas in feedback events.
   AGN_delta_T_K:                    3.16228e8  # Change in temperature to apply to the gas particle in an AGN feedback event in Kelvin.