Use a better value (the default one) for the gas fraction assumed by the EAGLE...

Use a better value (the default one) for the gas fraction assumed by the EAGLE SF model in the EAGLE low-z examples.

examples/EAGLE_low_z/EAGLE_12/eagle_12.yml

@@ -27,7 +27,7 @@ Snapshots:
   basename:            eagle # Common part of the name of output files
   scale_factor_first:  0.91  # Scale-factor of the first snaphot (cosmological run)
   time_first:          0.01  # Time of the first output (non-cosmological run) (in internal units)
-  delta_time:          1.01  # Time difference between consecutive outputs (in internal units)
+  delta_time:          1.002  # Time difference between consecutive outputs (in internal units)
   compression:         1
 
 # Parameters governing the conserved quantities statistics
@@ -83,7 +83,6 @@ EAGLEStarFormation:
   EOS_density_norm_H_p_cm3:          0.1       # Physical density used for the normalisation of the EOS assumed for the star-forming gas in Hydrogen atoms per cm^3.
   EOS_temperature_norm_K:            8000      # Temperature om the polytropic EOS assumed for star-forming gas at the density normalisation in Kelvin.
   EOS_gamma_effective:               1.3333333 # Slope the of the polytropic EOS assumed for the star-forming gas.
-  gas_fraction:                      0.3       # The gas fraction used internally by the model.
   KS_normalisation:                  1.515e-4  # The normalization of the Kennicutt-Schmidt law in Msun / kpc^2 / yr.
   KS_exponent:                       1.4       # The exponent of the Kennicutt-Schmidt law.
   KS_min_over_density:               57.7      # The over-density above which star-formation is allowed.

examples/EAGLE_low_z/EAGLE_25/eagle_25.yml

@@ -90,7 +90,6 @@ EAGLEStarFormation:
   EOS_density_norm_H_p_cm3:          0.1       # Physical density used for the normalisation of the EOS assumed for the star-forming gas in Hydrogen atoms per cm^3.
   EOS_temperature_norm_K:            8000      # Temperature om the polytropic EOS assumed for star-forming gas at the density normalisation in Kelvin.
   EOS_gamma_effective:               1.3333333 # Slope the of the polytropic EOS assumed for the star-forming gas.
-  gas_fraction:                      0.3       # The gas fraction used internally by the model.
   KS_normalisation:                  1.515e-4  # The normalization of the Kennicutt-Schmidt law in Msun / kpc^2 / yr.
   KS_exponent:                       1.4       # The exponent of the Kennicutt-Schmidt law.
   KS_min_over_density:               57.7      # The over-density above which star-formation is allowed.

examples/EAGLE_low_z/EAGLE_50/eagle_50.yml

@@ -85,7 +85,6 @@ EAGLEStarFormation:
   EOS_density_norm_H_p_cm3:          0.1       # Physical density used for the normalisation of the EOS assumed for the star-forming gas in Hydrogen atoms per cm^3.
   EOS_temperature_norm_K:            8000      # Temperature om the polytropic EOS assumed for star-forming gas at the density normalisation in Kelvin.
   EOS_gamma_effective:               1.3333333 # Slope the of the polytropic EOS assumed for the star-forming gas.
-  gas_fraction:                      0.3       # The gas fraction used internally by the model.
   KS_normalisation:                  1.515e-4  # The normalization of the Kennicutt-Schmidt law in Msun / kpc^2 / yr.
   KS_exponent:                       1.4       # The exponent of the Kennicutt-Schmidt law.
   KS_min_over_density:               57.7      # The over-density above which star-formation is allowed.

examples/EAGLE_low_z/EAGLE_6/eagle_6.yml

@@ -94,7 +94,6 @@ EAGLEStarFormation:
   EOS_density_norm_H_p_cm3:          0.1       # Physical density used for the normalisation of the EOS assumed for the star-forming gas in Hydrogen atoms per cm^3.
   EOS_temperature_norm_K:            8000      # Temperature om the polytropic EOS assumed for star-forming gas at the density normalisation in Kelvin.
   EOS_gamma_effective:               1.3333333 # Slope the of the polytropic EOS assumed for the star-forming gas.
-  gas_fraction:                      0.3       # The gas fraction used internally by the model.
   KS_normalisation:                  1.515e-4  # The normalization of the Kennicutt-Schmidt law in Msun / kpc^2 / yr.
   KS_exponent:                       1.4       # The exponent of the Kennicutt-Schmidt law.
   KS_min_over_density:               57.7      # The over-density above which star-formation is allowed.