diff --git a/doc/RTD/source/SubgridModels/AGNSpinJets/params.rst b/doc/RTD/source/SubgridModels/AGNSpinJets/params.rst
index 1fda66ccbf660bb2ccda898a9fd897f017f28233..a4ac82e8de3e71c8dbc9d98c247a5ead87cd3cd3 100644
--- a/doc/RTD/source/SubgridModels/AGNSpinJets/params.rst
+++ b/doc/RTD/source/SubgridModels/AGNSpinJets/params.rst
@@ -69,7 +69,7 @@ Below we give an example of parameter choices applicable for e.g. a 50 Mpc box.
fix_jet_efficiency: 0 # Global switch whether to fix jet efficiency to a particular value [1], or use a spin-dependant formula [0]. If used, jets will be launched exclusively along the z axis. Should be set to 1 only for tests.
jet_efficiency: 0.1 # The constant jet efficiency used if 'fix_jet_efficiency' is set to 1.
fix_jet_direction: 0 # Global switch whether to fix the jet direction to be along the z-axis, instead of along the spin vector.
- accretion_efficiency: 1. # The accretion efficiency (suppression factor of the accretion rate) to use in the thick disc (ADAF), to represent the effects of subgrid winds that take away most of the mass flowing through the accretion disc.
+ accretion_efficiency: 0.1 # The accretion efficiency (suppression factor of the accretion rate) to use in the thick disc (ADAF), to represent the effects of subgrid winds that take away most of the mass flowing through the accretion disc.
fix_radiative_efficiency: 0 # Global switch whether to fix the radiative efficiency to a particular value [1], or use a spin-dependant formula [0].
radiative_efficiency: 0.1 # The constant jet efficiency used if 'fix_radiative_efficiency' is set to 1. Otherwise, this value is used to define the Eddington accretion rate.
TD_region: B # How to treat the subgrid accretion disk if it is thin, according to the Shakura & Sunyaev (1973) model. If set to B, region b will be used. If set to C, region c will be used.
@@ -78,7 +78,7 @@ Below we give an example of parameter choices applicable for e.g. a 50 Mpc box.
turn_off_secondary_feedback: 1 # If set to 1, there will be only radiative (thermal) feedback in the thin disk mode, and only jets in the thick disk mode.
jet_h_r_slope: 1. # The slope of the dependence of jet efficiency on aspect ratio of the subgrid accretion disk, H/R. Default value is 1, and another reasonable value is 0 (same jet efficiency for all disks). Reality could be anything in between. This parameter is only used if turn_off_secondary_feedback is set to 0.
delta_ADAF: 0.2 # Electron heating parameter, which controls the strength of radiative feedback in thick disks. Should be between 0.1 and 0.5. This parameter is only used if turn_off_secondary_feedback is set to 0.
- include_slim_disk: 1 # Global switch whether to include super-Eddington accretion, modeled as the slim disk. If set to 0, disks will be considered thin even at very large accretion rates.
+ include_slim_disk: 0 # Global switch whether to include super-Eddington accretion, modeled as the slim disk. If set to 0, disks will be considered thin even at very large accretion rates.
Most of these parameters should work well generally, and should not be changed except for tests. We will discuss only some of the more important ones. You can choose whether to have only the thick and thin disk (low and high BH accretion rates, respectively), or you can also include the slim disk at super-Eddington rates with ``include_slim_disk``. You can control what type of feedback you (do not) want with ``include_jets`` and ``turn_off_radiative_feedback``. If you choose to turn off jets, everything will be modeled as a thin disk (regardless of accretion rate), since jets go hand-in-hand with the thick and the slim disk. Similarly, if you turn off radiation, everything will be treated as a thick disk.
diff --git a/examples/IdealisedCluster/IdealisedCluster_M13/idealised_cluster_M13.yml b/examples/IdealisedCluster/IdealisedCluster_M13/idealised_cluster_M13.yml
index 2a195a5737402af5babb2c00f4f980cb8acabde0..e94b56a79e262b0836224f3ec7251185d09b60e7 100644
--- a/examples/IdealisedCluster/IdealisedCluster_M13/idealised_cluster_M13.yml
+++ b/examples/IdealisedCluster/IdealisedCluster_M13/idealised_cluster_M13.yml
@@ -299,4 +299,6 @@ SPINJETAGN:
turn_off_secondary_feedback: 1 # Whether to turn off radiative feedback at very low accretion rates and jets at moderate accretion rates.
fix_jet_direction: 1 # Whether to fix the jet direction to be along the z-axis.
fix_radiative_efficiency: 0 # Whether to fix the radiative efficiency to a constant value.
- include_GRMHD_spindown: 0 # Use GRMHD simulation-derived formulas for spindown of BHs, or an analytical formula.
\ No newline at end of file
+ include_GRMHD_spindown: 0 # Use GRMHD simulation-derived formulas for spindown of BHs, or an analytical formula.
+ accretion_efficiency: 1. # The accretion efficiency (suppression factor of the accretion rate) to use in the thick disc (ADAF), to represent the effects of subgrid winds that take away most of the mass flowing through the accretion disc.
+
diff --git a/examples/IdealisedCluster/IdealisedCluster_M135/idealised_cluster_M135.yml b/examples/IdealisedCluster/IdealisedCluster_M135/idealised_cluster_M135.yml
index 5a6f29eaf0e04ef0ba3ecbb43871207ce327b4cf..ff3fbff68c733a702641229ed99717da452232dd 100644
--- a/examples/IdealisedCluster/IdealisedCluster_M135/idealised_cluster_M135.yml
+++ b/examples/IdealisedCluster/IdealisedCluster_M135/idealised_cluster_M135.yml
@@ -300,3 +300,5 @@ SPINJETAGN:
fix_jet_direction: 1 # Whether to fix the jet direction to be along the z-axis.
fix_radiative_efficiency: 0 # Whether to fix the radiative efficiency to a constant value.
include_GRMHD_spindown: 0 # Use GRMHD simulation-derived formulas for spindown of BHs, or an analytical formula.
+ accretion_efficiency: 1. # The accretion efficiency (suppression factor of the accretion rate) to use in the thick disc (ADAF), to represent the effects of subgrid winds that take away most of the mass flowing through the accretion disc.
+
diff --git a/examples/IdealisedCluster/IdealisedCluster_M14/idealised_cluster_M14.yml b/examples/IdealisedCluster/IdealisedCluster_M14/idealised_cluster_M14.yml
index 07fb7247338b34d9656cd0417883ab227ae50cee..fd8534d25f42e8bbdf34d7abc4b0b08069c6fe1d 100644
--- a/examples/IdealisedCluster/IdealisedCluster_M14/idealised_cluster_M14.yml
+++ b/examples/IdealisedCluster/IdealisedCluster_M14/idealised_cluster_M14.yml
@@ -300,3 +300,4 @@ SPINJETAGN:
fix_jet_direction: 1 # Whether to fix the jet direction to be along the z-axis.
fix_radiative_efficiency: 0 # Whether to fix the radiative efficiency to a constant value.
include_GRMHD_spindown: 0 # Use GRMHD simulation-derived formulas for spindown of BHs, or an analytical formula.
+ accretion_efficiency: 1. # The accretion efficiency (suppression factor of the accretion rate) to use in the thick disc (ADAF), to represent the effects of subgrid winds that take away most of the mass flowing through the accretion disc.
diff --git a/examples/IdealisedCluster/IdealisedCluster_M15/idealised_cluster_M15.yml b/examples/IdealisedCluster/IdealisedCluster_M15/idealised_cluster_M15.yml
index 71dbf91abb66f2fecd039314d7671a17b16d7cfe..edb92fa35b9507484c5b2e4bf9de34d190fbe7b8 100644
--- a/examples/IdealisedCluster/IdealisedCluster_M15/idealised_cluster_M15.yml
+++ b/examples/IdealisedCluster/IdealisedCluster_M15/idealised_cluster_M15.yml
@@ -299,4 +299,5 @@ SPINJETAGN:
turn_off_secondary_feedback: 1 # Whether to turn off radiative feedback at very low accretion rates and jets at moderate accretion rates.
fix_jet_direction: 1 # Whether to fix the jet direction to be along the z-axis.
fix_radiative_efficiency: 0 # Whether to fix the radiative efficiency to a constant value.
- include_GRMHD_spindown: 0 # Use GRMHD simulation-derived formulas for spindown of BHs, or an analytical formula.
\ No newline at end of file
+ include_GRMHD_spindown: 0 # Use GRMHD simulation-derived formulas for spindown of BHs, or an analytical formula.
+ accretion_efficiency: 1. # The accretion efficiency (suppression factor of the accretion rate) to use in the thick disc (ADAF), to represent the effects of subgrid winds that take away most of the mass flowing through the accretion disc.
diff --git a/examples/parameter_example.yml b/examples/parameter_example.yml
index 06f73b8e2b94176ad2c5a669af5f06705b9f89a4..6c07371a47d7b0b15113e80b602ba5e197661bec 100644
--- a/examples/parameter_example.yml
+++ b/examples/parameter_example.yml
@@ -807,7 +807,7 @@ SPINJETAGN:
fix_jet_efficiency: 0 # Global switch whether to fix jet efficiency to a particular value [1], or use a spin-dependant formula [0].
jet_efficiency: 0.1 # The constant jet efficiency used if 'fix_jet_efficiency' is set to 1.
fix_jet_direction: 0 # Global switch whether to fix the jet direction to be along the z-axis, instead of along the spin vector.
- accretion_efficiency: 1. # The accretion efficiency (suppression factor of the accretion rate) to use in the thick disc (ADAF), to represent the effects of subgrid winds that take away most of the mass flowing through the accretion disc.
+ accretion_efficiency: 0.1 # The accretion efficiency (suppression factor of the accretion rate) to use in the thick disc (ADAF), to represent the effects of subgrid winds that take away most of the mass flowing through the accretion disc.
fix_radiative_efficiency: 0 # Global switch whether to fix the radiative efficiency to a particular value [1], or use a spin-dependant formula [0].
radiative_efficiency: 0.1 # The constant jet efficiency used if 'fix_radiative_efficiency' is set to 1. Otherwise, this value is used to define the Eddington accretion rate.
TD_region: B # How to treat the subgrid accretion disk if it is thin, according to the Shakura & Sunyaev (1973) model. If set to B, region b will be used. If set to C, region c will be used.
@@ -815,7 +815,7 @@ SPINJETAGN:
turn_off_secondary_feedback: 1 # If set to 1, there will be only radiative (thermal) feedback in the thin disk mode, and only jets in the thick disk mode.
jet_h_r_slope: 1. # The slope of the dependence of jet efficiency on aspect ratio of the subgrid accretion disk, H/R. Default value is 1, and another reasonable value is 0 (same jet efficiency for all disks). Reality could be anything in between. This parameter is only used if turn_off_secondary_feedback is set to 0.
delta_ADAF: 0.2 # Electron heating parameter, which controls the strength of radiative feedback in thick disks. Should be between 0.1 and 0.5. This parameter is only used if turn_off_secondary_feedback is set to 0.
- include_slim_disk: 1 # Global switch whether to include super-Eddington accretion, modeled as the slim disk. If set to 0, disks will be considered thin even at very large accretion rates.
+ include_slim_disk: 0 # Global switch whether to include super-Eddington accretion, modeled as the slim disk. If set to 0, disks will be considered thin even at very large accretion rates.
# Parameters related to the neutrinos --------------------------------------------