diff --git a/examples/EAGLE_ICs/EAGLE_100/vrconfig_3dfof_subhalos_SO_hydro.cfg b/examples/EAGLE_ICs/EAGLE_100/vrconfig_3dfof_subhalos_SO_hydro.cfg index bb01aeed3acd0fc104aaf19472e99d3bef6d671d..84bd67c0e83c805edd391fd2fa9d1353fc55fb1f 100644 --- a/examples/EAGLE_ICs/EAGLE_100/vrconfig_3dfof_subhalos_SO_hydro.cfg +++ b/examples/EAGLE_ICs/EAGLE_100/vrconfig_3dfof_subhalos_SO_hydro.cfg @@ -16,6 +16,7 @@ Input_includes_wind_particle=0 #include wind particles in hydro input (used by I Input_includes_tracer_particle=0 #include tracer particles in hydro input (used by Illustris). Here shown as example Input_includes_extradm_particle=0 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Particle_type_for_reference_frames=1 #use DM particles to define reference frame Halo_core_phase_merge_dist=0.25 #merge substructures if difference in dispersion normalised distance is < this value Apply_phase_merge_to_host=1 #merge substructures with background if centrally located and phase-distance is small diff --git a/examples/EAGLE_ICs/EAGLE_12/vrconfig_3dfof_subhalos_SO_hydro.cfg b/examples/EAGLE_ICs/EAGLE_12/vrconfig_3dfof_subhalos_SO_hydro.cfg index bb01aeed3acd0fc104aaf19472e99d3bef6d671d..84bd67c0e83c805edd391fd2fa9d1353fc55fb1f 100644 --- a/examples/EAGLE_ICs/EAGLE_12/vrconfig_3dfof_subhalos_SO_hydro.cfg +++ b/examples/EAGLE_ICs/EAGLE_12/vrconfig_3dfof_subhalos_SO_hydro.cfg @@ -16,6 +16,7 @@ Input_includes_wind_particle=0 #include wind particles in hydro input (used by I Input_includes_tracer_particle=0 #include tracer particles in hydro input (used by Illustris). Here shown as example Input_includes_extradm_particle=0 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Particle_type_for_reference_frames=1 #use DM particles to define reference frame Halo_core_phase_merge_dist=0.25 #merge substructures if difference in dispersion normalised distance is < this value Apply_phase_merge_to_host=1 #merge substructures with background if centrally located and phase-distance is small diff --git a/examples/EAGLE_ICs/EAGLE_25/vrconfig_3dfof_subhalos_SO_hydro.cfg b/examples/EAGLE_ICs/EAGLE_25/vrconfig_3dfof_subhalos_SO_hydro.cfg index bb01aeed3acd0fc104aaf19472e99d3bef6d671d..84bd67c0e83c805edd391fd2fa9d1353fc55fb1f 100644 --- a/examples/EAGLE_ICs/EAGLE_25/vrconfig_3dfof_subhalos_SO_hydro.cfg +++ b/examples/EAGLE_ICs/EAGLE_25/vrconfig_3dfof_subhalos_SO_hydro.cfg @@ -16,6 +16,7 @@ Input_includes_wind_particle=0 #include wind particles in hydro input (used by I Input_includes_tracer_particle=0 #include tracer particles in hydro input (used by Illustris). Here shown as example Input_includes_extradm_particle=0 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Particle_type_for_reference_frames=1 #use DM particles to define reference frame Halo_core_phase_merge_dist=0.25 #merge substructures if difference in dispersion normalised distance is < this value Apply_phase_merge_to_host=1 #merge substructures with background if centrally located and phase-distance is small diff --git a/examples/EAGLE_ICs/EAGLE_50/vrconfig_3dfof_subhalos_SO_hydro.cfg b/examples/EAGLE_ICs/EAGLE_50/vrconfig_3dfof_subhalos_SO_hydro.cfg index bb01aeed3acd0fc104aaf19472e99d3bef6d671d..84bd67c0e83c805edd391fd2fa9d1353fc55fb1f 100644 --- a/examples/EAGLE_ICs/EAGLE_50/vrconfig_3dfof_subhalos_SO_hydro.cfg +++ b/examples/EAGLE_ICs/EAGLE_50/vrconfig_3dfof_subhalos_SO_hydro.cfg @@ -16,6 +16,7 @@ Input_includes_wind_particle=0 #include wind particles in hydro input (used by I Input_includes_tracer_particle=0 #include tracer particles in hydro input (used by Illustris). Here shown as example Input_includes_extradm_particle=0 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Particle_type_for_reference_frames=1 #use DM particles to define reference frame Halo_core_phase_merge_dist=0.25 #merge substructures if difference in dispersion normalised distance is < this value Apply_phase_merge_to_host=1 #merge substructures with background if centrally located and phase-distance is small diff --git a/examples/EAGLE_ICs/EAGLE_50_low_res/vrconfig_3dfof_subhalos_SO_hydro.cfg b/examples/EAGLE_ICs/EAGLE_50_low_res/vrconfig_3dfof_subhalos_SO_hydro.cfg index ad342fa599468bf459df22f9ba145209db476170..84bd67c0e83c805edd391fd2fa9d1353fc55fb1f 100644 --- a/examples/EAGLE_ICs/EAGLE_50_low_res/vrconfig_3dfof_subhalos_SO_hydro.cfg +++ b/examples/EAGLE_ICs/EAGLE_50_low_res/vrconfig_3dfof_subhalos_SO_hydro.cfg @@ -1,5 +1,5 @@ #Configuration file for analysing Hydro -#runs 3DFOF + substructure algorithm, demands subhalos and FOF halos be self-bound, calculates many properties +#runs 6DFOF + substructure algorithm, demands subhalos and FOF halos be self-bound, calculates many properties #Units currently set to take in as input, Mpc, 1e10 solar masses, km/s, output in same units #To set temporally unique halo ids, alter Snapshot_value=SNAP to appropriate value. Ie: for snapshot 12, change SNAP to 12 @@ -16,6 +16,7 @@ Input_includes_wind_particle=0 #include wind particles in hydro input (used by I Input_includes_tracer_particle=0 #include tracer particles in hydro input (used by Illustris). Here shown as example Input_includes_extradm_particle=0 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Particle_type_for_reference_frames=1 #use DM particles to define reference frame Halo_core_phase_merge_dist=0.25 #merge substructures if difference in dispersion normalised distance is < this value Apply_phase_merge_to_host=1 #merge substructures with background if centrally located and phase-distance is small @@ -26,6 +27,7 @@ Mass_input_unit_conversion_to_output_unit=1.0 #default mass unit, #assumes input is in 1e10 msun, Mpc and km/s and output units are the same Gravity=43.0211349 #for 1e10 Msun, km/s and Mpc Hubble_unit=100.0 # assuming units are km/s and Mpc, then value of Hubble in km/s/Mpc + #converting hydro quantities Stellar_age_input_is_cosmological_scalefactor=1 Metallicity_input_unit_conversion_to_output_unit=1.0 @@ -39,8 +41,8 @@ Length_unit_to_kpc=1000.0 Velocity_to_kms=1.0 #conversion of output mass units to solar masses Mass_to_solarmass=1.0e10 -#1 / 0.012 -Metallicity_to_solarmetallicity=83.33 + +Metallicity_to_solarmetallicity=83.33 #1 / 0.012 Star_formation_rate_to_solarmassperyear=97.78 Stellar_age_to_yr=1.0 #ensures that output is physical and not comoving distances per little h @@ -112,7 +114,7 @@ Halo_core_num_loops=8 #number of loops to iteratively search for cores Halo_core_loop_ellx_fac=0.75 #how much to change the configuration space linking per iteration Halo_core_loop_ellv_fac=1.0 #how much to change the velocity space linking per iteration Halo_core_loop_elln_fac=1.2 #how much to change the min number of particles per iteration -Halo_core_phase_significance=2.0 #how significant a core must be in terms of dispersions (sigma) significance +Halo_core_phase_significance=5.0 #how significant a core must be in terms of dispersions (sigma) significance ################################ #Unbinding options (VELOCIraptor is able to accurately identify tidal debris so particles need not be bound to a structure) @@ -134,6 +136,7 @@ Frac_pot_ref=1.0 Min_npot_ref=20 #reference frame only meaningful if calculating velocity frame using subset of particles in object. Can use radially sorted fraction of particles about minimum potential or centre of mass Kinetic_reference_frame_type=0 +#extra options in new unbinding optimisation Unbinding_max_unbound_removal_fraction_per_iteration=0.5 Unbinding_max_unbound_fraction=0.95 Unbinding_max_unbound_fraction_allowed=0.005 @@ -203,6 +206,4 @@ Snapshot_value=SNAP ################################ #other options ################################ -Verbose=0 #how talkative do you want the code to be, 0 not much, 1 a lot, 2 chatterbox - - +Verbose=1 #how talkative do you want the code to be, 0 not much, 1 a lot, 2 chatterbox diff --git a/examples/EAGLE_ICs/EAGLE_6/vrconfig_3dfof_subhalos_SO_hydro.cfg b/examples/EAGLE_ICs/EAGLE_6/vrconfig_3dfof_subhalos_SO_hydro.cfg index bb01aeed3acd0fc104aaf19472e99d3bef6d671d..84bd67c0e83c805edd391fd2fa9d1353fc55fb1f 100644 --- a/examples/EAGLE_ICs/EAGLE_6/vrconfig_3dfof_subhalos_SO_hydro.cfg +++ b/examples/EAGLE_ICs/EAGLE_6/vrconfig_3dfof_subhalos_SO_hydro.cfg @@ -16,6 +16,7 @@ Input_includes_wind_particle=0 #include wind particles in hydro input (used by I Input_includes_tracer_particle=0 #include tracer particles in hydro input (used by Illustris). Here shown as example Input_includes_extradm_particle=0 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Particle_type_for_reference_frames=1 #use DM particles to define reference frame Halo_core_phase_merge_dist=0.25 #merge substructures if difference in dispersion normalised distance is < this value Apply_phase_merge_to_host=1 #merge substructures with background if centrally located and phase-distance is small diff --git a/examples/SmallCosmoVolume/SmallCosmoVolume_VELOCIraptor/vrconfig_3dfof_subhalos_SO_hydro.cfg b/examples/SmallCosmoVolume/SmallCosmoVolume_VELOCIraptor/vrconfig_3dfof_subhalos_SO_hydro.cfg index 8590cbf5bc77e8d7a956d210339cced4bbdc692c..5198c63de5f469ec8bf6e857940ced30b3214cfd 100644 --- a/examples/SmallCosmoVolume/SmallCosmoVolume_VELOCIraptor/vrconfig_3dfof_subhalos_SO_hydro.cfg +++ b/examples/SmallCosmoVolume/SmallCosmoVolume_VELOCIraptor/vrconfig_3dfof_subhalos_SO_hydro.cfg @@ -1,5 +1,5 @@ #Configuration file for analysing Hydro -#runs 3DFOF + substructure algorithm, demands subhalos and FOF halos be self-bound, calculates many properties +#runs 6DFOF + substructure algorithm, demands subhalos and FOF halos be self-bound, calculates many properties #Units currently set to take in as input, Mpc, 1e10 solar masses, km/s, output in same units #To set temporally unique halo ids, alter Snapshot_value=SNAP to appropriate value. Ie: for snapshot 12, change SNAP to 12 @@ -10,12 +10,13 @@ HDF_name_convention=6 #HDF SWIFT naming convention Input_includes_dm_particle=1 #include dark matter particles in hydro input Input_includes_gas_particle=1 #include gas particles in hydro input -Input_includes_star_particle=1 #include star particles in hydro input -Input_includes_bh_particle=1 #include bh particles in hydro input +Input_includes_star_particle=0 #include star particles in hydro input +Input_includes_bh_particle=0 #include bh particles in hydro input Input_includes_wind_particle=0 #include wind particles in hydro input (used by Illustris and moves particle type 0 to particle type 3 when decoupled from hydro forces). Here shown as example Input_includes_tracer_particle=0 #include tracer particles in hydro input (used by Illustris). Here shown as example Input_includes_extradm_particle=0 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Particle_type_for_reference_frames=1 #use DM particles to define reference frame Halo_core_phase_merge_dist=0.25 #merge substructures if difference in dispersion normalised distance is < this value Apply_phase_merge_to_host=1 #merge substructures with background if centrally located and phase-distance is small @@ -26,6 +27,7 @@ Mass_input_unit_conversion_to_output_unit=1.0 #default mass unit, #assumes input is in 1e10 msun, Mpc and km/s and output units are the same Gravity=43.0211349 #for 1e10 Msun, km/s and Mpc Hubble_unit=100.0 # assuming units are km/s and Mpc, then value of Hubble in km/s/Mpc + #converting hydro quantities Stellar_age_input_is_cosmological_scalefactor=1 Metallicity_input_unit_conversion_to_output_unit=1.0 @@ -39,8 +41,8 @@ Length_unit_to_kpc=1000.0 Velocity_to_kms=1.0 #conversion of output mass units to solar masses Mass_to_solarmass=1.0e10 -#1 / 0.012 -Metallicity_to_solarmetallicity=83.33 + +Metallicity_to_solarmetallicity=83.33 #1 / 0.012 Star_formation_rate_to_solarmassperyear=97.78 Stellar_age_to_yr=1.0 #ensures that output is physical and not comoving distances per little h @@ -112,7 +114,7 @@ Halo_core_num_loops=8 #number of loops to iteratively search for cores Halo_core_loop_ellx_fac=0.75 #how much to change the configuration space linking per iteration Halo_core_loop_ellv_fac=1.0 #how much to change the velocity space linking per iteration Halo_core_loop_elln_fac=1.2 #how much to change the min number of particles per iteration -Halo_core_phase_significance=2.0 #how significant a core must be in terms of dispersions (sigma) significance +Halo_core_phase_significance=5.0 #how significant a core must be in terms of dispersions (sigma) significance ################################ #Unbinding options (VELOCIraptor is able to accurately identify tidal debris so particles need not be bound to a structure) @@ -134,6 +136,7 @@ Frac_pot_ref=1.0 Min_npot_ref=20 #reference frame only meaningful if calculating velocity frame using subset of particles in object. Can use radially sorted fraction of particles about minimum potential or centre of mass Kinetic_reference_frame_type=0 +#extra options in new unbinding optimisation Unbinding_max_unbound_removal_fraction_per_iteration=0.5 Unbinding_max_unbound_fraction=0.95 Unbinding_max_unbound_fraction_allowed=0.005 @@ -186,6 +189,4 @@ Snapshot_value=SNAP ################################ #other options ################################ -Verbose=0 #how talkative do you want the code to be, 0 not much, 1 a lot, 2 chatterbox - - +Verbose=1 #how talkative do you want the code to be, 0 not much, 1 a lot, 2 chatterbox diff --git a/examples/SmallCosmoVolume/SmallCosmoVolume_hydro/vrconfig_3dfof_subhalos_SO_hydro.cfg b/examples/SmallCosmoVolume/SmallCosmoVolume_hydro/vrconfig_3dfof_subhalos_SO_hydro.cfg index 8590cbf5bc77e8d7a956d210339cced4bbdc692c..5198c63de5f469ec8bf6e857940ced30b3214cfd 100644 --- a/examples/SmallCosmoVolume/SmallCosmoVolume_hydro/vrconfig_3dfof_subhalos_SO_hydro.cfg +++ b/examples/SmallCosmoVolume/SmallCosmoVolume_hydro/vrconfig_3dfof_subhalos_SO_hydro.cfg @@ -1,5 +1,5 @@ #Configuration file for analysing Hydro -#runs 3DFOF + substructure algorithm, demands subhalos and FOF halos be self-bound, calculates many properties +#runs 6DFOF + substructure algorithm, demands subhalos and FOF halos be self-bound, calculates many properties #Units currently set to take in as input, Mpc, 1e10 solar masses, km/s, output in same units #To set temporally unique halo ids, alter Snapshot_value=SNAP to appropriate value. Ie: for snapshot 12, change SNAP to 12 @@ -10,12 +10,13 @@ HDF_name_convention=6 #HDF SWIFT naming convention Input_includes_dm_particle=1 #include dark matter particles in hydro input Input_includes_gas_particle=1 #include gas particles in hydro input -Input_includes_star_particle=1 #include star particles in hydro input -Input_includes_bh_particle=1 #include bh particles in hydro input +Input_includes_star_particle=0 #include star particles in hydro input +Input_includes_bh_particle=0 #include bh particles in hydro input Input_includes_wind_particle=0 #include wind particles in hydro input (used by Illustris and moves particle type 0 to particle type 3 when decoupled from hydro forces). Here shown as example Input_includes_tracer_particle=0 #include tracer particles in hydro input (used by Illustris). Here shown as example Input_includes_extradm_particle=0 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Particle_type_for_reference_frames=1 #use DM particles to define reference frame Halo_core_phase_merge_dist=0.25 #merge substructures if difference in dispersion normalised distance is < this value Apply_phase_merge_to_host=1 #merge substructures with background if centrally located and phase-distance is small @@ -26,6 +27,7 @@ Mass_input_unit_conversion_to_output_unit=1.0 #default mass unit, #assumes input is in 1e10 msun, Mpc and km/s and output units are the same Gravity=43.0211349 #for 1e10 Msun, km/s and Mpc Hubble_unit=100.0 # assuming units are km/s and Mpc, then value of Hubble in km/s/Mpc + #converting hydro quantities Stellar_age_input_is_cosmological_scalefactor=1 Metallicity_input_unit_conversion_to_output_unit=1.0 @@ -39,8 +41,8 @@ Length_unit_to_kpc=1000.0 Velocity_to_kms=1.0 #conversion of output mass units to solar masses Mass_to_solarmass=1.0e10 -#1 / 0.012 -Metallicity_to_solarmetallicity=83.33 + +Metallicity_to_solarmetallicity=83.33 #1 / 0.012 Star_formation_rate_to_solarmassperyear=97.78 Stellar_age_to_yr=1.0 #ensures that output is physical and not comoving distances per little h @@ -112,7 +114,7 @@ Halo_core_num_loops=8 #number of loops to iteratively search for cores Halo_core_loop_ellx_fac=0.75 #how much to change the configuration space linking per iteration Halo_core_loop_ellv_fac=1.0 #how much to change the velocity space linking per iteration Halo_core_loop_elln_fac=1.2 #how much to change the min number of particles per iteration -Halo_core_phase_significance=2.0 #how significant a core must be in terms of dispersions (sigma) significance +Halo_core_phase_significance=5.0 #how significant a core must be in terms of dispersions (sigma) significance ################################ #Unbinding options (VELOCIraptor is able to accurately identify tidal debris so particles need not be bound to a structure) @@ -134,6 +136,7 @@ Frac_pot_ref=1.0 Min_npot_ref=20 #reference frame only meaningful if calculating velocity frame using subset of particles in object. Can use radially sorted fraction of particles about minimum potential or centre of mass Kinetic_reference_frame_type=0 +#extra options in new unbinding optimisation Unbinding_max_unbound_removal_fraction_per_iteration=0.5 Unbinding_max_unbound_fraction=0.95 Unbinding_max_unbound_fraction_allowed=0.005 @@ -186,6 +189,4 @@ Snapshot_value=SNAP ################################ #other options ################################ -Verbose=0 #how talkative do you want the code to be, 0 not much, 1 a lot, 2 chatterbox - - +Verbose=1 #how talkative do you want the code to be, 0 not much, 1 a lot, 2 chatterbox diff --git a/examples/nIFTyCluster/Baryonic/vrconfig_swift.cfg b/examples/nIFTyCluster/Baryonic/vrconfig_swift.cfg index 92b8d2f8f2c82a79215ac2ee6cbd00db121a08e3..5198c63de5f469ec8bf6e857940ced30b3214cfd 100644 --- a/examples/nIFTyCluster/Baryonic/vrconfig_swift.cfg +++ b/examples/nIFTyCluster/Baryonic/vrconfig_swift.cfg @@ -1,8 +1,7 @@ #Configuration file for analysing Hydro -#runs 3DFOF + substructure algorithm, demands subhalos and FOF halos be self-bound, calculates many properties +#runs 6DFOF + substructure algorithm, demands subhalos and FOF halos be self-bound, calculates many properties #Units currently set to take in as input, Mpc, 1e10 solar masses, km/s, output in same units #To set temporally unique halo ids, alter Snapshot_value=SNAP to appropriate value. Ie: for snapshot 12, change SNAP to 12 -# This is the same as the configuration file used in the EAGLE examples. ################################ #input options @@ -15,8 +14,9 @@ Input_includes_star_particle=0 #include star particles in hydro input Input_includes_bh_particle=0 #include bh particles in hydro input Input_includes_wind_particle=0 #include wind particles in hydro input (used by Illustris and moves particle type 0 to particle type 3 when decoupled from hydro forces). Here shown as example Input_includes_tracer_particle=0 #include tracer particles in hydro input (used by Illustris). Here shown as example -Input_includes_extradm_particle=1 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Input_includes_extradm_particle=0 #include extra dm particles stored in particle type 2 and type 3, useful for zooms +Particle_type_for_reference_frames=1 #use DM particles to define reference frame Halo_core_phase_merge_dist=0.25 #merge substructures if difference in dispersion normalised distance is < this value Apply_phase_merge_to_host=1 #merge substructures with background if centrally located and phase-distance is small @@ -27,6 +27,7 @@ Mass_input_unit_conversion_to_output_unit=1.0 #default mass unit, #assumes input is in 1e10 msun, Mpc and km/s and output units are the same Gravity=43.0211349 #for 1e10 Msun, km/s and Mpc Hubble_unit=100.0 # assuming units are km/s and Mpc, then value of Hubble in km/s/Mpc + #converting hydro quantities Stellar_age_input_is_cosmological_scalefactor=1 Metallicity_input_unit_conversion_to_output_unit=1.0 @@ -40,8 +41,9 @@ Length_unit_to_kpc=1000.0 Velocity_to_kms=1.0 #conversion of output mass units to solar masses Mass_to_solarmass=1.0e10 -Metallicity_to_solarmetallicity=1.0 -Star_formation_rate_to_solarmassperyear=1.0 + +Metallicity_to_solarmetallicity=83.33 #1 / 0.012 +Star_formation_rate_to_solarmassperyear=97.78 Stellar_age_to_yr=1.0 #ensures that output is physical and not comoving distances per little h Comoving_units=0 @@ -112,7 +114,7 @@ Halo_core_num_loops=8 #number of loops to iteratively search for cores Halo_core_loop_ellx_fac=0.75 #how much to change the configuration space linking per iteration Halo_core_loop_ellv_fac=1.0 #how much to change the velocity space linking per iteration Halo_core_loop_elln_fac=1.2 #how much to change the min number of particles per iteration -Halo_core_phase_significance=2.0 #how significant a core must be in terms of dispersions (sigma) significance +Halo_core_phase_significance=5.0 #how significant a core must be in terms of dispersions (sigma) significance ################################ #Unbinding options (VELOCIraptor is able to accurately identify tidal debris so particles need not be bound to a structure) @@ -134,6 +136,7 @@ Frac_pot_ref=1.0 Min_npot_ref=20 #reference frame only meaningful if calculating velocity frame using subset of particles in object. Can use radially sorted fraction of particles about minimum potential or centre of mass Kinetic_reference_frame_type=0 +#extra options in new unbinding optimisation Unbinding_max_unbound_removal_fraction_per_iteration=0.5 Unbinding_max_unbound_fraction=0.95 Unbinding_max_unbound_fraction_allowed=0.005 @@ -186,6 +189,4 @@ Snapshot_value=SNAP ################################ #other options ################################ -Verbose=0 #how talkative do you want the code to be, 0 not much, 1 a lot, 2 chatterbox - - +Verbose=1 #how talkative do you want the code to be, 0 not much, 1 a lot, 2 chatterbox