SAGE26 Parameter Reference
This document is the canonical reference for every parameter accepted by SAGE26
parameter files (input/*.par). Parameter files are parsed by
src/core_read_parameter_file.c.
Syntax: ParameterName value % optional comment
Lines beginning with % are comments. Required parameters must be present;
optional parameters take the listed default if omitted.
Output
Parameter |
Type |
Required |
Default |
Description |
|---|---|---|---|---|
|
string |
yes |
— |
Base name for output files (e.g. |
|
string |
yes |
— |
Directory for galaxy output. Created if absent. |
|
string |
no |
|
|
|
int |
no |
|
Number of snapshot outputs; |
|
0/1 |
no |
|
Store per-snapshot SFR history arrays ( |
|
0/1 |
no |
|
Record satellite disruption contributions to ICS ( |
Simulation
Parameter |
Type |
Required |
Default |
Description |
|---|---|---|---|---|
|
string |
yes |
— |
Merger tree format: |
|
string |
yes |
— |
Tree file basename (files are named |
|
string |
yes |
— |
Directory containing tree files. |
|
string |
yes |
— |
File listing snapshot scale factors, one per line. |
|
int |
yes |
— |
First tree file index to process. |
|
int |
yes |
— |
Last tree file index to process (inclusive). |
|
int |
yes |
— |
Total number of tree files (may differ from FirstFile–LastFile range). |
|
int |
yes |
— |
Index of the final snapshot in the tree files. |
|
double |
yes |
— |
Matter density parameter Ω_m. |
|
double |
yes |
— |
Dark energy density parameter Ω_Λ. |
|
double |
yes |
— |
Universal baryon fraction f_b = Ω_b / Ω_m. |
|
double |
yes |
— |
Dimensionless Hubble parameter h (H₀ = 100 h km/s/Mpc). |
|
double |
yes |
— |
N-body particle mass in 10¹⁰ M_sun/h. |
|
double |
yes |
— |
Simulation box side length in Mpc/h. |
Units
Parameter |
Type |
Required |
Default |
Description |
|---|---|---|---|---|
|
double |
yes |
— |
1 internal length unit in cm. Typically |
|
double |
yes |
— |
1 internal mass unit in g. Typically |
|
double |
yes |
— |
1 internal velocity unit in cm/s. Typically |
Physics switches
Parameter |
Type |
No |
Default |
Values and meaning |
|---|---|---|---|---|
|
int |
no |
|
Star formation prescription: 0=Croton+06; 1=Blitz & Rosolowsky 06 H₂; 2=Somerville+25 SFR; 3=Somerville+25 SFR+H₂; 4=Krumholz & Dekel 12; 5=KMT 09; 6=Krumholz 13; 7=Gnedin & Draine 14. |
|
int |
no |
|
AGN feedback: 0=off; 1=empirical; 2=Bondi-Hoyle; 3=cold cloud accretion. |
|
0/1 |
no |
|
SN feedback: 0=off; 1=Croton+16 reheating/ejection. |
|
0/1 |
no |
|
Reionization suppression of infall: 0=off; 1=Kravtsov+04 analytic fit. |
|
0/1 |
no |
|
Disk instability: 0=off; 1=Toomre criterion drives bulge and BH growth. |
|
0/1 |
no |
|
Two-regime CGM model: 0=off (classical C16 cooling only); 1=on. |
|
0/1 |
no |
|
FIRE stellar feedback: 0=off; 1=on. |
|
int |
no |
|
Feedback-free burst galaxies: 0=off; 1=Li+24 sigmoid; 2=BK25 (Ishiyama+21 c); 3=BK25 (ConcentrationOn method); 4=BK25 + log-normal c scatter; 5=Li+24 sharp; 6=Li+24 sigmoid + H₂ SF; 7=BK25 log-normal c scatter + H₂ SF. |
|
int |
no |
|
Halo concentration method: 0=off; 1=Ishiyama+21 table; 2=V_max/V_vir; 3=V_max/V_vir with infall freeze for satellites. |
|
int |
no |
|
Bulge radius model: 0=off; 1=Shen+2003 eq.33; 2=Shen+2003 eq.32; 3=Tonini+2016 (separate merger and instability channels, mass-weighted average). |
|
0/1 |
no |
|
Include cold gas contribution during merger starbursts. |
|
int |
no |
|
ICS-vs-BCG split for disrupted satellite stellar mass: 0=fixed fraction |
CGM model parameters
Parameter |
Type |
Required |
Default |
Description |
|---|---|---|---|---|
|
int |
no |
|
CGM gas density profile for precipitation: 0=uniform; 1=NFW; 2=beta (β=2/3). |
|
0/1 |
no |
|
Enable AGN heating coupling to the CGM-regime cooling path. |
FFB parameters
Parameter |
Type |
Required |
Default |
Description |
|---|---|---|---|---|
|
double |
no |
|
Maximum star formation efficiency during FFB bursts. |
|
double |
no |
|
Log-normal scatter in halo concentration used by |
|
0/1 |
no |
|
Apply FFB criterion regardless of CGM regime classification. |
|
0/1 |
no |
|
Use random number scatter in FFB threshold instead of deterministic sigmoid. |
|
double |
no |
|
Redshift exponent in the FFB mass threshold scaling (Li+24 eq. 2). |
H₂ star formation parameters
Parameter |
Type |
Required |
Default |
Description |
|---|---|---|---|---|
|
int |
no |
|
Disk area for H₂ surface density: 1=π r_disk²; 2=π (3 r_disk)²; 3=2π r_disk². |
|
0/1 |
no |
|
Use radial ring integration for H₂ fraction (more accurate, slower). |
|
int |
no |
|
Number of radial bins for the ring integration. |
|
double |
no |
|
Outer integration radius as a multiple of the disk scale radius. |
Model parameters
Star formation
Parameter |
Units |
Default |
Description |
|---|---|---|---|
|
dimensionless |
|
Cold/H2 gas consumption efficiency per dynamical time. Used by SFprescription 0, 1, 4, 5, 7 unconditionally, and by 6 (K13) only in the single-slab path ( |
|
dimensionless |
|
Fraction of stellar mass instantaneously recycled to cold gas. |
|
dimensionless |
|
Fraction of stellar mass returned as metals. |
|
dimensionless |
|
Fraction of newly produced metals transferred directly to hot gas. |
Supernova feedback
Parameter |
Units |
Default |
Description |
|---|---|---|---|
|
dimensionless |
|
Mass of cold gas reheated per unit of stellar mass formed (Martin 1999). |
|
dimensionless |
|
Fraction of SN energy deposited into hot gas for ejection. |
|
erg |
|
Energy per supernova event. |
|
M_sun⁻¹ |
|
Number of supernovae per solar mass of stars formed. |
AGN feedback
Parameter |
Units |
Default |
Description |
|---|---|---|---|
|
dimensionless |
|
AGN radio-mode heating efficiency (AGNrecipeOn=2). |
|
dimensionless |
|
AGN quasar-mode wind heating efficiency (AGNrecipeOn > 0). |
|
dimensionless |
|
Fraction of cold gas accreted onto the BH during mergers (AGNrecipeOn > 0). |
Mergers
Parameter |
Units |
Default |
Description |
|---|---|---|---|
|
dimensionless |
|
Mass ratio above which a merger is classified as major. |
|
dimensionless |
|
M_vir-to-baryonic mass ratio below which a satellite is disrupted rather than merged. |
|
dimensionless |
|
Fixed fraction of disrupted satellite stellar mass that goes to ICS (vs. central BCG). Used when |
|
dimensionless |
|
Power-law exponent for the mass-dependent disruption split. |
|
dimensionless |
|
Reference concentration for the disruption split. |
Gas cycling
Parameter |
Units |
Default |
Description |
|---|---|---|---|
|
dimensionless |
|
Fraction of ejected mass reincorporated per dynamical time. |
Reionization
Parameter |
— |
Default |
Description |
|---|---|---|---|
|
— |
|
Characteristic redshift for reionization suppression (Kravtsov+04). |
|
— |
|
Width parameter for reionization suppression. |
See the FFB parameters section above for FFBMaxEfficiency,
FFBConcSigma, and RedshiftPowerLawExponent.
MPI forest distribution
Parameter |
Type |
Required |
Default |
Description |
|---|---|---|---|---|
|
string |
no |
|
How forests are distributed over MPI tasks: |
|
double |
no |
|
Exponent for |