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Table 1.
Parameters involved in the code.
Parameter | Type | Default value | Description |
---|---|---|---|
Administrative parameters | |||
silent | Boolean | False | Allows MINOT to provide information when running |
output_dir | String | “./minot_output” | Full path to the output directory for products saving |
Global physical properties | |||
cosmo | Cosmology (a) | Planck15 | Cosmological model |
name | String | “Cluster” | Name of the cluster |
coord | SkyCoord (b) | [0, 0] deg | Coordinates of the cluster center |
redshift | Float | 0.01 | redshift of the cluster |
D_ang | Quantity (c) | (⋆) | Angular diameter distance |
D_lum | Quantity (c) | (⋆) | Luminosity distance |
M500 | Quantity (c) | 1015 M⊙ | Characteristic cluster mass |
R500 | Quantity (c) | (⋆) | Characteristic cluster physical radius |
theta500 | Quantity (c) | (⋆) | Characteristic cluster angular radius |
R_truncation | Quantity (c) | 3 × R500 | Physical extent (boundary) of the cluster |
theta_truncation | Quantity (c) | 3 × θ500 | Angular extent (boundary) of the cluster |
helium_mass_fraction | Float | 0.2735 | Helium mass fraction |
metallicity_sol | Float | 0.0153 | Reference metallically of the Sun |
abundance | Float | 0.3 | The metal abundance relative to the solar value |
EBL_model | String | “dominguez” | Name of the extragalactic background light model |
hse_bias | Float | 0.2 | Hydrostatic mass bias |
Epmin | Quantity (c) | ∼1.22 GeV | Minimal energy of the CRp |
Epmax | Quantity (c) | 10 PeV | Maximal energy of the CRp |
Eemin | Quantity (c) | mec2 | Minimal energy of the CRe1 |
Eemax | Quantity (c) | 10 PeV | Maximal energy of the CRe1 |
pp_interaction_model | String | “Pythia8” | Name of the proton-proton interaction model |
cre1_loss_model | String | “None” | Loss model to apply to the input primary CRe distribution |
Radial and spectral modeling | |||
pressure_gas_model | Dict | P13UPP (d) | Model to be used for the thermal gas pressure profile |
density_gas_model | Dict | ![]() |
Model to be used for the thermal gas number density profile |
magfield_model | Dict | ![]() |
Model to be used for the magnetic field profile |
X_crp_E | Dict | 1% within R500 | CRp to thermal energy ratio and reference radius |
X_cre1_E | Dict | 1% within R500 | CRe1 to thermal energy ratio and reference radius |
density_crp_model | Dict | ∝Pe(r) | Model to be used for the CRp number density profile |
density_cre1_model | Dict | ∝Pe(r) | Model to be used for CRe1 number density profile |
spectrum_crp_model | Dict | Index 2.5 power law | Model to be used for the CRp spectrum |
spectrum_cre1_model | Dict | Index 3.0 power law | Model to be used for CRe1 spectrum |
Sampling parameters | |||
Rmin | Quantity (c) | 1 kpc | Minimum radius used for log integration |
Npt_per_decade_integ | Int | 30 | Number of points per decade |
map_coord | SkyCoord (b) | [0, 0] deg | Coordinates of the map center |
map_reso | Quantity (c) | 0.01 deg | Map resolution (pixel size) |
map_fov | Quantity (c) list | [5, 5] deg | Map field-of-view size along RA and Dec |
map_header | String | None | Header of the map |
Notes.
(d)
Universal pressure profile based on mass and redshift, from Planck Collaboration V (2013).
(⋆)Quantities that are computed from other parameters.
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