diff options
Diffstat (limited to 'fg21sim')
| -rw-r--r-- | fg21sim/configs/config.spec | 22 |
1 files changed, 15 insertions, 7 deletions
diff --git a/fg21sim/configs/config.spec b/fg21sim/configs/config.spec index 9a466d1..5d13bed 100644 --- a/fg21sim/configs/config.spec +++ b/fg21sim/configs/config.spec @@ -147,14 +147,16 @@ stream = option("stderr", "stdout", "", default="stderr") [galactic] + # # Synchrotron emission component (unpolarized) + # [[synchrotron]] # The template map for the simulation, e.g., Haslam 408 MHz survey. # Unit: [K] (Kelvin) template = string(default=None) # The frequency of the template map. # Unit: [MHz] - template_freq = float(default=None, min=0) + template_freq = float(default=None) # Spectral index map indexmap = string(default=None) @@ -174,7 +176,10 @@ stream = option("stderr", "stdout", "", default="stderr") # Output directory to save the simulated results output_dir = string(default=None) + + # # Free-free bremsstrahlung emission component + # [[freefree]] # The Hα map from which to derive the free-free emission # Unit: [Rayleigh] @@ -185,7 +190,7 @@ stream = option("stderr", "stdout", "", default="stderr") dustmap = string(default=None) # Effective dust fraction in the LoS actually absorbing Halpha - dust_fraction = float(default=0.33, min=0.1, max=1) + dust_fraction = float(default=0.33, min=0, max=1) # Halpha absorption threshold: # When the dust absorption goes rather large, the true Halpha @@ -199,14 +204,17 @@ stream = option("stderr", "stdout", "", default="stderr") # The electron temperature assumed for the ionized interstellar medium # that generating Hα emission. # Unit: [K] - electron_temperature = float(default=7000, min=1000) + electron_temperature = float(default=7000) # Filename prefix for this component prefix = string(default="gfree") # Output directory to save the simulated results output_dir = string(default=None) + + # # Supernova remnants emission + # [[snr]] # The Galactic SNRs catalog data (CSV file) catalog = string(default=None) @@ -216,7 +224,7 @@ stream = option("stderr", "stdout", "", default="stderr") # Resolution for simulating each SNR template, which are finally # mapped to the all-sky HEALPix map if used. # Unit: [arcsec] - resolution = float(default=30, min=5) + resolution = float(default=30) # Filename prefix for this component prefix = string(default="gsnr") @@ -269,7 +277,7 @@ stream = option("stderr", "stdout", "", default="stderr") # Shape: (len(z), len(mass)) # Differential mass function in terms of natural log of M. # Unit: [Mpc^-3] (the little "h" is folded into the values) - dndlnm_outfile = string(default=None) + dndlnm_outfile = string(default="dndlnm.npz") # @@ -280,7 +288,7 @@ stream = option("stderr", "stdout", "", default="stderr") [[clusters]] # Output CSV file of the cluster catalog containing the simulated # mass, redshift, position, shape, recent merger info, etc. - catalog_outfile = string(default=None) + catalog_outfile = string(default="cluster.catalog.csv") # Whether to dump the raw data of the simulated cluster catalog in # Python native pickle format (i.e., ".pkl") to a file with the same @@ -306,7 +314,7 @@ stream = option("stderr", "stdout", "", default="stderr") # Output CSV file of the halos catalog containing the calculated # properties of the simulated halos. - halos_catalog_outfile = string(default=None) + halos_catalog_outfile = string(default="cluster.halos.csv") # Whether to dump the whole data of the simulated halos in Python # native pickle format (i.e., ".pkl") to a file with the same basename |