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diff --git a/docs/fg21sim.conf.example b/docs/fg21sim.conf.example deleted file mode 100644 index b1f964e..0000000 --- a/docs/fg21sim.conf.example +++ /dev/null @@ -1,333 +0,0 @@ -# Example configuration file for "fg21sim" -# -*- mode: conf -*- -# -# Syntax: `ConfigObj`, https://github.com/DiffSK/configobj -# -# This file contains all the configuration options accepted by "fg21sim", -# which control the simulation parameters, inputs data and outputs products, -# as well as some general behaviors. -# -# Some options already have a default value been set in the bundled -# configuration specifications, which will be further described below with -# their default values and be commented out. -# -# However, there is not a sensible default value for other options, -# therefore, users should explicitly set their values before carrying out -# the simulations.  These options are also explained in details below, and -# marked with "REQUIRED". -# -# NOTE: -# - The input templates for simulations should be HEALPix full-sky maps. -# - The input catalog should be in CSV format. - - -# Common/general configurations for the simulation -[common] -# HEALPix Nside value, i.e., pixel resolution -# NOTE: also update "lmax" below. -#nside = 1024 - -# Range of multipole monents (l) of the angular power spectrum. -# The power spectrum will be cut off to a constant for multipole l < lmin. -# Generally, lmax = 3 * nside - 1 -#lmin = 10 -#lmax = 3071 - -# List of foreground components to be simulated: -# + galactic/synchrotron: -#       Diffuse Galactic synchrotron emission (unpolarized) -# + galactic/freefree: -#       Diffuse Galactic free-free emission -# + galactic/snr: -#       Galactic supernova remnants emission -# + extragalactic/clusters: -#       Extragalactic clusters of galaxies emission -# + extragalactic/pointsources: -#       Emission from multiple types of extragalactic point sources -#       NOTE: This component is not well integrated and tested at the moment -# NOTE: -# If only one component is enabled, do NOT omit the trailing comma "," -# e.g., components = "galaxies/synchrotron", -#components = "galactic/synchrotron", "galactic/freefree", "galactic/snr", "extragalactic/clusters" - - -# Frequencies specification of the simulation products -[frequency] -# Unit of the frequency value -#unit = "MHz" - -# How to specify the frequencies -# + custom: -#       directly specify the frequency values using the "frequencies" config -# + calc: -#       calculate the frequency values by "start", "stop", and "step" -#type = "custom" - -# The frequency values to be simulated if above "type" is "custom". -# [REQUIRED: if "frequency/type" = "custom"] -#frequencies = - -# Parameters to calculate the frequencies -# start and stop frequency value (both inclusive) -# [REQUIRED: if "frequency/type" = "calc"] -#start = -#stop = -#step = - - -# Configuration for output products -[output] -# Unit of the sky map pixel value -#unit = "K" - -# Use single-precision float instead of double (also save spaces) -#use_float = True - -# Filetype used to store the products (default: fits) -#filetype = "fits" - -# Filename pattern (without extension) for the output products, which will -# be finally formatted using `str.format()`. -#filename_pattern = "{prefix}_{frequency:05.1f}" - -# Whether calculate the checksum for the output file (e.g., "CHECKSUM" -# keyword in FITS header)? -# NOTE: -# FITS checksum calculation may account for half the time to output the data. -#checksum = False - -# Whether overwrite existing files -#clobber = False - -# Whether combine all components and output -#combine = True - -# Prefix for the combined files -#combine_prefix = "fg" - -# Output directory to place the combined products -# NOTE: This config is mandatory and should be provided by the user -#       if above "combine=True". -# [REQUIRED: if "output/combine" = True] -#output_dir = - -# Filename of the simulation products manifest (JSON format) -#manifest = "products_manifest.json" - - -# Cosmological parameters -[cosmology] -# Hubble constant at z=0 [ km/s/Mpc ] -#H0 = 71.0 - -# Density of non-relativistic matter in units of the critical density at z=0 -#OmegaM0 = 0.27 - - -# Configurations for initialization/reconfiguration of the `logging` module -[logging] -# DEBUG:    Detailed information, typically of interest only when diagnosing -#           problems. -# INFO:     Confirmation that things are working as expected. -# WARNING:  An dinciation that something unexpected happended, or indicative -#           of some problem in the near future (e.g., "disk space low"). -#           The software is still working as expected. -# ERROR:    Due to a more serious problem, the software has not been able to -#           perform some function. -# CRITICAL: A serious error, indicating that the program itself may be unable -#           to continue running. -#level = "DEBUG" - -# Set the format of displayed messages -#format = "%(asctime)s [%(levelname)s] <%(name)s> %(message)s" - -# Set the date/time format in messages -#datefmt = "%Y-%m-%dT%H:%M:%S" - -# Set the logging filename (will create a `FileHandler`) -# If set to "" (empty string), then the `FileHandler` will be disabled. -#filename = "" - -# Whether append messages to the above logging file instead of overwrite -#appendmode = True - -# Set the stream used to initialize the `StreamHandler` -# If set to "" (empty string), then the `StreamHandler` will be disabled. -#stream = "stderr" - - -# Options corresponding the Galactic emission components, which currently -# includes the following components: -# - synchrotron : Galactic synchrotron emission (unpolarized) -# - freefree : Galactic free-free emission -# - snr : Galactic supernovae remnants -[galactic] - -  # Synchrotron emission component (unpolarized) -  [[synchrotron]] -  # The template map for the simulation. -  # [REQUIRED] -  #template = - -  # The frequency of the template map (same unit as in [frequency] section) -  # [REQUIRED] -  #template_freq = - -  # The unit of the template map pixel -  # [REQUIRED] -  #template_unit = - -  # Spectral index map -  # [REQUIRED] -  #indexmap = - -  # Whether add fluctuations on the small scales -  #add_smallscales = True - -  # Filename prefix for this component -  #prefix = "gsync" - -  # Whether save this component to disk -  #save = True - -  # Output directory to save the simulated results -  # [REQUIRED: if "galactic/synchrotron/save" = True] -  #output_dir = - -  # Free-free bremsstrahlung emission component -  [[freefree]] -  # The H{\alpha} map used as the free-free emission template -  # [REQUIRED] -  #halphamap = - -  # The unit of the H{\alpha} template (e.g., "Rayleigh") -  # [REQUIRED] -  #halphamap_unit = - -  # The 100-{\mu}m dust map used for dust absorption correction -  # [REQUIRED] -  #dustmap = - -  # The unit of the above dust map (e.g., "MJy/sr") -  # [REQUIRED] -  #dustmap_unit = - -  # Filename prefix for this component -  #prefix = "gfree" - -  # Whether save this component to disk -  #save = True - -  # Output directory to save the simulated results -  # [REQUIRED: if "galactic/freefree/save" = True] -  #output_dir = - -  # Supernova remnants emission -  [[snr]] -  # The Galactic SNRs catalog data (CSV file) -  # [REQUIRED] -  #catalog = - -  # Output the effective/inuse SNRs catalog data (CSV file) -  # NOTE: if not specified, then do not save the effective/inuse catalog -  #catalog_outfile = - -  # Resolution (unit: arcmin) for simulating each SNR, which are finally -  # mapped to the HEALPix map of Nside specified in "[common]" section. -  #resolution = 1.0 - -  # Filename prefix for this component -  #prefix = "gsnr" - -  # Whether save this component to disk -  #save = True - -  # Output directory to save the simulated results -  # [REQUIRED: if "galactic/snr/save" = True] -  #output_dir = - - -# Options corresponding the extragalactic emission components, which -# currently includes the following components: -# - clusters : clusters of galaxies -# - pointsources : multiple types of discrete point sources -[extragalactic] - -  # Emissions from the clusters of galaxies -  [[clusters]] -  # The clusters catalog derived from the Hubble Volume Project (CSV file) -  # [REQUIRED] -  #catalog = - -  # Output the effective/inuse clusters catalog data (CSV file) -  # NOTE: if not specified, then do not save the effective/inuse catalog -  #catalog_outfile = - -  # The fraction that a cluster hosts a radio halo -  # [REQUIRED] -  #halo_fraction = - -  # Resolution (unit: arcmin) for simulating each cluster, which are finally -  # mapped to the HEALPix map of Nside specified in "[common]" section. -  #resolution = 0.5 - -  # Filename prefix for this component -  #prefix = "egcluster" - -  # Whether save this component to disk -  #save = True - -  # Output directory to save the simulated results -  # [REQUIRED: if "extragalactic/clusters/save" = True] -  #output_dir = - -  # Extragalactic point sources -  [[pointsources]] -  # Whether save this point source catelogue to disk -  #save = True - -  # Output directory to save the simulated catelogues -  #output_dir = "PS_tables" - -  # PS components to be simulated -  # [REQUIRED] -  #pscomponents = - -  # Resolution [arcmin] -  #resolution = 0.6 - -    # Star forming -    [[[starforming]]] -    # Number of samples -    #numps = 1000 - -    # Prefix -    #prefix = "SF" - -    [[[starbursting]]] -    # Number of samples -    #numps = 1000 - -    # Prefix -    #prefix = "SB" - -    [[[radioquiet]]] -    # Number of samples -    #numps = 1000 - -    # Prefix -    #prefix = "RQ" - -    [[[FRI]]] -    # Number of samples -    #numps = 1000 - -    # Prefix -    #prefix = "FRI" - -    [[[FRII]]] -    # Number of samples -    #numps = 1000 - -    # Prefix -    #prefix = "FRII"  | 
