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authorAaron LI <aly@aaronly.me>2018-07-10 11:47:48 +0800
committerAaron LI <aly@aaronly.me>2018-07-10 11:47:48 +0800
commit9cf46ee6ced07282a7c51baedf3aabd938676f98 (patch)
tree31ac446399c1c69c793be10162c9269d3109cc19 /docs/fg21sim.conf.example
parent88d1d4151a093facf32a33b52d6b687686989666 (diff)
downloadfg21sim-9cf46ee6ced07282a7c51baedf3aabd938676f98.tar.bz2
docs: Replace the outdated config example with the current specification
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-# 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"