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authorAaron LI <aly@aaronly.me>2018-10-30 19:59:07 +0800
committerAaron LI <aly@aaronly.me>2018-10-30 19:59:07 +0800
commit86aaceba1a64255bf3ce46b6d2ea98615e6b21af (patch)
tree026140d10092edd97492d2fefa37a9253cee89a8 /fg21sim/configs
parent25f19ca897ccce5eb0cd7a8bc84e143d3e5a0feb (diff)
downloadfg21sim-86aaceba1a64255bf3ce46b6d2ea98615e6b21af.tar.bz2
configs: Merge config specs into one single file
Diffstat (limited to 'fg21sim/configs')
-rw-r--r--fg21sim/configs/00-general.conf.spec151
-rw-r--r--fg21sim/configs/10-galactic.conf.spec89
-rw-r--r--fg21sim/configs/config.spec (renamed from fg21sim/configs/20-extragalactic.conf.spec)238
-rw-r--r--fg21sim/configs/manager.py19
4 files changed, 234 insertions, 263 deletions
diff --git a/fg21sim/configs/00-general.conf.spec b/fg21sim/configs/00-general.conf.spec
deleted file mode 100644
index 353e2cf..0000000
--- a/fg21sim/configs/00-general.conf.spec
+++ /dev/null
@@ -1,151 +0,0 @@
-# Configurations for "fg21sim"
-# -*- mode: conf -*-
-#
-# Syntax: `ConfigObj`, https://github.com/DiffSK/configobj
-#
-# This file contains the general configurations, which control the general
-# behaviors, or will be used in other configuration sections.
-
-
-# Foreground components to be simulated
-[foregrounds]
-# Diffuse Galactic synchrotron emission (unpolarized)
-galactic/synchrotron = boolean(default=False)
-
-# Diffuse Galactic free-free emission
-galactic/freefree = boolean(default=False)
-
-# Galactic supernova remnants emission
-galactic/snr = boolean(default=False)
-
-# Extragalactic clusters of galaxies emission
-extragalactic/clusters = boolean(default=False)
-
-# Emission from multiple types of extragalactic point sources
-# NOTE: This component is not well integrated and tested at the moment
-extragalactic/pointsources = boolean(default=False)
-
-
-# Simulation sky/region configurations
-[sky]
-# Type of the input/output simulation sky
-# + patch:
-# Input/output sky template is only a (square) patch of the sky.
-# The simulated output maps have the same coverage/field as the
-# input template, as well as the coordinate projection.
-# + healpix:
-# Input/output sky template covers (almost) all sky, and stored
-# in HEALPix format. The simulated output maps will also be
-# all-sky using the HEALPix projection.
-type = option("patch", "healpix", default="patch")
-
- # Configurations for input/output sky patch
- [[patch]]
- # The (R.A., Dec.) coordinate of the sky patch center
- # Unit: [deg]
- # (MWA EoR0 field center: (0, -27))
- xcenter = float(default=0.0, min=0.0, max=360.0)
- ycenter = float(default=-27.0, min=-90.0, max=90.0)
-
- # The image dimensions (i.e., number of pixels) of the sky patch,
- # along the X (R.A./longitude) and Y (Dec./latitude) axes.
- # Default: 1800x1800 => 10x10 [deg^2] (20 arcsec/pixel)
- xsize = integer(default=1800, min=1)
- ysize = integer(default=1800, min=1)
-
- # Pixel size [arcsec]
- pixelsize = float(default=20.0, min=0.0)
-
- # Configurations for input/output HEALPix sky
- [[healpix]]
- # HEALPix Nside value, i.e., pixel resolution
- nside = integer(default=1024, min=128)
-
-
-# Frequencies specification of the simulation products
-[frequency]
-# 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 = option("custom", "calc", default="custom")
-
-# The frequency values to be simulated if above "type" is "custom".
-# Unit: [MHz]
-frequencies = float_list(default=list())
-
-# Parameters to calculate the frequencies
-# NOTE: "start" and "stop" frequencies are both inclusive.
-# Unit: [MHz]
-start = float(default=None, min=0.0)
-stop = float(default=None, min=0.0)
-step = float(default=None, min=0.0)
-
-
-# Configuration for output products
-[output]
-# Filename pattern for the output products, which will be finally
-# formatted using `str.format()`.
-filename_pattern = string(default="{prefix}_{frequency:06.2f}.fits")
-
-# Use single-precision float instead of double (to save spaces)
-float32 = boolean(default=True)
-
-# Whether to calculate the checksum for the output FITS file?
-# NOTE: May cost significantly more time on writing FITS file.
-checksum = boolean(default=False)
-
-# Whether to overwrite existing files (e.g., maps, catalogs, manifest, ...)
-clobber = boolean(default=False)
-
-# Filename of the simulation products manifest (JSON format), which
-# records all output products together with their sizes and MD5 hashes.
-# Do not create such a manifest if this option is not specified.
-manifest = string(default=None)
-
-
-# Cosmological parameters
-# References: Komatsu et al. 2011, ApJS, 192, 18; Tab.(1)
-[cosmology]
-# Hubble constant at z=0; [km/s/Mpc]
-H0 = float(default=71.0, min=0.0)
-# Density of non-relativistic matter in units of the critical density at z=0
-OmegaM0 = float(default=0.27, min=0.0, max=1.0)
-# Density of the baryon at present day
-Omegab0 = float(default=0.046, min=0.0, max=1.0)
-# Present-day CMB temperature; [K]
-Tcmb0 = float(default=2.725)
-# Present-day rms density fluctuations on a scale of 8 h^-1 [Mpc]
-sigma8 = float(default=0.81, min=0.0)
-# Scalar spectral index
-ns = float(default=0.96, min=0.0)
-
-
-# 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 indication 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 = option("debug", "info", "warning", "error", "critical", default="info")
-
-# Set the format of displayed messages
-format = string(default="%(asctime)s [%(levelname)s] <%(name)s:%(lineno)d> %(message)s")
-
-# Set the date/time format in messages
-datefmt = string(default="%H:%M:%S")
-
-# Set the logging filename (will create a `FileHandler`)
-# If set to "" (empty string), then the `FileHandler` will be disabled.
-filename = string(default="")
-
-# Set the stream used to initialize the `StreamHandler`
-# If set to "" (empty string), then the `StreamHandler` will be disabled.
-stream = option("stderr", "stdout", "", default="stderr")
diff --git a/fg21sim/configs/10-galactic.conf.spec b/fg21sim/configs/10-galactic.conf.spec
deleted file mode 100644
index 9185dc0..0000000
--- a/fg21sim/configs/10-galactic.conf.spec
+++ /dev/null
@@ -1,89 +0,0 @@
-# Configurations for "fg21sim"
-# -*- mode: conf -*-
-#
-# Syntax: `ConfigObj`, https://github.com/DiffSK/configobj
-#
-# This file contains the options corresponding the Galactic emission
-# components, which currently includes the following components:
-# - synchrotron
-# - freefree
-# - snr
-
-
-[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=0.0)
-
- # Spectral index map
- indexmap = string(default=None)
-
- # Whether add fluctuations on the small scales according the angular
- # power spectrum prediction?
- add_smallscales = boolean(default=False)
- # Range of multipole moments (l) of the angular power spectrum.
- # The power spectrum will be cut off to a constant for multipole l < lmin.
- # NOTE: Update the ``lmax`` accordingly w.r.t. ``sky/healpix/nside``.
- # Generally, lmax = 3 * nside - 1
- lmin = integer(min=0, default=10)
- lmax = integer(min=1, default=3071)
-
- # Filename prefix for this component
- prefix = string(default="gsync")
- # 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]
- halphamap = string(default=None)
-
- # The 100-μm dust map used to correct Hα dust absorption
- # Unit: [MJy/sr]
- dustmap = string(default=None)
-
- # Effective dust fraction in the LoS actually absorbing Halpha
- dust_fraction = float(default=0.33, min=0.1, max=1.0)
-
- # Halpha absorption threshold:
- # When the dust absorption goes rather large, the true Halpha
- # absorption can not well determined. This configuration sets the
- # threshold below which the dust absorption can be well determined,
- # while the sky regions with higher absorption are masked out due
- # to unreliable absorption correction.
- # Unit: [mag]
- halpha_abs_th = float(default=1.0)
-
- # The electron temperature assumed for the ionized interstellar medium
- # that generating H{\alpha} emission.
- # Unit: [K]
- electron_temperature = float(default=7000.0, min=1000)
-
- # 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)
- # Output the effective/inuse SNRs catalog data (CSV file)
- catalog_outfile = string(default=None)
-
- # Resolution for simulating each SNR template, which are finally
- # mapped to the all-sky HEALPix map if used.
- # Unit: [arcsec]
- resolution = float(default=30.0, min=5.0)
-
- # Filename prefix for this component
- prefix = string(default="gsnr")
- # Output directory to save the simulated results
- output_dir = string(default=None)
diff --git a/fg21sim/configs/20-extragalactic.conf.spec b/fg21sim/configs/config.spec
index 943c7e0..6b871e4 100644
--- a/fg21sim/configs/20-extragalactic.conf.spec
+++ b/fg21sim/configs/config.spec
@@ -1,14 +1,240 @@
-# Configurations for "fg21sim"
-# -*- mode: conf -*-
#
+# Configurations for "fg21sim"
# Syntax: `ConfigObj`, https://github.com/DiffSK/configobj
#
-# This file contains the options corresponding the extragalactic emission
-# components, which currently includes the following components:
-# - clusters: halos
-# - pointsources
+# Foreground components to be simulated
+[foregrounds]
+# Diffuse Galactic synchrotron emission (unpolarized)
+galactic/synchrotron = boolean(default=False)
+
+# Diffuse Galactic free-free emission
+galactic/freefree = boolean(default=False)
+
+# Galactic supernova remnants emission
+galactic/snr = boolean(default=False)
+
+# Extragalactic clusters of galaxies emission
+extragalactic/clusters = boolean(default=False)
+
+# Emission from multiple types of extragalactic point sources
+# NOTE: This component is not well integrated and tested at the moment
+extragalactic/pointsources = boolean(default=False)
+
+
+# Simulation sky/region configurations
+[sky]
+# Type of the input/output simulation sky
+# + patch:
+# Input/output sky template is only a (square) patch of the sky.
+# The simulated output maps have the same coverage/field as the
+# input template, as well as the coordinate projection.
+# + healpix:
+# Input/output sky template covers (almost) all sky, and stored
+# in HEALPix format. The simulated output maps will also be
+# all-sky using the HEALPix projection.
+type = option("patch", "healpix", default="patch")
+
+ # Configurations for input/output sky patch
+ [[patch]]
+ # The (R.A., Dec.) coordinate of the sky patch center
+ # Unit: [deg]
+ # (MWA EoR0 field center: (0, -27))
+ xcenter = float(default=0.0, min=0.0, max=360.0)
+ ycenter = float(default=-27.0, min=-90.0, max=90.0)
+
+ # The image dimensions (i.e., number of pixels) of the sky patch,
+ # along the X (R.A./longitude) and Y (Dec./latitude) axes.
+ # Default: 1800x1800 => 10x10 [deg^2] (20 arcsec/pixel)
+ xsize = integer(default=1800, min=1)
+ ysize = integer(default=1800, min=1)
+
+ # Pixel size [arcsec]
+ pixelsize = float(default=20.0, min=0.0)
+
+ # Configurations for input/output HEALPix sky
+ [[healpix]]
+ # HEALPix Nside value, i.e., pixel resolution
+ nside = integer(default=1024, min=128)
+
+
+# Frequencies specification of the simulation products
+[frequency]
+# 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 = option("custom", "calc", default="custom")
+
+# The frequency values to be simulated if above "type" is "custom".
+# Unit: [MHz]
+frequencies = float_list(default=list())
+
+# Parameters to calculate the frequencies
+# NOTE: "start" and "stop" frequencies are both inclusive.
+# Unit: [MHz]
+start = float(default=None, min=0.0)
+stop = float(default=None, min=0.0)
+step = float(default=None, min=0.0)
+
+
+# Configuration for output products
+[output]
+# Filename pattern for the output products, which will be finally
+# formatted using `str.format()`.
+filename_pattern = string(default="{prefix}_{frequency:06.2f}.fits")
+
+# Use single-precision float instead of double (to save spaces)
+float32 = boolean(default=True)
+
+# Whether to calculate the checksum for the output FITS file?
+# NOTE: May cost significantly more time on writing FITS file.
+checksum = boolean(default=False)
+
+# Whether to overwrite existing files (e.g., maps, catalogs, manifest, ...)
+clobber = boolean(default=False)
+
+# Filename of the simulation products manifest (JSON format), which
+# records all output products together with their sizes and MD5 hashes.
+# Do not create such a manifest if this option is not specified.
+manifest = string(default=None)
+
+
+# Cosmological parameters
+# References: Komatsu et al. 2011, ApJS, 192, 18; Tab.(1)
+[cosmology]
+# Hubble constant at z=0; [km/s/Mpc]
+H0 = float(default=71.0, min=0.0)
+# Density of non-relativistic matter in units of the critical density at z=0
+OmegaM0 = float(default=0.27, min=0.0, max=1.0)
+# Density of the baryon at present day
+Omegab0 = float(default=0.046, min=0.0, max=1.0)
+# Present-day CMB temperature; [K]
+Tcmb0 = float(default=2.725)
+# Present-day rms density fluctuations on a scale of 8 h^-1 [Mpc]
+sigma8 = float(default=0.81, min=0.0)
+# Scalar spectral index
+ns = float(default=0.96, min=0.0)
+
+
+# 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 indication 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 = option("debug", "info", "warning", "error", "critical", default="info")
+
+# Set the format of displayed messages
+format = string(default="%(asctime)s [%(levelname)s] <%(name)s:%(lineno)d> %(message)s")
+
+# Set the date/time format in messages
+datefmt = string(default="%H:%M:%S")
+
+# Set the logging filename (will create a `FileHandler`)
+# If set to "" (empty string), then the `FileHandler` will be disabled.
+filename = string(default="")
+
+# Set the stream used to initialize the `StreamHandler`
+# If set to "" (empty string), then the `StreamHandler` will be disabled.
+stream = option("stderr", "stdout", "", default="stderr")
+
+
+#
+# Galactic emission components
+#
+
+[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=0.0)
+
+ # Spectral index map
+ indexmap = string(default=None)
+
+ # Whether add fluctuations on the small scales according the angular
+ # power spectrum prediction?
+ add_smallscales = boolean(default=False)
+ # Range of multipole moments (l) of the angular power spectrum.
+ # The power spectrum will be cut off to a constant for multipole l < lmin.
+ # NOTE: Update the ``lmax`` accordingly w.r.t. ``sky/healpix/nside``.
+ # Generally, lmax = 3 * nside - 1
+ lmin = integer(min=0, default=10)
+ lmax = integer(min=1, default=3071)
+
+ # Filename prefix for this component
+ prefix = string(default="gsync")
+ # 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]
+ halphamap = string(default=None)
+
+ # The 100-μm dust map used to correct Hα dust absorption
+ # Unit: [MJy/sr]
+ dustmap = string(default=None)
+
+ # Effective dust fraction in the LoS actually absorbing Halpha
+ dust_fraction = float(default=0.33, min=0.1, max=1.0)
+
+ # Halpha absorption threshold:
+ # When the dust absorption goes rather large, the true Halpha
+ # absorption can not well determined. This configuration sets the
+ # threshold below which the dust absorption can be well determined,
+ # while the sky regions with higher absorption are masked out due
+ # to unreliable absorption correction.
+ # Unit: [mag]
+ halpha_abs_th = float(default=1.0)
+
+ # The electron temperature assumed for the ionized interstellar medium
+ # that generating H{\alpha} emission.
+ # Unit: [K]
+ electron_temperature = float(default=7000.0, min=1000)
+
+ # 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)
+ # Output the effective/inuse SNRs catalog data (CSV file)
+ catalog_outfile = string(default=None)
+
+ # Resolution for simulating each SNR template, which are finally
+ # mapped to the all-sky HEALPix map if used.
+ # Unit: [arcsec]
+ resolution = float(default=30.0, min=5.0)
+
+ # Filename prefix for this component
+ prefix = string(default="gsnr")
+ # Output directory to save the simulated results
+ output_dir = string(default=None)
+
+
+#
+# Extragalactic emission components
+#
+
[extragalactic]
#
# Press-Schechter formalism to determine the cluster distributions
diff --git a/fg21sim/configs/manager.py b/fg21sim/configs/manager.py
index e2103da..07f6f77 100644
--- a/fg21sim/configs/manager.py
+++ b/fg21sim/configs/manager.py
@@ -31,22 +31,6 @@ from ..errors import ConfigError
logger = logging.getLogger(__name__)
-def _get_configspec():
- """Found and read all the configuration specifications"""
- files = sorted(pkg_resources.resource_listdir(__name__, ""))
- specfiles = [fn for fn in files if fn.endswith(".conf.spec")]
- if os.environ.get("DEBUG_FG21SIM"):
- print("DEBUG: Found config specifications: %s" % ", ".join(specfiles),
- file=sys.stderr)
- # NOTE:
- # `resource_string()` returns the resource in *binary/bytes* string
- configspec = "\n".join([
- pkg_resources.resource_string(__name__, fn).decode("utf-8")
- for fn in specfiles
- ]).split("\n")
- return configspec
-
-
def _flatten_dict(d, sep="/", parent_key=""):
"""
Recursively flatten a nested dictionary with keys compressed.
@@ -147,7 +131,8 @@ class ConfigManager:
If the ``userconfig`` provided, the user configurations is also
loaded, validated, and merged.
"""
- configspec = _get_configspec()
+ configspec = pkg_resources.resource_string(
+ __name__, "config.spec").decode("utf-8")
self._configspec = ConfigObj(configspec, interpolation=False,
list_values=False, _inspec=True,
encoding="utf-8")