From 86aaceba1a64255bf3ce46b6d2ea98615e6b21af Mon Sep 17 00:00:00 2001
From: Aaron LI <aly@aaronly.me>
Date: Tue, 30 Oct 2018 19:59:07 +0800
Subject: configs: Merge config specs into one single file

---
 fg21sim/configs/10-galactic.conf.spec | 89 -----------------------------------
 1 file changed, 89 deletions(-)
 delete mode 100644 fg21sim/configs/10-galactic.conf.spec

(limited to 'fg21sim/configs/10-galactic.conf.spec')

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)
-- 
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