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author | Aaron LI <aly@aaronly.me> | 2017-08-27 12:37:23 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2017-08-27 12:37:23 +0800 |
commit | f29d5f6b4027d8f356e76528247d4b8b070b9c90 (patch) | |
tree | 1058f9a074d3a291b22044d4b30ccad7ca7bfedc | |
parent | 466eec34aab338757e59a06b8b0d38c37047f19f (diff) | |
download | fg21sim-f29d5f6b4027d8f356e76528247d4b8b070b9c90.tar.bz2 |
configs: synchrotron: default to not add smallscales
-rw-r--r-- | fg21sim/configs/10-galactic.conf.spec | 8 |
1 files changed, 5 insertions, 3 deletions
diff --git a/fg21sim/configs/10-galactic.conf.spec b/fg21sim/configs/10-galactic.conf.spec index cf2eef1..43e84c9 100644 --- a/fg21sim/configs/10-galactic.conf.spec +++ b/fg21sim/configs/10-galactic.conf.spec @@ -23,9 +23,11 @@ # Synchrotron emission component (unpolarized) [[synchrotron]] - # The template map for the simulation. + # 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 (same unit as in [frequency] section) + # The frequency of the template map. + # Unit: [MHz] template_freq = float(default=None, min=0.0) # Spectral index map @@ -33,7 +35,7 @@ # Whether add fluctuations on the small scales according the angular # power spectrum prediction? - add_smallscales = boolean(default=True) + 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``. |