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author | Aaron LI <aly@aaronly.me> | 2017-10-19 13:21:01 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2017-10-19 13:21:01 +0800 |
commit | 128d5e3745a19c956556bfbecbd66ee8f1fb5dc2 (patch) | |
tree | 4bea5242158821dd583bbb3ee59d9caaa677298c | |
parent | 08e33b8617f4f702a97e3aeacc5260b2254c7523 (diff) | |
download | fg21sim-128d5e3745a19c956556bfbecbd66ee8f1fb5dc2.tar.bz2 |
clusters: Update configuration defaults and description
-rw-r--r-- | fg21sim/configs/20-extragalactic.conf.spec | 24 |
1 files changed, 12 insertions, 12 deletions
diff --git a/fg21sim/configs/20-extragalactic.conf.spec b/fg21sim/configs/20-extragalactic.conf.spec index df5ea86..2c879ac 100644 --- a/fg21sim/configs/20-extragalactic.conf.spec +++ b/fg21sim/configs/20-extragalactic.conf.spec @@ -20,12 +20,12 @@ # The model of the fitting function for halo mass distribution # For all models and more details: # https://hmf.readthedocs.io/en/latest/_autosummary/hmf.fitting_functions.html - model = option("jenkins", "ps", "smt", default="smt") + model = option("smt", "jenkins", "ps", default="smt") - # The minimum (inclusive) and maximum (exclusive) halo mass (dark + # The minimum (inclusive) and maximum (exclusive!) halo mass (dark # matter only) within which to calculate the halo mass distribution. # Unit: [Msun] - M_min = float(default=1e13, min=1e10, max=1e14) + M_min = float(default=1e12, min=1e10, max=1e14) M_max = float(default=1e16, min=1e14, max=1e18) # The logarithmic (base 10) step size for the halo masses; therefore # the number of intervals is: (log10(M_max) - log10(M_min)) / M_step @@ -60,8 +60,8 @@ # mass, redshift, position, shape, and the recent major merger info. catalog_outfile = string(default=None) - # Directly use the (previously simulated) catalog file specified - # as the above "catalog_outfile" option. + # Whether to directly use the (previously simulated) catalog file + # specified as the above "catalog_outfile" option? # NOTE: # By using an existing catalog, the steps to derive these data are # simply skipped. @@ -96,7 +96,7 @@ # The minimum mass for clusters when to determine the galaxy clusters # total counts and their distributions. # Unit: [Msun] - mass_min = float(default=2e14, min=1e12) + mass_min = float(default=1e14, min=1e12) # Boost the number of expected cluster number within the sky coverage # by the specified times. @@ -150,13 +150,13 @@ gamma_max = float(default=1e5) # Number of momentum points/cells for solving the Fokker-Planck # equation. - gamma_np = integer(default=200, min=50) + gamma_np = integer(default=200, min=100) - # Number of grid points used as the buffer region near the lower - # boundary, and the value within this buffer region will be fixed to - # avoid unphysical pile-up of low-energy electrons. - # Reference: Donnert & Brunetti 2014, MNRAS, 443, 3564, Sec.(3.3) - buffer_np = integer(default=5, min=0) + # Number of cells used as the buffer regions near both the lower + # and upper boundaries, and the value within the buffer regions will + # be fixed to avoid unphysical pile-ups. + # It is suggested to be about 5%-10% of the above ``gamma_np``. + buffer_np = integer(default=10, min=0) # Time step for solving the Fokker-Planck equation # Unit: [Gyr] |