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author | Aaron LI <aly@aaronly.me> | 2019-02-27 22:00:44 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2019-02-27 23:57:12 +0800 |
commit | eddca6e37e3d8079a4f2bf4653588dd98f789f37 (patch) | |
tree | 919e743258c2c19878e1a2857052a3fd8fe08502 | |
parent | 963f6f4015c856f2f695f3634b47ed903ade5adf (diff) | |
download | fg21sim-eddca6e37e3d8079a4f2bf4653588dd98f789f37.tar.bz2 |
Several minor cleanups
-rw-r--r-- | fg21sim/configs/config.spec | 8 | ||||
-rw-r--r-- | fg21sim/extragalactic/clusters/main.py | 4 |
2 files changed, 6 insertions, 6 deletions
diff --git a/fg21sim/configs/config.spec b/fg21sim/configs/config.spec index 5a0731d..38e07d1 100644 --- a/fg21sim/configs/config.spec +++ b/fg21sim/configs/config.spec @@ -254,7 +254,7 @@ stream = option("stderr", "stdout", "", default="stderr") # Unit: [Msun] 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 10-based logarithmic step size for the halo masses; therefore # the number of intervals is: (log10(M_max) - log10(M_min)) / M_step M_step = float(default=0.01, min=0.001, max=0.1) @@ -272,11 +272,11 @@ stream = option("stderr", "stdout", "", default="stderr") # Redshifts where the halo mass distribution is calculated. # * ``mass``: # (Logarithmic-distributed) mass points. - # Unit: [Msun] (the little "h" is folded into the values) + # Unit: [Msun] (NOTE: the little "h" is folded into the values) # * ``dndlnm``: # Shape: (len(z), len(mass)) - # Differential mass function in terms of natural log of M. - # Unit: [Mpc^-3] (the little "h" is folded into the values) + # Differential mass function in terms of ln(M). + # Unit: [Mpc^-3] (NOTE: the little "h" is folded into the values) dndlnm_outfile = string(default="dndlnm.npz") diff --git a/fg21sim/extragalactic/clusters/main.py b/fg21sim/extragalactic/clusters/main.py index cfeaf80..201ceed 100644 --- a/fg21sim/extragalactic/clusters/main.py +++ b/fg21sim/extragalactic/clusters/main.py @@ -453,8 +453,8 @@ class GalaxyClusters: the corresponding halo within the ``self.halos``. The templates are normalized to have *mean* value of 1. """ - idx_kept = [idx for idx, cdict in enumerate(self.halos) - if cdit["genuine"] and not cdict.get("drop", False)] + idx_kept = [idx for idx, hdict in enumerate(self.halos) + if hdit["genuine"] and not hdict.get("drop", False)] num = len(idx_kept) logger.info("Draw template images for %d halos ..." % num) for i, idx in enumerate(idx_kept): |