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author | Aaron LI <aaronly.me@gmail.com> | 2016-05-27 22:47:24 +0800 |
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committer | Aaron LI <aaronly.me@gmail.com> | 2016-05-27 22:47:24 +0800 |
commit | ffd178e0bd72562a3c2cff9747b6e656edc881dc (patch) | |
tree | 8800b7b5b2e8bc3df1a6760df5cd54eaaa686702 /mass_profile/extract_tcool.py | |
parent | 5c35fad9240fb42c1371c721e0b2af7379bd9ea0 (diff) | |
download | chandra-acis-analysis-ffd178e0bd72562a3c2cff9747b6e656edc881dc.tar.bz2 |
Add mass_profile tools
* These tools are mainly use to calculate the total gravitational mass
profile, as well as the intermediate products (e.g., surface
brightness profile fitting, gas density profile, NFW fitting, etc.)
* There are additional tools for calculating the luminosity and flux.
* These tools mainly developed by Junhua GU, and contributed by
Weitian (Aaron) LI, and Zhenghao ZHU.
Diffstat (limited to 'mass_profile/extract_tcool.py')
-rwxr-xr-x | mass_profile/extract_tcool.py | 12 |
1 files changed, 12 insertions, 0 deletions
diff --git a/mass_profile/extract_tcool.py b/mass_profile/extract_tcool.py new file mode 100755 index 0000000..393af27 --- /dev/null +++ b/mass_profile/extract_tcool.py @@ -0,0 +1,12 @@ +#!/usr/bin/env python + +import sys +rcool=float(sys.argv[1]) + +for l in open('cooling_time.dat'): + r,t=l.split() + r=float(r) + t=float(t) + if r>rcool: + print("cooling time at %f kpc=%f Gyr"%(rcool,t)) + sys.exit(0) |