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authorAaron LI <aaronly.me@gmail.com>2016-06-07 19:52:19 +0800
committerAaron LI <aaronly.me@gmail.com>2016-06-07 19:52:19 +0800
commit4ff0cbc8879f4a2c50a14a9c8373f4eea61a2184 (patch)
tree046225fa500b2bb87247a589b14c3f08010e81d3 /mass_profile
parent43692e5f1d9ac09eb67bd1555b71f24ec8d86bf4 (diff)
downloadchandra-acis-analysis-4ff0cbc8879f4a2c50a14a9c8373f4eea61a2184.tar.bz2
fit_sbp.sh: update comment; use cosmo_calc
Diffstat (limited to 'mass_profile')
-rwxr-xr-xmass_profile/fit_sbp.sh12
1 files changed, 9 insertions, 3 deletions
diff --git a/mass_profile/fit_sbp.sh b/mass_profile/fit_sbp.sh
index 76aaaaf..666be2f 100755
--- a/mass_profile/fit_sbp.sh
+++ b/mass_profile/fit_sbp.sh
@@ -1,5 +1,12 @@
#!/bin/sh
#
+# Handy script for SBP fitting.
+# This script wraps the 'fit_beta_sbp' and 'fit_dbeta_sbp',
+# and automatically determine the sbp model according to the config file.
+#
+# Weitian LI
+# 2013-02-20
+#
if [ $# -ne 1 ]; then
printf "usage: $0 <mass_conf>\n"
@@ -19,8 +26,8 @@ t_param_file=`grep '^t_param_file' $cfg_file | awk '{ print $2 }'`
nh=`grep '^nh' $cfg_file | awk '{ print $2 }'`
abund=`grep '^abund' $cfg_file | awk '{ print $2 }'`
z=`grep '^z' $sbp_cfg | awk '{ print $2 }'`
-cm_per_pixel=`${base_path}/calc_distance ${z} | grep 'cm_per_pixel' | awk '{ print $2 }'`
-sed -i'' "s/^cm_per_pixel.*$/cm_per_pixel ${cm_per_pixel}/" ${sbp_cfg}
+cm_per_pixel=`cosmo_calc ${z} | grep 'cm/pixel' | awk -F':' '{ print $2 }'`
+sed -i'' "s/^cm_per_pixel.*$/cm_per_pixel ${cm_per_pixel}/" ${sbp_cfg}
cfunc_file=`grep '^cfunc_file' $sbp_cfg | awk '{ print $2 }'`
T_file=`grep '^T_file' $sbp_cfg | awk '{ print $2 }'`
@@ -40,4 +47,3 @@ fi
$base_path/$PROG $sbp_cfg
printf "## MODEL: ${MODEL}\n"
printf "## z: ${z}\n"
-