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authorAaron LI <aaronly.me@outlook.com>2017-02-20 09:15:35 +0800
committerAaron LI <aaronly.me@outlook.com>2017-02-20 09:15:35 +0800
commit79f878f1c578eb4c85563a6f36170e6527f71b3b (patch)
tree44485f043062b6dbc2dd2abc94f560880802c54d /scripts
parentcdc927778f0c61dcff7e566eec0d038737f8e526 (diff)
downloadchandra-acis-analysis-79f878f1c578eb4c85563a6f36170e6527f71b3b.tar.bz2
Add scripts/cosmo_calc.py
* This 'cosmo_calc.py' replaces the original C++ version 'cosmo_calc' * Also fix a issue in 'acispy/cosmo.py'
Diffstat (limited to 'scripts')
-rwxr-xr-xscripts/cosmo_calc.py91
1 files changed, 91 insertions, 0 deletions
diff --git a/scripts/cosmo_calc.py b/scripts/cosmo_calc.py
new file mode 100755
index 0000000..7381da0
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+++ b/scripts/cosmo_calc.py
@@ -0,0 +1,91 @@
+#!/usr/bin/env python3
+#
+# Copyright (c) 2017 Weitian LI <liweitianux@live.com>
+# MIT license
+
+"""
+Cosmology calculator with support of Chandra ACIS-specific quantities.
+"""
+
+import argparse
+
+from context import acispy
+from acispy.cosmo import Calculator
+
+
+def main():
+ parser = argparse.ArgumentParser(
+ description="Cosmology calculator with Chandra-specific quantities")
+ parser.add_argument("-H", "--hubble", dest="H0",
+ type=float, default=71.0,
+ help="Present-day Hubble parameter " +
+ "(default: 71 km/s/Mpc)")
+ parser.add_argument("-M", "--omega-m", dest="Om0",
+ type=float, default=0.27,
+ help="Present-day matter density (default: 0.27")
+ parser.add_argument("-b", "--brief", dest="brief", action="store_true",
+ help="be brief")
+ parser.add_argument("-U", "--unit", dest="unit",
+ help="unit for output quantity if supported")
+ group = parser.add_mutually_exclusive_group(required=True)
+ group.add_argument("-L", "--luminosity-distance",
+ dest="luminosity_distance",
+ action="store_true",
+ help="calculate the luminosity distance (DL)")
+ group.add_argument("-A", "--angular-diameter-distance",
+ dest="angular_diameter_distance",
+ action="store_true",
+ help="calculate the angular diameter distance (DA)")
+ group.add_argument("--kpc-per-arcsec", dest="kpc_per_arcsec",
+ action="store_true",
+ help="calculate the transversal length [kpc] " +
+ "w.r.t. 1 arcsec at DA(z)")
+ group.add_argument("--kpc-per-pix", dest="kpc_per_pix",
+ action="store_true",
+ help="calculate the transversal length [kpc] " +
+ "w.r.t. 1 ACIS pixel (0.492 arcsec) at DA(z)")
+ group.add_argument("--cm-per-pix", dest="cm_per_pix",
+ action="store_true",
+ help="calculate the transversal length [cm] " +
+ "w.r.t. 1 ACIS pixel (0.492 arcsec) at DA(z)")
+ group.add_argument("--norm-apec", dest="norm_apec",
+ action="store_true",
+ help="calculate the normalization factor " +
+ "of the XSPEC APEC model assuming EM=1")
+ parser.add_argument("z", type=float, help="redshift")
+ args = parser.parse_args()
+
+ cosmocalc = Calculator(H0=args.H0, Om0=args.Om0)
+
+ if args.luminosity_distance:
+ kwargs = {"z": args.z}
+ kwargs["unit"] = args.unit if args.unit else "Mpc"
+ label = "Luminosity distance [%s]" % kwargs["unit"]
+ value = cosmocalc.luminosity_distance(**kwargs)
+ elif args.angular_diameter_distance:
+ kwargs = {"z": args.z}
+ kwargs["unit"] = args.unit if args.unit else "Mpc"
+ label = "Angular diameter distance [%s]" % kwargs["unit"]
+ value = cosmocalc.angular_diameter_distance(**kwargs)
+ elif args.kpc_per_arcsec:
+ label = "kpc/arcsec (DA)"
+ value = cosmocalc.kpc_per_arcsec(args.z)
+ elif args.kpc_per_pix:
+ label = "kpc/pix (DA)"
+ value = cosmocalc.kpc_per_pix(args.z)
+ elif args.cm_per_pix:
+ label = "cm/pix (DA)"
+ value = cosmocalc.cm_per_pix(args.z)
+ elif args.norm_apec:
+ label = "norm (APEC) [cm^-5]"
+ value = cosmocalc.norm_apec(args.z)
+ else:
+ raise ValueError("no quantity to calculate")
+
+ if not args.brief:
+ print(label + ": ", end="", flush=True)
+ print(value)
+
+
+if __name__ == "__main__":
+ main()