#!/usr/bin/env python3 # # Copyright (c) 2017 Weitian LI # 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()