Commit 937b71e2f6e9ab41e56148712ca3eab461ef1647
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scripts/cta_kb_bkgrates.py
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| 1 | +#! /usr/bin/env python | |
| 2 | +# ========================================================================== | |
| 3 | +# This script converts the background rates in Konrad's performance files | |
| 4 | +# into a column separated file function table. The table is automatically | |
| 5 | +# named "bkg_XXX.txt" where "XXX" is for example "kb_E_50h_v3". | |
| 6 | +# | |
| 7 | +# Copyright (C) 2011 Jurgen Knodlseder | |
| 8 | +# | |
| 9 | +# This program is free software: you can redistribute it and/or modify | |
| 10 | +# it under the terms of the GNU General Public License as published by | |
| 11 | +# the Free Software Foundation, either version 3 of the License, or | |
| 12 | +# (at your option) any later version. | |
| 13 | +# | |
| 14 | +# This program is distributed in the hope that it will be useful, | |
| 15 | +# but WITHOUT ANY WARRANTY; without even the implied warranty of | |
| 16 | +# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the | |
| 17 | +# GNU General Public License for more details. | |
| 18 | +# | |
| 19 | +# You should have received a copy of the GNU General Public License | |
| 20 | +# along with this program. If not, see <http://www.gnu.org/licenses/>. | |
| 21 | +# | |
| 22 | +# ========================================================================== | |
| 23 | +from gammalib import * | |
| 24 | +import math | |
| 25 | +import sys | |
| 26 | + | |
| 27 | + | |
| 28 | +# ================================= # | |
| 29 | +# Generate file function from model # | |
| 30 | +# ================================= # | |
| 31 | +def make_file_function(irfname, filename): | |
| 32 | + """ | |
| 33 | + Generate file function from model. | |
| 34 | + | |
| 35 | + Parameters: | |
| 36 | + irfname - IRF filename | |
| 37 | + filename - File function filename | |
| 38 | + """ | |
| 39 | + # Open performance file and file function | |
| 40 | + irf = open(irfname, "r") | |
| 41 | + file = open(filename, "w") | |
| 42 | + | |
| 43 | + # Read data | |
| 44 | + for row in irf: | |
| 45 | + | |
| 46 | + # Skip header and trailer | |
| 47 | + if row.find("log(E)") != -1: | |
| 48 | + continue | |
| 49 | + if row.find("--------") != -1: | |
| 50 | + break | |
| 51 | + | |
| 52 | + # Extract data | |
| 53 | + fields = row.replace(" ",",").replace(",,",",").rstrip("\n").split(",") | |
| 54 | + logE = float(fields[0]) | |
| 55 | + aeff = float(fields[1]) | |
| 56 | + r68 = float(fields[2]) | |
| 57 | + r80 = float(fields[3]) | |
| 58 | + eres = float(fields[4]) | |
| 59 | + bgd = float(fields[5]) | |
| 60 | + sens = float(fields[6]) | |
| 61 | + | |
| 62 | + # Compute energy (in MeV) | |
| 63 | + energy = math.pow(10.0, logE)*1.0e6 | |
| 64 | + | |
| 65 | + # Compute solid angle of r68 region in sr | |
| 66 | + omega = 2.0 * math.pi * (1.0 - math.cos(math.radians(r68))) | |
| 67 | + | |
| 68 | + # Compute background rate per steradian and MeV | |
| 69 | + bkg_rate = bgd/omega/energy | |
| 70 | + | |
| 71 | + # Write | |
| 72 | + file.write(str(energy)+" "+str(bkg_rate)+"\n") | |
| 73 | + | |
| 74 | + print logE, energy, bgd, omega, bkg_rate | |
| 75 | + | |
| 76 | + # Close files | |
| 77 | + irf.close() | |
| 78 | + file.close() | |
| 79 | + | |
| 80 | + # Return | |
| 81 | + return | |
| 82 | + | |
| 83 | + | |
| 84 | +# ================ # | |
| 85 | +# Main entry point # | |
| 86 | +# ================ # | |
| 87 | +if __name__ == '__main__': | |
| 88 | + """ | |
| 89 | + Main entry point | |
| 90 | + """ | |
| 91 | + # Get IRF from command line argument | |
| 92 | + if (len(sys.argv) > 1): | |
| 93 | + irf = sys.argv[1] | |
| 94 | + else: | |
| 95 | + irf = "kb_E_50h_v3" | |
| 96 | + | |
| 97 | + # Set parameters | |
| 98 | + caldb = "/usr/local/gamma/share/caldb/cta" | |
| 99 | + | |
| 100 | + # Set filenames | |
| 101 | + irfname = caldb+"/"+irf+".dat" | |
| 102 | + filename = "bkg_"+irf+".txt" | |
| 103 | + | |
| 104 | + # Read | |
| 105 | + make_file_function(irfname, filename) | ... | ... |