test_cslightcrv.py
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#! /usr/bin/env python
# ==========================================================================
# This scripts performs unit tests for the cslightcrv script.
#
# Copyright (C) 2016-2020 Juergen Knoedlseder
#
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
#
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License
# along with this program. If not, see <http://www.gnu.org/licenses/>.
#
# ==========================================================================
import gammalib
import cscripts
from testing import test
# ================================ #
# Test class for cslightcrv script #
# ================================ #
class Test(test):
"""
Test class for cslightcrv script
This test class makes unit tests for the cslightcrv script by using it
from the command line and from Python.
"""
# Constructor
def __init__(self):
"""
Constructor
"""
# Call base class constructor
test.__init__(self)
# Add off-axis events for classical analysis
self._offaxis_events = self._datadir + '/crab_offaxis1.fits'
self._model_onoff = self._datadir + '/crab_onoff.xml'
# Return
return
# Set test functions
def set(self):
"""
Set all test functions.
"""
# Set test name
self.name('cslightcrv')
# Append tests
self.append(self._test_cmd, 'Test cslightcrv on command line')
self.append(self._test_python, 'Test cslightcrv from Python')
self.append(self._test_pickeling, 'Test cslightcrv pickeling')
# Return
return
# Test cslightcrv on command line
def _test_cmd(self):
"""
Test cslightcrv on the command line.
"""
# Set script name
cslightcrv = self._script('cslightcrv')
# Setup cslightcrv command
cmd = cslightcrv+' inobs="'+self._events+'"'+ \
' inmodel="'+self._model+'" srcname="Crab"'+ \
' caldb="'+self._caldb+'" irf="'+self._irf+'"'+ \
' tbinalg=LIN '+ \
' tmin=2020-01-01T00:00:00 tmax=2020-01-01T00:05:00'+ \
' tbins=2 method=3D enumbins=0 emin=1.0 emax=100.0'+ \
' outfile="lightcurve_cmd1.fits"'+ \
' logfile="cslightcrv_cmd1.log" chatter=1'
# Check if execution was successful
self.test_assert(self._execute(cmd) == 0,
'Check successful execution from command line')
# Check light curve
self._check_light_curve('lightcurve_cmd1.fits', 2)
# Setup cslightcrv command
cmd = cslightcrv+' inobs="events_that_do_not_exist.fits"'+ \
' inmodel="'+self._model+'" srcname="Crab"'+ \
' caldb="'+self._caldb+'" irf="'+self._irf+'"'+ \
' tbinalg=LIN '+ \
' tmin=2020-01-01T00:00:00 tmax=2020-01-01T00:05:00'+ \
' tbins=2 method=3D enumbins=0 emin=1.0 emax=100.0'+ \
' outfile="lightcurve_cmd1.fits"'+ \
' logfile="cslightcrv_cmd2.log" debug=yes'
# Check if execution failed
self.test_assert(self._execute(cmd, success=False) != 0,
'Check invalid input file when executed from command line')
# Check cslightcrv --help
self._check_help(cslightcrv)
# Return
return
# Test cslightcrv from Python
def _test_python(self):
"""
Test cslightcrv from Python
"""
# Set-up unbinned cslightcrv
lcrv = cscripts.cslightcrv()
lcrv['inobs'] = self._events
lcrv['inmodel'] = self._model
lcrv['srcname'] = 'Crab'
lcrv['caldb'] = self._caldb
lcrv['irf'] = self._irf
lcrv['tbinalg'] = 'LIN'
lcrv['tmin'] = '2020-01-01T00:00:00'
lcrv['tmax'] = '2020-01-01T00:05:00'
lcrv['tbins'] = 2
lcrv['method'] = '3D'
lcrv['enumbins'] = 0
lcrv['emin'] = 1.0
lcrv['emax'] = 100.0
lcrv['outfile'] = 'cslightcrv_py1.fits'
lcrv['logfile'] = 'cslightcrv_py1.log'
lcrv['chatter'] = 2
lcrv['publish'] = True
# Run cslightcrv script and save light curve
lcrv.logFileOpen() # Make sure we get a log file
lcrv.run()
lcrv.save()
# Check light curve
self._check_light_curve('cslightcrv_py1.fits', 2)
# Now use FILE as time bin algorithm. For this we need first to
# create an ASCII file. We use now 2 time bins. The ASCII file
# is saved into the file "lightcurve_py2.dat".
csv = gammalib.GCsv(2,2)
tmin = 58849.00
tdelta = 0.0017361
for i in range(csv.nrows()):
csv[i,0] = '%.5f' % (tmin + i * tdelta)
csv[i,1] = '%.5f' % (tmin + (i+1) * tdelta)
csv.save('cslightcrv_py2.dat', ' ', True)
# Set-up unbinned cslightcrv
lcrv = cscripts.cslightcrv()
lcrv['inobs'] = self._events
lcrv['inmodel'] = self._model
lcrv['srcname'] = 'Crab'
lcrv['caldb'] = self._caldb
lcrv['irf'] = self._irf
lcrv['tbinalg'] = 'FILE'
lcrv['tbinfile'] = 'cslightcrv_py2.dat'
lcrv['method'] = '3D'
lcrv['enumbins'] = 0
lcrv['emin'] = 1.0
lcrv['emax'] = 100.0
lcrv['fix_bkg'] = True
lcrv['outfile'] = 'cslightcrv_py2.fits'
lcrv['logfile'] = 'cslightcrv_py2.log'
lcrv['chatter'] = 3
# Execute cslightcrv script
lcrv.execute()
# Check light curve
self._check_light_curve('cslightcrv_py2.fits', 2)
# Now we setup an observation container on input. We attached the
# model to the observation container so that cslightcrv should
# no longer query for the parameter.
cta = gammalib.GCTAObservation(self._events)
obs = gammalib.GObservations()
obs.append(cta)
obs.models(self._model)
# Set-up unbinned cslightcrv from observation container. Now use
# the GTI algorithm so that we test all timing algorithms.
lcrv = cscripts.cslightcrv(obs)
lcrv['srcname'] = 'Crab'
lcrv['caldb'] = self._caldb
lcrv['irf'] = self._irf
lcrv['tbinalg'] = 'GTI'
lcrv['method'] = '3D'
lcrv['enumbins'] = 0
lcrv['emin'] = 1.0
lcrv['emax'] = 100.0
lcrv['outfile'] = 'cslightcrv_py3.fits'
lcrv['logfile'] = 'cslightcrv_py3.log'
lcrv['chatter'] = 4
# Execute cslightcrv script
lcrv.execute()
# Check light curve
self._check_light_curve('cslightcrv_py3.fits', 1)
# Binned cslightcrv
lcrv = cscripts.cslightcrv()
lcrv['inobs'] = self._events
lcrv['inmodel'] = self._model
lcrv['srcname'] = 'Crab'
lcrv['caldb'] = self._caldb
lcrv['irf'] = self._irf
lcrv['tbinalg'] = 'LIN'
lcrv['tmin'] = '2020-01-01T00:00:00'
lcrv['tmax'] = '2020-01-01T00:05:00'
lcrv['tbins'] = 2
lcrv['method'] = '3D'
lcrv['emin'] = 1.0
lcrv['emax'] = 100.0
lcrv['enumbins'] = 3
lcrv['coordsys'] = 'CEL'
lcrv['proj'] = 'TAN'
lcrv['xref'] = 83.63
lcrv['yref'] = 22.01
lcrv['nxpix'] = 10
lcrv['nypix'] = 10
lcrv['binsz'] = 0.04
lcrv['outfile'] = 'cslightcrv_py4.fits'
lcrv['logfile'] = 'cslightcrv_py4.log'
lcrv['chatter'] = 4
# Execute cslightcrv script
lcrv.execute()
# Check light curve
self._check_light_curve('cslightcrv_py4.fits', 2)
# cslightcrv with classical analysis
lcrv = cscripts.cslightcrv()
lcrv['inobs'] = self._offaxis_events
lcrv['inmodel'] = self._model_onoff
lcrv['srcname'] = 'Crab'
lcrv['caldb'] = self._caldb
lcrv['irf'] = self._irf
lcrv['tbinalg'] = 'LIN'
lcrv['tmin'] = '2020-01-01T00:00:00'
lcrv['tmax'] = '2020-01-01T00:05:00'
lcrv['tbins'] = 2
lcrv['method'] = 'ONOFF'
lcrv['srcshape'] = 'CIRCLE'
lcrv['use_model_bkg'] = False # Needed even if WSTAT
lcrv['emin'] = 1.0
lcrv['emax'] = 100.0
lcrv['enumbins'] = 2
lcrv['coordsys'] = 'CEL'
lcrv['xref'] = 83.63
lcrv['yref'] = 22.01
lcrv['rad'] = 0.2
lcrv['etruemin'] = 1.0
lcrv['etruemax'] = 100.0
lcrv['etruebins'] = 5
lcrv['statistic'] = 'WSTAT'
lcrv['outfile'] = 'cslightcrv_py5.fits'
lcrv['logfile'] = 'cslightcrv_py5.log'
lcrv['chatter'] = 4
# Execute cslightcrv script
lcrv.execute()
# Check light curve
self._check_light_curve('cslightcrv_py5.fits', 2)
# Set-up cslightcrv without multiprocessing
lcrv = cscripts.cslightcrv()
lcrv['inobs'] = self._events
lcrv['inmodel'] = self._model
lcrv['srcname'] = 'Crab'
lcrv['caldb'] = self._caldb
lcrv['irf'] = self._irf
lcrv['tbinalg'] = 'LIN'
lcrv['tmin'] = '2020-01-01T00:00:00'
lcrv['tmax'] = '2020-01-01T00:05:00'
lcrv['tbins'] = 2
lcrv['method'] = '3D'
lcrv['enumbins'] = 0
lcrv['emin'] = 1.0
lcrv['emax'] = 100.0
lcrv['outfile'] = 'cslightcrv_py6.fits'
lcrv['logfile'] = 'cslightcrv_py6.log'
lcrv['chatter'] = 2
lcrv['publish'] = True
lcrv['nthreads'] = 1
# Run cslightcrv script and save light curve
lcrv.logFileOpen() # Make sure we get a log file
lcrv.run()
lcrv.save()
# Check light curve
self._check_light_curve('cslightcrv_py6.fits', 2)
# Return
return
# Test cslightcrv pickeling
def _test_pickeling(self):
"""
Test cslightcrv pickeling
"""
# Perform pickeling tests of empty class
self._pickeling(cscripts.cslightcrv())
# Set-up unbinned cslightcrv
lcrv = cscripts.cslightcrv()
lcrv['inobs'] = self._events
lcrv['inmodel'] = self._model
lcrv['srcname'] = 'Crab'
lcrv['caldb'] = self._caldb
lcrv['irf'] = self._irf
lcrv['tbinalg'] = 'LIN'
lcrv['tmin'] = '2020-01-01T00:00:00'
lcrv['tmax'] = '2020-01-01T00:05:00'
lcrv['tbins'] = 2
lcrv['method'] = '3D'
lcrv['enumbins'] = 0
lcrv['emin'] = 1.0
lcrv['emax'] = 100.0
lcrv['outfile'] = 'cslightcrv_py1_pickle.fits'
lcrv['logfile'] = 'cslightcrv_py1_pickle.log'
lcrv['chatter'] = 2
lcrv['publish'] = True
# Perform pickeling tests of filled class
obj = self._pickeling(lcrv)
# Run cslightcrv script and save light curve
obj.logFileOpen() # Make sure we get a log file
obj.run()
obj.save()
# Check light curve
self._check_light_curve('cslightcrv_py1_pickle.fits', 2)
# Return
return
# Check light curve result file
def _check_light_curve(self, filename, bins, prefactor=5.7e-16):
"""
Check light curve file
"""
# Expected column names
cols = ['MJD', 'e_MJD', 'Prefactor', 'e_Prefactor',
'Index', 'e_Index', 'TS', 'DiffUpperLimit',
'FluxUpperLimit', 'EFluxUpperLimit']
# Open FITS file
fits = gammalib.GFits(filename)
# Check FITS file structure
self.test_value(fits.size(), 2,
'Check for 2 extensions in light curve FITS file')
self.test_assert(fits.contains('LIGHTCURVE'),
'FITS file contains "LIGHTCURVE" extension')
# Get LIGHTCURVE table
table = fits['LIGHTCURVE']
# Check FITS table structure
self.test_value(table.ncols(), len(cols),
'Check for %d columns in light curve FITS table' % len(cols))
self.test_value(table.nrows(), bins,
'Check for %d rows in light curve FITS table' % bins)
for col in cols:
self.test_assert(table.contains(col),
'FITS file contains "'+col+'" column')
# Check that the Prefactor has the right order of magnitude
for s in range(table.nrows()):
self.test_value(table['Prefactor'][s], prefactor, 0.9*prefactor,
'Check prefactor value')
# Close FITS file
fits.close()
# Return
return