csresspec.py
25.9 KB
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
275
276
277
278
279
280
281
282
283
284
285
286
287
288
289
290
291
292
293
294
295
296
297
298
299
300
301
302
303
304
305
306
307
308
309
310
311
312
313
314
315
316
317
318
319
320
321
322
323
324
325
326
327
328
329
330
331
332
333
334
335
336
337
338
339
340
341
342
343
344
345
346
347
348
349
350
351
352
353
354
355
356
357
358
359
360
361
362
363
364
365
366
367
368
369
370
371
372
373
374
375
376
377
378
379
380
381
382
383
384
385
386
387
388
389
390
391
392
393
394
395
396
397
398
399
400
401
402
403
404
405
406
407
408
409
410
411
412
413
414
415
416
417
418
419
420
421
422
423
424
425
426
427
428
429
430
431
432
433
434
435
436
437
438
439
440
441
442
443
444
445
446
447
448
449
450
451
452
453
454
455
456
457
458
459
460
461
462
463
464
465
466
467
468
469
470
471
472
473
474
475
476
477
478
479
480
481
482
483
484
485
486
487
488
489
490
491
492
493
494
495
496
497
498
499
500
501
502
503
504
505
506
507
508
509
510
511
512
513
514
515
516
517
518
519
520
521
522
523
524
525
526
527
528
529
530
531
532
533
534
535
536
537
538
539
540
541
542
543
544
545
546
547
548
549
550
551
552
553
554
555
556
557
558
559
560
561
562
563
564
565
566
567
568
569
570
571
572
573
574
575
576
577
578
579
580
581
582
583
584
585
586
587
588
589
590
591
592
593
594
595
596
597
598
599
600
601
602
603
604
605
606
607
608
609
610
611
612
613
614
615
616
617
618
619
620
621
622
623
624
625
626
627
628
629
630
631
632
633
634
635
636
637
638
639
640
641
642
643
644
645
646
647
648
649
650
651
652
653
654
655
656
657
658
659
660
661
662
663
664
665
666
667
668
669
670
671
672
673
674
675
676
677
678
679
680
681
682
683
684
685
686
687
688
689
690
691
692
693
694
695
696
697
698
699
700
701
702
703
704
705
706
707
708
709
710
711
712
713
714
715
716
#! /usr/bin/env python
# ==========================================================================
# Generates a residual spectrum.
#
# Copyright (C) 2017-2018 Luigi Tibaldo
#
# 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 ctools
from cscripts import obsutils
import sys
# =============== #
# csresspec class #
# =============== #
class csresspec(ctools.csobservation):
"""
Generates a residual spectrum
"""
# Constructor
def __init__(self, *argv):
"""
Constructor
"""
# Initialise application by calling the appropriate class constructor
self._init_csobservation(self.__class__.__name__, ctools.__version__,
argv)
# Initialise class members
self._use_maps = False
self._stack = False
self._mask = False
self._fits = gammalib.GFits()
# Return
return
# Private methods
def _get_parameters(self):
"""
Get parameters from parfile and setup the observation
"""
# Setup observations (require response and allow event list as well as
# counts cube)
self._setup_observations(self.obs(), True, True, True)
# Set observation statistic
self._set_obs_statistic(gammalib.toupper(self['statistic'].string()))
# Collect number of unbinned, binned and On/Off observations in
# observation container
n_unbinned = 0
n_binned = 0
n_onoff = 0
for obs in self.obs():
if obs.classname() == 'GCTAObservation':
if obs.eventtype() == 'CountsCube':
n_binned += 1
else:
n_unbinned += 1
elif obs.classname() == 'GCTAOnOffObservation':
n_onoff += 1
n_cta = n_unbinned + n_binned + n_onoff
n_other = self.obs().size() - n_cta
# Query whether to compute model for individual components
components = self['components'].boolean()
# If there is only one binned observation and no model for individual
# components is required, query for precomputed model file and set
# use_maps to True
if self.obs().size() == 1 and n_binned == 1 and not components:
modcube = self['modcube'].filename()
if modcube != 'NONE':
self._use_maps = True
# If there are unbinned observations query the energy binning parameters
if n_unbinned != 0:
self['ebinalg'].string()
if self['ebinalg'].string() == 'FILE':
self['ebinfile'].filename()
else:
self['emin'].real()
self['emax'].real()
self['enumbins'].integer()
if n_cta > n_unbinned:
n_notunbin = n_cta - n_unbinned
# If there is more than one observation, and observations are all
# unbinned or all onoff query user to know if they wish stacked results
if self.obs().size() > 1 and \
(n_unbinned == self.obs().size() or n_onoff == self.obs().size()):
self._stack = self['stack'].boolean()
# If we are to stack event lists query parameters for cube creation
if self._stack and n_unbinned == self.obs().size():
self['coordsys'].string()
self['proj'].string()
self['xref'].real()
self['yref'].real()
self['nxpix'].integer()
self['nypix'].integer()
self['binsz'].real()
# If we are not using a precomputed model and no models are available
# in the observation container query input XML model file
if not self._use_maps and self.obs().models().size() == 0:
self.obs().models(self['inmodel'].filename())
# Unless all observations are On/Off query for mask definition
if n_onoff == n_cta:
pass
else:
self._mask = self['mask'].boolean()
if self._mask:
self['ra'].real()
self['dec'].real()
self['rad'].real()
self['regfile'].filename()
# Unless all observations are On/Off, or we are using precomputed model
# maps query whether to use energy dispersion
if n_onoff == n_cta or self._use_maps:
pass
else:
self['edisp'].boolean()
# Query algorithm for residual computation
self['algorithm'].string()
# Read ahead output parameters
if self._read_ahead():
self['outfile'].filename()
# Write input parameters into logger
self._log_parameters(gammalib.TERSE)
# Write header for observation census
self._log_header1(gammalib.TERSE, 'Observation census')
# Log census of input observations
self._log_value(gammalib.NORMAL, 'Unbinned CTA observations', n_unbinned)
self._log_value(gammalib.NORMAL, 'Binned CTA observations', n_binned)
self._log_value(gammalib.NORMAL, 'On/off CTA observations', n_onoff)
self._log_value(gammalib.NORMAL, 'Other observations', n_other)
if n_other > 0:
msg = 'WARNING: Only CTA observation can be handled, all non-CTA ' \
+ 'observations will be ignored.'
self._log_string(gammalib.TERSE, msg)
# Log for unbinned observations
if n_unbinned != 0:
msg = ' User defined energy binning will be used for %d unbinned '\
'observations.' % (n_unbinned)
self._log_string(gammalib.TERSE, msg)
if n_cta > n_unbinned:
msg = ' The intrinsic binning will be used for the remaining '\
'%d CTA observations.' % (n_notunbin)
self._log_string(gammalib.TERSE, msg)
# Signal how energy dispersion is applied
if n_onoff == n_cta or self._use_maps:
msg = ' Energy dispersion is applied based on the input data/model ' \
+ 'and not according to the edisp parameter'
self._log_string(gammalib.TERSE, msg)
# Return
return
def _stack_observations(self):
"""
Stack multiple observations and replace observation container
with single stacked observation
Returns
-------
obs : `~gammalib.GObservations'
Observation container with a single stacked observation
"""
# Use first observation to determine the type and apply the
# appropriate stacking method
# If On/Off use the GCTAOnOffObservation constructor
if self.obs()[0].classname() == 'GCTAOnOffObservation':
msg = 'Stacking %d On/Off observations.' % (self.obs().size())
self._log_string(gammalib.NORMAL, msg)
stacked = gammalib.GCTAOnOffObservation(self.obs())
stacked_obs = gammalib.GObservations()
stacked_obs.append(stacked)
stacked_obs.models(self.obs().models())
# If event list then bin observations
elif self.obs()[0].classname() == 'GCTAObservation':
msg = 'Stacking %d event lists.' % (self.obs().size())
self._log_string(gammalib.NORMAL, msg)
stacked_obs = obsutils.get_stacked_obs(self, self.obs())
# Return
return stacked_obs
def _bin_evlist(self, obs):
"""
Turn single event list into counts cube
Parameters
----------
obs : `~gammalib.GObservations()`
Observation container with single event list
Returns
-------
obs : `~gammalib.GObservations()`
Binned observation container dict with event list ROI and energy
range information
"""
# Retrieve information about ROI in event list
roi = obs[0].roi()
ra = roi.centre().dir().ra_deg()
dec = roi.centre().dir().dec_deg()
rad = roi.radius()
# We will cover the whole ROI with 0.02 deg binning
npix = int(2.0 * rad / 0.02) + 1
# Log binning of events
self._log_string(gammalib.EXPLICIT, 'Binning events')
# Bin events
cntcube = ctools.ctbin(obs)
cntcube['xref'] = ra
cntcube['yref'] = dec
cntcube['binsz'] = 0.02
cntcube['nxpix'] = npix
cntcube['nypix'] = npix
cntcube['proj'] = 'TAN'
cntcube['coordsys'] = 'CEL'
cntcube['ebinalg'] = self['ebinalg'].string()
if self['ebinalg'].string() == 'FILE':
cntcube['ebinfile'] = self['ebinfile'].filename()
else:
cntcube['enumbins'] = self['enumbins'].integer()
cntcube['emin'] = self['emin'].real()
cntcube['emax'] = self['emax'].real()
cntcube.run()
# Retrieve the binned observation container
binned_obs = cntcube.obs().copy()
# Check if energy boundaries provided by user extend beyond the
# content of the event list
if self['emin'].real() > obs[0].events().emin().TeV():
emin = 'INDEF'
else:
emin = obs[0].events().emin().TeV()
if self['emax'].real() < obs[0].events().emax().TeV():
emax = 'INDEF'
else:
emax = obs[0].events().emax().TeV()
# Put ROI and E bound info in dictionary
info = {'was_list': True, 'roi_ra': ra, 'roi_dec': dec, 'roi_rad': rad,
'emin': emin, 'emax': emax}
# Return new oberservation container
return binned_obs, info
def _masked_cube(self, cube, ra, dec, rad, emin='INDEF', emax='INDEF',
regfile='NONE'):
"""
Mask an event cube and returns the masked cube
Parameters
----------
cube : `~gammalib.GCTAEventCube()`
Event cube
ra : float (str 'INDEF' for no selection on direction)
Right Ascension (deg)
dec : float (str 'INDEF' for no selection on direction)
Declination (deg)
rad : float (str 'INDEF' for no selection on direction)
Radius (deg)
emin : float (str 'INDEF' for no selection on energy)
Minimum energy (TeV)
emax : float (str 'INDEF' for no selection on energy)
Maximum energy (TeV)
Returns
-------
cube : `~gammalib.GCTAEventCube()`
Event cube
"""
# Turn cube into observation container to feed to ctcubemask
obs = gammalib.GCTAObservation()
obs.events(cube)
obs_cont = gammalib.GObservations()
obs_cont.append(obs)
# Use ctcubemask to mask event cube pixels
cubemask = ctools.ctcubemask(obs_cont)
cubemask['ra'] = ra
cubemask['dec'] = dec
cubemask['rad'] = rad
cubemask['emin'] = emin
cubemask['emax'] = emax
cubemask['regfile'] = regfile
cubemask.run()
# Extract copy of cube from observation container (copy is needed to
# avoid memory leaks in SWIG)
cube = cubemask.obs()[0].events().copy()
# Return cube
return cube
def _cube_to_spectrum(self, cube, evlist_info):
"""
Derive from event cube a count spectrum
If data come from event list use only the ROI and energy range of
the original data. Apply user defined mask if requested.
Parameters
----------
cube : `~gammalib.GCTAEventCube()`
Event cube
evlist_info : dict
Dictionary with information on original event list
Returns
-------
array : `~gammalib.GNdarray()'
Counts spectrum
"""
# If we started from event list mask the ROI only
# for residual computation
if evlist_info['was_list']:
msg = 'Masking ROI from original event list'
self._log_string(gammalib.EXPLICIT, msg)
cube = self._masked_cube(cube, evlist_info['roi_ra'],
evlist_info['roi_dec'],
evlist_info['roi_rad'],
emin=evlist_info['emin'],
emax=evlist_info['emax'])
# Apply user mask
if self._mask:
msg = 'Masking ROI requested by user'
self._log_string(gammalib.EXPLICIT, msg)
cube = self._masked_cube(cube, self['ra'], self['dec'],
self['rad'],
regfile=self['regfile'])
# Extract skymap and clip at 0 to null masked areas
counts = cube.counts().copy()
counts = counts.clip(0.)
# Convert skymap into GNdarray count spectrum
counts = counts.counts()
# Return
return counts
def _residuals_table(self, obs_id, ebounds, counts, model, residuals):
"""
Create a Fits Table and store counts, model, and residuals
Parameters
----------
obs_id : str
Observation id
ebounds : `~gammalib.GEbounds()'
Energy boundaries
counts : `~gammalib.GNdarray()'
Counts spectrum
model : `~gammalib.GNdarray()'
Model spectrum
residuals : `~gammalib.GNdarray()'
Residual spectrum
Returns
-------
table : `~gammalib.GFitsBinTable()'
Residual spectrum as FITS binary table
"""
# Create FITS table columns
nrows = ebounds.size()
energy_low = gammalib.GFitsTableDoubleCol('Emin', nrows)
energy_high = gammalib.GFitsTableDoubleCol('Emax', nrows)
counts_col = gammalib.GFitsTableDoubleCol('Counts', nrows)
model_col = gammalib.GFitsTableDoubleCol('Model', nrows)
resid_col = gammalib.GFitsTableDoubleCol('Residuals', nrows)
energy_low.unit('TeV')
energy_high.unit('TeV')
# Fill FITS table columns
for i in range(nrows):
energy_low[i] = ebounds.emin(i).TeV()
energy_high[i] = ebounds.emax(i).TeV()
counts_col[i] = counts[i]
model_col[i] = model[i]
resid_col[i] = residuals[i]
# Initialise FITS Table with extension set to obs id
table = gammalib.GFitsBinTable(nrows)
# If name not empty add leading blank
if obs_id != '':
obs_id = ' ' + obs_id
table.extname('RESIDUALS' + obs_id)
# Add Header card to specify algorithm used for residual computation
table.card('ALGORITHM', self['algorithm'].string(),
'Algorithm used for computation of residuals')
# Append filled columns to fits table
table.append(energy_low)
table.append(energy_high)
table.append(counts_col)
table.append(model_col)
table.append(resid_col)
# Return binary table
return table
def _append_column(self, table, name, data):
"""
Append optional column to residual table
Parameters
----------
table : `~gammalib.GFitsBinTable()'
FITS binary table
name : str
Column name
data : `~gammalib.GEbounds()'
Data to be filled into new column
Returns
-------
table : `~gammalib.GFitsBinTable()'
FITS binary table
"""
# Check size compatibility
if table.nrows() == data.size():
pass
# Otherwise throw error
else:
msg = 'csresspec._append_column: FITS table and data have ' \
'incompatible size.'
raise RuntimeError(msg)
# Create column
column = gammalib.GFitsTableDoubleCol(name, table.nrows())
# Fill data
for i, value in enumerate(data):
column[i] = value
# Append new column to table
table.append(column)
# Return modified table
return table
# Public methods
def run(self):
"""
Run the script
"""
# Switch screen logging on in debug mode
if self._logDebug():
self._log.cout(True)
# Get parameters
self._get_parameters()
# Write observation into logger
self._log_observations(gammalib.NORMAL, self.obs(), 'Observation')
# Stack observations if requested
if self._stack:
self._log_header1(gammalib.TERSE, 'Stacking Observations')
self.obs(self._stack_observations())
# Log processing header
self._log_header1(gammalib.TERSE, 'Processing Observations')
# Loop over observations and calculate residuals
for s, observation in enumerate(self.obs()):
# Retrieve and store obs id
obs_id = observation.id()
# If observation id is empty and there is more than one observation
# replace with incremental number
if obs_id == '' and self.obs().size() > 1:
obs_id = str(s)
# Log processing of observation
if self.obs().size() > 1:
self._log_header2(gammalib.NORMAL,
'Processing observation %s' % obs_id)
# Turn into observation container and assign models
obs = gammalib.GObservations()
obs.append(observation)
obs.models(self.obs().models())
# if 3D observation
if obs[0].classname() == 'GCTAObservation':
# If already binned set the evlist_info dictionary to have
# attribute was_list False
if obs[0].eventtype() == 'CountsCube':
evlist_info = {'was_list': False}
# ... otherwise bin now
else:
# we remember if we binned an event list so that we can
# mask only the ROI for residual calculation
msg = 'Setting up binned observation'
self._log_string(gammalib.NORMAL, msg)
obs, evlist_info = self._bin_evlist(obs)
# Calculate Model and residuals. If model cube is provided load
# it
if self._use_maps:
modcube = gammalib.GCTAEventCube(self['inmodel'].filename())
# ... otherwise calculate it now
else:
msg = 'Computing model cube'
self._log_string(gammalib.NORMAL, msg)
modelcube = ctools.ctmodel(obs)
modelcube['edisp'] = self['edisp'].boolean()
modelcube.run()
modcube = modelcube.cube().copy()
# Extract cntcube for residual computation
cntcube = obs[0].events().copy()
# Derive count spectra from cubes
msg = 'Computing counts, model, and residual spectra'
self._log_string(gammalib.NORMAL, msg)
counts = self._cube_to_spectrum(cntcube, evlist_info)
model = self._cube_to_spectrum(modcube, evlist_info)
# Calculate residuals
residuals = obsutils.residuals(self, counts, model)
# Extract energy bounds
ebounds = cntcube.ebounds()
# Fill results table
msg = 'Filling residual table'
self._log_string(gammalib.NORMAL, msg)
table = self._residuals_table(obs_id, ebounds, counts, model,
residuals)
# Calculate models of individual components if requested
if self['components'].boolean():
for component in obs.models():
# Log component
self._log_value(gammalib.NORMAL,
'Computing model component',
component.name())
# Set model cube models to individual component
model_cont = gammalib.GModels()
model_cont.append(component)
modelcube.obs().models(model_cont)
# Run model cube
modelcube['edisp'] = self['edisp'].boolean()
modelcube.run()
# Extract spectrum of individual component
modcube = modelcube.cube().copy()
model = self._cube_to_spectrum(modcube, evlist_info)
# append component to table
table = self._append_column(table, component.name(),
model)
# otherwise, if On/Off
elif obs[0].classname() == 'GCTAOnOffObservation':
onoff = obs[0]
# Calculate Counts, Model and residuals
msg = 'Computing counts, model, and residual spectra'
self._log_string(gammalib.NORMAL, msg)
# On spectrum
counts = onoff.on_spec().counts_spectrum()
# Model for On region
background = onoff.model_background(obs.models()).counts_spectrum()
alpha = onoff.on_spec().backscal_spectrum()
model = background.copy()
model *= alpha
model += onoff.model_gamma(obs.models()).counts_spectrum()
# On Residuals
residuals = obsutils.residuals(self, counts, model)
# Extract energy bounds
ebounds = onoff.on_spec().ebounds()
# Fill results table
msg = 'Filling residual table'
self._log_string(gammalib.NORMAL, msg)
table = self._residuals_table(obs_id, ebounds, counts, model,
residuals)
# Get Off spectrum and add to table
msg = 'Computing counts, model, and residual spectra for Off regions'
self._log_string(gammalib.NORMAL, msg)
counts_off = onoff.off_spec().counts_spectrum()
table = self._append_column(table, 'Counts_Off',
counts_off)
# Add background/Off model to table
table = self._append_column(table, 'Model_Off',
background)
# Calculate Off residuals and add to table
residuals_off = obsutils.residuals(self, counts_off, background)
table = self._append_column(table, 'Residuals_Off',
residuals_off)
# Calculate models of individual components if requested
if self['components'].boolean():
for component in obs.models():
# If background pass
# We always add the background at the end so that
# we accommodate WSTAT for which the background is not
# mandatory in the model
if component.classname() == 'GCTAModelIrfBackground':
pass
# Otherwise calculate gamma component and append to Table
else:
self._log_value(gammalib.NORMAL,
'Computing model for component',
component.name())
# Create observation container for individual components
model_cont = gammalib.GModels()
model_cont.append(component)
# Calculate gamma model
model = onoff.model_gamma(model_cont)
model = model.counts_spectrum()
# Append to table
table = self._append_column(table, component.name(),
model)
# Add background already calculated
self._log_value(gammalib.NORMAL,
'Computing model for component',
'Background')
background *= onoff.on_spec().backscal_spectrum()
table = self._append_column(table, 'Background',
background)
# Append results table to output file
self._fits.append(table)
# Return
return
def save(self):
"""
Save residuals
"""
# Write header
self._log_header1(gammalib.TERSE, 'Save residuals')
# Continue only if FITS file is valid
if self._fits != None:
# Get outfile parameter
outfile = self['outfile'].filename()
# Log file name
self._log_value(gammalib.NORMAL, 'Residuals file', outfile.url())
# Save residuals
self._fits.saveto(outfile, self['clobber'].boolean())
# Return
return
# ======================== #
# Main routine entry point #
# ======================== #
if __name__ == '__main__':
# Create instance of application
app = csresspec(sys.argv)
# Execute application
app.execute()