NEWS
9.04 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
New Features and Important Changes in ctools 1.7.0
15 July 2020
Introduction
------------
This document briefly summarizes the changes that have been made in this
ctools release with respect to the precedent release.
Configuration
-------------
None
Documentation
-------------
Update user manual to indicate where to get the latest CTA IRF (#3075).
Python interface
----------------
None
Support model
-------------
None
Base classes
------------
The headers in the log files created by cscripts that were derived from the
ctools.cscript base class were repeated. This repetition was not present in
the other base classes due to a reopening of the log file in those classes.
The logic was changed so that the cscripts now behave like the ctools. A log
file is not written by default in Python, the logFileOpen() method needs to
be called for that. And the header is only written once in the log file (#3066).
ctbin - CTA event binning
-------------------------
Add ebingamma parameter and support for POW binning (#2881).
ctbkgcube - CTA background cube generation
------------------------------------------
None
ctbutterfly - Generate butterfly diagrams
-----------------------------------------
None
ctcubemask - CTA cube filtering
-------------------------------
None
ctedispcube - CTA energy dispersion cube generation
---------------------------------------------------
Add ebingamma parameter and support for POW binning (#2881).
cterror - Likelihood profile error computation
----------------------------------------------
None
ctexpcube - CTA exposure cube generation
----------------------------------------
Add ebingamma parameter and support for POW binning (#2881).
ctfindvar - Variability search
------------------------------
None
ctlike - Maximum likelihood fitting
-----------------------------------
None
ctmapcube - CTA map cube generation
-----------------------------------
Add ebingamma parameter and support for POW binning (#2881).
ctmodel - CTA counts cube modelling
-----------------------------------
Add ebingamma parameter and support for POW binning (#2881).
ctobssim - CTA observation simulation
-------------------------------------
None
ctphase - Event phase computation
---------------------------------
None
ctprob - Event probability computation
--------------------------------------
None
ctpsfcube - CTA point spread function cube generation
-----------------------------------------------------
Add ebingamma parameter and support for POW binning (#2881).
ctselect - CTA event selection
------------------------------
None
ctskymap - CTA sky mapping
--------------------------
Added ctskymap::fits() method to allow access of FITS file object before
saving the object to disk. This allows manipulation of ctskymap results without
writing a FITS file (#2925).
cttsmap - Generation of Test Statistic map
------------------------------------------
Remove response cache for test source before fitting the source (#2973).
ctulimit - Compute upper limit
------------------------------
None
support - Support classes
-------------------------
None
csbkgmodel - Generate background model for 3D analysis
------------------------------------------------------
None
cscaldb - Inspect calibration database
--------------------------------------
None
csebins - Generate energy boundaries
------------------------------------
None
csfindobs - Find IACT observations
----------------------------------
None
csiactcopy - Copy IACT observations
-----------------------------------
None
csiactdata - Inspect IACT data store
------------------------------------
None
csiactobs - Inspect IACT observation definition XML file
--------------------------------------------------------
None
cslightcrv - Generate light curve
---------------------------------
None
csmodelinfo - Return model information
--------------------------------------
None
csmodelmerge - Merge models
---------------------------
None
csmodelselect - Select models
-----------------------------
None
csmodelsois - Puts selected sources in diffuse model cube
---------------------------------------------------------
None
csobs2caldb - Generate calibration database entry for an IACT observation
-------------------------------------------------------------------------
None
csobsdef - Generate observation definition XML file
---------------------------------------------------
None
csobsinfo - Return observation definition information
-----------------------------------------------------
None
csobsselect - Select observations
---------------------------------
None
csphagen - Generate On/Off observations
---------------------------------------
The handling of reflected regions in the presence of exclusion regions was
improved. In the presence of exclusion regions, the number of Off regions is
slighty shift in position (#2976).
Setting the exclusion map via csphagen.exclusion_map(object=<map>) will now
actually use the exclusion map even if the "inexclusion" parameter is not set.
Before, the only exclusion that would be used was the exclusion passed via the
"inexclusion" "parameter. If re-running csphagen using the "inexclusion"
parameter after setting the map with csphagen.exclusion_map() you should first
call csphagen.exclusion_map(object=gammalib.GSkyRegionMap()). This makes the
map empty and csphagen then checks the "inexclusion" "parameter (#2925).
Add ebingamma parameter and support for POW binning (#2881).
csphasecrv - Generate phase curve
---------------------------------
None
cspull - Generate pull distributions
------------------------------------
None
csresmap - Generate residual map
--------------------------------
Add ebingamma parameter and support for POW binning (#2881).
csresspec - Generate residual spectrum
--------------------------------------
Add ebingamma parameter and support for POW binning (#2881).
csroot2caldb - Generates calibration database from ROOT file
------------------------------------------------------------
None
csscs - Spectral component separation
-------------------------------------
Add new script that performs a spectral component separation analysis. A
tutorial and reference manual is included that explains how the script
works (#2961).
cssens - Computes sensitivity curve
-----------------------------------
Allow using spectral models without "Prefactor" parameter for sensitivity
computation (#1889).
csspec - Generates Spectral Energy Distribution
-----------------------------------------------
Support to generate Castro plots was added and the relevant information is
now sorted in the output FITS file (#2938).
Add ebingamma parameter and support for POW binning (#2881).
cssrcdetect - Detects sources in sky map
----------------------------------------
The using of a smoothing kernel in the _map_moments() method can lead to
negative squared standard deviations that lead to an exception when the
square root is taken. A filter was introduced that sets all small values
of mean and std to zero, avoiding thus the exception.
cstsdist - Computes Test Statistic distribution
-----------------------------------------------
Allow using spectral models without "Prefactor" parameter for computation of
TS distribution (#1889).
cstsmapmerge - Merge Test Statistic maps
----------------------------------------
None
cstsmapsplit - Prepare split Test Statistic computation
-------------------------------------------------------
None
csviscube - Generate visibility cube
------------------------------------
Moon contraints were added to compute a more accurate visibility cube. So far
there are two constraints:
- moonzenith, which specifies a minimum allow zenith angle for the Moon. In
other words, if the Moon is higher in the sky than the specified zenith
angle, the corresponding times are excluded from the visibility cube.
- maxfli, which specifies the maximum fraction of lunar illumination. If the
Moon has an illumination that is equal or larger than this fraction, the
corresponding times are excluded from the visibility cube.
(#3065).
csworkflow - Execute workflow
-----------------------------
None
calutils - Calibration utilities
--------------------------------
None
ioutils - Input/Output utilities
--------------------------------
None
modutils - Model utilities
--------------------------
Allow using spectral models without "Prefactor" parameter as test source in
test_source() function. Add normalisation_parameter() function to retrieve
spectral normalisation parameter from any model (#1889).
mputils - Multiprocessing utilities
-----------------------------------
None
obsutils - Observation utilities
--------------------------------
None
Examples
--------
In show_pull_histogram.py relpaced the call to mlab.normpdf() by a direct
computation of the normalisation, so that the code also works for matplotlib
> 3.1.0 (#3156).
The show_viscube.py script was added to display a visibility cube (#3065).
The example scripts show_butterfly.py, show_spectrum.py, show_residuals.py
and show_significance_distribution.py can now be run using objects that only
exist in memory (#2925).
caldb
-----
None
models
------
None