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ChangeLog
NEWS
| 1 | -New Features and Important Changes in ctools 1.7.0 | |
| 1 | +New Features and Important Changes in ctools 1.7.1 | |
| 2 | 2 | |
| 3 | -15 July 2020 | |
| 3 | +20 July 2020 | |
| 4 | 4 | |
| 5 | 5 | |
| 6 | 6 | Introduction |
| ... | ... | @@ -16,12 +16,7 @@ None |
| 16 | 16 | |
| 17 | 17 | Documentation |
| 18 | 18 | ------------- |
| 19 | -Add Interface Manual to User documentation that provides links to the | |
| 20 | -ctools and GammaLib Doxygen documentation (#3163). | |
| 21 | - | |
| 22 | -Add On/Off analysis to ctlike reference manual (#3154). | |
| 23 | - | |
| 24 | -Update user manual to indicate where to get the latest CTA IRF (#3075). | |
| 19 | +None | |
| 25 | 20 | |
| 26 | 21 | |
| 27 | 22 | Python interface |
| ... | ... | @@ -36,17 +31,13 @@ None |
| 36 | 31 | |
| 37 | 32 | Base classes |
| 38 | 33 | ------------ |
| 39 | -The headers in the log files created by cscripts that were derived from the | |
| 40 | -ctools.cscript base class were repeated. This repetition was not present in | |
| 41 | -the other base classes due to a reopening of the log file in those classes. | |
| 42 | -The logic was changed so that the cscripts now behave like the ctools. A log | |
| 43 | -file is not written by default in Python, the logFileOpen() method needs to | |
| 44 | -be called for that. And the header is only written once in the log file (#3066). | |
| 34 | +None | |
| 45 | 35 | |
| 46 | 36 | |
| 47 | 37 | ctbin - CTA event binning |
| 48 | 38 | ------------------------- |
| 49 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 39 | +The code was refactored so that parallel processing using OpenMP is now | |
| 40 | +considerably faster when data are stacked (#3275). | |
| 50 | 41 | |
| 51 | 42 | |
| 52 | 43 | ctbkgcube - CTA background cube generation |
| ... | ... | @@ -66,7 +57,7 @@ None |
| 66 | 57 | |
| 67 | 58 | ctedispcube - CTA energy dispersion cube generation |
| 68 | 59 | --------------------------------------------------- |
| 69 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 60 | +None | |
| 70 | 61 | |
| 71 | 62 | |
| 72 | 63 | cterror - Likelihood profile error computation |
| ... | ... | @@ -76,7 +67,7 @@ None |
| 76 | 67 | |
| 77 | 68 | ctexpcube - CTA exposure cube generation |
| 78 | 69 | ---------------------------------------- |
| 79 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 70 | +None | |
| 80 | 71 | |
| 81 | 72 | |
| 82 | 73 | ctfindvar - Variability search |
| ... | ... | @@ -91,12 +82,12 @@ None |
| 91 | 82 | |
| 92 | 83 | ctmapcube - CTA map cube generation |
| 93 | 84 | ----------------------------------- |
| 94 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 85 | +None | |
| 95 | 86 | |
| 96 | 87 | |
| 97 | 88 | ctmodel - CTA counts cube modelling |
| 98 | 89 | ----------------------------------- |
| 99 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 90 | +None | |
| 100 | 91 | |
| 101 | 92 | |
| 102 | 93 | ctobssim - CTA observation simulation |
| ... | ... | @@ -116,7 +107,7 @@ None |
| 116 | 107 | |
| 117 | 108 | ctpsfcube - CTA point spread function cube generation |
| 118 | 109 | ----------------------------------------------------- |
| 119 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 110 | +None | |
| 120 | 111 | |
| 121 | 112 | |
| 122 | 113 | ctselect - CTA event selection |
| ... | ... | @@ -126,14 +117,12 @@ None |
| 126 | 117 | |
| 127 | 118 | ctskymap - CTA sky mapping |
| 128 | 119 | -------------------------- |
| 129 | -Added ctskymap::fits() method to allow access of FITS file object before | |
| 130 | -saving the object to disk. This allows manipulation of ctskymap results without | |
| 131 | -writing a FITS file (#2925). | |
| 120 | +None | |
| 132 | 121 | |
| 133 | 122 | |
| 134 | 123 | cttsmap - Generation of Test Statistic map |
| 135 | 124 | ------------------------------------------ |
| 136 | -Remove response cache for test source before fitting the source (#2973). | |
| 125 | +None | |
| 137 | 126 | |
| 138 | 127 | |
| 139 | 128 | ctulimit - Compute upper limit |
| ... | ... | @@ -228,19 +217,7 @@ None |
| 228 | 217 | |
| 229 | 218 | csphagen - Generate On/Off observations |
| 230 | 219 | --------------------------------------- |
| 231 | -The handling of reflected regions in the presence of exclusion regions was | |
| 232 | -improved. In the presence of exclusion regions, the number of Off regions is | |
| 233 | -slighty shift in position (#2976). | |
| 234 | - | |
| 235 | -Setting the exclusion map via csphagen.exclusion_map(object=<map>) will now | |
| 236 | -actually use the exclusion map even if the "inexclusion" parameter is not set. | |
| 237 | -Before, the only exclusion that would be used was the exclusion passed via the | |
| 238 | -"inexclusion" "parameter. If re-running csphagen using the "inexclusion" | |
| 239 | -parameter after setting the map with csphagen.exclusion_map() you should first | |
| 240 | -call csphagen.exclusion_map(object=gammalib.GSkyRegionMap()). This makes the | |
| 241 | -map empty and csphagen then checks the "inexclusion" "parameter (#2925). | |
| 242 | - | |
| 243 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 220 | +None | |
| 244 | 221 | |
| 245 | 222 | |
| 246 | 223 | csphasecrv - Generate phase curve |
| ... | ... | @@ -255,12 +232,12 @@ None |
| 255 | 232 | |
| 256 | 233 | csresmap - Generate residual map |
| 257 | 234 | -------------------------------- |
| 258 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 235 | +None | |
| 259 | 236 | |
| 260 | 237 | |
| 261 | 238 | csresspec - Generate residual spectrum |
| 262 | 239 | -------------------------------------- |
| 263 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 240 | +None | |
| 264 | 241 | |
| 265 | 242 | |
| 266 | 243 | csroot2caldb - Generates calibration database from ROOT file |
| ... | ... | @@ -270,39 +247,27 @@ None |
| 270 | 247 | |
| 271 | 248 | csscs - Spectral component separation |
| 272 | 249 | ------------------------------------- |
| 273 | -Add new script that performs a spectral component separation analysis. A | |
| 274 | -tutorial and reference manual is included that explains how the script | |
| 275 | -works (#2961). | |
| 250 | +None | |
| 276 | 251 | |
| 277 | 252 | |
| 278 | 253 | cssens - Computes sensitivity curve |
| 279 | 254 | ----------------------------------- |
| 280 | -Allow using spectral models without "Prefactor" parameter for sensitivity | |
| 281 | -computation (#1889). | |
| 255 | +None | |
| 282 | 256 | |
| 283 | 257 | |
| 284 | 258 | csspec - Generates Spectral Energy Distribution |
| 285 | 259 | ----------------------------------------------- |
| 286 | -Support to generate Castro plots was added and the relevant information is | |
| 287 | -now sorted in the output FITS file (#2938). | |
| 288 | - | |
| 289 | -Add ebingamma parameter and support for POW binning (#2881). | |
| 260 | +None | |
| 290 | 261 | |
| 291 | 262 | |
| 292 | 263 | cssrcdetect - Detects sources in sky map |
| 293 | 264 | ---------------------------------------- |
| 294 | -The using of a smoothing kernel in the _map_moments() method can lead to | |
| 295 | -negative squared standard deviations that lead to an exception when the square | |
| 296 | -root is taken. To avoid negative values, the minimum pixel values for the | |
| 297 | -standard deviation map is computed and, if the minimum value is negative, | |
| 298 | -subtracted from the standard deviation map. Therefore, by definition, the | |
| 299 | -standard deviation map is non negative for all pixels (#3261). | |
| 265 | +None | |
| 300 | 266 | |
| 301 | 267 | |
| 302 | 268 | cstsdist - Computes Test Statistic distribution |
| 303 | 269 | ----------------------------------------------- |
| 304 | -Allow using spectral models without "Prefactor" parameter for computation of | |
| 305 | -TS distribution (#1889). | |
| 270 | +None | |
| 306 | 271 | |
| 307 | 272 | |
| 308 | 273 | cstsmapmerge - Merge Test Statistic maps |
| ... | ... | @@ -317,15 +282,7 @@ None |
| 317 | 282 | |
| 318 | 283 | csviscube - Generate visibility cube |
| 319 | 284 | ------------------------------------ |
| 320 | -Moon contraints were added to compute a more accurate visibility cube. So far | |
| 321 | -there are two constraints: | |
| 322 | -- moonzenith, which specifies a minimum allow zenith angle for the Moon. In | |
| 323 | - other words, if the Moon is higher in the sky than the specified zenith | |
| 324 | - angle, the corresponding times are excluded from the visibility cube. | |
| 325 | -- maxfli, which specifies the maximum fraction of lunar illumination. If the | |
| 326 | - Moon has an illumination that is equal or larger than this fraction, the | |
| 327 | - corresponding times are excluded from the visibility cube. | |
| 328 | -(#3065). | |
| 285 | +None | |
| 329 | 286 | |
| 330 | 287 | |
| 331 | 288 | csworkflow - Execute workflow |
| ... | ... | @@ -345,9 +302,7 @@ None |
| 345 | 302 | |
| 346 | 303 | modutils - Model utilities |
| 347 | 304 | -------------------------- |
| 348 | -Allow using spectral models without "Prefactor" parameter as test source in | |
| 349 | -test_source() function. Add normalisation_parameter() function to retrieve | |
| 350 | -spectral normalisation parameter from any model (#1889). | |
| 305 | +None | |
| 351 | 306 | |
| 352 | 307 | |
| 353 | 308 | mputils - Multiprocessing utilities |
| ... | ... | @@ -357,20 +312,12 @@ None |
| 357 | 312 | |
| 358 | 313 | obsutils - Observation utilities |
| 359 | 314 | -------------------------------- |
| 360 | -Fix numerical glitch in residual computation in residuals() function (#2765). | |
| 315 | +None | |
| 361 | 316 | |
| 362 | 317 | |
| 363 | 318 | Examples |
| 364 | 319 | -------- |
| 365 | -In show_pull_histogram.py relpaced the call to mlab.normpdf() by a direct | |
| 366 | -computation of the normalisation, so that the code also works for matplotlib | |
| 367 | -> 3.1.0 (#3156). | |
| 368 | - | |
| 369 | -The show_viscube.py script was added to display a visibility cube (#3065). | |
| 370 | - | |
| 371 | -The example scripts show_butterfly.py, show_spectrum.py, show_residuals.py | |
| 372 | -and show_significance_distribution.py can now be run using objects that only | |
| 373 | -exist in memory (#2925). | |
| 320 | +None | |
| 374 | 321 | |
| 375 | 322 | |
| 376 | 323 | caldb | ... | ... |
doc/source/admin/release_history/1.7.1.rst
0 → 100644
| 1 | +.. _1.7.1: | |
| 2 | + | |
| 3 | +ctools 1.7.1 release (20 July 2020) | |
| 4 | +=================================== | |
| 5 | + | |
| 6 | +Overview | |
| 7 | +-------- | |
| 8 | + | |
| 9 | +ctools 1.7.1 is a bug fix release for ctools release 1.7. | |
| 10 | + | |
| 11 | +The following bugs were fixed: | |
| 12 | + | |
| 13 | +* ... | |
| 14 | + | |
| 15 | + | |
| 16 | +The following improvements were done: | |
| 17 | + | |
| 18 | +* [`3275 <https://cta-redmine.irap.omp.eu/issues/3275>`_] - | |
| 19 | + Speed-up ctbin for stacked event binning | ... | ... |