Commit b7130ada1b6587ebddc953ee574551379de51e87
1 parent
60b94c5c
Add "NODES" method to csspec to support non-CTA analysis (#1927)
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213 additions
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21 deletions
ChangeLog
| ... | ... | @@ -9,6 +9,7 @@ |
| 9 | 9 | Add keywords to sky maps produced by ctskymap (#2194) |
| 10 | 10 | Enhance efficiency of computations in ctmodel (#2189) |
| 11 | 11 | Add csmodelsois script (#2180) |
| 12 | + Add "NODES" method to csspec to support non-CTA analysis (#1927) | |
| 12 | 13 | Use t-type parameters for all "tmin" and "tmax" parameters (#1864) |
| 13 | 14 | |
| 14 | 15 | ... | ... |
NEWS
| ... | ... | @@ -140,6 +140,13 @@ for classical On/Off IACT analysis (#2208). |
| 140 | 140 | |
| 141 | 141 | The csspec script now can also handle On/Off spectra for SED generation (#2231). |
| 142 | 142 | |
| 143 | +The csspec script now can also handle non-CTA data. For that purpose a "method" | |
| 144 | +parameter has been introduced that allows to selected between slicing of the data | |
| 145 | +(method="SLICE"), which is only supported for CTA observations, and replacing of | |
| 146 | +the spectral model by a node function (method="NODES"). If method="AUTO" the tool | |
| 147 | +will use "SLICE" for observations containing only CTA data and "NODES" for observations | |
| 148 | +containing other data (#1927). | |
| 149 | + | |
| 143 | 150 | |
| 144 | 151 | Examples |
| 145 | 152 | -------- | ... | ... |
cscripts/csspec.par
| ... | ... | @@ -31,6 +31,7 @@ outfile, f, a, spectrum.fits,,, "Output spectrum file" |
| 31 | 31 | # |
| 32 | 32 | # Script parameters |
| 33 | 33 | #================== |
| 34 | +method, s, a, AUTO,SLICE|NODES|AUTO,, "Spectrum generation method" | |
| 34 | 35 | emin, r, a, 0.1,,, "Lower energy limit (TeV)" |
| 35 | 36 | emax, r, a, 100.0,,, "Upper energy limit (TeV)" |
| 36 | 37 | enumbins, i, a, 20,,, "Number of energy bins" | ... | ... |
cscripts/csspec.py
| ... | ... | @@ -29,7 +29,7 @@ import ctools |
| 29 | 29 | class csspec(ctools.cscript): |
| 30 | 30 | """ |
| 31 | 31 | Generates a spectrum |
| 32 | - | |
| 32 | + | |
| 33 | 33 | This class implements the generation of a spectral energy distribution |
| 34 | 34 | from data. |
| 35 | 35 | """ |
| ... | ... | @@ -48,6 +48,7 @@ class csspec(ctools.cscript): |
| 48 | 48 | self._fits = None |
| 49 | 49 | self._binned_mode = False |
| 50 | 50 | self._onoff_mode = False |
| 51 | + self._method = 'AUTO' | |
| 51 | 52 | |
| 52 | 53 | # Initialise observation container from constructor arguments |
| 53 | 54 | self._obs, argv = self._set_input_obs(argv) |
| ... | ... | @@ -75,16 +76,6 @@ class csspec(ctools.cscript): |
| 75 | 76 | if self._obs == None or self._obs.size() == 0: |
| 76 | 77 | self._require_inobs('csspec::get_parameters()') |
| 77 | 78 | self._obs = self._get_observations() |
| 78 | - # if we have one binned CTA observation, i.e. if we are in | |
| 79 | - # binned mode | |
| 80 | - #self._binned_mode = False | |
| 81 | - #self._onoff_mode = False | |
| 82 | - #if self._obs.size() == 1: | |
| 83 | - # if self._obs[0].classname() == 'GCTAObservation': | |
| 84 | - # if self._obs[0].eventtype() == 'CountsCube': | |
| 85 | - # self._binned_mode = True | |
| 86 | - # elif self._obs[0].classname() == 'GCTAOnOffObservation': | |
| 87 | - # self._onoff_mode = True | |
| 88 | 79 | |
| 89 | 80 | # Set models if we have none |
| 90 | 81 | if self._obs.models().size() == 0: |
| ... | ... | @@ -106,6 +97,8 @@ class csspec(ctools.cscript): |
| 106 | 97 | n_unbinned += 1 |
| 107 | 98 | elif obs.classname() == 'GCTAOnOffObservation': |
| 108 | 99 | n_onoff += 1 |
| 100 | + n_cta = n_unbinned + n_binned + n_onoff | |
| 101 | + n_other = self._obs.size() - n_cta | |
| 109 | 102 | |
| 110 | 103 | # Set script mode according to CTA observations |
| 111 | 104 | if n_unbinned == 0 and n_binned != 0 and n_onoff == 0: |
| ... | ... | @@ -126,6 +119,9 @@ class csspec(ctools.cscript): |
| 126 | 119 | # Set ebounds |
| 127 | 120 | self._set_ebounds() |
| 128 | 121 | |
| 122 | + # Get method | |
| 123 | + self._method = self['method'].string() | |
| 124 | + | |
| 129 | 125 | # Query other parameeters |
| 130 | 126 | self['edisp'].boolean() |
| 131 | 127 | self['calc_ulim'].boolean() |
| ... | ... | @@ -140,6 +136,35 @@ class csspec(ctools.cscript): |
| 140 | 136 | # Write input parameters into logger |
| 141 | 137 | self._log_parameters(gammalib.TERSE) |
| 142 | 138 | |
| 139 | + # Write spectrum method header and parameters | |
| 140 | + self._log_header1(gammalib.TERSE, 'Spectrum method') | |
| 141 | + self._log_value(gammalib.TERSE, 'Unbinned CTA observations', n_unbinned) | |
| 142 | + self._log_value(gammalib.TERSE, 'Binned CTA observations', n_binned) | |
| 143 | + self._log_value(gammalib.TERSE, 'On/off CTA observations', n_onoff) | |
| 144 | + self._log_value(gammalib.TERSE, 'Other observations', n_other) | |
| 145 | + | |
| 146 | + # If there are a mix of CTA and non-CTA observations and the method | |
| 147 | + # is 'SLICE' then log a warning that non-CTA observations will be | |
| 148 | + # ignored | |
| 149 | + if n_cta > 0 and n_other > 0 and self._method == 'SLICE': | |
| 150 | + self._log_string(TERSE, '\nWARNING: Only CTA observation can be ' | |
| 151 | + 'handled with the "SLICE" method, all ' | |
| 152 | + 'non-CTA observation will be ignored.') | |
| 153 | + | |
| 154 | + # If there are only non-CTA observations and the method is 'SLICE' | |
| 155 | + # then stop now | |
| 156 | + elif n_other > 0: | |
| 157 | + if self._method == 'SLICE': | |
| 158 | + msg = 'Selected "SLICE" method but none of the observations ' \ | |
| 159 | + 'is a CTA observation. Please select "AUTO" or "NODES" ' \ | |
| 160 | + 'if no CTA observation is provided.' | |
| 161 | + raise RuntimeError(msg) | |
| 162 | + else: | |
| 163 | + self._method = 'NODES' | |
| 164 | + | |
| 165 | + # Log selected spectrum method | |
| 166 | + self._log_value(gammalib.TERSE, 'Selected spectrum method', self._method) | |
| 167 | + | |
| 143 | 168 | # Return |
| 144 | 169 | return |
| 145 | 170 | |
| ... | ... | @@ -311,6 +336,56 @@ class csspec(ctools.cscript): |
| 311 | 336 | # Return |
| 312 | 337 | return |
| 313 | 338 | |
| 339 | + def _set_replace_src_spectrum_by_nodes(self): | |
| 340 | + """ | |
| 341 | + Replace source spectrum by node function | |
| 342 | + """ | |
| 343 | + # Initialise model container | |
| 344 | + models = gammalib.GModels() | |
| 345 | + | |
| 346 | + # Loop over model containers | |
| 347 | + for model in self._obs.models(): | |
| 348 | + | |
| 349 | + # If we deal with source model then replace the spectral model | |
| 350 | + # by a node function | |
| 351 | + if model.name() == self['srcname'].string(): | |
| 352 | + | |
| 353 | + # Setup energies at log mean energies of bins | |
| 354 | + energies = gammalib.GEnergies() | |
| 355 | + for i in range(self._ebounds.size()): | |
| 356 | + energies.append(self._ebounds.elogmean(i)) | |
| 357 | + | |
| 358 | + # Setup spectral node function | |
| 359 | + spectrum = gammalib.GModelSpectralNodes(model.spectral(), energies) | |
| 360 | + spectrum.autoscale() | |
| 361 | + | |
| 362 | + # Make sure that all nodes are positive | |
| 363 | + for i in range(spectrum.nodes()): | |
| 364 | + par = spectrum[i*2+1] | |
| 365 | + value = par.value() | |
| 366 | + min = 1.0e-30 * value | |
| 367 | + if min <= 0.0: | |
| 368 | + min = 1.0e-50 | |
| 369 | + if min < value: | |
| 370 | + value = min | |
| 371 | + par.value(value) | |
| 372 | + par.min(min) | |
| 373 | + | |
| 374 | + # Set spectral component of source model | |
| 375 | + model.spectral(spectrum) | |
| 376 | + | |
| 377 | + # Append model | |
| 378 | + models.append(model) | |
| 379 | + | |
| 380 | + # ... otherwise just append model | |
| 381 | + else: | |
| 382 | + models.append(model) | |
| 383 | + | |
| 384 | + # Put new model in observation containers | |
| 385 | + self._obs.models(models) | |
| 386 | + | |
| 387 | + # Return | |
| 388 | + return | |
| 314 | 389 | |
| 315 | 390 | def _select_onoff_obs(self, obs, emin, emax): |
| 316 | 391 | """ |
| ... | ... | @@ -444,10 +519,10 @@ class csspec(ctools.cscript): |
| 444 | 519 | |
| 445 | 520 | # Use ctselect for unbinned analysis |
| 446 | 521 | else: |
| 447 | - | |
| 522 | + | |
| 448 | 523 | # Write header |
| 449 | 524 | self._log_header3(gammalib.EXPLICIT, 'Selecting events') |
| 450 | - | |
| 525 | + | |
| 451 | 526 | # Select events |
| 452 | 527 | select = ctools.ctselect(self._obs) |
| 453 | 528 | select['ra'] = 'UNDEFINED' |
| ... | ... | @@ -458,7 +533,7 @@ class csspec(ctools.cscript): |
| 458 | 533 | select['tmin'] = 'UNDEFINED' |
| 459 | 534 | select['tmax'] = 'UNDEFINED' |
| 460 | 535 | select.run() |
| 461 | - | |
| 536 | + | |
| 462 | 537 | # Retrieve observation |
| 463 | 538 | obs = select.obs().copy() |
| 464 | 539 | |
| ... | ... | @@ -610,6 +685,95 @@ class csspec(ctools.cscript): |
| 610 | 685 | # Return results |
| 611 | 686 | return results |
| 612 | 687 | |
| 688 | + def _fit_model(self): | |
| 689 | + """ | |
| 690 | + Fit model to observations | |
| 691 | + | |
| 692 | + Returns | |
| 693 | + ------- | |
| 694 | + results : list of dict | |
| 695 | + List of dictionaries with fit results | |
| 696 | + """ | |
| 697 | + # Write header | |
| 698 | + self._log_header1(gammalib.TERSE, 'Generate spectrum') | |
| 699 | + | |
| 700 | + # Write header for fitting | |
| 701 | + self._log_header3(gammalib.EXPLICIT, 'Performing fit') | |
| 702 | + | |
| 703 | + # Perform maximum likelihood fit | |
| 704 | + like = ctools.ctlike(self._obs) | |
| 705 | + like['edisp'] = self['edisp'].boolean() | |
| 706 | + like.run() | |
| 707 | + | |
| 708 | + # Initialise fit results | |
| 709 | + results = [] | |
| 710 | + | |
| 711 | + # Extract fit results | |
| 712 | + model = like.obs().models()[self['srcname'].string()] | |
| 713 | + spectrum = model.spectral() | |
| 714 | + ts = model.ts() | |
| 715 | + | |
| 716 | + # Loop over all nodes | |
| 717 | + for i in range(spectrum.nodes()): | |
| 718 | + | |
| 719 | + # Get energy boundaries | |
| 720 | + emin = self._ebounds.emin(i) | |
| 721 | + emax = self._ebounds.emax(i) | |
| 722 | + elogmean = self._ebounds.elogmean(i) | |
| 723 | + | |
| 724 | + # Initialise dictionary | |
| 725 | + result = {'energy': elogmean.TeV(), | |
| 726 | + 'energy_low': (elogmean - emin).TeV(), | |
| 727 | + 'energy_high': (emax - elogmean).TeV(), | |
| 728 | + 'flux': 0.0, | |
| 729 | + 'flux_err': 0.0, | |
| 730 | + 'TS': 0.0, | |
| 731 | + 'ulimit': 0.0, | |
| 732 | + 'Npred': 0.0} | |
| 733 | + | |
| 734 | + # Convert differential flux and flux error to nuFnu | |
| 735 | + norm = elogmean.MeV() * elogmean.MeV() * gammalib.MeV2erg | |
| 736 | + result['flux'] = spectrum[i*2+1].value() * norm | |
| 737 | + result['flux_err'] = spectrum[i*2+1].error() * norm | |
| 738 | + | |
| 739 | + # Compute TS | |
| 740 | + if self['calc_ts'].boolean(): | |
| 741 | + | |
| 742 | + # Copy observation container | |
| 743 | + obs = like.obs().copy() | |
| 744 | + | |
| 745 | + # Set intensity of node to tiny value | |
| 746 | + par = obs.models()[self['srcname'].string()].spectral()[i*2+1] | |
| 747 | + value = 1.0e-30 * par.value() | |
| 748 | + if par.min() > value: | |
| 749 | + par.min(value) | |
| 750 | + par.value(value) | |
| 751 | + par.fix() | |
| 752 | + | |
| 753 | + # Perform maximum likelihood fit | |
| 754 | + tslike = ctools.ctlike(obs) | |
| 755 | + tslike['edisp'] = self['edisp'].boolean() | |
| 756 | + tslike.run() | |
| 757 | + | |
| 758 | + # Store Test Statistic | |
| 759 | + model = tslike.obs().models()[self['srcname'].string()] | |
| 760 | + result['TS'] = ts - model.ts() | |
| 761 | + | |
| 762 | + # Log information | |
| 763 | + value = '%e +/- %e' % (result['flux'], result['flux_err']) | |
| 764 | + if self['calc_ulim'].boolean() and result['ulimit'] > 0.0: | |
| 765 | + value += ' [< %e]' % (result['ulimit']) | |
| 766 | + value += ' erg/cm2/s' | |
| 767 | + if self['calc_ts'].boolean() and result['TS'] > 0.0: | |
| 768 | + value += ' (TS = %.3f)' % (result['TS']) | |
| 769 | + self._log_value(gammalib.TERSE, 'Bin '+str(i+1), value) | |
| 770 | + | |
| 771 | + # Append results | |
| 772 | + results.append(result) | |
| 773 | + | |
| 774 | + # Return results | |
| 775 | + return results | |
| 776 | + | |
| 613 | 777 | def _create_fits(self, results): |
| 614 | 778 | """ |
| 615 | 779 | Create FITS file |
| ... | ... | @@ -688,14 +852,26 @@ class csspec(ctools.cscript): |
| 688 | 852 | # Write input observation container into logger |
| 689 | 853 | self._log_observations(gammalib.NORMAL, self._obs, 'Input observation') |
| 690 | 854 | |
| 855 | + # Write spectral binning into logger | |
| 856 | + self._log_spectral_binning() | |
| 857 | + | |
| 691 | 858 | # Adjust model parameters dependent on input user parameters |
| 692 | 859 | self._adjust_model_pars() |
| 693 | 860 | |
| 694 | - # Write spectral binning into logger | |
| 695 | - self._log_spectral_binning() | |
| 861 | + # Case A: "SLICE" method | |
| 862 | + if self._method == 'SLICE': | |
| 696 | 863 | |
| 697 | - # Fit energy bins | |
| 698 | - results = self._fit_energy_bins() | |
| 864 | + # Fit energy bins | |
| 865 | + results = self._fit_energy_bins() | |
| 866 | + | |
| 867 | + # Case B: "NODES" method | |
| 868 | + elif self._method == 'NODES': | |
| 869 | + | |
| 870 | + # Replace source spectrum by nodes function | |
| 871 | + self._set_replace_src_spectrum_by_nodes() | |
| 872 | + | |
| 873 | + # Fit model | |
| 874 | + results = self._fit_model() | |
| 699 | 875 | |
| 700 | 876 | # Create FITS file |
| 701 | 877 | self._create_fits(results) |
| ... | ... | @@ -738,7 +914,7 @@ class csspec(ctools.cscript): |
| 738 | 914 | |
| 739 | 915 | # Get outmap parameter |
| 740 | 916 | outfile = self['outfile'].filename() |
| 741 | - | |
| 917 | + | |
| 742 | 918 | # Log file name |
| 743 | 919 | self._log_value(gammalib.NORMAL, 'Spectrum file', outfile.url()) |
| 744 | 920 | ... | ... |
doc/source/admin/release_history/1.5.rst
| ... | ... | @@ -31,6 +31,8 @@ Improvements |
| 31 | 31 | Add keywords to sky maps produced by :ref:`ctskymap` |
| 32 | 32 | * [`2189 <https://cta-redmine.irap.omp.eu/issues/2189>`_] - |
| 33 | 33 | Enhance efficiency of computations in :ref:`ctmodel` |
| 34 | +* [`1927 <https://cta-redmine.irap.omp.eu/issues/1927>`_] - | |
| 35 | + Add ``NODES`` method to :ref:`csspec` to support non-CTA analysis | |
| 34 | 36 | |
| 35 | 37 | |
| 36 | 38 | New features | ... | ... |
doc/source/users/reference_manual/csspec.rst
| ... | ... | @@ -79,8 +79,13 @@ General parameters |
| 79 | 79 | Name of the source in the source model XML file which should be used |
| 80 | 80 | for sensitivity computation. |
| 81 | 81 | |
| 82 | -``outfile [file]`` | |
| 83 | - Output source spectrum file. | |
| 82 | +``outfile <SLICE|NODES|AUTO> [file]`` | |
| 83 | + Spectrum generation method. | |
| 84 | + ``SLICE``: Slice energy interval into ``enumbins`` independent bins. | |
| 85 | + ``NODES``: Replace spectral model by node function with ``enumbins`` nodes. | |
| 86 | + ``AUTO`` : Automatically select method based on input data. Will use ``SLICE`` | |
| 87 | + for CTA-only observations and ``NODES`` for observations including | |
| 88 | + non-CTA data. | |
| 84 | 89 | |
| 85 | 90 | ``emin [real]`` |
| 86 | 91 | Lower energy limit of events (in TeV). | ... | ... |