Commit 3186c66e81ccba1c3eabdebfbc603ed71196fa1c
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48526cfc
Update CTA developed test scripts
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429 additions
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1 deletions
inst/cta/test/dev/README.md
| @@ -32,16 +32,38 @@ if needed. | @@ -32,16 +32,38 @@ if needed. | ||
| 32 | > matplotlib is installed, the simulated photons are shown as | 32 | > matplotlib is installed, the simulated photons are shown as |
| 33 | > a spectrum. | 33 | > a spectrum. |
| 34 | 34 | ||
| 35 | +`show_model_mc.py` | ||
| 36 | +> For a given model, compares Monte Carlo simulation to model | ||
| 37 | +> ecaluation. | ||
| 38 | + | ||
| 39 | +`test_background_integration.py` | ||
| 40 | +> Test the event simulation using GCTAModelBackground. | ||
| 41 | + | ||
| 42 | +`test_cta_bkgcube.py` | ||
| 43 | +> Test energy integration of GCTABackground3D. | ||
| 44 | + | ||
| 35 | `test_gauss.py` | 45 | `test_gauss.py` |
| 36 | > Test Gaussian. | 46 | > Test Gaussian. |
| 37 | 47 | ||
| 48 | +`test_irf_elliptical.py` | ||
| 49 | +> Test the response computation for elliptical models. | ||
| 50 | + | ||
| 38 | `test_irf_offset.py` | 51 | `test_irf_offset.py` |
| 39 | > Creates images of source models for various offset angles. This | 52 | > Creates images of source models for various offset angles. This |
| 40 | > tests the IRF variation with offset angle. | 53 | > tests the IRF variation with offset angle. |
| 41 | 54 | ||
| 55 | +`test_irf_radial.py` | ||
| 56 | +> Test the response computation for radial models. | ||
| 57 | + | ||
| 42 | `test_irf_trafo.py` | 58 | `test_irf_trafo.py` |
| 43 | > Test coordinate transformations for IRF computation. | 59 | > Test coordinate transformations for IRF computation. |
| 44 | 60 | ||
| 61 | +`test_likelihood_profile.py` | ||
| 62 | +> Performs likelihood profile computation. | ||
| 63 | + | ||
| 64 | +`test_ml_fitting.py` | ||
| 65 | +> Performs a binned maximum likelihood analysis. | ||
| 66 | + | ||
| 45 | `test_model.py` | 67 | `test_model.py` |
| 46 | > Creates images of sources models convolved with the CTA instrument | 68 | > Creates images of sources models convolved with the CTA instrument |
| 47 | > response function. Also allows the creation of gradient images. | 69 | > response function. Also allows the creation of gradient images. |
| @@ -49,15 +71,27 @@ if needed. | @@ -49,15 +71,27 @@ if needed. | ||
| 49 | `test_npred_computation.py` | 71 | `test_npred_computation.py` |
| 50 | > Test the Npred computation of the CTA response. | 72 | > Test the Npred computation of the CTA response. |
| 51 | 73 | ||
| 74 | +`test_npred_elliptical.py` | ||
| 75 | +> Test the Npred computation of the CTA response for elliptical models. | ||
| 76 | + | ||
| 52 | `test_npred_integration.py` | 77 | `test_npred_integration.py` |
| 53 | > Compare numerical to analytical Npred computation for CTA response. | 78 | > Compare numerical to analytical Npred computation for CTA response. |
| 54 | 79 | ||
| 80 | +`test_psf_radial.py` | ||
| 81 | +> Tests the radial response computation. | ||
| 82 | + | ||
| 83 | +`test_psf_shape.py` | ||
| 84 | +> Simulates the PSF distribution. | ||
| 85 | + | ||
| 55 | `test_radial_acceptance.py` | 86 | `test_radial_acceptance.py` |
| 56 | > Displays the various radial acceptance models. | 87 | > Displays the various radial acceptance models. |
| 57 | 88 | ||
| 58 | `test_response_table.py` | 89 | `test_response_table.py` |
| 59 | > Display CTA response table. | 90 | > Display CTA response table. |
| 60 | 91 | ||
| 92 | +`test_shell.py` | ||
| 93 | +> Shows the shell model radial distribution. | ||
| 94 | + | ||
| 61 | `test_sim_edisp.py` | 95 | `test_sim_edisp.py` |
| 62 | > Compares energy dispersion simulation to energy dispersion | 96 | > Compares energy dispersion simulation to energy dispersion |
| 63 | > model. | 97 | > model. |
inst/cta/test/dev/show_model_mc.py
0 → 100755
| 1 | +#! /usr/bin/env python | ||
| 2 | +# ========================================================================== | ||
| 3 | +# Show simulation - model for a given model | ||
| 4 | +# | ||
| 5 | +# Copyright (C) 2018 Juergen Knoedlseder | ||
| 6 | +# | ||
| 7 | +# This program is free software: you can redistribute it and/or modify | ||
| 8 | +# it under the terms of the GNU General Public License as published by | ||
| 9 | +# the Free Software Foundation, either version 3 of the License, or | ||
| 10 | +# (at your option) any later version. | ||
| 11 | +# | ||
| 12 | +# This program is distributed in the hope that it will be useful, | ||
| 13 | +# but WITHOUT ANY WARRANTY; without even the implied warranty of | ||
| 14 | +# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the | ||
| 15 | +# GNU General Public License for more details. | ||
| 16 | +# | ||
| 17 | +# You should have received a copy of the GNU General Public License | ||
| 18 | +# along with this program. If not, see <http://www.gnu.org/licenses/>. | ||
| 19 | +# | ||
| 20 | +# ========================================================================== | ||
| 21 | +import os | ||
| 22 | +import math | ||
| 23 | +import gammalib | ||
| 24 | +import ctools | ||
| 25 | +import cscripts | ||
| 26 | +from cscripts import obsutils | ||
| 27 | +import matplotlib.pyplot as plt | ||
| 28 | + | ||
| 29 | + | ||
| 30 | +# ====================== # | ||
| 31 | +# Plot residual spectrum # | ||
| 32 | +# ====================== # | ||
| 33 | +def plot_resspec(frame, energies, resspec, errspec, emin=0.1, emax=100.0): | ||
| 34 | + """ | ||
| 35 | + Plot residual spectrum | ||
| 36 | + | ||
| 37 | + Parameters | ||
| 38 | + ---------- | ||
| 39 | + frame : pyplot | ||
| 40 | + Frame for spectrum | ||
| 41 | + """ | ||
| 42 | + # Set axes scales and limit | ||
| 43 | + frame.set_xscale('log') | ||
| 44 | + frame.set_xlim([emin, emax]) | ||
| 45 | + | ||
| 46 | + # Counts and model | ||
| 47 | + frame.errorbar(energies, resspec, yerr=errspec, | ||
| 48 | + fmt='ko', capsize=0, linewidth=2, zorder=2, label='Data') | ||
| 49 | + frame.plot(frame.get_xlim(),[0,0], 'r-') | ||
| 50 | + frame.set_xlabel('Energy (TeV)') | ||
| 51 | + frame.set_ylabel('Simulation - Model') | ||
| 52 | + | ||
| 53 | + # Return | ||
| 54 | + return | ||
| 55 | + | ||
| 56 | + | ||
| 57 | +# ================= # | ||
| 58 | +# Plot residual map # | ||
| 59 | +# ================= # | ||
| 60 | +def plot_resmap(plt1, plt2, map, error, steps=1): | ||
| 61 | + """ | ||
| 62 | + Plot pull histogram | ||
| 63 | + | ||
| 64 | + Parameters | ||
| 65 | + ---------- | ||
| 66 | + plt1 : pyplot | ||
| 67 | + Frame for first map | ||
| 68 | + plt2 : pyplot | ||
| 69 | + Frame for second map | ||
| 70 | + map : `~gammalib.GSkyMap()` | ||
| 71 | + Sky map | ||
| 72 | + error : `~gammalib.GSkyMap()` | ||
| 73 | + Sky map | ||
| 74 | + steps : int | ||
| 75 | + Number of steps for rebinning | ||
| 76 | + """ | ||
| 77 | + # Create longitude array from skymap | ||
| 78 | + x_lon = [] | ||
| 79 | + y_lon = [] | ||
| 80 | + e_lon = [] | ||
| 81 | + for ix in range(0, map.nx(), steps): | ||
| 82 | + value = 0.0 | ||
| 83 | + err = 0.0 | ||
| 84 | + for istep in range(steps): | ||
| 85 | + if istep+ix < map.nx(): | ||
| 86 | + for iy in range(map.ny()): | ||
| 87 | + index = istep+ix+iy*map.nx() | ||
| 88 | + value += map[index] | ||
| 89 | + err += error[index]*error[index] | ||
| 90 | + x_lon.append(ix) | ||
| 91 | + y_lon.append(value) | ||
| 92 | + e_lon.append(math.sqrt(err)) | ||
| 93 | + | ||
| 94 | + # Create latitude array from skymap | ||
| 95 | + x_lat = [] | ||
| 96 | + y_lat = [] | ||
| 97 | + e_lat = [] | ||
| 98 | + for iy in range(0, map.ny(), steps): | ||
| 99 | + value = 0.0 | ||
| 100 | + err = 0.0 | ||
| 101 | + for istep in range(steps): | ||
| 102 | + if istep+iy < map.ny(): | ||
| 103 | + for ix in range(map.nx()): | ||
| 104 | + index = ix+(istep+iy)*map.nx() | ||
| 105 | + value += map[index] | ||
| 106 | + err += error[index]*error[index] | ||
| 107 | + x_lat.append(iy) | ||
| 108 | + y_lat.append(value) | ||
| 109 | + e_lat.append(math.sqrt(err)) | ||
| 110 | + | ||
| 111 | + # Plot longitude distribution | ||
| 112 | + plt1.errorbar(x_lon, y_lon, yerr=e_lon, | ||
| 113 | + fmt='ko', capsize=0, linewidth=2, zorder=2) | ||
| 114 | + plt1.axhline(0, color='r', linestyle='--') | ||
| 115 | + plt1.set_xlabel('Right Ascension (pixels)') | ||
| 116 | + plt1.set_ylabel('Simulation - Model') | ||
| 117 | + plt1.grid(True) | ||
| 118 | + | ||
| 119 | + # Plot latitude distribution | ||
| 120 | + plt2.errorbar(x_lat, y_lat, yerr=e_lat, | ||
| 121 | + fmt='ko', capsize=0, linewidth=2, zorder=2) | ||
| 122 | + plt2.axhline(0, color='r', linestyle='--') | ||
| 123 | + plt2.set_xlabel('Declination (pixels)') | ||
| 124 | + plt2.set_ylabel('Simulation - Model') | ||
| 125 | + plt2.grid(True) | ||
| 126 | + | ||
| 127 | + # Return | ||
| 128 | + return | ||
| 129 | + | ||
| 130 | + | ||
| 131 | +# ======== # | ||
| 132 | +# Plot map # | ||
| 133 | +# ======== # | ||
| 134 | +def plot_map(frame, map, smooth=0.0): | ||
| 135 | + """ | ||
| 136 | + Plot Aitoff map | ||
| 137 | + | ||
| 138 | + Parameters | ||
| 139 | + ---------- | ||
| 140 | + frame : pyplot | ||
| 141 | + Frame for map | ||
| 142 | + map : `~gammalib.GSkyMap()` | ||
| 143 | + Sky map | ||
| 144 | + smooth : float, optional | ||
| 145 | + Map smoothing parameter (degrees) | ||
| 146 | + """ | ||
| 147 | + # Optionally smooth map | ||
| 148 | + if smooth > 0.0: | ||
| 149 | + _map = map.copy() | ||
| 150 | + _map.smooth('DISK', smooth) | ||
| 151 | + else: | ||
| 152 | + _map = map | ||
| 153 | + | ||
| 154 | + # Create array from skymap | ||
| 155 | + array = [] | ||
| 156 | + v_max = 0.0 | ||
| 157 | + for iy in range(_map.ny()): | ||
| 158 | + row = [] | ||
| 159 | + for ix in range(_map.nx()): | ||
| 160 | + index = ix+iy*_map.nx() | ||
| 161 | + value = _map[index] | ||
| 162 | + row.append(value) | ||
| 163 | + array.append(row) | ||
| 164 | + | ||
| 165 | + # Show Aitoff projection | ||
| 166 | + c = frame.imshow(array, aspect=1.0) | ||
| 167 | + cbar = plt.colorbar(c, orientation='vertical', shrink=0.7) | ||
| 168 | + frame.grid(True) | ||
| 169 | + frame.set_xlabel('Right Ascension (pixels)') | ||
| 170 | + frame.set_ylabel('Declination (pixels)') | ||
| 171 | + | ||
| 172 | + # Return | ||
| 173 | + return | ||
| 174 | + | ||
| 175 | + | ||
| 176 | +# =========================== # | ||
| 177 | +# Determine spatial residuals # | ||
| 178 | +# =========================== # | ||
| 179 | +def residual_spatial(countscube, modelcube): | ||
| 180 | + """ | ||
| 181 | + Determine spatial residuals | ||
| 182 | + | ||
| 183 | + Parameters | ||
| 184 | + ---------- | ||
| 185 | + countscube : `~gammalib.GCTAEventCube` | ||
| 186 | + Simulated counts cube | ||
| 187 | + modelcube : `~gammalib.GCTAEventCube` | ||
| 188 | + Model cube | ||
| 189 | + | ||
| 190 | + Returns | ||
| 191 | + ------- | ||
| 192 | + map, error : `~gammalib.GSkyMap()` | ||
| 193 | + Residual sky map and error | ||
| 194 | + """ | ||
| 195 | + # Get model cube maps | ||
| 196 | + map1 = countscube.counts() | ||
| 197 | + map2 = modelcube.counts() | ||
| 198 | + | ||
| 199 | + # Generate residual map | ||
| 200 | + map = map1 - map2 | ||
| 201 | + map.stack_maps() | ||
| 202 | + | ||
| 203 | + # Generate residual error bars | ||
| 204 | + error = map2.copy() | ||
| 205 | + error.stack_maps() | ||
| 206 | + error = error.sqrt() | ||
| 207 | + | ||
| 208 | + # Return residual map and error map | ||
| 209 | + return map, error | ||
| 210 | + | ||
| 211 | + | ||
| 212 | +# ============================ # | ||
| 213 | +# Determine spectral residuals # | ||
| 214 | +# ============================ # | ||
| 215 | +def residual_spectral(countscube, modelcube): | ||
| 216 | + """ | ||
| 217 | + Determine spectral residuals | ||
| 218 | + | ||
| 219 | + Parameters | ||
| 220 | + ---------- | ||
| 221 | + countscube : `~gammalib.GCTAEventCube` | ||
| 222 | + Simulated counts cube | ||
| 223 | + modelcube : `~gammalib.GCTAEventCube` | ||
| 224 | + Model cube | ||
| 225 | + | ||
| 226 | + Returns | ||
| 227 | + ------- | ||
| 228 | + map, error : list | ||
| 229 | + Residual vector | ||
| 230 | + """ | ||
| 231 | + # Get model cube maps | ||
| 232 | + map1 = countscube.counts() | ||
| 233 | + map2 = modelcube.counts() | ||
| 234 | + | ||
| 235 | + # Compute spectra | ||
| 236 | + spec1 = [] | ||
| 237 | + spec2 = [] | ||
| 238 | + residual = [] | ||
| 239 | + error = [] | ||
| 240 | + energies = [] | ||
| 241 | + for ieng in range(map1.nmaps()): | ||
| 242 | + sum1 = 0.0 | ||
| 243 | + sum2 = 0.0 | ||
| 244 | + for ipix in range(map1.npix()): | ||
| 245 | + sum1 += map1[ipix, ieng] | ||
| 246 | + sum2 += map2[ipix, ieng] | ||
| 247 | + spec1.append(sum1) | ||
| 248 | + spec2.append(sum2) | ||
| 249 | + residual.append(sum1 - sum2) | ||
| 250 | + error.append(math.sqrt(sum2)) | ||
| 251 | + energies.append(modelcube.energy(ieng).TeV()) | ||
| 252 | + | ||
| 253 | + # Return residual and error | ||
| 254 | + return energies, residual, error | ||
| 255 | + | ||
| 256 | + | ||
| 257 | +# ==================== # | ||
| 258 | +# Simulate counts cube # | ||
| 259 | +# ==================== # | ||
| 260 | +def simulate_counts_cube(obs, ra=83.63, dec=22.01, npix=50, binsz=0.02, | ||
| 261 | + emin=0.1, emax=100.0, ebins=20, seed=1, edisp=False): | ||
| 262 | + """ | ||
| 263 | + Simulate counts cube | ||
| 264 | + | ||
| 265 | + Parameters | ||
| 266 | + ---------- | ||
| 267 | + obs : `~gammalib.GObservations` | ||
| 268 | + Observation container | ||
| 269 | + ebins : int, optional | ||
| 270 | + Number of energy bins for binned or stacked analysis | ||
| 271 | + edisp : boolean, optional | ||
| 272 | + Use energy dispersion | ||
| 273 | + """ | ||
| 274 | + # Simulate events | ||
| 275 | + ctobssim = ctools.ctobssim(obs) | ||
| 276 | + ctobssim['seed'] = seed | ||
| 277 | + ctobssim['edisp'] = edisp | ||
| 278 | + ctobssim.run() | ||
| 279 | + | ||
| 280 | + # Create counts cube | ||
| 281 | + ctbin = ctools.ctbin(ctobssim.obs()) | ||
| 282 | + ctbin['stack'] = True | ||
| 283 | + ctbin['ebinalg'] = 'LOG' | ||
| 284 | + ctbin['emin'] = emin | ||
| 285 | + ctbin['emax'] = emax | ||
| 286 | + ctbin['enumbins'] = ebins | ||
| 287 | + ctbin['coordsys'] = 'CEL' | ||
| 288 | + ctbin['proj'] = 'CAR' | ||
| 289 | + ctbin['xref'] = ra | ||
| 290 | + ctbin['yref'] = dec | ||
| 291 | + ctbin['nxpix'] = npix | ||
| 292 | + ctbin['nypix'] = npix | ||
| 293 | + ctbin['binsz'] = binsz | ||
| 294 | + ctbin.run() | ||
| 295 | + | ||
| 296 | + # Return counts cube | ||
| 297 | + return ctbin.cube().copy() | ||
| 298 | + | ||
| 299 | + | ||
| 300 | +# ================= # | ||
| 301 | +# Create model cube # | ||
| 302 | +# ================= # | ||
| 303 | +def create_model_cube(obs, countscube, edisp=False): | ||
| 304 | + """ | ||
| 305 | + Create model cube | ||
| 306 | + | ||
| 307 | + Parameters | ||
| 308 | + ---------- | ||
| 309 | + obs : `~gammalib.GObservations` | ||
| 310 | + Observation container | ||
| 311 | + countscube : `~gammalib.GCTAEventCube` | ||
| 312 | + Counts cube for binning | ||
| 313 | + edisp : boolean, optional | ||
| 314 | + Use energy dispersion | ||
| 315 | + """ | ||
| 316 | + # Create model cube | ||
| 317 | + ctmodel = ctools.ctmodel(obs) | ||
| 318 | + ctmodel.cube(countscube) | ||
| 319 | + ctmodel['edisp'] = edisp | ||
| 320 | + ctmodel.run() | ||
| 321 | + | ||
| 322 | + # Return model cube | ||
| 323 | + return ctmodel.cube().copy() | ||
| 324 | + | ||
| 325 | + | ||
| 326 | +# ================= # | ||
| 327 | +# Show model and MC # | ||
| 328 | +# ================= # | ||
| 329 | +def show_model_mc(modelname, duration=180000.0, caldb='prod2', irf='South_50h', | ||
| 330 | + ebins=20, edisp=False): | ||
| 331 | + """ | ||
| 332 | + """ | ||
| 333 | + # Set pointing direction | ||
| 334 | + pntdir = gammalib.GSkyDir() | ||
| 335 | + pntdir.radec_deg(83.63, 22.01) | ||
| 336 | + | ||
| 337 | + # Set single CTA observation | ||
| 338 | + run = obsutils.set_obs(pntdir, duration=duration, caldb=caldb, irf=irf) | ||
| 339 | + | ||
| 340 | + # Set observation container | ||
| 341 | + obs = gammalib.GObservations() | ||
| 342 | + obs.append(run) | ||
| 343 | + | ||
| 344 | + # Load and append model | ||
| 345 | + models = gammalib.GModels(modelname) | ||
| 346 | + obs.models(models) | ||
| 347 | + | ||
| 348 | + # Create simulated counts cube | ||
| 349 | + countscube = simulate_counts_cube(obs, npix=400, binsz=0.002, ebins=ebins, | ||
| 350 | + edisp=edisp) | ||
| 351 | + print(countscube) | ||
| 352 | + | ||
| 353 | + # Create model cube | ||
| 354 | + modelcube = create_model_cube(obs, countscube, edisp=edisp) | ||
| 355 | + print(modelcube) | ||
| 356 | + | ||
| 357 | + # Create residual map and spectrum | ||
| 358 | + resmap, errmap = residual_spatial(countscube, modelcube) | ||
| 359 | + energies, resspec, errspec = residual_spectral(countscube, modelcube) | ||
| 360 | + | ||
| 361 | + # Create figure | ||
| 362 | + fig = plt.figure(figsize=(14,5)) | ||
| 363 | + | ||
| 364 | + # Create subplot for residual spectrum | ||
| 365 | + frame1 = fig.add_subplot(131) | ||
| 366 | + plot_resspec(frame1, energies, resspec, errspec, emin=0.05, emax=150.0) | ||
| 367 | + | ||
| 368 | + # Create subplots for residual profiles | ||
| 369 | + frame2 = fig.add_subplot(232) | ||
| 370 | + frame3 = fig.add_subplot(235) | ||
| 371 | + plot_resmap(frame2, frame3, resmap, errmap, steps=5) | ||
| 372 | + | ||
| 373 | + # Create subplot for residual map | ||
| 374 | + frame4 = fig.add_subplot(133) | ||
| 375 | + plot_map(frame4, resmap, smooth=0.02) | ||
| 376 | + | ||
| 377 | + # Show figure | ||
| 378 | + plt.show() | ||
| 379 | + | ||
| 380 | + # Return | ||
| 381 | + return | ||
| 382 | + | ||
| 383 | + | ||
| 384 | +# ======================== # | ||
| 385 | +# Main routine entry point # | ||
| 386 | +# ======================== # | ||
| 387 | +if __name__ == '__main__': | ||
| 388 | + | ||
| 389 | + # Set model name | ||
| 390 | + modelname = 'crab.xml' | ||
| 391 | + | ||
| 392 | + # Show model and MC | ||
| 393 | + #show_model_mc(modelname, ebins=50, edisp=False) | ||
| 394 | + show_model_mc(modelname, ebins=50, edisp=True) |
inst/cta/test/dev/test_background_integration.py
| 1 | #! /usr/bin/env python | 1 | #! /usr/bin/env python |
| 2 | # ========================================================================== | 2 | # ========================================================================== |
| 3 | -# This energy integration of GCTABackground3D | 3 | +# Test energy integration of GCTABackground3D |
| 4 | # | 4 | # |
| 5 | # Copyright (C) 2017 Juergen Knoedlseder | 5 | # Copyright (C) 2017 Juergen Knoedlseder |
| 6 | # | 6 | # |