Coverage for tests/test_calibrateImage.py: 16%

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21 

22import unittest 

23import tempfile 

24 

25import astropy.units as u 

26from astropy.coordinates import SkyCoord 

27import numpy as np 

28 

29import lsst.afw.image as afwImage 

30import lsst.afw.table as afwTable 

31import lsst.daf.base 

32import lsst.daf.butler.tests as butlerTests 

33import lsst.geom 

34import lsst.meas.algorithms 

35from lsst.meas.algorithms import testUtils 

36import lsst.meas.extensions.psfex 

37import lsst.meas.base.tests 

38import lsst.pipe.base.testUtils 

39from lsst.pipe.tasks.calibrateImage import CalibrateImageTask 

40import lsst.utils.tests 

41 

42 

43class CalibrateImageTaskTests(lsst.utils.tests.TestCase): 

44 

45 def setUp(self): 

46 # Different x/y dimensions so they're easy to distinguish in a plot, 

47 # and non-zero minimum, to help catch xy0 errors. 

48 bbox = lsst.geom.Box2I(lsst.geom.Point2I(5, 4), lsst.geom.Point2I(205, 184)) 

49 self.sky_center = lsst.geom.SpherePoint(245.0, -45.0, lsst.geom.degrees) 

50 self.photo_calib = 12.3 

51 dataset = lsst.meas.base.tests.TestDataset(bbox, crval=self.sky_center, calibration=self.photo_calib) 

52 # sqrt of area of a normalized 2d gaussian 

53 psf_scale = np.sqrt(4*np.pi*(dataset.psfShape.getDeterminantRadius())**2) 

54 noise = 10.0 # stddev of noise per pixel 

55 # Sources ordered from faintest to brightest. 

56 self.fluxes = np.array((6*noise*psf_scale, 

57 12*noise*psf_scale, 

58 45*noise*psf_scale, 

59 150*noise*psf_scale, 

60 400*noise*psf_scale, 

61 1000*noise*psf_scale)) 

62 self.centroids = np.array(((162, 22), 

63 (40, 70), 

64 (100, 160), 

65 (50, 120), 

66 (92, 35), 

67 (175, 154)), dtype=np.float32) 

68 for flux, centroid in zip(self.fluxes, self.centroids): 

69 dataset.addSource(instFlux=flux, centroid=lsst.geom.Point2D(centroid[0], centroid[1])) 

70 

71 # Bright extended source in the center of the image: should not appear 

72 # in any of the output catalogs. 

73 center = lsst.geom.Point2D(100, 100) 

74 shape = lsst.afw.geom.Quadrupole(8, 9, 3) 

75 dataset.addSource(instFlux=500*noise*psf_scale, centroid=center, shape=shape) 

76 

77 schema = dataset.makeMinimalSchema() 

78 self.truth_exposure, self.truth_cat = dataset.realize(noise=noise, schema=schema) 

79 # To make it look like a version=1 (nJy fluxes) refcat 

80 self.truth_cat = self.truth_exposure.photoCalib.calibrateCatalog(self.truth_cat) 

81 self.ref_loader = testUtils.MockReferenceObjectLoaderFromMemory([self.truth_cat]) 

82 metadata = lsst.daf.base.PropertyList() 

83 metadata.set("REFCAT_FORMAT_VERSION", 1) 

84 self.truth_cat.setMetadata(metadata) 

85 

86 # TODO: a cosmic ray (need to figure out how to insert a fake-CR) 

87 # self.truth_exposure.image.array[10, 10] = 100000 

88 # self.truth_exposure.variance.array[10, 10] = 100000/noise 

89 

90 # Copy the truth exposure, because CalibrateImage modifies the input. 

91 # Post-ISR ccds only contain: initial WCS, VisitInfo, filter 

92 self.exposure = afwImage.ExposureF(self.truth_exposure.maskedImage) 

93 self.exposure.setWcs(self.truth_exposure.wcs) 

94 self.exposure.info.setVisitInfo(self.truth_exposure.visitInfo) 

95 # "truth" filter, to match the "truth" refcat. 

96 self.exposure.setFilter(lsst.afw.image.FilterLabel(physical='truth', band="truth")) 

97 

98 # Test-specific configuration: 

99 self.config = CalibrateImageTask.ConfigClass() 

100 # We don't have many sources, so have to fit simpler models. 

101 self.config.psf_detection.background.approxOrderX = 1 

102 self.config.star_detection.background.approxOrderX = 1 

103 # Only insert 2 sky sources, for simplicity. 

104 self.config.star_sky_sources.nSources = 2 

105 # Use PCA psf fitter, as psfex fails if there are only 4 stars. 

106 self.config.psf_measure_psf.psfDeterminer = 'pca' 

107 # We don't have many test points, so can't match on complicated shapes. 

108 self.config.astrometry.matcher.numPointsForShape = 3 

109 # ApFlux has more noise than PsfFlux (the latter unrealistically small 

110 # in this test data), so we need to do magnitude rejection at higher 

111 # sigma, otherwise we can lose otherwise good sources. 

112 # TODO DM-39203: Once we are using Compensated Gaussian Fluxes, we 

113 # will use those fluxes here, and hopefully can remove this. 

114 self.config.astrometry.magnitudeOutlierRejectionNSigma = 9.0 

115 

116 # find_stars needs an id generator. 

117 self.id_generator = lsst.meas.base.IdGenerator() 

118 

119 # Something about this test dataset prefers the older fluxRatio here. 

120 self.config.star_catalog_calculation.plugins['base_ClassificationExtendedness'].fluxRatio = 0.925 

121 

122 def _check_run(self, calibrate, result): 

123 """Test the result of CalibrateImage.run(). 

124 

125 Parameters 

126 ---------- 

127 calibrate : `lsst.pipe.tasks.calibrateImage.CalibrateImageTask` 

128 Configured task that had `run` called on it. 

129 result : `lsst.pipe.base.Struct` 

130 Result of calling calibrate.run(). 

131 """ 

132 # Background should have 4 elements: 3 from compute_psf and one from 

133 # re-estimation during source detection. 

134 self.assertEqual(len(result.background), 4) 

135 

136 # Check that the summary statistics are reasonable. 

137 summary = result.output_exposure.info.getSummaryStats() 

138 self.assertFloatsAlmostEqual(summary.psfSigma, 2.0, rtol=1e-2) 

139 self.assertFloatsAlmostEqual(summary.ra, self.sky_center.getRa().asDegrees(), rtol=1e-7) 

140 self.assertFloatsAlmostEqual(summary.dec, self.sky_center.getDec().asDegrees(), rtol=1e-7) 

141 

142 # Returned photoCalib should be the applied value, not the ==1 one on the exposure. 

143 self.assertFloatsAlmostEqual(result.applied_photo_calib.getCalibrationMean(), 

144 self.photo_calib, rtol=2e-3) 

145 # Should have flux/magnitudes in the afw and astropy catalogs 

146 self.assertIn("slot_PsfFlux_flux", result.stars_footprints.schema) 

147 self.assertIn("slot_PsfFlux_mag", result.stars_footprints.schema) 

148 self.assertEqual(result.stars["slot_PsfFlux_flux"].unit, u.nJy) 

149 self.assertEqual(result.stars["slot_PsfFlux_mag"].unit, u.ABmag) 

150 

151 # Should have detected all S/N >= 10 sources plus 2 sky sources, whether 1 or 2 snaps. 

152 self.assertEqual(len(result.stars), 7) 

153 # Did the psf flags get propagated from the psf_stars catalog? 

154 self.assertEqual(result.stars["calib_psf_used"].sum(), 3) 

155 

156 # Check that all necessary fields are in the output. 

157 lsst.pipe.base.testUtils.assertValidOutput(calibrate, result) 

158 

159 def test_run(self): 

160 """Test that run() returns reasonable values to be butler put. 

161 """ 

162 calibrate = CalibrateImageTask(config=self.config) 

163 calibrate.astrometry.setRefObjLoader(self.ref_loader) 

164 calibrate.photometry.match.setRefObjLoader(self.ref_loader) 

165 result = calibrate.run(exposures=self.exposure) 

166 

167 self._check_run(calibrate, result) 

168 

169 def test_run_2_snaps(self): 

170 """Test that run() returns reasonable values to be butler put, when 

171 passed two exposures to combine as snaps. 

172 """ 

173 calibrate = CalibrateImageTask(config=self.config) 

174 calibrate.astrometry.setRefObjLoader(self.ref_loader) 

175 calibrate.photometry.match.setRefObjLoader(self.ref_loader) 

176 # Halve the flux in each exposure to get the expected visit sum. 

177 self.exposure.image /= 2 

178 self.exposure.variance /= 2 

179 result = calibrate.run(exposures=[self.exposure, self.exposure]) 

180 

181 self._check_run(calibrate, result) 

182 

183 def test_handle_snaps(self): 

184 calibrate = CalibrateImageTask(config=self.config) 

185 self.assertEqual(calibrate._handle_snaps(self.exposure), self.exposure) 

186 self.assertEqual(calibrate._handle_snaps((self.exposure, )), self.exposure) 

187 self.assertEqual(calibrate._handle_snaps(self.exposure), self.exposure) 

188 with self.assertRaisesRegex(RuntimeError, "Can only process 1 or 2 snaps, not 0."): 

189 calibrate._handle_snaps([]) 

190 with self.assertRaisesRegex(RuntimeError, "Can only process 1 or 2 snaps, not 3."): 

191 calibrate._handle_snaps(3*[self.exposure]) 

192 

193 def test_compute_psf(self): 

194 """Test that our brightest sources are found by _compute_psf(), 

195 that a PSF is assigned to the expopsure. 

196 """ 

197 calibrate = CalibrateImageTask(config=self.config) 

198 psf_stars, background, candidates = calibrate._compute_psf(self.exposure) 

199 

200 # Background should have 3 elements: initial subtraction, and two from 

201 # re-estimation during the two detection passes. 

202 self.assertEqual(len(background), 3) 

203 

204 # Only the point-sources with S/N > 50 should be in this output. 

205 self.assertEqual(psf_stars["calib_psf_used"].sum(), 3) 

206 # Sort in order of brightness, to easily compare with expected positions. 

207 psf_stars.sort(psf_stars.getPsfFluxSlot().getMeasKey()) 

208 for record, flux, center in zip(psf_stars[::-1], self.fluxes, self.centroids[self.fluxes > 50]): 

209 self.assertFloatsAlmostEqual(record.getX(), center[0], rtol=0.01) 

210 self.assertFloatsAlmostEqual(record.getY(), center[1], rtol=0.01) 

211 # PsfFlux should match the values inserted. 

212 self.assertFloatsAlmostEqual(record["slot_PsfFlux_instFlux"], flux, rtol=0.01) 

213 

214 # TODO: While debugging DM-32701, we're using PCA instead of psfex. 

215 # Check that we got a useable PSF. 

216 # self.assertIsInstance(self.exposure.psf, lsst.meas.extensions.psfex.PsfexPsf) 

217 self.assertIsInstance(self.exposure.psf, lsst.meas.algorithms.PcaPsf) 

218 # TestDataset sources have PSF radius=2 pixels. 

219 radius = self.exposure.psf.computeShape(self.exposure.psf.getAveragePosition()).getDeterminantRadius() 

220 self.assertFloatsAlmostEqual(radius, 2.0, rtol=1e-2) 

221 

222 # To look at images for debugging (`setup display_ds9` and run ds9): 

223 # import lsst.afw.display 

224 # display = lsst.afw.display.getDisplay() 

225 # display.mtv(self.exposure) 

226 

227 def test_measure_aperture_correction(self): 

228 """Test that _measure_aperture_correction() assigns an ApCorrMap to the 

229 exposure. 

230 """ 

231 calibrate = CalibrateImageTask(config=self.config) 

232 psf_stars, background, candidates = calibrate._compute_psf(self.exposure) 

233 

234 # First check that the exposure doesn't have an ApCorrMap. 

235 self.assertIsNone(self.exposure.apCorrMap) 

236 calibrate._measure_aperture_correction(self.exposure, psf_stars) 

237 self.assertIsInstance(self.exposure.apCorrMap, afwImage.ApCorrMap) 

238 

239 def test_find_stars(self): 

240 """Test that _find_stars() correctly identifies the S/N>10 stars 

241 in the image and returns them in the output catalog. 

242 """ 

243 calibrate = CalibrateImageTask(config=self.config) 

244 psf_stars, background, candidates = calibrate._compute_psf(self.exposure) 

245 calibrate._measure_aperture_correction(self.exposure, psf_stars) 

246 

247 stars = calibrate._find_stars(self.exposure, background, self.id_generator) 

248 

249 # Background should have 4 elements: 3 from compute_psf and one from 

250 # re-estimation during source detection. 

251 self.assertEqual(len(background), 4) 

252 

253 # Only 5 psf-like sources with S/N>10 should be in the output catalog, 

254 # plus two sky sources. 

255 self.assertEqual(len(stars), 7) 

256 self.assertTrue(stars.isContiguous()) 

257 # Sort in order of brightness, to easily compare with expected positions. 

258 stars.sort(stars.getPsfFluxSlot().getMeasKey()) 

259 for record, flux, center in zip(stars[::-1], self.fluxes, self.centroids[self.fluxes > 50]): 

260 self.assertFloatsAlmostEqual(record.getX(), center[0], rtol=0.01) 

261 self.assertFloatsAlmostEqual(record.getY(), center[1], rtol=0.01) 

262 self.assertFloatsAlmostEqual(record["slot_PsfFlux_instFlux"], flux, rtol=0.01) 

263 

264 def test_astrometry(self): 

265 """Test that the fitted WCS gives good catalog coordinates. 

266 """ 

267 calibrate = CalibrateImageTask(config=self.config) 

268 calibrate.astrometry.setRefObjLoader(self.ref_loader) 

269 psf_stars, background, candidates = calibrate._compute_psf(self.exposure) 

270 calibrate._measure_aperture_correction(self.exposure, psf_stars) 

271 stars = calibrate._find_stars(self.exposure, background, self.id_generator) 

272 

273 calibrate._fit_astrometry(self.exposure, stars) 

274 

275 # Check that we got reliable matches with the truth coordinates. 

276 sky = stars["sky_source"] 

277 fitted = SkyCoord(stars[~sky]['coord_ra'], stars[~sky]['coord_dec'], unit="radian") 

278 truth = SkyCoord(self.truth_cat['coord_ra'], self.truth_cat['coord_dec'], unit="radian") 

279 idx, d2d, _ = fitted.match_to_catalog_sky(truth) 

280 np.testing.assert_array_less(d2d.to_value(u.milliarcsecond), 35.0) 

281 

282 def test_photometry(self): 

283 """Test that the fitted photoCalib matches the one we generated, 

284 and that the exposure is calibrated. 

285 """ 

286 calibrate = CalibrateImageTask(config=self.config) 

287 calibrate.astrometry.setRefObjLoader(self.ref_loader) 

288 calibrate.photometry.match.setRefObjLoader(self.ref_loader) 

289 psf_stars, background, candidates = calibrate._compute_psf(self.exposure) 

290 calibrate._measure_aperture_correction(self.exposure, psf_stars) 

291 stars = calibrate._find_stars(self.exposure, background, self.id_generator) 

292 calibrate._fit_astrometry(self.exposure, stars) 

293 

294 stars, matches, meta, photoCalib = calibrate._fit_photometry(self.exposure, stars) 

295 

296 # NOTE: With this test data, PhotoCalTask returns calibrationErr==0, 

297 # so we can't check that the photoCal error has been set. 

298 self.assertFloatsAlmostEqual(photoCalib.getCalibrationMean(), self.photo_calib, rtol=2e-3) 

299 # The exposure should be calibrated by the applied photoCalib. 

300 self.assertFloatsAlmostEqual(self.exposure.image.array/self.truth_exposure.image.array, 

301 self.photo_calib, rtol=2e-3) 

302 # PhotoCalib on the exposure must be identically 1. 

303 self.assertEqual(self.exposure.photoCalib.getCalibrationMean(), 1.0) 

304 

305 # Check that we got reliable magnitudes and fluxes vs. truth, ignoring 

306 # sky sources. 

307 sky = stars["sky_source"] 

308 fitted = SkyCoord(stars[~sky]['coord_ra'], stars[~sky]['coord_dec'], unit="radian") 

309 truth = SkyCoord(self.truth_cat['coord_ra'], self.truth_cat['coord_dec'], unit="radian") 

310 idx, _, _ = fitted.match_to_catalog_sky(truth) 

311 # Because the input variance image does not include contributions from 

312 # the sources, we can't use fluxErr as a bound on the measurement 

313 # quality here. 

314 self.assertFloatsAlmostEqual(stars[~sky]['slot_PsfFlux_flux'], 

315 self.truth_cat['truth_flux'][idx], 

316 rtol=0.1) 

317 self.assertFloatsAlmostEqual(stars[~sky]['slot_PsfFlux_mag'], 

318 self.truth_cat['truth_mag'][idx], 

319 rtol=0.01) 

320 

321 def test_match_psf_stars(self): 

322 """Test that _match_psf_stars() flags the correct stars as psf stars 

323 and candidates. 

324 """ 

325 calibrate = CalibrateImageTask(config=self.config) 

326 psf_stars, background, candidates = calibrate._compute_psf(self.exposure) 

327 calibrate._measure_aperture_correction(self.exposure, psf_stars) 

328 stars = calibrate._find_stars(self.exposure, background, self.id_generator) 

329 

330 # There should be no psf-related flags set at first. 

331 self.assertEqual(stars["calib_psf_candidate"].sum(), 0) 

332 self.assertEqual(stars["calib_psf_used"].sum(), 0) 

333 self.assertEqual(stars["calib_psf_reserved"].sum(), 0) 

334 

335 calibrate._match_psf_stars(psf_stars, stars) 

336 

337 # Sort in order of brightness; the psf stars are the 3 brightest, with 

338 # two sky sources as the faintest. 

339 stars.sort(stars.getPsfFluxSlot().getMeasKey()) 

340 # sort() above leaves the catalog non-contiguous. 

341 stars = stars.copy(deep=True) 

342 np.testing.assert_array_equal(stars["calib_psf_candidate"], 

343 [False, False, False, False, True, True, True]) 

344 np.testing.assert_array_equal(stars["calib_psf_used"], [False, False, False, False, True, True, True]) 

345 # Too few sources to reserve any in these tests. 

346 self.assertEqual(stars["calib_psf_reserved"].sum(), 0) 

347 

348 

349class CalibrateImageTaskRunQuantumTests(lsst.utils.tests.TestCase): 

350 """Tests of ``CalibrateImageTask.runQuantum``, which need a test butler, 

351 but do not need real images. 

352 """ 

353 def setUp(self): 

354 instrument = "testCam" 

355 exposure0 = 101 

356 exposure1 = 101 

357 visit = 100101 

358 detector = 42 

359 

360 # Create a and populate a test butler for runQuantum tests. 

361 self.repo_path = tempfile.TemporaryDirectory(ignore_cleanup_errors=True) 

362 self.repo = butlerTests.makeTestRepo(self.repo_path.name) 

363 

364 # A complete instrument record is necessary for the id generator. 

365 instrumentRecord = self.repo.dimensions["instrument"].RecordClass( 

366 name=instrument, visit_max=1e6, exposure_max=1e6, detector_max=128, 

367 class_name="lsst.obs.base.instrument_tests.DummyCam", 

368 ) 

369 self.repo.registry.syncDimensionData("instrument", instrumentRecord) 

370 

371 # dataIds for fake data 

372 butlerTests.addDataIdValue(self.repo, "exposure", exposure0) 

373 butlerTests.addDataIdValue(self.repo, "exposure", exposure1) 

374 butlerTests.addDataIdValue(self.repo, "visit", visit) 

375 butlerTests.addDataIdValue(self.repo, "detector", detector) 

376 

377 # inputs 

378 butlerTests.addDatasetType(self.repo, "postISRCCD", {"instrument", "exposure", "detector"}, 

379 "ExposureF") 

380 butlerTests.addDatasetType(self.repo, "gaia_dr3_20230707", {"htm7"}, "SimpleCatalog") 

381 butlerTests.addDatasetType(self.repo, "ps1_pv3_3pi_20170110", {"htm7"}, "SimpleCatalog") 

382 

383 # outputs 

384 butlerTests.addDatasetType(self.repo, "initial_pvi", {"instrument", "visit", "detector"}, 

385 "ExposureF") 

386 butlerTests.addDatasetType(self.repo, "initial_stars_footprints_detector", 

387 {"instrument", "visit", "detector"}, 

388 "SourceCatalog") 

389 butlerTests.addDatasetType(self.repo, "initial_stars_detector", 

390 {"instrument", "visit", "detector"}, 

391 "ArrowAstropy") 

392 butlerTests.addDatasetType(self.repo, "initial_photoCalib_detector", 

393 {"instrument", "visit", "detector"}, 

394 "PhotoCalib") 

395 # optional outputs 

396 butlerTests.addDatasetType(self.repo, "initial_pvi_background", {"instrument", "visit", "detector"}, 

397 "Background") 

398 butlerTests.addDatasetType(self.repo, "initial_psf_stars_footprints_detector", 

399 {"instrument", "visit", "detector"}, 

400 "SourceCatalog") 

401 butlerTests.addDatasetType(self.repo, "initial_psf_stars_detector", 

402 {"instrument", "visit", "detector"}, 

403 "ArrowAstropy") 

404 butlerTests.addDatasetType(self.repo, 

405 "initial_astrometry_match_detector", 

406 {"instrument", "visit", "detector"}, 

407 "Catalog") 

408 butlerTests.addDatasetType(self.repo, 

409 "initial_photometry_match_detector", 

410 {"instrument", "visit", "detector"}, 

411 "Catalog") 

412 

413 # dataIds 

414 self.exposure0_id = self.repo.registry.expandDataId( 

415 {"instrument": instrument, "exposure": exposure0, "detector": detector}) 

416 self.exposure1_id = self.repo.registry.expandDataId( 

417 {"instrument": instrument, "exposure": exposure1, "detector": detector}) 

418 self.visit_id = self.repo.registry.expandDataId( 

419 {"instrument": instrument, "visit": visit, "detector": detector}) 

420 self.htm_id = self.repo.registry.expandDataId({"htm7": 42}) 

421 

422 # put empty data 

423 self.butler = butlerTests.makeTestCollection(self.repo) 

424 self.butler.put(afwImage.ExposureF(), "postISRCCD", self.exposure0_id) 

425 self.butler.put(afwTable.SimpleCatalog(), "gaia_dr3_20230707", self.htm_id) 

426 self.butler.put(afwTable.SimpleCatalog(), "ps1_pv3_3pi_20170110", self.htm_id) 

427 

428 def tearDown(self): 

429 self.repo_path.cleanup() 

430 

431 def test_runQuantum(self): 

432 task = CalibrateImageTask() 

433 lsst.pipe.base.testUtils.assertValidInitOutput(task) 

434 

435 quantum = lsst.pipe.base.testUtils.makeQuantum( 

436 task, self.butler, self.visit_id, 

437 {"exposures": [self.exposure0_id], 

438 "astrometry_ref_cat": [self.htm_id], 

439 "photometry_ref_cat": [self.htm_id], 

440 # outputs 

441 "output_exposure": self.visit_id, 

442 "stars": self.visit_id, 

443 "stars_footprints": self.visit_id, 

444 "background": self.visit_id, 

445 "psf_stars": self.visit_id, 

446 "psf_stars_footprints": self.visit_id, 

447 "applied_photo_calib": self.visit_id, 

448 "initial_pvi_background": self.visit_id, 

449 "astrometry_matches": self.visit_id, 

450 "photometry_matches": self.visit_id, 

451 }) 

452 mock_run = lsst.pipe.base.testUtils.runTestQuantum(task, self.butler, quantum) 

453 

454 # Ensure the reference loaders have been configured. 

455 self.assertEqual(task.astrometry.refObjLoader.name, "gaia_dr3_20230707") 

456 self.assertEqual(task.photometry.match.refObjLoader.name, "ps1_pv3_3pi_20170110") 

457 # Check that the proper kwargs are passed to run(). 

458 self.assertEqual(mock_run.call_args.kwargs.keys(), {"exposures", "id_generator"}) 

459 

460 def test_runQuantum_2_snaps(self): 

461 task = CalibrateImageTask() 

462 lsst.pipe.base.testUtils.assertValidInitOutput(task) 

463 

464 quantum = lsst.pipe.base.testUtils.makeQuantum( 

465 task, self.butler, self.visit_id, 

466 {"exposures": [self.exposure0_id, self.exposure1_id], 

467 "astrometry_ref_cat": [self.htm_id], 

468 "photometry_ref_cat": [self.htm_id], 

469 # outputs 

470 "output_exposure": self.visit_id, 

471 "stars": self.visit_id, 

472 "stars_footprints": self.visit_id, 

473 "background": self.visit_id, 

474 "psf_stars": self.visit_id, 

475 "psf_stars_footprints": self.visit_id, 

476 "applied_photo_calib": self.visit_id, 

477 "initial_pvi_background": self.visit_id, 

478 "astrometry_matches": self.visit_id, 

479 "photometry_matches": self.visit_id, 

480 }) 

481 mock_run = lsst.pipe.base.testUtils.runTestQuantum(task, self.butler, quantum) 

482 

483 # Ensure the reference loaders have been configured. 

484 self.assertEqual(task.astrometry.refObjLoader.name, "gaia_dr3_20230707") 

485 self.assertEqual(task.photometry.match.refObjLoader.name, "ps1_pv3_3pi_20170110") 

486 # Check that the proper kwargs are passed to run(). 

487 self.assertEqual(mock_run.call_args.kwargs.keys(), {"exposures", "id_generator"}) 

488 

489 def test_runQuantum_no_optional_outputs(self): 

490 config = CalibrateImageTask.ConfigClass() 

491 config.optional_outputs = None 

492 task = CalibrateImageTask(config=config) 

493 lsst.pipe.base.testUtils.assertValidInitOutput(task) 

494 

495 quantum = lsst.pipe.base.testUtils.makeQuantum( 

496 task, self.butler, self.visit_id, 

497 {"exposures": [self.exposure0_id], 

498 "astrometry_ref_cat": [self.htm_id], 

499 "photometry_ref_cat": [self.htm_id], 

500 # outputs 

501 "output_exposure": self.visit_id, 

502 "stars": self.visit_id, 

503 "stars_footprints": self.visit_id, 

504 "applied_photo_calib": self.visit_id, 

505 "background": self.visit_id, 

506 }) 

507 mock_run = lsst.pipe.base.testUtils.runTestQuantum(task, self.butler, quantum) 

508 

509 # Ensure the reference loaders have been configured. 

510 self.assertEqual(task.astrometry.refObjLoader.name, "gaia_dr3_20230707") 

511 self.assertEqual(task.photometry.match.refObjLoader.name, "ps1_pv3_3pi_20170110") 

512 # Check that the proper kwargs are passed to run(). 

513 self.assertEqual(mock_run.call_args.kwargs.keys(), {"exposures", "id_generator"}) 

514 

515 def test_lintConnections(self): 

516 """Check that the connections are self-consistent. 

517 """ 

518 Connections = CalibrateImageTask.ConfigClass.ConnectionsClass 

519 lsst.pipe.base.testUtils.lintConnections(Connections) 

520 

521 

522def setup_module(module): 

523 lsst.utils.tests.init() 

524 

525 

526class MemoryTestCase(lsst.utils.tests.MemoryTestCase): 

527 pass 

528 

529 

530if __name__ == "__main__": 530 ↛ 531line 530 didn't jump to line 531, because the condition on line 530 was never true

531 lsst.utils.tests.init() 

532 unittest.main()