Use a real star selector when measuring aperture corrections.

lsst-dm · May 15, 2016 · 9c0d070 · 9c0d070
1 parent 3e63661
commit 9c0d070
Showing 1 changed file with 4 additions and 2 deletions.
diff --git a/config/processCcd.py b/config/processCcd.py
@@ -18,10 +18,12 @@
 config.charImage.detectAndMeasure.measurement.slots.apFlux = "base_CircularApertureFlux_7_0"
 config.charImage.detectAndMeasure.measurement.slots.calibFlux = "base_CircularApertureFlux_7_0"
 
+# we rarely run PSF determination on SDSS data, so we have to run our own star selector instead
+from lsst.meas.algorithms import ObjectSizeStarSelectorTask
+config.charImage.detectAndMeasure.measureApCorr.starSelector.retarget(ObjectSizeStarSelectorTask)
+
 config.calibrate.detectAndMeasure.detection.background.binSize = 512
 config.calibrate.detectAndMeasure.detection.background.binSize = 512
-# we rarely run PSF determination on SDSS data, so use the output of the star selector instead
-config.calibrate.detectAndMeasure.measureApCorr.inputFilterFlag = "calib_psfCandidate"
 
 # use the WCS determined by SDSS (why?)
 config.calibrate.astrometry.forceKnownWcs = True