DM-43176: Flag sources with no flux after re-distribution. #93
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fred3m
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TallJimbo
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Mar 12, 2024
| footprint = afwFootprint(SpanSet(spanList)) | ||
| footprint.setPeakCatalog(heavy.peaks) | ||
| zeroImage = afwImage(array=np.array([[0]], dtype=np.float32), xy0=center, dtype=dtype) | ||
| heavy = makeHeavyFootprint(footprint, MaskedImage(zeroImage, dtype=dtype)) |
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| heavy = makeHeavyFootprint(footprint, MaskedImage(zeroImage, dtype=dtype)) | |
| heavy = HeavyFootprintF(footprint) | |
| heavy.getImageArray()[0] = 0.0 |
is probably a bit more efficient (no need for Image or MaskedImage temporaries), but I'm not sure it's enough better to merit another Jenkins run. Just another way to do it.
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Good idea. I have to rebase the other packages anyway, so I'll make this change, rebase all of them, and just Jenkins without the ci packages.
Sometimes errors in the pipelines, like incorrect PSF modeling, can cause sources with valid scarlet models to have no flux after flux re-distribution when the footprints are being reconstructed. This commit adds a `deblend_zeroFlux` column to identify sources that have zero flux in a given band for follow-up.
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Sometimes errors in the pipelines, like incorrect PSF modeling, can cause sources with valid scarlet models to have no flux after flux re-distribution when the footprints are being reconstructed. This commit adds a
deblend_zeroFluxcolumn to identify sources that have zero flux in a given band for follow-up.