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The `imProc.sources.forcedPhot` function is intended for performing forced photometry on given source coordinates. Generally, the function is invoked as follows:
```
FP = imProc.sources.forcedPh…
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By default **imProc.calib.photometricZP** relies on SN_2 column (previously it was SN_3) in the source catalog.
Once we use **imProc.sources.findMeasureSources** with an empirically measured PSF rath…
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We have a pipeline with simple synchronisation.
Provide a copy script that gathers input form the user to perform the extractions automatically.
The extraction should output and register raw photomet…
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Pipeline not well laid out - works out catalogues to be processed, but doesn't use this and then recalculates in class.
Mostly fixed
Better logging needed at ingest stage to show how much left - to …
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Load csv file saved in step 1 (at USAGE)
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From the [Requirements Doc](https://docs.google.com/document/d/1czDIkTisJEv5T40j3PCGRrUSoPRdz-jqkV_9mMcA14g/edit?tab=t.0#heading=h.3wcu7fhoej8h) we have a basic definition of inputs and outputs for th…
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The CLI needs to be a little intuitive and clearly self documented. The options below are listed to meet the current requirements.
Implementation can use `argparse` package. LSST pipelines pass …
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From FY24 Q2 QU
> We will also use the new HSC+VIDEO images and catalogues produced from the above pipeline run, to search for dwarf galaxies and test whether the addition of the near infrared photom…
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Hello,
I recently graduated with a masters degree and my thesis was on W UMa binary stars and I created a package for analyzing these systems. I am working on creating a pipeline for Ball State Uni…
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Unfortunately, another update of pyKLIP JWST.py is needed. Currently, the pixel scale is taken as the square root of the PIXAR_A2 header keyword, but this header keyword does not exist if the photomet…