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I was thinking we could add PSF photometry to the pipeline as this would be more appropriate for galaxies.
Probably the easiest way to implement this would be by using sextractor as this software …
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We need to add in color terms post photometry to calculate natural system photometry. This means keeping track of the color terms used for each image in some way. The simplest is to of course append t…
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Pipeline needs an additional stage to properly normalize the photometric calibration between datasets of the same field pointing and filter taken with different cameras.
This code should be run a…
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Issue [JDA-30](https://jira.stsci.edu/browse/JDA-30) was created by Ben Sunnquist:
Data used: Mirage NIRCam imaging simulations of Candels/GOODS-S processed through level 3 of the JWST Pipeline
Da…
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### Instrument
MIRI (Stages 1-3)
### What is your suggestion?
For MIRI imaging (especially with long wavelength filters), the observations are quite background noise limited. Rather than just…
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# ML Inference for Photo-Z/Physical Properties
Building inference baselines for Photo-Z and Physical Property Prediction.
Contacts: Liam Parker, Kartheik Iyer
Participants: Liam Parker, Karthe…
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Bouts of poor weather, particularly periods of low sky transparency due to cloud cause photometric scatter that is not taken into account in the photometric noise model for the pipeline.
A post-pro…
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rknop updated
5 months ago
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As pointed out by @coclar in #80, the PSF photometry option simply fits circularly symmetric PSFs to the stars in the images.
The parameters for these PSFs are simply copied across from those foun…
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_Issue [JP-3115](https://jira.stsci.edu/browse/JP-3115) was created on JIRA by [Ori Fox](https://jira.stsci.edu/secure/ViewProfile.jspa?name=ofox):_
Add PSF photometry to the pipeline. This will im…