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Improved model for MIRI cruciform artifact, part 1 #837
Improved model for MIRI cruciform artifact, part 1 #837
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Hello @mperrin, Thank you for updating !
Comment last updated at 2024-05-17 14:57:33 UTC |
FYI to @merope82 and @mlibralato - here's an update to improve cruciform artifact models in webbpsf. |
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This looks good to me. I did a comparison at different wavelengths with some PSF subtraction and, even close to the center of the detector, there is a better residual at lower wavelengths.
Summary:
This PR implements an improved model for the cruciform artifact seen in MIRI, in particular modeling the shifts of the cruciform lines as a function of position. This is motivated by comparisons with actual MIRI ePSFs by Libralato et al. 2024.
The key changes are
Example plots showing the outputs and comparing to data are included below.
This is intended as the first PR of at least two for improving the MIRI ePSFs (broken up for complexity and to keep the reviews more manageable / bite-sized). A next step would add in models for the 'peaks' in the cruciform, as predicted by Gaspar et al, and as observed in MIRI LRS ePSFs.
A few additional pieces
There's also a little helper function for displaying the cruciform models, which is not used in calculations but helps visualize what's going on:
As you can see in the above, this PR also adds a model for the diffuse radial halo part of the "cruciform". See Figure 12 of Gaspar et al. 2021. This is a small but nonzero portion of the cruciform physics which we previously have neglected; this portion of the model is harder to base in empirical data given SNR of available ePSFs, but it seems
Example outputs and comparisons with data
Comparisons: F560W
Comparisons: F770W