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For MIRI imaging (especially with long wavelength filters), the observations are quite background noise limited. Rather than just doing simple aperture photometry, it might be better to do optimal photometric extraction using code very similar to our optimal spectral extraction.
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The text was updated successfully, but these errors were encountered:
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 doing simple aperture photometry, it might be better to do optimal photometric extraction using code very similar to our optimal spectral extraction.
Error traceback output
No response
What operating system are you using?
No response
What version of Python are you running?
No response
What Python packages do you have installed?
No response
Code of Conduct
The text was updated successfully, but these errors were encountered: