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Thirty days after launch, the detectors will provide their first "thumbprint images," which according to Ressler will allow the team to verify that the entire data chain is functional and that data will be collected as expected when the instrument is in its final cooled state.
From that point on for MIRI, approximately 63 days of cool down operations will follow as the cryocooler drives the instrument down to 6 Kelvin. Once there, approximately 93 or 94 days after launch, the first actual MIRI images will be collected… of the inside of the cover to continue verifying that all is operational with the instrument.
That calibration will take approximately two days, after which, MIRI will be ready for calibration with known star clusters.
"So there are two regions of the sky that JWST is always able to image, the north ecliptic pole and south ecliptic pole," said Ressler. "So we have specific targets chosen in those two ecliptic poles that will let us measure the plate scale how many arc seconds per pixel we've got. It'll let us check our distortion."
"So there's well-characterized clusters of stars that other missions have used. They're patches of sky that we understand very well. They'll be relatively photogenic. So yes these are images of things in the sky, but they are calibration fields that are commonly used to do instrument checkouts like this."