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Submitted version of IR linearity monitor WFC3/IR proposal 16404, continuation of 15724. Warnings for orbital length slightly exceeded shouldn't be a problem as the orbits are fully internal and can be scheduled anytime in the first quarter of Cycle 28. We prefer the first half because the Cycle 27 calibrations were taken on Oct 1-2, 2019, and we prefer to have between 1 and 1.25 years between the datasets. Please let me know if you encounter any processing issues.
-616417474
----- Attempting Submission 1 (Thu Aug 06 19:26:11 GMT 2020) -----
Internal-only calibration proposals do not need to resolve with the visit planner.
WFC3 IR Linearity Monitor
The WFC3/IR detector exhibits a non-linear response to incident flux. The data reduction pipeline provides a correction for the non-linearity, which depends on accurate characterization of the response of the detector. To monitor the non-linearity of the WFC3/IR detector, we use a dark observation followed by two internal flats using the Tungsten lamp at different sampling rates, and a trailing dark. Any changes measured in the non-linearity will be updated in the calibration reference file, crucial to providing a correction for accurate photometry. This program is a continuation of the cycle 27 (program 15724) linearity calibration program.
To monitor the non-linearity of the WFC3/IR detector, we use a dark observation followed by two internal flats using the Tungsten lamp. We begin with a narrow band flat to ensure that the lamp is warm and stable, but not so bright as to cause persistence, observing the Tungsten lamp with F126N (half SPARS10 and half SPARS50). Then we take internal flats though the F127M filter at different signal levels and sampling sequence (half SPARS10 and half SPARS25). After the F127M flat, a dark is obtained to measure the persistence decay rate.
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