The list of Investigators does not match the STScI records for this program.
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
Couldn't read CASM results
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
Couldn't read CASM results
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
Couldn't read CASM results
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
Couldn't read CASM results
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
Couldn't read CASM results
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
Couldn't read CASM results
Couldn't read CASM results
Couldn't read CASM results
Couldn't read CASM results
Couldn't read CASM results
I'm not sure what is causing the errors in the Visit Planner - it seems that some formatting has changed? Please advise whether/how to resubmit without errors.
The internal visit length slightly exceeding 1800s is acceptable.
The warning about co-Is is because Varun Bajaj has been (re-)added as co-I.
-1687023922
----- Attempting Submission 1 (Fri Jun 30 18:59:03 GMT 2023) -----
I'm not sure what is causing the errors in the Visit Planner - it seems that some formatting has changed? Please advise whether/how to resubmit without errors.
The internal visit length slightly exceeding 1800s is acceptable.
The warning about co-Is is because Varun Bajaj has been (re-)added as co-I.
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 30 (program 17012) 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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