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   Phase="Phase II"
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            <ErrorText>The list of Investigators does not match the STScI records for this program.
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
MAXIMUM DURATION EXCEEDED FOR INTERNAL OR EARTH CALIB SU
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser
FLASH level may be too low for this exposure or a short subexposure.  See extended explanation in the diagnostic browser</ErrorText>
            
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            <SubmissionLog>----- Attempting Submission 1 (Tue Jun 29 18:29:39 GMT 2021) -----
HST Phase II Proposal 16585  successfully submitted.
Receipt: # 16585-1

----- Attempting Submission 2 (Tue Jun 29 19:38:41 GMT 2021) -----</SubmissionLog>
            
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      PureParallelProposal="false"
      Cycle="29"
      STScIEditNumber="0">
      
      <Title>WFC3 UVIS Internal Flats</Title>
      
      <Abstract>Internal flats are taken across all 62 UVIS filters in order to track the stability of the UVIS pixel-to-pixel sensitivity, the functionality of the filters, and the operation of the Tungsten lamp. The monitor uses both the Tungsten and Deuterium lamps, the former for optical and the latter for UV wavelengths. This is a continuation of the following proposals:

12337 (Cy 18), 12711 (Cy 19), 13097 (Cy 20), 13568 (Cy 21), 14028 (Cy 22)
14390 (Cy 23), 14547 (Cy 24), 14997 (Cy 25), 15590 (Cy 26), 15730 (Cy 27)
16410 (Cy 28)</Abstract>
      
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         FirstName="Harish"
         LastName="Khandrika"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="17320"
         Institution="Space Telescope Science Institute"
         Country="USA"
         State="MD"
         Contact="true" />
      
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         LastName="Kuhn"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="27117"
         Institution="Space Telescope Science Institute"
         Country="USA"
         State="MD"
         Contact="true"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Ms."
         FirstName="Jennifer"
         LastName="Mack"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="6012"
         Institution="Space Telescope Science Institute"
         Country="USA"
         State="MD"
         Contact="true"
         AdminUSPI="false" />
      
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            <ObservingDescription>This program consists of 3 orbits with the Deuterium (D2) lamp for the following filters: F218W, F200LP, F225W, F275W, F280N, F300X, F336W, F343N, F373N, F390M, F390W, F395N, FQ232N, FQ243N, FQ378N, and FQ387N. 
8 orbits will be taken with the Tungsten lamp for the remaining 46 filters. 

Observations in the 4 filters, F390W, F438W, F606W, and F814W with the Tungsten lamp will be repeated 2 times over the cycle for a total of 2 orbits.

------ Calibration Justification -------

We will compare the flat fields taken in this cycle to the SMOV flat fields to check for any temporal change in the illumination pattern/brightness of the lamps, and serves as a way to monitor the health of all of the UVIS filters. Current analysis of the UVIS flat fields is underway by Khandrika and Kuhn (2021 ISR TBD). Analysis shows partial degradation in lamp performance, possibly due to photometric sensitivity loss but also overall tungsten lamp degradation. Deuterium lamp analysis is to be determined as well.</ObservingDescription>
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