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<HSTProposal
   Phase2ID="17020"
   Phase="Phase II"
   AptVersion="Version 2022.4  JWST PRD: PRDOPSSOC-052 ">
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   <!--This file is automatically generated and should not be edited by hand. Editing this file directly is at your own risk.-->
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   <!--APT Version: Version 2022.4  JWST PRD: PRDOPSSOC-052 -->
   <!--Date: Fri Jul 08 20:22:34 GMT 2022-->
   
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            SubmissionMode="STScI"
            SubmissionCounter="1"
            SubmissionSuccessCounter="0"
            HasErrors="true"
            Cycle="30"
            IncludeSysInfo="true"
            NotificationAddress="hkhandrika@stsci.edu">
            
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               os.name="Mac OS X"
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            <ErrorText>The list of Investigators does not match the STScI records for this program.
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
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
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
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
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</ErrorText>
            
            <SubmissionComments />
            
            <SubmissionCommentsCheckSum>0</SubmissionCommentsCheckSum>
            
            <SubmissionLog>----- Attempting Submission 1 (Fri Jul 08 20:22:34 GMT 2022) -----</SubmissionLog>
            
            <Phase2DiagnosticJustification>Should be good to go</Phase2DiagnosticJustification>
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   <ProposalInformation
      Category="CAL/WFC3"
      SnapPriority="Normal Priority"
      PureParallelProposal="false"
      Cycle="30"
      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), 16585 (Cy 29)</Abstract>
      
      <PrincipalInvestigator
         Honorific="Mr."
         FirstName="Harish"
         LastName="Khandrika"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="17320"
         Institution="Space Telescope Science Institute"
         Country="USA"
         State="MD"
         Contact="true" />
      
      <CoInvestigator
         FirstName="Benjamin"
         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" />
      
      <Questions>
         
         <Phase2Questions>
            
            <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 completed by Khandrika and
Kuhn (2021-15) and Kuhn and Khandrika (2021-16). Analysis shows partial degradation in lamp performance, possibly due to photometric
sensitivity loss but also overall tungsten and deuterium lamp degradation. The bluer filters show greater reduction, indicating that the two lamps may
be reddening over time. New never-before-seen artifacts have been discovered in the flat field ratios, including a dark region named the bowling pin
between amp A and B quadrants as well as a dark vertical box in amp B dubbed the roller shade. New data and further analysis will help with determining how much more degradation will occur and help keep track of any further issues.</ObservingDescription>
         </Phase2Questions>
      </Questions>
      
      <Orbits
         ThisCycle2GyroPrimary="1" />
      
      <Phase1ProposalInformation>
         
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            Default="true">0</ProprietaryPeriod>
         
         <CalibProp>false</CalibProp>
         
         <FundamentalPhysics>false</FundamentalPhysics>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="true"
         ProposalSize="EXEMPT">
         
         <Availability>RESTRICTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
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