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----- Attempting Submission 1 (Fri Apr 10 20:11:35 GMT 2015) -----</SubmissionLog>
            
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            <SubmissionComments>I am unsure of the optimal values for NSAMP and SAMP-SEQ for the WFC3/IR obs,
I have asked the Contact Scientist for advice on this.

Also, there is a possibility that my target will not be visible when these observations 
are taken (it is an evolving transient that may have faded away completely). In this case
deep observations are still useful as they can set limits on the source magnitude, but
I was unclear whether this would affect the acquisition of the target.

Regards and thanks,

Morgan Fraser</SubmissionComments>
            
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            <SubmissionLog>----- Attempting Submission 1 (Wed Jul 22 21:52:14 GMT 2015) -----</SubmissionLog>
            
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      <Title>Searching for the disappearance of the progenitor of the unique SN 2009ip</Title>
      
      <Abstract>We request HST time in order to obtain late-time imaging of SN 2009ip, where for the first time in the history of astronomy we have monitored a star for many years before it has (possibly) exploded as a supernova (SN). SN 2009ip was first discovered as a giant outburst of a luminous blue variable star in 2009, and three years later an explosive event caused it to reach SN-like luminosities of M_V~-18, and a bolometric luminosity of 10E43 erg/s. We have monitored SN 2009ip extensively over the following 2.5 years, and now seek to conduct the definitive test of whether SN 2009ip exploded as a core-collapse supernova or not, by observing whether SN 2009ip fades below or remains above the progenitor magnitude.</Abstract>
      
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         Institution="University of Cambridge"
         Country="GBR"
         State="England"
         Contact="true" />
      
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         FirstName="Rubina"
         LastName="Kotak"
         ESAMember="true"
         Retired="false"
         UniqueID="12646"
         Institution="The Queen's University of Belfast"
         Country="GBR"
         State="Northern Ireland"
         Contact="false"
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         LastName="Pastorello"
         ESAMember="true"
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         Institution="Osservatorio Astronomico di Padova"
         Country="ITA"
         Contact="false"
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            <ObservingDescription>We wish to obtain deep imaging of the nearby supernova/supernova impostor SN 2009ip, to confirm (or otherwise) the disappearance of the progenitor candidate seen in pre-explosion WFPC2  imaging. We will observe SN 2009ip with ACS/WFC F606W and F814W, with WFC3/UVIS F438W, and with WFC3/IR F606W. As the target is still fading, we wish to observe it as late as possible in Cycle 23 to ensure that it will have faded below the expected flux level of the progenitor.</ObservingDescription>
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         <ScientificCategory>HOT STARS</ScientificCategory>
         
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            <Description>LUMINOUS BLUE VARIABLE</Description>
            
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         <Comments>WFC3 imaging in F435W and F160W</Comments>
         
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