<?xml version="1.0" encoding="ISO-8859-1"?>

<HSTProposal
   Phase1ID="10828"
   Phase2ID="10828"
   Phase="Phase II"
   AptVersion="Version 16.0.2 ">
   <!--**********************************************************************************************************************-->
   <!--This file is automatically generated and should not be edited by hand. Editing this file directly is at your own risk.-->
   <!--**********************************************************************************************************************-->
   
   <ToolData />
   
   <ProposalInformation
      Category="GO"
      PureParallelProposal="false"
      Cycle="15"
      STScIEditNumber="1">
      
      <Title>Debris Disks Around Nearby Young M Dwarfs</Title>
      
      <Abstract>We propose to obtain HST/ACS F606W coronagraphic imaging of two young (10--50 Myr), nearby (25--55 pc) M dwarfs to resolve their debris disks in scattered light.  Little is known about debris disks around M dwarfs, as very few examples are known and only one, the AU Mic debris disk, has been spatially resolved thus far.  IR/sub-mm photometry of our targets indicate large quantities of exceptionally cold dust, comparable to the prototype AU Mic system, and make them excellent candidates for resolved studies with physical resolutions of 1-2 AU.  HST/ACS provides an excellent capability for detection of disks in scattered light.  Modeling the disk images will allow us to quantify the radial and vertical structure and to search for disk sub-structure, a potential probe of the planet formation process in these young systems. Our program can expand the census of young resolved debris disks, of which very few are currently known.  M dwarfs have been largely over-looked in myriad imaging searches: our program will complement the many current programs focusing on the higher-mass AFGK stars.  Because our targets belong to nearby young moving groups with known resolved disks around higher mass stars, a key potential outcome of our program is comparative study of coeval debris disks over a range of stellar masses.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Michael"
         MiddleInitial="C."
         LastName="Liu"
         ESAMember="false"
         UniqueID="4308"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="University of Hawaii"
            USState="HI"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="David"
         MiddleInitial="R."
         LastName="Ardila"
         ESAMember="false"
         UniqueID="6478"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="California Institute of Technology"
            USState="CA"
            Country="USA" />
      </CoInvestigator>
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription>We will use the ACS/HRC coronagraph with the 0.9'' mask to resolve disks around two M dwarfs. For each target and PSF reference star we will take short, non-coronagraphic, and long (one orbit each) coronagraphic exposures. The PSF reference star is a star of the same spectral type but brighter and as spatially close to the target as possible. The coronagraphic observations will be done using the F606W filter, which is well calibrated and has been used in the past for this kind of work. Target acquisition is done in a narrow-band filter to avoid saturation. For each target, two orbits are necessary, one for the target and the other for the PSF reference.</ObservingDescription>
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
         </Phase2Questions>
      </Questions>
      
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         ThisCycle2GyroPrimary="4"
         ThisCycle2GyroParallel="0"
         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
         AfterNext2GyroPrimary="0"
         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/local/d1/APT1522/C:\local\d1\proposals\hst\mdwarfs_cyc15\mdwarfs_v3.pdf">
         
         <ScientificCategory>ISM AND CIRCUMSTELLAR MATTER</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="DUST" />
         
         <ScientificKeyword2
            Keyword="PROTO-PLANETARY DISKS" />
         
         <ScientificKeyword3
            Keyword="VERY LOW MASS STARS AND BROWN DWARFS" />
         
         <ScientificKeyword4
            Keyword="EXTRA-SOLAR PLANETS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
         
         <Spitzer>false</Spitzer>
         
         <Survey>false</Survey>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="true">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
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         ReferenceFrame="ICRS"
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         DecPM="-0.09394"
         Epoch="1991.25">
         
         <PrimaryCategory>STAR</PrimaryCategory>
         
         <PrimaryDescription>
            
            <Description>M V-IV</Description>
         </PrimaryDescription>
         
         <Comments>Hipparcos Coordinates
V=10.1
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         Epoch="2000.0">
         
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         <PrimaryDescription>
            
            <Description>M V-IV</Description>
         </PrimaryDescription>
         
         <Comments>Tycho Coordinates
V=11.65
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               Magnitude="11.06" />
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            <Configuration>
               
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            <Configuration>
               
               <Config>ACS/HRC</Config>
               
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            </Configuration>
            
            <Configuration>
               
               <Config>ACS/HRC</Config>
               
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               <Config>ACS/HRC</Config>
               
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