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   Phase2ID="13508"
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----- Attempting Submission 1 (Mon Aug 26 13:00:42 GMT 2013) -----
  HST Phase I Proposal 2184 (kraemer.pdf.apt) successfully submitted.</SubmissionLog>
            
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            <SubmissionLog>----- Attempting Submission 1 (Thu Sep 26 20:33:22 GMT 2013) -----</SubmissionLog>
            
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Object has been observed numerous time with STIS/E140M, so BOT not needed.</Phase2DiagnosticJustification>
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      Category="GO"
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      <Title>Resolved Spectroscopy of the Extended X-ray Emission in NGC 4151:  New Insights  into AGN-driven Outflows</Title>
      
      <Abstract>AGN feedback, in the form of winds or jets, is likely the mechanism that connects the growth of galactic bulges and their super-massive black holes.  AGN-driven winds are most directly studied at the spatial scale of the narrow line region (NLR), but little is known of NLR X-ray emitting gas, which may be the dominant component in mass outflows.  Given its brightness and orientation, the Seyfert 1 galaxy NGC 4151 is one of the few AGN for which we can resolve the X-ray NLR. We will obtain a 250 ksec Chandra/HETG observation, at a roll angle which will permit us to map the kinematics and ionization structure of the high-ionization gas.  We will use these data to determine the mass outflow rate and kinetic luminosity of the X-ray gas, and, thus, its role in AGN feedback.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Prof."
         FirstName="Steven"
         LastName="Kraemer"
         ESAMember="false"
         UniqueID="4182"
         Institution="Catholic University of America"
         Country="USA"
         State="DC"
         Contact="true" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="T."
         MiddleInitial="Jane"
         LastName="Turner"
         ESAMember="false"
         UniqueID="4739"
         Institution="University of Maryland Baltimore County"
         Country="USA"
         State="MD"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="D."
         MiddleInitial="Michael"
         LastName="Crenshaw"
         ESAMember="false"
         UniqueID="447"
         Institution="Georgia State University Research Foundation"
         Country="USA"
         State="GA"
         Contact="false"
         AdminUSPI="false" />
      
      <Questions>
         
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            <ObservingDescription>we will obtain {\it HST}/STIS spectra of the nucleus of NGC~4151 with the 
E140M grating to cover the important UV absorption lines in the range 1150 --
1710 \AA~ at a velocity resolution of $\sim$7 km s$^{-1}$ (NGC~4151 is the only 
Seyfert galaxy too bright to be observed by COS). Using the STIS exposure 
time calculator and the average continuum flux of 2.8 $\times$ 10$^{-13}$ 
ergs s$^{-1}$ cm$^{-2}$ \AA$^{-1}$~ at 1345 \AA, we will obtain a S/N 
$\approx$ 5 per resolution element with an exposure time of 5100 s (2 
orbits), similar to spectra we have obtained of this AGN over the years.</ObservingDescription>
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
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         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
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         AfterNext2GyroParallel="0" />
      
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         TotalTargets="1"
         Attachment="/Users/blacker/Desktop/Chandra-Approved-15/15700502_skraemer_merged.pdf"
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         <ScientificCategory />
         
         <ProprietaryPeriod>Default</ProprietaryPeriod>
         
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         <UvInit>false</UvInit>
         
         <Treasury>false</Treasury>
         
         <MultiCycleTreasury>false</MultiCycleTreasury>
         
         <Theory>false</Theory>
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         PCFlag="true"
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         <Availability>SUPPORTED</Availability>
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         Name="NGC-4151"
         Number="1"
         ReferenceFrame="ICRS"
         ProvisionalCoordinates="12 10 32.5740 +39 24 20.88">
         
         <PrimaryCategory>GALAXY</PrimaryCategory>
         
         <PrimaryDescription>
            
            <Description>NLR</Description>
            
            <Description>SEYFERT</Description>
            
            <Description>WIND</Description>
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         <Comments>This object was generated by the targetselector and retrieved from the SIMBAD database.</Comments>
         
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            <Equinox>J2000</Equinox>
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         <Equinox>J2000</Equinox>
         
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               Magnitude="11.48" />
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         TotalOrbits="2"
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         CoordinatedParallel="false"
         TargetOfOpportunity="No"
         CVZ="false"
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               <Coronography>No</Coronography>
               
               <Polarimetry>No</Polarimetry>
               
               <SpectralElement>E140M</SpectralElement>
               
               <Wavelength>1425</Wavelength>
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