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      <Title>The Black Hole Population in Galactic Globular Clusters</Title>
      
      <Abstract>We are engaged in a systematic search for stellar-mass black holes (BHs) in Galactic globular clusters, using a combination of deep radio continuum data, high-resolution X-ray observations, and optical images.  Here we request 128 ksec of Chandra/ACIS observations to image the seven GCs in our sample with no or minimal archival Chandra data, enabling differentiation between accreting BHs, neutron stars, cataclysmic variables, and background galaxies.  We also request two orbits of HST imaging to detect the optical counterpart to a BH candidate in one of these clusters.</Abstract>
      
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         LastName="Chomiuk"
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         Institution="Michigan State University"
         Country="USA"
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         Institution="Michigan State University"
         Country="USA"
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         Institution="University of Alberta"
         Country="CAN"
         State="Edmonton"
         Contact="false"
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         Institution="Curtin University"
         Country="AUS"
         State="Australia"
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         Institution="Texas Tech University"
         Country="USA"
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         Institution="University of Alberta"
         Country="CAN"
         State="Edmonton"
         Contact="false"
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