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    <titleInfo>
        <title>High-Contrast Observations with an Integral Field Spectrograph</title>
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    <name type="personal" ID="ntz2101">
        <namePart type="family">Zimmerman</namePart>
        <namePart type="given">Neil Thomas</namePart>
        <role>
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        <affiliation>Columbia University. Astronomy and Astrophysics</affiliation>
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    <name type="personal" ID="bro1">
        <namePart type="family">Oppenheimer</namePart>
        <namePart type="given">Ben R.</namePart>
        <role>
            <roleTerm type="text">thesis advisor</roleTerm>
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        <affiliation>Columbia University. Astronomy and Astrophysics</affiliation>
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        <namePart>Columbia University. Astronomy and Astrophysics</namePart>
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        <dateIssued keyDate="yes">2011</dateIssued>
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    <abstract>This thesis is comprised of work carried out during the commissioning phase of Project 1640, a combined coronagraph--integral field spectrograph for Palomar Observatory&apos;s adaptive optics-equipped 200&apos;&apos; Hale Telescope. I have divided my investigations into three chapters. First, I describe the data reduction pipeline software, which solves a number of data extraction and calibration challenges unique to this kind of instrument. In the second chapter, I demonstrate a novel method for faint companion discovery which takes advantage of the high-precision relative astrometry enabled by a pupil plane reticle grid. This tool, in combination with the spectrophotometric capability of the integral field spectrograph, reveal that the A5V star Alcor has a heretofore unknown M-dwarf companion. In my third chapter, I explore the suitability of combining the non-redundant aperture mask interferometry technique with an integral field spectrograph. In the proof-of-concept observation of the spectroscopic binary star Beta CrB, I retrieve the first near-infrared spectrum of its F-dwarf companion.</abstract>
    <note>Ph.D., Columbia University.</note>
    <subject>
        <topic>Astronomy</topic>
    </subject>
    <identifier type="hdl">http://hdl.handle.net/10022/AC:P:10968</identifier>
    
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