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    <title>Balloon-borne Large Aperture Submillimeter Telescope</title>
    <shortName>BLAST</shortName>
    <identifier>ivo://irsa.ipac/BLAST/Images</identifier>
    <curation>
        <publisher ivo-id="ivo://irsa.ipac/IRSA">NASA/IPAC Infrared Science Archive</publisher>
        <creator>
            <name>BLAST team</name>
            <logo/>
        </creator>
        <date role="update">2011-02-24</date>
        <contact>
            <name>IRSA Support Team</name>
            <address/>
            <email>irsasupport@ipac.caltech.edu</email>
            <telephone/>
        </contact>
    </curation>
    <content>
        <subject>submillimeter survey</subject>
        <description>The Balloon-borne Large-Aperture Sub-millimeter Telescope (BLAST) is a
2-m telescope that conducted the first wide-area (&gt; many square
degrees) sub-mm surveys at wavelengths 250--500 um. Built and flown by
an international collaboration headed by the University of
Pennsylvania (P.I. Mark Devlin), the telescope uses a prototype of the
SPIRE camera for the Herschel satellite.  Despite parts of this band
being available to ground-based telescopes from high-altitude sites
such as Mauna Kea (e.g. JCMT) and Chile (e.g. future ALMA site), BLAST
surveys are currently un-matched in sensitivity and area given the
comparatively negligible atmospheric water vapour at 38 km
altitude.</description>
        <referenceURL>https://irsa.ipac.caltech.edu/data/BLAST/overview.html</referenceURL>
        <type>Archive</type>
        <contentLevel>Research</contentLevel>
    </content>
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        <imageServiceType>Pointed</imageServiceType>
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        <maxImageSize>5500</maxImageSize>
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    <capability>
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            <accessURL>https://irsa.ipac.caltech.edu/data/BLAST</accessURL>
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    </capability>
    <coverage>
        <waveband>Millimeter</waveband>
    </coverage>
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