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    <title>Herschel Oxygen Project</title>
    <shortName>HOP</shortName>
    <identifier>ivo://irsa.ipac/Herschel/Spectra/HOP</identifier>
    <curation>
        <publisher ivo-id="ivo://irsa.ipac/IRSA">NASA/IPAC Infrared Science Archive</publisher>
        <creator>
            <name>HOP Team</name>
        </creator>
        <date role="creation">2024-10-02</date>
        <contact>
            <name>IRSA Support Team</name>
            <address/>
            <email>irsasupport@ipac.caltech.edu</email>
            <telephone/>
        </contact>
    </curation>
    <content>
        <subject/>
        <description>The Herschel Oxygen Project (HOP) is Herschel Open Time Key Program (KPOT_pgolds01_1). The main goal of HOP was to use HIFI to probe a range of molecular cloud environments to detect molecular oxygen. The three strongest transitions in the range covered by HIFI from energy levels lower than 120 K above the ground state were selected (487.3 GHz, 773.8 GHz and 1120.7 GHz) for the following targets: Sgr A, Sgr B2(S), OMC-1(Peak 1), Orion Bar, rho Oph A, NGC 1333 IRAS 4A, NGC 6334I and AFGL 2591. Both single LOs and Spectral scans are available. This program also provides a spectral map of rhoOph. The spectra are provided at the four positions indicated in Liseau et al. (2012).</description>
        <referenceURL>https://irsa.ipac.caltech.edu/data/Herschel/HOP/overview.html</referenceURL>
        <type>Survey</type>
        <contentLevel>Research</contentLevel>
    </content>
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            <accessURL use="base">https://irsa.ipac.caltech.edu/SSA?COLLECTION=herschel_hop&amp;</accessURL>
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        <dataSource>survey</dataSource>
        <creationType>archival</creationType>
        <supportedFrame>ICRS</supportedFrame>
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            <pos>
                <long>307.352917</long>
                <lat>40.188611</lat>
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            <size>0.5</size>
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    </capability>
    <coverage>
        <waveband>Millimeter</waveband>
    </coverage>
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