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    <title>Auriga-California Molecular Cloud Catalog</title>
    <shortName>ACMC Catalog</shortName>
    <identifier>ivo://irsa.ipac/Herschel/Catalog/ACMC</identifier>
    <curation>
        <publisher ivo-id="ivo://irsa.ipac/IRSA">NASA/IPAC Infrared Science Archive</publisher>
        <creator>
            <name>Harvey et al. (2013)</name>
        </creator>
        <date role="update">2013-08-22</date>
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            <address/>
            <email>irsasupport@ipac.caltech.edu</email>
            <telephone/>
        </contact>
    </curation>
    <content>
        <subject>star formation</subject>
        <description>The Auriga-California molecular cloud is a large region of relatively modest star formation that is part of the Gould Belt. The "Auriga-California Molecular Cloud" (ACMC) Herschel program observed a 14.5 square degree area in five far-infrared bands.

The ACMC catalog provides photometry for the 60 point-like and very compact sources in each band: PACS 70 and 160 microns, SPIRE 250, 350, and 500 microns.</description>
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    <coverage>
        <waveband>Infrared</waveband>
        <waveband>Millimeter</waveband>
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            <title>HERSCHEL</title>
            <description>The Herschel Auriga-California Molecular Cloud (ACMC)</description>
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                <description>Auriga-California Molecular Cloud Catalog</description>
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