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    <title>Evolution of Interstellar Dust</title>
    <shortName>SAG-4</shortName>
    <identifier>ivo://irsa.ipac/Herschel/Spectra/SAG-4</identifier>
    <curation>
        <publisher ivo-id="ivo://irsa.ipac/IRSA">NASA/IPAC Infrared Science Archive</publisher>
        <creator>
            <name>SAG-4 team</name>
        </creator>
        <date role="creation">2017-10-27</date>
        <contact>
            <name>IRSA Support Team</name>
            <email>irsasupport@ipac.caltech.edu</email>
        </contact>
    </curation>
    <content>
        <subject/>
        <description>The goal of the "Evolution of interstellar dust" guaranteed time key project (PI: A. Abergel &amp; A. Zavagno) is to explore with Herschel the far-infrared (FIR) to submillimeter (submm) emission properties of dust particles in a wide range of regions within our Galaxy, from very diffuse clouds to sites of star formation and proto-stars. Photometric data taken with SPIRE and PACS are complemented with spectroscopy using the FTS of SPIRE and PACS to derive the physical conditions of the gas from the lines of [CI], the high-level rotational lines of CO, and the major cooling lines of [CII] and [OI].</description>
        <referenceURL>https://irsa.ipac.caltech.edu/data/Herschel/SAG-4/overview.html</referenceURL>
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        <contentLevel>Research</contentLevel>
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    <coverage>
        <waveband>Infrared</waveband>
        <waveband>Millimeter</waveband>
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