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    <Identification_Area>
        <logical_identifier>urn:jaxa:darts:context:instrument:mascot.micromega</logical_identifier>
        <version_id>1.0</version_id>
        <title>MicrOmega for MASCOT</title>
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        <Modification_History>
            <Modification_Detail>
                <modification_date>2021-02-10</modification_date>
                <version_id>1.0</version_id>
                <description>Initial version.</description>
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    </Identification_Area>
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        <Internal_Reference>
            <lid_reference>urn:jaxa:darts:context:instrument_host:lander.mascot</lid_reference>
            <reference_type>instrument_to_instrument_host</reference_type>
        </Internal_Reference>
        <External_Reference>
            <doi>10.1007/s11214-017-0335-y</doi>
            <reference_text>
                J.-P. Bibring, V. Hamm, Y. Langevin, C. Pilorget, A. Arondel, M. Bouzit, M. Chaigneau,
                B. Crane, A. Darié, C. Evesque, J. Hansotte, V. Gardien, L. Gonnod, J.-C. Leclec'h,
                L. Meslier, T. Redon, C. Tamiatto, S. Tosti, N. Thoores,
                The MicrOmega Investigation Onboard Hayabusa2,
                Space Sci. Rev., 208, 401-412, 2017.
            </reference_text>
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            </ctli:Type_List>
        </Type_List_Area>
        <naif_instrument_id>-37730</naif_instrument_id>
        <description>MicrOmega is a near-IR hyperspectral microscope and is designed to determine the mineralogical composition of the asteroid surface.</description>
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