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        <logical_identifier>urn:nasa:pds:uranus_occ_u14_opmt_200cm:data</logical_identifier>
        <version_id>2.0</version_id>
        <title>Data Collection for Uranus System Occultation of Star u14 (Hipparcos 79085) Observed from the OPMT 200cm Telescope</title>
        <information_model_version>1.14.0.0</information_model_version>
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        <Citation_Information>
            <author_list>French, Richard G.; McGhee-French, Colleen A.; Gordon, Mitchell K.</author_list>
            <publication_year>2020</publication_year>
            <keyword>uranus rings</keyword>
            <keyword>uranus rings stellar occultation</keyword>
            <keyword>uranus rings stellar occultation radial profiles</keyword>
            <description>This collection contains calibrated and derived data resulting from the occultation of star u14 (Hipparcos 79085) by the rings of Uranus.</description>
        </Citation_Information>
        <Modification_History>
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            <Modification_Detail>
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                <description>Corrected Pic du Midi context product LID, and updated VIDs in collection_data.csv</description>
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            <processing_level>Derived</processing_level>
            <description>This collection contains calibrated and derived data resulting from the occultation of star u14 (Hipparcos 79085) by the rings of Uranus.</description>
            <Science_Facets>
                <wavelength_range>Infrared</wavelength_range>
                <discipline_name>Ring-Moon Systems</discipline_name>
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            <Observing_System_Component>
                <name>Bernard Lyot 2.0m</name>
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            <alternate_designation>U Rings</alternate_designation>
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                Any or all of the rings in the ring system of Uranus.
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                LID of central body: urn:nasa:pds:context:target:planet.uranus;
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                        <geom:spice_kernel_file_name>ura111.bsp</geom:spice_kernel_file_name>
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            <reference_type>collection_to_document</reference_type>
            <comment>The User Guide for Earth-based Uranus Stellar Occultations.</comment>
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            <comment>Diagram of the Uranus system showing the occultation track.</comment>
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            <comment>Illustrates some of the processing steps involved in normalizing a time-series occultation light curve from counts per second to units of stellar flux.</comment>
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        <Internal_Reference>
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            <comment>Gallery of square-well diffraction model fits to individual ring profiles.</comment>
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        <Internal_Reference>
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            <comment>The support bundle for all of the Earth-based Uranus system occultations.</comment>
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        <Internal_Reference>
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            <reference_type>collection_to_resource</reference_type>
            <comment>The fitted model of the ring system upon which the data are based.</comment>
        </Internal_Reference>
        <External_Reference>
            <reference_text>Elliot et al. (1984). "Structure of the Uranian rings. I. Square-well model and particle-size constraints" Astron J. 89, 1587-1603. http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1984AJ.....89.1587E&amp;data_type=PDF_HIGH&amp;whole_paper=YES&amp;type=PRINTER&amp;filetype=.pdf</reference_text>
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    </Reference_List>
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            <creation_date_time>2024-03-18T16:34:04Z</creation_date_time>
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