<?xml version="1.0" encoding="UTF-8"?>
<?xml-model href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1G00.sch" schematypens="http://purl.oclc.org/dsdl/schematron"?>

<Product_Context xmlns="http://pds.nasa.gov/pds4/pds/v1"
    xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
    xsi:schemaLocation="http://pds.nasa.gov/pds4/pds/v1 http://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1G00.xsd">
    <Identification_Area>
        <logical_identifier>urn:nasa:pds:context:telescope:las_campanas.magellan_clay_6m5</logical_identifier>
        <version_id>1.0</version_id>
        <title>Landon T. Clay Telescope at Las Campanas Observatory</title>
        <information_model_version>1.16.0.0</information_model_version>
        <product_class>Product_Context</product_class>
        
        <Modification_History>
            <Modification_Detail>
                <modification_date>2021-08-12</modification_date>
                <version_id>1.0</version_id>
                <description>
                    Created by A.C.Raugh from information downloaded from the 
                    Las Campanas Observatory web site on 2021-08-21.
                </description>
            </Modification_Detail>
        </Modification_History>
    </Identification_Area>
    
    <Reference_List>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:facility:observatory.las_campanas</lid_reference>
            <reference_type>telescope_to_facility</reference_type>
        </Internal_Reference>
    </Reference_List>
    
    <Telescope>
        <aperture unit="m">6.5</aperture>
        <telescope_altitude unit="m">2400</telescope_altitude>
        <description>
            The Landon T. Clay telescope is one of a twin pair (with the Walter Baade)
            located on Cerro Manqui at Las Campanas Observatory. The primary mirror is
            an f/1.25 parabaloid with a honeycomb internal structure to reduce weight.
            The telescope optics include active controls, including correction of 
            low-order aberrations by controlling the figure of the primary mirror.
        </description>
    </Telescope>
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