<?xml version='1.0' encoding='UTF-8'?>
<?xml-model href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1P00.sch" schematypens="http://purl.oclc.org/dsdl/schematron"?>
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<Product_Context xmlns="http://pds.nasa.gov/pds4/pds/v1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:ctli="http://pds.nasa.gov/pds4/ctli/v2" xsi:schemaLocation="http://pds.nasa.gov/pds4/pds/v1 https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1P00.xsd http://pds.nasa.gov/pds4/ctli/v2 https://pds.nasa.gov/pds4/ctli/v2/PDS4_CTLI_1P00_2300.xsd">
  <Identification_Area>
    <logical_identifier>urn:nasa:pds:context:instrument:orm.int2m54.ids</logical_identifier>
    <version_id>1.3</version_id>
    <title>Intermediate Dispersion Spectrograph (IDS)</title>
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      <Modification_Detail>
        <modification_date>2025-12-24</modification_date>
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      </Modification_Detail>
      <Modification_Detail>
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        <description>Updated schema version. Adding missing "telescope" references. Update instrument type/subtype to use valid CTLI LDD.</description>
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      <Modification_Detail>
        <modification_date>2021-09-22</modification_date>
        <version_id>1.0</version_id>
        <description>Initial export from OLAF</description>
      </Modification_Detail>
    </Modification_History>
  </Identification_Area>
  <Reference_List>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:context:telescope:orm.int2m54</lid_reference>
      <reference_type>instrument_to_telescope</reference_type>
    </Internal_Reference>
  </Reference_List>
  <Instrument>
    <name>Intermediate Dispersion Spectrograph (IDS)</name>
    <Type_List_Area>
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          <ctli:type>Camera</ctli:type>
        </ctli:Type_List>
        <ctli:Type_List>
          <ctli:type>Spectrometer</ctli:type>
        </ctli:Type_List>
      </ctli:Type_List_Set>
    </Type_List_Area>
    <description>Intermediate Dispersion Spectrograph (IDS) of the 2.5m Isaac Newton Telescope is a long-slit spectrograph. Two 4096x2048 CCD detectors are available, the red-sensitive RED+2 and blue-sensitive EEV10. 16 gratings are also available. Possible grating and CCD combinations  allow dispersions between 0.24 and 4 √Ö per pixel. The spatial scale is 0.4 and 0.44 arcsec per pixel for EEV10 and RED+2 detector, respectively. The full unvignetted slit length is 3.3 arcmin.</description>
  </Instrument>
</Product_Context>
