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    xmlns="http://pds.nasa.gov/pds4/pds/v1"
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  <Identification_Area>
    <logical_identifier>urn:nasa:pds:context:telescope:orm.int2m54</logical_identifier>
    <version_id>1.1</version_id>
    <title>2.54-m Isaac Newton Grubb-Parsons Cass. equat. refl. (INT)</title>
    <information_model_version>1.19.0.0</information_model_version>
    <product_class>Product_Context</product_class>
    <Modification_History>
      <Modification_Detail>
        <modification_date>2021-09-22</modification_date>
        <version_id>1.0</version_id>
        <description>Initial export from OLAF</description>
      </Modification_Detail>
      <Modification_Detail>
        <modification_date>2023-03-02</modification_date>
        <version_id>1.1</version_id>
        <description>Added reference to ids and wfc</description>
      </Modification_Detail>
    </Modification_History>
  </Identification_Area>
  <Reference_List>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:context:instrument:orm.int2m54.wfc</lid_reference>
      <reference_type>telescope_to_instrument</reference_type>
    </Internal_Reference>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:context:instrument:orm.int2m54.ids</lid_reference>
      <reference_type>telescope_to_instrument</reference_type>
    </Internal_Reference>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:context:facility:observatory.orm</lid_reference>
      <reference_type>telescope_to_facility</reference_type>
    </Internal_Reference>
  </Reference_List>
  <Telescope>
    <aperture unit="m">2.54</aperture>
    <telescope_longitude unit="deg">342.12236</telescope_longitude>
    <telescope_latitude unit="deg">28.762056</telescope_latitude>
    <telescope_altitude unit="m">2336</telescope_altitude>
    <coordinate_source>Geodetic - WGS 84 datum</coordinate_source>
    <description>The Isaac Newton Telescope or INT is a 2.54 m (100 in.) optical telescope run by the
ING at Roque de los Muchachos Observatory on La Palma in the Canary Islands since
1984.

The La Palma INT is a Cassegrain telescope, with a 2.54 m diameter primary mirror and
a focal length of 8.36 m. The f/3.29 Prime focus, used with the Wide Field Camera,
allows an unvignetted field of view of 33 arcminutes (approximately 0.3 square
degrees). There is also a secondary focal station, the f/15 Cassegrain focus, which
possesses a 20 arcminute field of view and is the mount point for the Intermediate
Dispersion Spectrograph.

The pointing accuracy of the telescope is around 5 arcseconds, but a sophisticated
autoguider, which tracks a given guide star and makes small corrections to the
telescope tracking, allows a guiding accuracy of better than an arcsecond on better
than 20th magnitude guide stars in support of the typical 0.8-1.5 arcsec seeing at
the INT.</description>
  </Telescope>
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