<?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"?>
<?xml-model href="https://pds.nasa.gov/pds4/ctli/v2/PDS4_CTLI_1P00_2300.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" 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:ctio-cerro_tololo.smarts_1m0.fruttispec</logical_identifier>
    <version_id>1.4</version_id>
    <title>CTIO 1.0m 2DFrutti Spectrograph</title>
    <information_model_version>1.25.0.0</information_model_version>
    <product_class>Product_Context</product_class>
    <Alias_List>
      <Alias>
        <alternate_title>urn:nasa:pds:context:instrument:ctio.smarts1m0.fruttispec</alternate_title>
      </Alias>
      <!-- deprecated LID -->
    </Alias_List>
    <Modification_History>
      <Modification_Detail>
        <modification_date>2026-07-07</modification_date>
        <version_id>1.4</version_id>
        <description>Removed duplicate Internal_Reference entries from Reference_List.</description>
      </Modification_Detail>
      <Modification_Detail>
        <modification_date>2025-12-24</modification_date>
        <version_id>1.3</version_id>
        <description>Adding missing "facility" references. Adding missing "telescope" references.</description>
      </Modification_Detail>
      <Modification_Detail>
        <modification_date>2025-12-24</modification_date>
        <version_id>1.2</version_id>
        <description>Updated schema version. Adding missing "facility" references. Adding missing "telescope" references.</description>
      </Modification_Detail>
      <Modification_Detail>
        <modification_date>2025-01-02</modification_date>
        <version_id>1.1</version_id>
        <description>Updated schema version. Adding missing "telescope" references.</description>
      </Modification_Detail>
      <Modification_Detail>
        <modification_date>2021-12-07</modification_date>
        <version_id>1.0</version_id>
        <description>per RMS, deprecated ctio in favor of ctio-cerro_tololo</description>
      </Modification_Detail>
    </Modification_History>
  </Identification_Area>
  <Reference_List>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:context:telescope:ctio-cerro_tololo.smarts_1m0</lid_reference>
      <reference_type>instrument_to_telescope</reference_type>
    </Internal_Reference>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:context:facility:observatory.ctio-cerro_tololo</lid_reference>
      <reference_type>instrument_to_facility</reference_type>
    </Internal_Reference>
  </Reference_List>
  <Instrument>
    <name>CTIO 1.0m 2DFrutti Spectrograph</name>
    <Type_List_Area>
      <ctli:Type_List>
        <ctli:type>Spectrometer</ctli:type>
      </ctli:Type_List>
    </Type_List_Area>
    <description>The Boller &amp; Chivens fast uv-transmitting image tube spectrograph was used at the f/10 focus of the 1.0m telescope.  Plate Scale (at f/10 focal plane)      19.5 arcsec/mm Slit Length     19mm mm, 370 arcsec Collimator Focal Length         900 mm Point source collimated beam diameter   90 mm Collimator-to-Camera Angle      49 degrees Grating size    128[INVALID_PDS_CHARACTER]102 mm Camera Focal Length     140 mm Demagnification         6.455 Plate Scale (at detector)     125 arcsec/mm  The 2D-Frutti was a two-dimensional photon counting detector, originally developed by Steve Shectman then of the Mt Wilson and Las Campanas Observatories. The sensitivity of this detector is determined by the S-20 photocathode of the Carnegie image tube which provides the first intensification stage.  This peaks at ~ 4200A, declining slowly toward the red, so that 7300A can be taken as its red limit.  In the UV, the 2D-Frutti was sensitive down to the atmospheric cutoff (3200A).  The 2D-Frutti offered a format up to 1.5-M pixels, zero readout noise, and low dark current ( &lt; 1 count/pixel/hour for 1x1 binning). Conversely the 2D-Frutti could be irreversibly damaged by over illumination and count rates must be further limited to typically &lt; 1 cts/pixel/second, because of coincidence losses. Even with these precautions, the 2D-Frutti was not really all that linear.         </description>
  </Instrument>
</Product_Context>
