<?xml version="1.0" encoding="UTF-8"?>
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<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 https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1A00.xsd">
  <Identification_Area>
    <logical_identifier>urn:nasa:pds:context:instrument:multi-host.dbp</logical_identifier>
    <version_id>1.0</version_id>
    <title>Dual Beam Photometer</title>
    <information_model_version>1.10.0.0</information_model_version>
    <product_class>Product_Context</product_class>
    <Modification_History>
      <Modification_Detail>
        <modification_date>2020-06-12</modification_date>
        <version_id>1.0</version_id>
        <description>Creation</description>
      </Modification_Detail>
    </Modification_History>
  </Identification_Area>
  <Reference_List>
    <External_Reference>
      <reference_text>McCord, T.B., A Double Beam Astronomical Photometer, Applied Optics, vol. 7, pp.
475-478, 1968.</reference_text>
    </External_Reference>
  </Reference_List>
  <Instrument>
    <name>Dual Beam Photometer</name>
    <type>Photometer</type>
    <description>Instrument Overview
===================
The dual beam photometer is designed to provide object and sky
photoelectric photometry through a series of 24 filters.  The light
passes through a field lens and then through a 24-position filter
wheel the positions of which are selectable by means of a stepper
motor.  The next element in the optical path is a chopping mirror
which alternates at a rate of 24 Hz between the object and a nearby
patch of sky.  The resulting beam then enters the detector.  A
choice among three different available detectors was made on the
basis of the required sensitivity and wavelength range for the given
object.  The three available detectors include a high quantum
efficiency GaInAs photomultiplier, an S-20 photomultiplier, and an
S-1 photomultiplier.</description>
  </Instrument>
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