<?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:dushanbe.rcc.sanglok</logical_identifier>
    <version_id>1.4</version_id>
    <title>Sanglok Observatory Photometer-Polarimeter</title>
    <information_model_version>1.25.0.0</information_model_version>
    <product_class>Product_Context</product_class>
    <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 "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 "telescope" references.</description>
      </Modification_Detail>
      <Modification_Detail>
        <modification_date>2025-01-02</modification_date>
        <version_id>1.1</version_id>
        <description>Updated schema version. Update instrument type/subtype to use valid CTLI LDD.</description>
      </Modification_Detail>
      <Modification_Detail>
        <modification_date>2020-02-18</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:dushanbe.rcc</lid_reference>
      <reference_type>instrument_to_telescope</reference_type>
    </Internal_Reference>
    <External_Reference>
      <reference_text>Kayumov V.V., N.N. Kiselev, P.A. Pushnin, V.Yu. Rakhimov, V.I. Siklitskij, K.V.
Tarasov, G.P. Chernova, and V.N. Yakutovich, The investigation of the
photometer-polarimeter of the 1-m RCC telescope. Bull. Inst. Astrophyz. Tadjik Acad.
Sci. No. 78, p. 10-16 (in Russian), 1989.</reference_text>
    </External_Reference>
  </Reference_List>
  <Instrument>
    <name>Sanglok Observatory Photometer-Polarimeter</name>
    <Type_List_Area>
      <ctli:Type_List>
        <ctli:type>Polarimeter</ctli:type>
      </ctli:Type_List>
    </Type_List_Area>
    <description>The single-channel photometer-polarimeter at Sanglok Observatory was built at the Institute of Astrophysics of Tadjik Academy of Sciences. It allowed quasi-simultaneous photometric and polarimetric observations. The useble wavelength range was 0.35-0.75 microns. The polarimeter worked on the modulation principle with a rapidly-rotating polarizer as the analyzer. The rotation frequency of the polarizer was about 33 revolutions per second. Four impulse counters were used to registrate impulses during each quarter of a polarizer revolution. The total number of impulses in four positions of the polarizer allow the derivation of the values of the Stokes Q and U parameters and hence the value of the degree of linear polarization and the position angle. The observing procedure included consecutive measurements of an object and a sky background near the object with the same diaphragm.  To control the stability of instrument operation the measurements of a built-in signal generator were used.  For more information, see  Kayumov V.V., Kiselev N.N., Pushnin P.A., Rakhimov V.Yu., Siklitskij V.I., Tarasov K.V., Chernova G.P., Yakutovich V.N. The investigation of the photometer-polarimeter of the 1-m RCC telescope. Bull. Inst. Astrophyz. Tadjik Acad. Sci No. 78, p. 10-16, 1989 (in Russian).</description>
  </Instrument>
</Product_Context>
