<?xml version="1.0" encoding="utf-8"?>
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  xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_2_2.xsd">
  <Version>2.2.2</Version>
<Instrument>
    <ResourceID>spase://SMWG/Instrument/OAC/OACT</ResourceID>
    <ResourceHeader>
      <ResourceName>OACT (VSO notation)</ResourceName>
      <ReleaseDate>2012-04-12T00:00:00Z</ReleaseDate>
      <Description>The Catania Astrophysicsl Observatory (OAC)
Telescope (OACT) used for solar observations has a
Ha Lyot-filter (bandwidth of 0.25 - 0.50 Angstrom, tunable filter 
range +/- 16 Angstrom) and a 1360 x 1200 Astromed TE4 CCD array. 
In patrol full-disk mode the camera can taken images every 60 s, 
with a dynamical range of 16 bit.  It has an H-alpha Halle filter
with a camera for limb observations.  It has a 150 mm refractor 
with a focal length of 230 cm.  A Cook refractor is used to make 
daily drawings of sunspot-groups from visual observation.  See 
http://web.ct.astro.it/sun/instrument.htm.</Description>
      <Contact>
        <PersonID>spase://SMWG/Person/Francesca.Zuccarelli</PersonID>
        <Role>GeneralContact</Role>
      </Contact>
      <PriorID>spase://vspo/instrument/171</PriorID>
    </ResourceHeader>
    <InstrumentType>Imager</InstrumentType>
    <InvestigationName>OACT (VSO notation) on OAC</InvestigationName>
    <ObservatoryID>spase://SMWG/Observatory/OAC</ObservatoryID>
  </Instrument>
</Spase>