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  <front>
    <journal-meta>
      <journal-id journal-id-type="ojs">aat</journal-id>
      <journal-id journal-id-type="publisher-id" xml:lang="en">
                       Acta Astrophys. Tau.
                </journal-id>
      <journal-title-group>
        <journal-title xml:lang="en">
                    Acta Astrophysica Taurica
                </journal-title>
      </journal-title-group>
      <issn pub-type="epub">2712-925X</issn>
      <publisher>
        <publisher-name>Kiselev Nikolai Nikolaevich,  Mosсow, settlement Moskovskii, Tat'yanin Park Str., 12, Moscow, Russia.</publisher-name>
        <publisher-loc>RU</publisher-loc>
      </publisher>
      <self-uri xlink:href="https://astrophysicatauricum.org/index.php/aat"/>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="publisher-id">9</article-id>
      <article-id pub-id-type="doi">10.31059/aat.vol1.iss1.pp33-38</article-id>
      <article-categories>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Research articles</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="en">Echelle spectrograph at the 2.6 m Shajn telescope</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Lagutin</surname>
              <given-names>Aleksandr</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-1"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Plachinda</surname>
              <given-names>Sergei</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-2"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Shakhovskoi</surname>
              <given-names>Dmitrii </given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-3"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Nekhai</surname>
              <given-names>Evgenii</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-4"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Baklanova</surname>
              <given-names>Dilyara </given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-5"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname> Petrov</surname>
              <given-names>Petr</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-6"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory,  Nauchny 298409, Crimea</institution>
      </aff>
      <aff id="aff-2">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory,  Nauchny 298409, Crimea</institution>
      </aff>
      <aff id="aff-3">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory,  Nauchny 298409, Crimea</institution>
      </aff>
      <aff id="aff-4">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory,  Nauchny 298409, Crimea</institution>
      </aff>
      <aff id="aff-5">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory,  Nauchny 298409, Crimea</institution>
      </aff>
      <aff id="aff-6">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory,  Nauchny 298409, Crimea</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2020-04-15">
        <day>15</day>
        <month>04</month>
        <year>2020</year>
      </pub-date>
      <volume>1</volume>
      <issue>1</issue>
      <fpage>33</fpage>
      <lpage>38</lpage>
      <history>
        <date date-type="received" iso-8601-date="2020-04-10">
          <day>10</day>
          <month>04</month>
          <year>2020</year>
        </date>
      </history>
      <permissions>
        <copyright-statement xml:lang="en">Copyright (c) 2020 Lagutin A., Plachinda S., Shakhovskoi D., Nekhai E., Baklanova D., Petrov P.</copyright-statement>
        <copyright-year>
					2020
				</copyright-year>
        <copyright-holder xml:lang="en">Lagutin A., Plachinda S., Shakhovskoi D., Nekhai E., Baklanova D., Petrov P.</copyright-holder>
        <license license-type="open-access" xlink:href="http://creativecommons.org/licenses/by/4.0" xml:lang="en">
          <license-p> The metadata for this submission is licensed under a  Creative Commons Attribution 4.0 International License.  
 Copyright and publishing rights for texts published in  Acta Astrophysica Taurica  is retained by the authors, with first publication rights granted to the journal.Texts are free to use with proper attribution and link to the licensing  (Creative Commons Attribution 4.0 International).  
     </license-p>
        </license>
      </permissions>
      <self-uri xlink:href="https://astrophysicatauricum.org/index.php/aat/article/view/9"/>
      <abstract xml:lang="en">
        <p> The paper describes the high-resolution echelle spectrograph ESPL developed for the coude focus of the 2.6 m Shajn reflector of the Crimean Astrophysical Observatory.&amp;nbsp; The spectrograph has been regularly operated since 2013.&amp;nbsp; Efficiency of the spectrograph is estimated from observations of stars. </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>astronomy</kwd>
        <kwd>instruments</kwd>
        <kwd>observational facilities</kwd>
        <kwd>spectrometry</kwd>
      </kwd-group>
      <counts>
        <page-count count="6"/>
      </counts>
    </article-meta>
  </front>
  <body/>
  <back>
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</article>
