<?xml version="1.0" encoding="UTF-8"?>
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" article-type="instruments-and-methods" xml:lang="en">
  <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">121</article-id>
      <article-id pub-id-type="edn">UTTPNS</article-id>
      <article-categories>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Instruments and Methods</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="en">TeA – Telescope Analyzer</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Emelianov</surname>
              <given-names>Eduard</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-1"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">Special Astrophysical Observatory of the Russian Academy of Sciences, Nizhnij Arkhyz 369167, Zelenchukskiy region, Karachai-Cherkessian Republic, Russia</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2026-03-31">
        <day>31</day>
        <month>03</month>
        <year>2026</year>
      </pub-date>
      <volume>7</volume>
      <issue>1</issue>
      <fpage>8</fpage>
      <lpage>11</lpage>
      <history>
        <date date-type="received" iso-8601-date="2026-03-12">
          <day>12</day>
          <month>03</month>
          <year>2026</year>
        </date>
      </history>
      <permissions>
        <copyright-statement xml:lang="en">Copyright (c) 2026 Eduard Emelianov</copyright-statement>
        <copyright-year>
					2026
				</copyright-year>
        <copyright-holder xml:lang="en">Eduard Emelianov</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/121"/>
      <abstract xml:lang="en">
        <p> We have developed a multipurpose device for studying the optics and mechanics of the BTA and Zeiss-1000 telescopes. The heart of the device is a ZWO ASI 1600 MM Pro CMOS light detector mounted on a three-axis stage. The device was tested on the Zeiss-1000 and BTA telescopes. Based on the BTA tests, the spectrum of image oscillations along both axes was evaluated, as well as the possibility of using the device for estimating the aberration axis position (by direction of coma at the field of view), taking hartmannogramms, and recording images of stellar fields to measure coefficients of the pointing correction system. </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>instrumentation</kwd>
        <kwd>telescopes</kwd>
        <kwd>optics control</kwd>
      </kwd-group>
      <funding-group>
        <funding-statement xml:lang="en">
                                                    Information on funding is not available
                                                </funding-statement>
      </funding-group>
      <counts>
        <page-count count="4"/>
      </counts>
    </article-meta>
  </front>
  <body/>
</article>
