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<article article-type="research-article" dtd-version="1.3" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xml:lang="ru"><front><journal-meta><journal-id journal-id-type="publisher-id">izmertech</journal-id><journal-title-group><journal-title xml:lang="ru">Измерительная техника</journal-title><trans-title-group xml:lang="en"><trans-title>Izmeritel`naya Tekhnika</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">0368-1025</issn><issn pub-type="epub">2949-5237</issn><publisher><publisher-name>ФГУП "ВНИИФТРИ"</publisher-name></publisher></journal-meta><article-meta><article-id custom-type="elpub" pub-id-type="custom">izmertech-1368</article-id><article-categories><subj-group subj-group-type="heading"><subject>Research Article</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="ru"><subject>ОПТИКО-ФИЗИЧЕСКИЕ ИЗМЕРЕНИЯ</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>OPTICOPHYSICAL MEASUREMENTS</subject></subj-group></article-categories><title-group><article-title>Использование эталонного источника cинхротронного излучения для калибровки чувствительности телескопа с ПЗС-матрицей и высоким угловым разрешением</article-title><trans-title-group xml:lang="en"><trans-title></trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Аневский</surname><given-names>С. И.</given-names></name></name-alternatives><email xlink:type="simple">anevsky@vniiofi.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Золотаревский</surname><given-names>Ю. М.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Крутиков</surname><given-names>В. Н.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Лебедев</surname><given-names>А. М.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.ru</email><xref ref-type="aff" rid="aff-2"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Минаева</surname><given-names>О. А.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Минаев</surname><given-names>Р. В.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Сенин</surname><given-names>Д. С.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.ru</email><xref ref-type="aff" rid="aff-1"/></contrib><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Станкевич</surname><given-names>В. Г.</given-names></name></name-alternatives><email xlink:type="simple">noemail@neicon.ru</email><xref ref-type="aff" rid="aff-2"/></contrib></contrib-group><aff xml:lang="ru" id="aff-1"><institution>Всероссийский научно-исследовательский институт оптико-физических измерений</institution><country>Russian Federation</country></aff><aff xml:lang="ru" id="aff-2"><institution>Национальный исследовательский центр «Курчатовский институт»</institution><country>Russian Federation</country></aff><pub-date pub-type="collection"><year>2015</year></pub-date><pub-date pub-type="epub"><day>07</day><month>02</month><year>2023</year></pub-date><volume>0</volume><issue>5</issue><fpage>33</fpage><lpage>36</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; ФГУП "ВНИИФТРИ", 2023</copyright-statement><copyright-year>2023</copyright-year><copyright-holder xml:lang="ru">ФГУП "ВНИИФТРИ"</copyright-holder><copyright-holder xml:lang="en">ФГУП "ВНИИФТРИ"</copyright-holder><license xlink:href="https://www.izmt.ru/jour/about/submissions#copyrightNotice" xlink:type="simple"><license-p>https://www.izmt.ru/jour/about/submissions#copyrightNotice</license-p></license></permissions><self-uri xlink:href="https://www.izmt.ru/jour/article/view/1368">https://www.izmt.ru/jour/article/view/1368</self-uri><abstract><p>Рассмотрен метод использования первичного эталонного источника синхротронного излучения для высокоточной калибровки чувствительности телескопов с ПЗС-матрицей и высоким угловым разрешением. Метод основан на высокоточном воспроизведении спектральных энергетических характеристик, гауссовом распределении спектральной плотности энергетической яркости по излучающей области, стабильности и воспроизводимости характеристик синхротронного излучения в одноэлектронном режиме.</p></abstract><trans-abstract xml:lang="en"><p>A method of the use of the synchrotron radiation primary standard source for high accuracy calibration of telescopes with high of telescopes with high angular resolution is described. The method is based on a highly accurate reproduction of spectral energetic characteristics, Gaussian distribution of the spectral density of energetic irradiance by the emitting area, stability and reproducibility of the characteristics of synchrotron radiation in one-electron mode.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>эталонный источник</kwd><kwd>синхротронное излучение</kwd><kwd>электронное накопительное кольцо</kwd><kwd>спектральная плотность энергетической освещенности</kwd><kwd>ПЗС-матрица</kwd><kwd>телескоп</kwd><kwd>standard source</kwd><kwd>synchrotron radiation</kwd><kwd>electron storage ring</kwd><kwd>spectral density of energetic irradiance</kwd><kwd>CCD-matrix</kwd><kwd>telescope</kwd></kwd-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Ulm G. Radiometry with synchrotron radiation // Metrologia. 2003. N. 40. P. S101-106.</mixed-citation><mixed-citation xml:lang="en">Ulm G. Radiometry with synchrotron radiation // Metrologia. 2003. N. 40. P. S101-106.</mixed-citation></citation-alternatives></ref><ref id="cit2"><label>2</label><citation-alternatives><mixed-citation xml:lang="ru">Thornagel R., Klein R., Ulm G. The electron storage ring BESSY II as a primary source standard from the visible to the X-ray range // Metrologia. 2001. N. 38. P. 385-391.</mixed-citation><mixed-citation xml:lang="en">Thornagel R., Klein R., Ulm G. The electron storage ring BESSY II as a primary source standard from the visible to the X-ray range // Metrologia. 2001. N. 38. P. 385-391.</mixed-citation></citation-alternatives></ref><ref id="cit3"><label>3</label><citation-alternatives><mixed-citation xml:lang="ru">Klein R., Brandt G., Fliegauf R., Hoehl A., MЈuller R., Thornagel R., Ulm G. The Metrology Light Source operated as a primary source standard // Metrologia. 2009. N. 46. P. S266-271.</mixed-citation><mixed-citation xml:lang="en">Klein R., Brandt G., Fliegauf R., Hoehl A., MЈuller R., Thornagel R., Ulm G. The Metrology Light Source operated as a primary source standard // Metrologia. 2009. N. 46. P. S266-271.</mixed-citation></citation-alternatives></ref></ref-list><fn-group><fn fn-type="conflict"><p>The authors declare that there are no conflicts of interest present.</p></fn></fn-group></back></article>
