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<article 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" xmlns:ali="http://www.niso.org/schemas/ali/1.0/" article-type="research-article" dtd-version="1.2" xml:lang="en"><front><journal-meta><journal-id journal-id-type="publisher-id">Astronomy Reports</journal-id><journal-title-group><journal-title xml:lang="en">Astronomy Reports</journal-title><trans-title-group xml:lang="ru"><trans-title>Астрономический журнал</trans-title></trans-title-group></journal-title-group><issn publication-format="print">0004-6299</issn><issn publication-format="electronic">3034-5170</issn><publisher><publisher-name xml:lang="en">The Russian Academy of Sciences</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">690673</article-id><article-id pub-id-type="doi">10.31857/S0004629925060048</article-id><article-id pub-id-type="edn">qawhmy</article-id><article-categories><subj-group subj-group-type="toc-heading" xml:lang="en"><subject>Articles</subject></subj-group><subj-group subj-group-type="toc-heading" xml:lang="ru"><subject>СТАТЬИ</subject></subj-group><subj-group subj-group-type="article-type"><subject>Research Article</subject></subj-group></article-categories><title-group><article-title xml:lang="en">Detection of radio emission from magnetar RX J1605.3+3249 at frequency 111 MHz</article-title><trans-title-group xml:lang="ru"><trans-title>Обнаружение радиоизлучения от магнитара RX J1605.3+3249 на частоте 111 МГц</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Rodin</surname><given-names>A. E.</given-names></name><name xml:lang="ru"><surname>Родин</surname><given-names>А. Е.</given-names></name></name-alternatives><email>a.rodin@lebedev.ru</email><xref ref-type="aff" rid="aff1"/></contrib><contrib contrib-type="author"><name-alternatives><name xml:lang="en"><surname>Fedorova</surname><given-names>V. A.</given-names></name><name xml:lang="ru"><surname>Федорова</surname><given-names>В. А.</given-names></name></name-alternatives><email>v.fedorova@lebedev.ru</email><xref ref-type="aff" rid="aff1"/></contrib></contrib-group><aff-alternatives id="aff1"><aff><institution xml:lang="en">P. N. Lebedev Physical Institute of the Russian Academy of Sciences</institution></aff><aff><institution xml:lang="ru">Физический институт им. П. Н. Лебедева Российской академии наук</institution></aff></aff-alternatives><pub-date date-type="pub" iso-8601-date="2025-06-15" publication-format="electronic"><day>15</day><month>06</month><year>2025</year></pub-date><volume>102</volume><issue>6</issue><issue-title xml:lang="en">VOL 102, NO6 (2025)</issue-title><issue-title xml:lang="ru">ТОМ 102, №6 (2025)</issue-title><fpage>490</fpage><lpage>495</lpage><history><date date-type="received" iso-8601-date="2025-09-21"><day>21</day><month>09</month><year>2025</year></date></history><permissions><copyright-statement xml:lang="en">Copyright ©; 2025, Russian Academy of Sciences</copyright-statement><copyright-statement xml:lang="ru">Copyright ©; 2025, Российская академия наук</copyright-statement><copyright-year>2025</copyright-year><copyright-holder xml:lang="en">Russian Academy of Sciences</copyright-holder><copyright-holder xml:lang="ru">Российская академия наук</copyright-holder></permissions><self-uri xlink:href="https://journals.eco-vector.com/0004-6299/article/view/690673">https://journals.eco-vector.com/0004-6299/article/view/690673</self-uri><abstract xml:lang="en"><p>For the first time, pulsed radio emission from the magnetar RX J1605.3+3249, which is part of the “magnificent seven”, has been detected. Data obtained at the BSA LPI radio telescope at a frequency of 111 MHz in the period from 2012 to 2024 were processed. The peak flux density mJy and the dispersion measure pc/cm3 were measured.</p></abstract><trans-abstract xml:lang="ru"><p>Впервые зарегистрировано импульсное радиоизлучение от магнитара RX J1605.3+3249, входящего в “Великолепную семерку”. Были обработаны данные, полученные на радиотелескопе БСА ФИАН на частоте 111 МГц в период с 2012 по 2024 гг. Измерена пиковая плотность потока мЯн и мера дисперсии пк/см3.</p></trans-abstract><kwd-group xml:lang="en"><kwd>RBS 156</kwd><kwd>X-ray pulsars</kwd><kwd>magnetars</kwd><kwd>interstellar medium</kwd><kwd>source RX J1605.3+3249</kwd><kwd>RBS 1556</kwd></kwd-group><kwd-group xml:lang="ru"><kwd>рентгеновские пульсары</kwd><kwd>магнитары</kwd><kwd>межзвездная среда</kwd><kwd>источник RX J1605.3+3249</kwd></kwd-group></article-meta></front><body></body><back><ref-list><ref id="B1"><label>1.</label><mixed-citation>F.M. Walter, S.J. 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