{"id":60964,"date":"2025-04-29T19:09:06","date_gmt":"2025-04-29T19:09:06","guid":{"rendered":"https:\/\/www.europesays.com\/uk\/60964\/"},"modified":"2025-04-29T19:09:06","modified_gmt":"2025-04-29T19:09:06","slug":"astronomers-investigate-an-extremely-x-ray-luminous-radio-loud-quasar","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/uk\/60964\/","title":{"rendered":"Astronomers investigate an extremely X-ray-luminous, radio-loud quasar"},"content":{"rendered":"<p>            <img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.europesays.com\/uk\/wp-content\/uploads\/2025\/04\/russian-astronomers-in.jpg\" alt=\"Russian astronomers investigate an extremely X-ray luminous radio-loud quasar\" title=\"Smoothed X-ray image of SRGA J2306+1556. Credit: arXiv (2025). DOI: 10.48550\/arxiv.2504.13658\" width=\"800\" height=\"530\"\/><\/p>\n<p>                Smoothed X-ray image of SRGA J2306+1556. Credit: arXiv (2025). DOI: 10.48550\/arxiv.2504.13658<\/p>\n<p>Using the Spektr-RG (SRG) space observatory, astronomers from the Russian Academy of Sciences have inspected a radio-loud quasar known as SRGA J2306+1556, which is extremely luminous in the X-ray band. Results of the new study are <a href=\"https:\/\/arxiv.org\/abs\/2504.13658\" target=\"_blank\" rel=\"noopener\">reported<\/a> in a research paper published April 18 on the arXiv preprint server.<\/p>\n<p>Quasars, or quasi-stellar objects (QSOs), are <a href=\"https:\/\/phys.org\/tags\/active+galactic+nuclei\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">active galactic nuclei<\/a> (AGN) of very high luminosity powered by <a href=\"https:\/\/phys.org\/tags\/supermassive+black+holes\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">supermassive black holes<\/a> (SMBHs), emitting electromagnetic radiation observable in radio, infrared, visible, ultraviolet and X-ray wavelengths. They are among the brightest and most distant objects in the known universe, and serve as fundamental tools for numerous studies in astrophysics as well as cosmology.<\/p>\n<p>SRGA J2306+1556 is a radio-loud quasar at a redshift of approximately 0.44, discovered in 2022 with Spektr-RG. Previous observations of SRGA J2306+1556 have found that it is heavily obscured and its intrinsic X-ray luminosity exceeds 4.0 quattuordecillion erg\/s.<\/p>\n<p>Recently, a team of astronomers led by Grigory Uskov decided to re-investigate SRGA J2306+1556 with Spektr-RG in order to get more insights into its nature. Their study was complemented by data from NASA&#8217;s Swift spacecraft.<\/p>\n<p>&#8220;To study this interesting quasar in detail, we organized its follow-up pointed X-ray observations with SRG\/ART-XC and the XRT telescope aboard the Neil Gehrels Swift observatory, which revealed a strongly absorbed X-ray spectrum,&#8221; the researchers wrote in the paper.<\/p>\n<p>During the new observations, the unabsorbed X-ray luminosity of SRGA J2306+1556 ranged between 1.0 and 6.0 quattuordecillion erg\/s, and the source exhibited a strongly absorbed X-ray spectrum. The astronomers noted that such X-ray luminous obscured AGN are extremely rare at redshifts below 0.5.<\/p>\n<p>The collected data indicate that SRGA J2306+1556 experienced an X-ray outburst in 2020\u20132021 and was in a &#8220;low&#8221; state in June 2023. The researchers estimate that the outburst could have lasted about one year or more.<\/p>\n<p>Furthermore, it was found that SRGA J2306+1556 showcases a complex morphology in the radio band with a core and two extended radio lobes. The findings suggest that the radio counterpart of SRGA J2306+1556 is a giant radio galaxy (GRG) of the FR II type with a radio power at a level of 286 YW\/Hz, which is equivalent to 0.004 quattuordecillion erg\/s.<\/p>\n<p>The study also found that SRGA J2306+1556 has a bolometric luminosity of around 60 quattuordecillion erg\/s and that its central black hole has a mass of about 1.4 billion solar masses.<\/p>\n<p>Summing up the results, the authors of the paper underlined that SRGA J2306+1556 is one of the most luminous obscured quasars in the observable universe and accretes mass at a high rate.<\/p>\n<p><strong>More information:<\/strong><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tGrigory Uskov et al, SRGAJ230631.0+155633: an extremely X-ray luminous, heavily obscured, radio-loud quasar at z=0.44 discovered by SRG\/ART-XC, arXiv (2025). <a data-doi=\"1\" href=\"https:\/\/dx.doi.org\/10.48550\/arxiv.2504.13658\" target=\"_blank\" rel=\"noopener\">DOI: 10.48550\/arxiv.2504.13658<\/a><\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t\t\t<strong>Journal information:<\/strong><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<a href=\"https:\/\/phys.org\/journals\/arxiv\/\" target=\"_blank\" rel=\"noopener\">arXiv<\/a><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"icon_open\" href=\"http:\/\/arxiv.org\/\" target=\"_blank\" rel=\"nofollow noopener\"><\/p>\n<p>\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/p>\n<p class=\"article-main__note mt-4\">\n\t\t\t\t\t\t\t\t\t\t\t\t  \u00a9 2025 Science X Network\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t\t<strong>Citation<\/strong>:<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tAstronomers investigate an extremely X-ray-luminous, radio-loud quasar (2025, April 29)<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tretrieved 29 April 2025<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tfrom https:\/\/phys.org\/news\/2025-04-astronomers-extremely-ray-luminous-radio.html\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no<br \/>\n\t\t\t\t\t\t\t\t\t\t\t part may be reproduced without the written permission. The content is provided for information purposes only.\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n","protected":false},"excerpt":{"rendered":"Smoothed X-ray image of SRGA J2306+1556. Credit: arXiv (2025). DOI: 10.48550\/arxiv.2504.13658 Using the Spektr-RG (SRG) space observatory, astronomers&hellip;\n","protected":false},"author":2,"featured_media":60965,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[3845],"tags":[75,76,74,71,70,72,53,73,16,15],"class_list":{"0":"post-60964","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-physics","8":"tag-materials","9":"tag-nanotech","10":"tag-physics","11":"tag-physics-news","12":"tag-science","13":"tag-science-news","14":"tag-technology","15":"tag-technology-news","16":"tag-uk","17":"tag-united-kingdom"},"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@uk\/114422832852853688","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/60964","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/comments?post=60964"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/posts\/60964\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media\/60965"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/media?parent=60964"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/categories?post=60964"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/uk\/wp-json\/wp\/v2\/tags?post=60964"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}