{"id":258,"date":"2021-05-04T06:53:05","date_gmt":"2021-05-04T06:53:05","guid":{"rendered":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/?page_id=258"},"modified":"2024-11-28T11:22:03","modified_gmt":"2024-11-28T11:22:03","slug":"publications","status":"publish","type":"page","link":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:26% auto\"><figure class=\"wp-block-media-text__media\"><a href=\"https:\/\/arxiv.org\/abs\/2405.13630\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" width=\"1024\" height=\"884\" src=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/05\/quintin_Stonks-1024x884.png\" alt=\"\" class=\"wp-image-5658 size-full\" srcset=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/05\/quintin_Stonks-1024x884.png 1024w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/05\/quintin_Stonks-300x259.png 300w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/05\/quintin_Stonks-768x663.png 768w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/05\/quintin_Stonks-1536x1326.png 1536w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/05\/quintin_Stonks-2048x1768.png 2048w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/05\/quintin_Stonks-1251x1080.png 1251w\" sizes=\"(max-width: 1024px) 100vw, 1024px\" \/><\/a><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\"><\/p>\n\n\n\n<p><a href=\"https:\/\/arxiv.org\/abs\/2405.13630\" target=\"_blank\" rel=\"noreferrer noopener\">STONKS: Quasi-real time XMM-Newton transient detection system<\/a>, Quintin, E., et al.<\/p>\n\n\n\n<p>DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2024arXiv240513630Q\/doi:10.48550\/arXiv.2405.13630\" target=\"_blank\">10.48550\/arXiv.2405.13630<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-text-color has-background has-white-background-color has-white-color\"\/>\n\n\n\n<hr class=\"wp-block-separator\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:27% auto\"><figure class=\"wp-block-media-text__media\"><a href=\"https:\/\/arxiv.org\/abs\/2401.00045\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" width=\"1024\" height=\"884\" src=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/George-1024x884.png\" alt=\"\" class=\"wp-image-5465 size-full\" srcset=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/George-1024x884.png 1024w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/George-300x259.png 300w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/George-768x663.png 768w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/George-1536x1326.png 1536w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/George-2048x1768.png 2048w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/George-1251x1080.png 1251w\" sizes=\"(max-width: 1024px) 100vw, 1024px\" \/><\/a><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\"><\/p>\n\n\n\n<p><a rel=\"noreferrer noopener\" href=\"https:\/\/arxiv.org\/abs\/2401.00045\" target=\"_blank\">The link among X-ray spectral properties, AGN structure and the host galaxy<\/a>, Mountrichas, G., et al.<\/p>\n\n\n\n<p>DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2024arXiv240100045M\/doi:10.48550\/arXiv.2401.00045\" target=\"_blank\">10.48550\/arXiv.2401.00045<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-text-color has-background has-white-background-color has-white-color\"\/>\n\n\n\n<hr class=\"wp-block-separator is-style-wide\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:28% auto\"><figure class=\"wp-block-media-text__media\"><a href=\"https:\/\/arxiv.org\/abs\/2306.10868\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" width=\"1024\" height=\"884\" src=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/Keir-1024x884.png\" alt=\"\" class=\"wp-image-5464 size-full\" srcset=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/Keir-1024x884.png 1024w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/Keir-300x259.png 300w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/Keir-768x663.png 768w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/Keir-1536x1326.png 1536w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/Keir-2048x1768.png 2048w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2024\/02\/Keir-1251x1080.png 1251w\" sizes=\"(max-width: 1024px) 100vw, 1024px\" \/><\/a><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\"><\/p>\n\n\n\n<p><a href=\"https:\/\/arxiv.org\/abs\/2306.10868\" target=\"_blank\" rel=\"noreferrer noopener\">The relationship between the incidence of X-ray selected AGN in nearby galaxies &amp; star-formation rate<\/a>, Birchall, K., et al.<\/p>\n\n\n\n<p>DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2023MNRAS.523.4756B\/doi:10.48550\/arXiv.2306.10868\" target=\"_blank\">10.48550\/arXiv.2306.10868<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-text-color has-background has-white-background-color has-white-color\"\/>\n\n\n\n<hr class=\"wp-block-separator is-style-wide\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:29% auto\"><figure class=\"wp-block-media-text__media\"><a href=\"https:\/\/arxiv.org\/abs\/2306.00438\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" width=\"1024\" height=\"884\" src=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/06\/quintin-1024x884.png\" alt=\"\" class=\"wp-image-4659 size-full\" srcset=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/06\/quintin-1024x884.png 1024w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/06\/quintin-300x259.png 300w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/06\/quintin-768x663.png 768w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/06\/quintin-1536x1326.png 1536w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/06\/quintin-2048x1768.png 2048w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/06\/quintin-1251x1080.png 1251w\" sizes=\"(max-width: 1024px) 100vw, 1024px\" \/><\/a><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\"><\/p>\n\n\n\n<p><a rel=\"noreferrer noopener\" href=\"https:\/\/arxiv.org\/abs\/2306.00438\" target=\"_blank\">Tormund&rsquo;s return: Hints of quasi-periodic eruption features from a recent optical tidal disruption event<\/a>, Quintin, E., et al.<\/p>\n\n\n\n<p><\/p>\n\n\n\n<p>DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2023arXiv230600438Q\/doi:10.48550\/arXiv.2306.00438\" target=\"_blank\">10.48550\/arXiv.2306.00438<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-text-color has-background has-white-background-color has-white-color\"\/>\n\n\n\n<hr class=\"wp-block-separator is-style-wide\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:30% auto\"><figure class=\"wp-block-media-text__media\"><a href=\"https:\/\/arxiv.org\/abs\/2304.11216\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" width=\"1024\" height=\"884\" src=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/05\/hugo-1024x884.png\" alt=\"\" class=\"wp-image-4444 size-full\" srcset=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/05\/hugo-1024x884.png 1024w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/05\/hugo-300x259.png 300w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/05\/hugo-768x663.png 768w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/05\/hugo-1536x1326.png 1536w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/05\/hugo-2048x1768.png 2048w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/05\/hugo-1251x1080.png 1251w\" sizes=\"(max-width: 1024px) 100vw, 1024px\" \/><\/a><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\"><\/p>\n\n\n\n<p><a rel=\"noreferrer noopener\" href=\"https:\/\/arxiv.org\/abs\/2304.11216\" target=\"_blank\">Statistical study of a large and cleaned sample of ultraluminous and hyperluminous X-ray sources<\/a>, Tranin, H., et al.<\/p>\n\n\n\n<p><\/p>\n\n\n\n<p>DOI: <a href=\"https:\/\/doi.org\/10.48550\/arXiv.2304.11216\" target=\"_blank\" rel=\"noreferrer noopener\">10.48550\/arXiv.2304.11216<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-text-color has-background has-white-background-color has-white-color\"\/>\n\n\n\n<hr class=\"wp-block-separator is-style-wide\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><a href=\"https:\/\/arxiv.org\/abs\/2304.08828\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" width=\"1024\" height=\"884\" src=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/04\/Natalie_Tidal-3-1024x884.png\" alt=\"\" class=\"wp-image-4397 size-full\" srcset=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/04\/Natalie_Tidal-3-1024x884.png 1024w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/04\/Natalie_Tidal-3-300x259.png 300w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/04\/Natalie_Tidal-3-768x663.png 768w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/04\/Natalie_Tidal-3-1536x1326.png 1536w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/04\/Natalie_Tidal-3-2048x1768.png 2048w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/04\/Natalie_Tidal-3-1251x1080.png 1251w\" sizes=\"(max-width: 1024px) 100vw, 1024px\" \/><\/a><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\"><\/p>\n\n\n\n<p><a rel=\"noreferrer noopener\" href=\"https:\/\/arxiv.org\/abs\/2304.08828\" target=\"_blank\">Tidal disruption events and quasi periodic eruptions<\/a>, Webb N., et al.<\/p>\n\n\n\n<p>DOI: <a href=\"https:\/\/doi.org\/10.48550\/arXiv.2304.08828\" target=\"_blank\" rel=\"noreferrer noopener\">10.48550\/arXiv.2304.08828<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-text-color has-background has-white-background-color has-white-color\"\/>\n\n\n\n<hr class=\"wp-block-separator is-style-wide\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:31% auto\"><figure class=\"wp-block-media-text__media\"><a href=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/03\/Natalie.png\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" width=\"1024\" height=\"884\" src=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/03\/Natalie-1024x884.png\" alt=\"\" class=\"wp-image-4248 size-full\" srcset=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/03\/Natalie-1024x884.png 1024w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/03\/Natalie-300x259.png 300w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/03\/Natalie-768x663.png 768w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/03\/Natalie-1536x1326.png 1536w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/03\/Natalie-2048x1768.png 2048w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/03\/Natalie-1251x1080.png 1251w\" sizes=\"(max-width: 1024px) 100vw, 1024px\" \/><\/a><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-large-font-size\"><\/p>\n\n\n\n<p><a rel=\"noreferrer noopener\" href=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2023\/03\/Natalie.png\" target=\"_blank\">XMM2ATHENA, the H2020 project to improve XMM-Newtonanalysis software and prepare for Athena<\/a>, Webb N., et al.<\/p>\n\n\n\n<p><\/p>\n\n\n\n<p>DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2023arXiv230310097W\/doi:10.48550\/arXiv.2303.10097\" target=\"_blank\">10.48550\/arXiv.2303.10097<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator has-text-color has-background has-white-background-color has-white-color\"\/>\n\n\n\n<hr class=\"wp-block-separator is-style-wide\"\/>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:34% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" width=\"1024\" height=\"884\" src=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2022\/01\/newspaper-hugo-tranin-1024x884.png\" alt=\"\" class=\"wp-image-2199 size-full\" srcset=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2022\/01\/newspaper-hugo-tranin-1024x884.png 1024w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2022\/01\/newspaper-hugo-tranin-300x259.png 300w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2022\/01\/newspaper-hugo-tranin-768x663.png 768w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2022\/01\/newspaper-hugo-tranin-1536x1326.png 1536w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2022\/01\/newspaper-hugo-tranin-2048x1768.png 2048w, http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-content\/uploads\/2022\/01\/newspaper-hugo-tranin-1251x1080.png 1251w\" sizes=\"(max-width: 1024px) 100vw, 1024px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-text-align-left has-large-font-size\"><\/p>\n\n\n\n<p><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021arXiv211101489T\/abstract\" target=\"_blank\">Probabilistic classification of X-ray sources applied to <em>Swift<\/em>-XRT and XMM-<em>Newton<\/em> catalogs<\/a><\/mark>, by Tranin H., et al.<br><\/p>\n\n\n\n<p>DOI: <a href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2022A&amp;A...657A.138T\/doi:10.1051\/0004-6361\/202141259\" target=\"_blank\" rel=\"noreferrer noopener\">10.1051\/0004-6361\/202141259<\/a><\/p>\n<\/div><\/div>\n\n\n\n<hr class=\"wp-block-separator is-style-wide\"\/>\n\n\n\n<ul class=\"has-black-color has-text-color\"><li>XMM-Newton and SRG\/eROSITA observations of the isolated neutron star candidate 4XMM J022141.5\u2212735632, A. Pires, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2022A&amp;A...666A.148P\/doi:10.1051\/0004-6361\/202244514\" target=\"_blank\">10.1051\/0004-6361\/202244514<\/a><\/li><li>The co-evolution of supermassive black holes and galaxies in luminous AGN over a wide range of redshift, G. Mountrichas, DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2023A&amp;A...672A..98M\/doi:10.1051\/0004-6361\/202345924\" target=\"_blank\">10.1051\/0004-6361\/202345924<\/a><\/li><li>Link between star formation and the properties of supermassive black holes, G. Mountrichas, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2023A&amp;A...679A.151M\/doi:10.1051\/0004-6361\/202347392\" target=\"_blank\">10.1051\/0004-6361\/202347392<\/a><\/li><li>Universality of coronal properties in accreting black holes across mass and accretion rate, S. Chakraborty, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2023A&amp;A...676L..13C\/doi:10.1051\/0004-6361\/202347181\" target=\"_blank\">10.1051\/0004-6361\/202347181<\/a><\/li><li>Discovery of two promising isolated neutron star candidates in the SRG\/eROSITA All-Sky Survey, J. Kurpas, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2023A&amp;A...674A.155K\/doi:10.1051\/0004-6361\/202346375\" target=\"_blank\">10.1051\/0004-6361\/202346375<\/a><\/li><li>The relation of cosmic environment and morphology with the star formation and stellar populations of AGN and non-AGN galaxies, G. Mountrichas, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2023A&amp;A...675A.137M\/doi:10.1051\/0004-6361\/202346706\" target=\"_blank\">10.1051\/0004-6361\/202346706<\/a><\/li><li>Host galaxy properties of X-ray active galactic nuclei in the local Universe, L. Koutoulidis, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2022A&amp;A...658A..35K\/doi:10.1051\/0004-6361\/202142466\" target=\"_blank\">10.1051\/0004-6361\/202142466<\/a><\/li><li>XXL-HSC: Link between AGN activity and star formation in the early Universe (z \u2a7e 3.5), E. Pouliasis, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2022A&amp;A...667A..56P\/doi:10.1051\/0004-6361\/202243502\" target=\"_blank\">10.1051\/0004-6361\/202243502<\/a><\/li><li>The intrinsic X-ray luminosity distribution of an optically selected SDSS quasar population, A. Rankine, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2024MNRAS.527.9004R\/doi:10.1093\/mnras\/stad3686\" target=\"_blank\">10.1093\/mnras\/stad3686<\/a><\/li><li>The STATiX pipeline for the detection of X-ray transients in three dimensions, A. Ruiz, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2024MNRAS.527.3674R\/doi:10.1093\/mnras\/stad3339\" target=\"_blank\">10.1093\/mnras\/stad3339<\/a><\/li><li>Comparing the host galaxy ages of X-ray selected AGN in COSMOS. Obscured AGN are associated with older galaxies, I. Georgantopoulos, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2023A&amp;A...673A..67G\/doi:10.1051\/0004-6361\/202244875\" target=\"_blank\">10.1051\/0004-6361\/202244875<\/a><\/li><li>Phase-resolved X-ray spectroscopy of PSR B0656+14 with SRG\/eROSITA and XMM-Newton, A. Schwope, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2022A&amp;A...661A..41S\/doi:10.1051\/0004-6361\/202141105\" target=\"_blank\">10.1051\/0004-6361\/202141105<\/a><\/li><li>The properties of supermassive black holes and their host galaxies for type 1 and 2 active galactic nuclei in the eFEDS and COSMOS fields, G. Mountrichas, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2024A&amp;A...683A.160M\/doi:10.1051\/0004-6361\/202348156\" target=\"_blank\">10.1051\/0004-6361\/202348156<\/a><\/li><li>Comparative analysis of the SFR of AGN and non-AGN galaxies, as a function of stellar mass, AGN power, cosmic time, and obscuration, G. 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Kurpas, et al., DOI: <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2024A&amp;A...683A.164K\/doi:10.1051\/0004-6361\/202347967\" target=\"_blank\">10.1051\/0004-6361\/202347967<\/a><\/li><\/ul>\n","protected":false},"excerpt":{"rendered":"<p>STONKS: Quasi-real time XMM-Newton transient detection system, Quintin, E., et al. DOI: 10.48550\/arXiv.2405.13630 The link among X-ray spectral properties, AGN structure and the host galaxy, Mountrichas, G., et al. DOI: 10.48550\/arXiv.2401.00045 The relationship between the incidence of X-ray selected AGN in nearby galaxies &amp; star-formation rate, Birchall, K., et al. DOI: 10.48550\/arXiv.2306.10868 Tormund&rsquo;s return: Hints&hellip; <br \/> <a class=\"read-more\" href=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/publications\/\">Lire la suite<\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_eb_attr":"","_mi_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0},"_links":{"self":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/pages\/258"}],"collection":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/comments?post=258"}],"version-history":[{"count":23,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/pages\/258\/revisions"}],"predecessor-version":[{"id":5941,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/pages\/258\/revisions\/5941"}],"wp:attachment":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/media?parent=258"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}