{"id":1388,"date":"2021-10-25T10:02:17","date_gmt":"2021-10-25T10:02:17","guid":{"rendered":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/?page_id=1388"},"modified":"2024-05-29T11:29:40","modified_gmt":"2024-05-29T11:29:40","slug":"publicaciones","status":"publish","type":"page","link":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/es\/publicaciones\/","title":{"rendered":"Publicaciones"},"content":{"rendered":"\n
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STONKS: Quasi-real time XMM-Newton transient detection system<\/a>, Quintin, E., et al.<\/p>\n\n\n\n

DOI: 10.48550\/arXiv.2405.13630<\/a><\/p>\n<\/div><\/div>\n\n\n\n

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The link among X-ray spectral properties, AGN structure and the host galaxy, Mountrichas<\/a>, G., et al.<\/p>\n\n\n\n

DOI: 10.48550\/arXiv.2401.00045<\/a><\/p>\n<\/div><\/div>\n\n\n\n

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The relationship between the incidence of X-ray selected AGN in nearby galaxies and star-formation rate<\/a>, Birchall, K., et al.<\/p>\n\n\n\n

DOI: 10.48550\/arXiv.2306.10868<\/a><\/p>\n<\/div><\/div>\n\n\n\n

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Tormund’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

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DOI: 10.48550\/arXiv.2306.00438<\/a><\/p>\n<\/div><\/div>\n\n\n\n

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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

DOI: 10.48550\/arXiv.2304.11216<\/a><\/p>\n<\/div><\/div>\n\n\n\n

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Tidal disruption events and quasi periodic eruptions<\/a>, Webb N., et al.<\/p>\n\n\n\n

DOI: 10.48550\/arXiv.2304.08828<\/a><\/p>\n<\/div><\/div>\n\n\n\n

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XMM2ATHENA, the H2020 project to improve XMM-Newtonanalysis software and prepare for Athena<\/a>, Webb N. et al.<\/p>\n\n\n\n

DOI: 10.48550\/arXiv.2303.10097<\/a><\/p>\n<\/div><\/div>\n\n\n\n

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Probabilistic classification of X-ray sources applied to Swift<\/em>-XRT and XMM-Newton<\/em> catalogs<\/a>, Tranin H., et al.
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DOI: 10.1051\/0004-6361\/202141259<\/a><\/p>\n<\/div><\/div>\n","protected":false},"excerpt":{"rendered":"

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 and star-formation rate, Birchall, K., et al. DOI: 10.48550\/arXiv.2306.10868 Tormund’s return: Hints…
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\/1388"}],"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=1388"}],"version-history":[{"count":17,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/pages\/1388\/revisions"}],"predecessor-version":[{"id":5673,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/pages\/1388\/revisions\/5673"}],"wp:attachment":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/media?parent=1388"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}