{"id":4247,"date":"2023-03-24T13:45:44","date_gmt":"2023-03-24T13:45:44","guid":{"rendered":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/?p=4247"},"modified":"2023-10-26T10:46:19","modified_gmt":"2023-10-26T10:46:19","slug":"xmm2athena-the-h2020-project-to-improve-xmm-newtonanalysis-software-and-prepare-for-athena","status":"publish","type":"post","link":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/2023\/03\/24\/xmm2athena-the-h2020-project-to-improve-xmm-newtonanalysis-software-and-prepare-for-athena\/","title":{"rendered":"XMM2ATHENA, the H2020 project to improve XMM-Newtonanalysis software and prepare for Athena"},"content":{"rendered":"\n[24 March 2023]\n\n\n\n<p class=\"has-black-color has-text-color\">XMM-<em>Newton<\/em>, a European Space Agency observatory, has been observing the X-<br>ray, ultra-violet and optical sky for 23 years. During this time, astronomy has<br>evolved from mainly studying single sources to populations and from a single wave-<br>length, to multi-wavelength\/messenger data. We are also moving into an era of time<br>domain astronomy. New software and methods are required to accompany evolving<br>astronomy and prepare for the next generation X-ray observatory, Athena.<br>Here we present XMM2ATHENA, a programme funded by the European Union\u2019s<br>Horizon 2020 research and innovation programme. XMM2ATHENA builds on foun-<br>dations laid by the XMM-<em>Newton<\/em> Survey Science Centre (XMM-SSC), including key<br>members of this consortium and the Athena Science ground segment, along with<br>members of the X-ray community. The project is developing and testing new methods<br>and software to allow the community to follow the X-ray transient sky in quasi-real<br>time, identify multi-wavelength\/ messenger counterparts of XMM-<em>Newton<\/em> sources<br>and determine their nature using machine learning. We detail here the first milestone<br>delivery of the project, a new online, sensitivity estimator. We also outline other<br>products, including the forthcoming innovative stacking procedure and detection<br>algorithms to detect the faintest sources. These tools will then be adapted for Athena<br>and the newly detected\/ identified sources will enhance preparation for observing the<br>Athena X-ray sky.<\/p>\n\n\n\n<p class=\"has-black-color has-text-color\">Download full paper: <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023arXiv230310097W\/abstract\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/ui.adsabs.h<\/a><a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023arXiv2303100\" target=\"_blank\">arvard.edu\/abs\/2023arXiv2303100<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>[24 March 2023] XMM-Newton, a European Space Agency observatory, has been observing the X-ray, ultra-violet and optical sky for 23 years. During this time, astronomy hasevolved from mainly studying single sources to populations and from a single wave-length, to multi-wavelength\/messenger data. We are also moving into an era of timedomain astronomy. New software and methods&hellip; <br \/> <a class=\"read-more\" href=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/2023\/03\/24\/xmm2athena-the-h2020-project-to-improve-xmm-newtonanalysis-software-and-prepare-for-athena\/\">Lire la suite<\/a><\/p>\n","protected":false},"author":5,"featured_media":4248,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_eb_attr":"","_mi_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0},"categories":[1],"tags":[],"_links":{"self":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/posts\/4247"}],"collection":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/comments?post=4247"}],"version-history":[{"count":6,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/posts\/4247\/revisions"}],"predecessor-version":[{"id":5025,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/posts\/4247\/revisions\/5025"}],"wp:featuredmedia":[{"embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/media\/4248"}],"wp:attachment":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/media?parent=4247"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/categories?post=4247"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/tags?post=4247"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}