{"id":1297,"date":"2021-08-31T08:08:26","date_gmt":"2021-08-31T08:08:26","guid":{"rendered":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/?p=1297"},"modified":"2021-09-06T08:22:19","modified_gmt":"2021-09-06T08:22:19","slug":"new-versions-of-the-xmm-newton-serendipitous-source-catalogues-4xmm-dr11-and-4xmm-dr11s","status":"publish","type":"post","link":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/2021\/08\/31\/new-versions-of-the-xmm-newton-serendipitous-source-catalogues-4xmm-dr11-and-4xmm-dr11s\/","title":{"rendered":"New versions of the XMM-Newton Serendipitous Source Catalogues: 4XMM-DR11 and 4XMM-DR11s"},"content":{"rendered":"\n<p class=\"has-black-color has-text-color\">A new version of the XMM-Newton EPIC Serendipitous Source Catalogue, 4XMM-DR11, has been released on 18th August by the XMM-Newton Survey Science Centre (XMM-SSC) in collaboration with the SOC. This version includes an extra year of data with respect to 4XMM-DR10. 4XMM-DR11 includes 895,415 X-ray detections which relate to 602,543 unique X-ray sources from 12,210 observations that were public by the 31st December 2020. 4XMM-DR11 covers a total sky area, with at least 1 ks exposure, of 1,239 square degrees if overlaps are taken into account, where some regions of the sky have been pointed as many as 80 times. Around 13% of all the detections are classified as extended, and spectra and time series have been extracted for 36% of the detections. The median positional uncertainty of the catalogue detections is 1.57 arcseconds (with a standard deviation of 1.43). Median fluxes in the catalogue are ~5.2E-15 and ~1.2E-14 erg\/cm2\/s in the soft (0.2-2 keV) and hard (2-12 keV) X-ray band, respectively.<\/p>\n\n\n\n<p class=\"has-black-color has-text-color\">With 4XMM-DR11, we release 4XMM-DR11s, the catalogue version created from overlapping observations. Stacking observations provides longer effective exposure times, resulting in better source parameters and higher sensitivity. 4XMM-DR11s is built from 1,475 groups with 8,292 observations. Most of the stacks are composed of 2 observations and the largest has 357. The catalogue contains 35,8809 sources, of which 275,440 have several contributing observations. It reaches a median flux of ~3.3E-15 and ~1.1E-14 erg\/cm2\/s in the soft (0.2-2 keV) and hard (2-12 keV) X-ray band, respectively. 8587 good quality sources are variable on the long term.<\/p>\n\n\n\n<p class=\"has-black-color has-text-color\">The detection catalogue is described in the paper <a rel=\"noreferrer noopener\" href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...641A.136W\/abstract\" target=\"_blank\">Webb et al. (2020)<\/a> and the stacked catalogue is further described in <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...641A.137T\/abstract\" target=\"_blank\" rel=\"noreferrer noopener\">Traulsen et al. (2020)<\/a>.<br>Details of the catalogue, the catalogue files and full 4XMM documentation are available on the XMM-SSC webpages at:<\/p>\n\n\n\n<p><a rel=\"noreferrer noopener\" href=\"http:\/\/xmmssc.irap.omp.eu\/Catalogue\/4XMM-DR11\/4XMM_DR11.html\" target=\"_blank\">http:\/\/xmmssc.irap.omp.eu\/Catalogue\/4XMM-DR11\/4XMM_DR11.html<\/a>\u00a0<br><span class=\"has-inline-color has-black-color\">and<\/span><br><a href=\"https:\/\/xmmssc.aip.de\/cms\/catalogues\/4xmm-dr11s\/\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/xmmssc.aip.de\/cms\/catalogues\/catalogue-4xmm-dr11s\/<\/a>\u00a0<\/p>\n\n\n\n<p class=\"has-black-color has-text-color\">FITS files containing summary information about the observations used in the catalogue are also provided. FITS and CSV versions of the full 4XMM catalogue and a slimline version of the FITS file are also available for download at:<\/p>\n\n\n\n<p><a href=\"http:\/\/www.cosmos.esa.int\/web\/xmm-newton\/xsa\" target=\"_blank\" rel=\"noreferrer noopener\">http:\/\/www.cosmos.esa.int\/web\/xmm-newton\/xsa<\/a>&nbsp;<\/p>\n\n\n\n<p class=\"has-black-color has-text-color\">The slimline version of 4XMM-DR11 has only one row per unique source (rather than per detection as in the main catalogue) and a reduced number of columns that essentially pertain to the unique source quantities.<\/p>\n\n\n\n<p class=\"has-black-color has-text-color\">Alongside the XSA user interface, 4XMM is also distributed through:<\/p>\n\n\n\n<p><span class=\"has-inline-color has-black-color\">XCATDB<\/span>: <a rel=\"noreferrer noopener\" href=\"http:\/\/xcatdb.unistra.fr\/4xmmdr11\" target=\"_blank\">http:\/\/xcatdb.unistra.fr\/4xmmdr11<\/a>\u00a0<br><span class=\"has-inline-color has-black-color\">HEASARC<\/span>: <a href=\"https:\/\/heasarc.gsfc.nasa.gov\/w3browse\/all\/xmmssc.html\" target=\"_blank\" rel=\"noreferrer noopener\">https:\/\/heasarc.gsfc.nasa.gov\/w3browse\/all\/xmmssc.html\u00a0<\/a><br><span class=\"has-inline-color has-black-color\">IRAP<\/span>: <a rel=\"noreferrer noopener\" href=\"http:\/\/xmm-catalog.irap.omp.eu\/\" target=\"_blank\">http:\/\/xmm-catalog.irap.omp.eu\/<\/a>\u00a0<\/p>\n","protected":false},"excerpt":{"rendered":"<p>A new version of the XMM-Newton EPIC Serendipitous Source Catalogue, 4XMM-DR11, has been released on 18th August by the XMM-Newton Survey Science Centre (XMM-SSC) in collaboration with the SOC. This version includes an extra year of data with respect to 4XMM-DR10. 4XMM-DR11 includes 895,415 X-ray detections which relate to 602,543 unique X-ray sources from 12,210&hellip; <br \/> <a class=\"read-more\" href=\"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/2021\/08\/31\/new-versions-of-the-xmm-newton-serendipitous-source-catalogues-4xmm-dr11-and-4xmm-dr11s\/\">Lire la suite<\/a><\/p>\n","protected":false},"author":2,"featured_media":1309,"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\/1297"}],"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\/2"}],"replies":[{"embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/comments?post=1297"}],"version-history":[{"count":7,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/posts\/1297\/revisions"}],"predecessor-version":[{"id":1318,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/posts\/1297\/revisions\/1318"}],"wp:featuredmedia":[{"embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/media\/1309"}],"wp:attachment":[{"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/media?parent=1297"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/categories?post=1297"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/xmm-ssc.irap.omp.eu\/xmm2athena\/wp-json\/wp\/v2\/tags?post=1297"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}