{"id":2452,"date":"2023-05-26T12:57:25","date_gmt":"2023-05-26T11:57:25","guid":{"rendered":"https:\/\/ahead.iaps.inaf.it\/?page_id=2452"},"modified":"2023-05-26T13:00:41","modified_gmt":"2023-05-26T12:00:41","slug":"tools-for-high-energy-spectroscopy","status":"publish","type":"page","link":"https:\/\/ahead.iaps.inaf.it\/?page_id=2452","title":{"rendered":"Tools for High energy spectroscopy"},"content":{"rendered":"<p style=\"font-weight: 400;\">Two-dimensional maps that allowed us (Lovisari, Ettori et al. 2023, A&amp;A, submitted) to study the perturbations in the temperature (and density) distribution, evaluating and characterizing the level of inhomogeneities of the ICM in a subsample of the CHEX-MATE (website: <a href=\"http:\/\/xmm-heritage.oas.inaf.it\/\">http:\/\/xmm-heritage.oas.inaf.it\/<\/a>; reference: CHEX-MATE collaboration 2021 \/ <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021A&amp;A...650A.104C\/abstract\">https:\/\/ui.adsabs.harvard.edu\/abs\/2021A%26A&#8230;650A.104C\/abstract<\/a>) galaxy clusters.<br \/>\n(From left to right) bkg-subctracted and exposure-corrected XMM-Newton images in the 0.3-7 keV band; binned X-ray surface brightness maps; projected electron density maps; projected temperature maps obtained through the Weighted Voronoi Tesselation (WVT) method by requiring a signal-to-noise ratio S\/N~30 ; relative temperature error maps. The size of the boxes corresponds to R500 (~0.6 times the virial radius); the white circles in the Voronoi maps corresponds to 0.15 R500, 0.5 R500, and R500.<br \/>\n<a href=\"http:\/\/ahead.iaps.inaf.it\/wp-content\/uploads\/2023\/05\/HES.png\"><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter size-full wp-image-2456\" src=\"http:\/\/ahead.iaps.inaf.it\/wp-content\/uploads\/2023\/05\/HES.png\" alt=\"\" width=\"612\" height=\"792\" srcset=\"https:\/\/ahead.iaps.inaf.it\/wp-content\/uploads\/2023\/05\/HES.png 612w, https:\/\/ahead.iaps.inaf.it\/wp-content\/uploads\/2023\/05\/HES-232x300.png 232w\" sizes=\"auto, (max-width: 612px) 100vw, 612px\" \/><\/a><\/p>\n<div class=\"pdfprnt-buttons pdfprnt-buttons-page pdfprnt-bottom-right\"><a href=\"https:\/\/ahead.iaps.inaf.it\/index.php?rest_route=%2Fwp%2Fv2%2Fpages%2F2452&print=print\" class=\"pdfprnt-button pdfprnt-button-print\" target=\"_blank\" ><img decoding=\"async\" src=\"https:\/\/ahead.iaps.inaf.it\/wp-content\/plugins\/pdf-print\/images\/print.png\" alt=\"image_print\" title=\"Print Content\" \/><\/a><\/div>","protected":false},"excerpt":{"rendered":"<p>Two-dimensional maps that allowed us (Lovisari, Ettori et al. 2023, A&amp;A, submitted) to study the perturbations in the temperature (and density) distribution, evaluating and characterizing the level of inhomogeneities of the ICM in a subsample of the CHEX-MATE (website: http:\/\/xmm-heritage.oas.inaf.it\/; reference: CHEX-MATE collaboration 2021 \/ https:\/\/ui.adsabs.harvard.edu\/abs\/2021A%26A&#8230;650A.104C\/abstract) galaxy clusters. (From left to right) bkg-subctracted and exposure-corrected &#8230; <a title=\"Tools for High energy spectroscopy\" class=\"read-more\" href=\"https:\/\/ahead.iaps.inaf.it\/?page_id=2452\" aria-label=\"Read more about Tools for High energy spectroscopy\">Read more<\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-2452","page","type-page","status-publish"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.0 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Tools for High energy spectroscopy &#183; AHEAD<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/ahead.iaps.inaf.it\/?page_id=2452\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Tools for High energy spectroscopy &#183; AHEAD\" \/>\n<meta property=\"og:description\" content=\"Two-dimensional maps that allowed us (Lovisari, Ettori et al. 2023, A&amp;A, submitted) to study the perturbations in the temperature (and density) distribution, evaluating and characterizing the level of inhomogeneities of the ICM in a subsample of the CHEX-MATE (website: http:\/\/xmm-heritage.oas.inaf.it\/; reference: CHEX-MATE collaboration 2021 \/ https:\/\/ui.adsabs.harvard.edu\/abs\/2021A%26A&#8230;650A.104C\/abstract) galaxy clusters. (From left to right) bkg-subctracted and exposure-corrected ... 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(From left to right) bkg-subctracted and exposure-corrected ... 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