{"id":4007,"date":"2024-05-24T09:53:03","date_gmt":"2024-05-24T07:53:03","guid":{"rendered":"http:\/\/brera.inaf.it\/?post_type=progetti_ricerca&#038;p=4007"},"modified":"2024-10-30T10:25:53","modified_gmt":"2024-10-30T09:25:53","slug":"beatrix","status":"publish","type":"progetti_ricerca","link":"https:\/\/brera.inaf.it\/en\/progetti_ricerca\/beatrix\/","title":{"rendered":"BEaTriX"},"content":{"rendered":"\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-995f960e wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:33.33%\">\n<figure class=\"wp-block-image size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"800\" height=\"800\" src=\"http:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-beatrix.png\" alt=\"\" class=\"wp-image-979\"\/><\/figure>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\" style=\"flex-basis:66.66%\">\n<h5 class=\"wp-block-heading\">BEaTriX<\/h5>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>B<\/strong>eam <strong>E<\/strong>xpander <strong>T<\/strong>esting <strong>X<\/strong>-ray Facility <\/p>\n\n\n\n<h5 class=\"wp-block-heading\">SHORT DESCRIPTION<\/h5>\n\n\n\n<p class=\"has-text-align-left wp-block-paragraph\">BEaTriX is a facility installed at the INAF-Brera Astronomical Observatory in its seat Merate (Lecco). It is the first realization of an instrument that generates a parallel and wide X-ray beam within a small lab. The main objective of BEaTriX is to demonstrate that it is possible to perform acceptance tests of the optical modules of the ATHENA telescope, at a rate able to keep up with their manufacturing in series.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">ATHENA is an ESA X-ray observatory, scheduled for launch in 2030. The telescope consists of several hundred optical modules (Mirror Modules, MM) in silicon (Silicon Pore Optics, SPO) to be assembled. The MMs, produced with the well-established silicon technology used in the semiconductor industry, will be produced at a rate of 2 MMs\/day, each one needing to be tested for acceptance before integration.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">MMs are currently being tested at the Berlin synchrotron BESSY II, where the X-ray beam produced by a synchrotron is parallel but very small; hence, it does not allow illuminating the entire modules to be tested. The modules are also measured at PANTER, of the Max-Planck-Institut f\u00fcr Extra-terrestrische Physik, located in Germany near Munich; however, the vacuum chamber is extremely large and requires days to reach the vacuum necessary for the measurement.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Research entities involved in the BEaTriX project: <a href=\"http:\/\/www.inaf.it\/en?set_language=en\" target=\"_blank\" rel=\"noreferrer noopener\">INAF<\/a> &#8211; <a href=\"https:\/\/www.esa.int\/\" target=\"_blank\" rel=\"noreferrer noopener\">ESA<\/a> &#8211; <a href=\"https:\/\/www.esrf.fr\/\" target=\"_blank\" rel=\"noreferrer noopener\">ESRF<\/a> &#8211; <a href=\"https:\/\/www.imem.cnr.it\/en\/node\" target=\"_blank\" rel=\"noreferrer noopener\">IMEM<\/a> &#8211; <a href=\"https:\/\/www.mpe.mpg.de\/main\" target=\"_blank\" rel=\"noreferrer noopener\">MPE<\/a> &#8211; <a href=\"https:\/\/www.dtu.dk\/english\" target=\"_blank\" rel=\"noreferrer noopener\">DTU<\/a><br><span id=\"docs-internal-guid-7b8b8230-7fff-a8e2-a246-629c03da3c3c\"><\/span><\/p>\n\n\n\n<h5 class=\"wp-block-heading\">ROLE OF THE OBSERVATORY<\/h5>\n\n\n\n<p class=\"wp-block-paragraph\">In <strong>2012<\/strong>, INAF-OABrera began to design a unique structure in the world with the aim to overcome the limitations of existing laboratories, thanks to the initial funding of the <strong>AHEAD<\/strong> (Activities for the High-Energy Astrophysics Domain) project, a grant awarded by the <strong>European Horizon-2020 program<\/strong>.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Thanks to the results achieved, INAF-OABrera subsequently obtained more funding to build the laboratory at our headquarters in Merate (LC): an ESA contract, a second AHEAD funding, ASI funds, and other dedicated INAF funds.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">BEaTriX has been designed to ensure\u00a0 a certain flexibility, beyond its primary purpose for the ATHENA telescope, so as to be used in the future for other X-ray optics, i.e. optics of different sizes than the ATHENA MMs and different focal lengths.<\/p>\n\n\n\n<h5 class=\"wp-block-heading has-text-align-left\">BEaTriX TEAM<\/h5>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-995f960e wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<p class=\"wp-block-paragraph\"><strong>OAB<\/strong> <strong>Staff<\/strong><\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Gianpiero Tagliaferri &#8211; Project Leader &#8211; gianpiero.tagliaferri AT inaf.it<\/li>\n\n\n\n<li>Giovanni Pareschi &#8211; Deputy Project Leader &#8211; giovanni.pareschi AT inaf.it<\/li>\n\n\n\n<li>Bianca Salmaso &#8211; Program manager &amp; System Engineer &#8211; bianca.salmaso AT inaf.it<\/li>\n\n\n\n<li>Stefano Basso &#8211; AIT &amp; AIV Executive Manager &#8211; stefano.basso AT inaf.it<\/li>\n\n\n\n<li>Daniele Spiga &#8211; Optical design and simulations &#8211; daniele.spiga AT inaf.it<\/li>\n\n\n\n<li>Mauro Ghigo &#8211; Vacuum System, Polishing and figuring and control software &#8211; mauro.ghigo AT inaf.it<\/li>\n\n\n\n<li>Gabriele Vecchi &#8211; Mirror polishing and figuring &#8211; gabriele.vecchi AT inaf.it<\/li>\n\n\n\n<li>Giorgia Sironi \u2013 Mirror metrology &#8211; giorgia.sironi AT inaf.it<\/li>\n\n\n\n<li>Vincenzo Cotroneo \u2013 Mirror figuring &#8211; vincenzo.cotroneo AT inaf.it<\/li>\n\n\n\n<li>Andrea Bianco &#8211; Clean environment &#8211; andrea.bianco AT inaf.it<\/li>\n\n\n\n<li>Rachele Millul &#8211; Project Controller &#8211; rachele.millul AT inaf.it<\/li>\n\n\n\n<li>Roberto Moncalvi &#8211; Contract Officer &#8211; roberto.moncalvi AT inaf.it<\/li>\n<\/ul>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\">\n<p class=\"wp-block-paragraph\"><strong>Students and postdoc in OAB<\/strong><\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Davide Sisana &#8211; PhD Politecnico Milano<\/li>\n\n\n\n<li>Akanshu Chauan &#8211; Postdoc<\/li>\n\n\n\n<li>Simone Marini &#8211; MS Thesis Politecnico Milano<br><\/li>\n<\/ul>\n\n\n\n<p class=\"wp-block-paragraph\"><strong>Staff from other entities<\/strong><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">Claudio Ferrari \u2013 Crystal manufacturing and characterization \u2013 IMEM-CNR<br> Andrea Zappettini &#8211; Crystal manufacturing \u2013 IMEM-CNR<br> Vadim Burwitz \u2013 MM cross-validation \u2013 MPE<br> Manuel Sanchez del Rio &#8211; Crystal simulations \u2013 \u00a0ESRF<br> Michela Uslenghi \u2013 Detectors \u2013 INAF-IASF-MI<br> Mauro Fiorini \u2013 Electronics &#8211; INAF-IASF-MI<br> Finn Christensen &#8211; External advisor \u2013 DTU<br> \u00a0Desir\u00e9e Della Monica Ferreira \u2013 Mirror coating \u2013 DTU<br> Sonny Massahi \u00a0\u2013 Mirror coating \u2013 DTU<\/p>\n<\/div>\n<\/div>\n\n\n\n<h5 class=\"wp-block-heading\">TIMELINE<\/h5>\n\n\n\n<p class=\"wp-block-paragraph\">2012 &#8211; 2030<\/p>\n\n\n\n<h5 class=\"wp-block-heading\">WEBSITE<\/h5>\n\n\n\n<div class=\"wp-block-group is-layout-constrained wp-block-group-is-layout-constrained\">\n<div class=\"wp-block-group is-vertical is-layout-flex wp-container-core-group-is-layout-1f26014c wp-block-group-is-layout-flex\">\n<p class=\"wp-block-paragraph\">BEaTriX: <a href=\"http:\/\/www.brera.inaf.it\/beatrix-facility\/\">http:\/\/www.brera.inaf.it\/beatrix-facility\/<\/a><\/p>\n<\/div>\n<\/div>\n\n\n\n<h5 class=\"wp-block-heading\">CONTACT<\/h5>\n\n\n\n<p class=\"wp-block-paragraph\">bianca.salmaso AT inaf.it<\/p>\n\n\n\n<h5 class=\"wp-block-heading\">CREDIT<\/h5>\n\n\n\n<p class=\"wp-block-paragraph\">Web page content: B. Salmaso and D. Spiga for BEaTriX Team<\/p>\n<\/div>\n<\/div>\n\n\n\n<h5 class=\"wp-block-heading\"> Origin of the name BEaTriX by Daniele Spiga<\/h5>\n\n\n\n<p class=\"wp-block-paragraph\">As often happens with the names of scientific projects, it is an acronym: initials that form a word. And in this way, the word takes on two meanings: one &#8220;serious&#8221; and one more &#8220;transcendent&#8221;. Let&#8217;s start with the &#8220;serious&#8221; one: BEaTriX is the acronym for the \u201cBeam Expander testing X-ray facility\u201d, a complex equipment assembly, unique in the world, enabling the creation of a parallel and wide beam of X-rays. This, in turn, simulates an astronomical X-ray source, in order to carry out tests on modular optics for telescopes such as Athena. BEaTriX was born for the development of silicon pore optics, in the context of our collaboration with ESA and Cosine. And it is a facility that is drawing great attention worldwide.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><br>But BEaTriX, with this interlocking of letters, is also dedicated to Beatrice Portinari, the woman who inspired Dante to write the Divine Comedy; the immortal masterpiece that recounts his journey\u00a0 not only through the Cosmos known in his days, and into the depths of the human soul also. And our soul is not only made of rationality, but also of emotions and passions, sometimes destructive but &#8211;\u00a0 fortunately &#8211; also high and sublime, the same passions that can lift humanity from the hell of self-destruction to the paradise of the contemplation of the entire Universe. And just as Beatrice (&#8220;she who makes happy&#8221;) leads the Supreme Poet by the hand towards the sky, illuminating him with the reflection of divine light\u2026, so we want to illuminate (even in X-rays) the optics that will carry the Athena telescope to the sky. To reveal to mankind a face of the Universe that we do not know yet, and make them a little happier than now.<br><\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><br>&#8220;<em>Beatrice mi guard\u00f2 con li occhi pieni<br>di faville d\u2019amor cos\u00ec divini,<br>che, vinta, mia virtute di\u00e8 le reni,<br>e quasi mi perdei con li occhi chini.<\/em>&#8220;<br>(Paradiso, IV 139-142)<\/p>\n","protected":false},"excerpt":{"rendered":"<p>BEaTriX Beam Expander Testing X-ray Facility SHORT DESCRIPTION BEaTriX is a facility installed at the INAF-Brera Astronomical Observatory in its seat Merate (Lecco). It is the first realization of an instrument that generates a parallel and wide X-ray beam within a small lab. The main objective of BEaTriX is to demonstrate that it is possible [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":1193,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"closed","template":"","format":"standard","meta":{"footnotes":""},"categories":[25],"tags":[],"class_list":["post-4007","progetti_ricerca","type-progetti_ricerca","status-publish","format-standard","has-post-thumbnail","hentry","category-research-project"],"blocksy_meta":[],"featured_image_urls":{"full":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-beatrix.png",800,800,false],"thumbnail":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-beatrix.png",150,150,false],"medium":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-beatrix.png",300,300,false],"medium_large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-beatrix.png",768,768,false],"large":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-beatrix.png",800,800,false],"1536x1536":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-beatrix.png",800,800,false],"2048x2048":["https:\/\/brera.inaf.it\/wp-content\/uploads\/2024\/06\/Progetti-OAB-800x800-beatrix.png",800,800,false]},"post_excerpt_stackable":"<p>BEaTriX Beam Expander Testing X-ray Facility SHORT DESCRIPTION BEaTriX is a facility installed at the INAF-Brera Astronomical Observatory in its seat Merate (Lecco). It is the first realization of an instrument that generates a parallel and wide X-ray beam within a small lab. The main objective of BEaTriX is to demonstrate that it is possible to perform acceptance tests of the optical modules of the ATHENA telescope, at a rate able to keep up with their manufacturing in series. ATHENA is an ESA X-ray observatory, scheduled for launch in 2030. The telescope consists of several hundred optical modules (Mirror Modules,&hellip;<\/p>\n","category_list":"<a href=\"https:\/\/brera.inaf.it\/en\/category\/research-project\/\" rel=\"category tag\">Research project<\/a>","author_info":{"name":"Maria Rosa Panzera","url":"https:\/\/brera.inaf.it\/en\/author\/maria-rosa-panzera\/"},"comments_num":"0 comments","_links":{"self":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/progetti_ricerca\/4007","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/progetti_ricerca"}],"about":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/types\/progetti_ricerca"}],"author":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/comments?post=4007"}],"version-history":[{"count":10,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/progetti_ricerca\/4007\/revisions"}],"predecessor-version":[{"id":4059,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/progetti_ricerca\/4007\/revisions\/4059"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media\/1193"}],"wp:attachment":[{"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/media?parent=4007"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/categories?post=4007"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/brera.inaf.it\/en\/wp-json\/wp\/v2\/tags?post=4007"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}