{"id":6,"date":"2015-07-16T13:50:13","date_gmt":"2015-07-16T13:50:13","guid":{"rendered":"https:\/\/www.clues-project.org\/cms\/?page_id=6"},"modified":"2023-09-18T08:34:03","modified_gmt":"2023-09-18T08:34:03","slug":"home","status":"publish","type":"page","link":"https:\/\/www.clues-project.org\/cms\/","title":{"rendered":"CLUES &#8211; Constrained Local UniversE Simulations"},"content":{"rendered":"<p>The <a href=\"http:\/\/en.wikipedia.org\/wiki\/Local_Group\" target=\"_blank\" rel=\"noopener noreferrer\">Local Group<\/a> and its environment is the most well observed region of the universe. Only in this unique environment can we study structure formation on scales as small as that of very low mass dwarf galaxies. The main goal of the CLUES-project is to provide <a href=\"https:\/\/www.clues-project.org\/cms\/home\/constrained-simulations\/\">constrained simulations<\/a> of the local universe designed to be used as a numerical laboratory of the current paradigm. The simulations will be used for unprecedented analysis of the complex dark matter and gasdynamical processes which govern the formation of galaxies. The predictions of these experiments can be easily compared with the detailed observations of our galactic neighborhood.<\/p>\n<div align=\"center\">\u00a0 \u00a0 \u00a0Executive Board of the Collaboration:<\/div>\n<div align=\"center\"><a href=\"http:\/\/jennygsorce.appspot.com\/\">Jenny Sorce,<\/a> <a href=\"https:\/\/dicintioarianna.wixsite.com\/mysite\">Arianna Di Cintio<\/a>, <a href=\"http:\/\/www.aip.de\/Members\/nlibeskind\/\">Noam Libeskind,<\/a> <a href=\"http:\/\/popia.ft.uam.es\/aknebe\/\">Alexander Knebe<\/a><a href=\"https:\/\/ipnl.in2p3.fr\/perso\/courtois\">,<\/a><\/div>\n<div align=\"center\"><a href=\"http:\/\/astro.ft.uam.es\/%7Egustavo\/\">Gustavo Yepes,<\/a> <a href=\"https:\/\/phys.huji.ac.il\/contacts\/hoffman_yehuda\">Yehuda Hoffman,<\/a> <a href=\"http:\/\/www.aip.de\/People\/SGottloeber\/\">Stefan Gottl\u00f6ber<\/a><\/div>\n<div align=\"center\"><\/div>\n<div align=\"center\"><\/div>\n<div align=\"center\"><\/div>\n<div align=\"center\"><\/div>\n<table class=\"plain\" border=\"0\" width=\"600\" cellspacing=\"2\" cellpadding=\"10\" align=\"center\">\n<tbody>\n<tr>\n<td style=\"padding-right: 20px;\" colspan=\"1\" rowspan=\"1\" width=\"220\"><a href=\"https:\/\/www.clues-project.org\/cms\/wp-content\/uploads\/2015\/07\/Box160and64.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-medium wp-image-277\" src=\"https:\/\/www.clues-project.org\/cms\/wp-content\/uploads\/2015\/07\/Box160and64-300x300.jpg\" alt=\"Box160and64\" width=\"300\" height=\"300\" srcset=\"https:\/\/www.clues-project.org\/cms\/wp-content\/uploads\/2015\/07\/Box160and64-300x300.jpg 300w, https:\/\/www.clues-project.org\/cms\/wp-content\/uploads\/2015\/07\/Box160and64-150x150.jpg 150w, https:\/\/www.clues-project.org\/cms\/wp-content\/uploads\/2015\/07\/Box160and64.jpg 800w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><\/a><\/td>\n<td colspan=\"1\" rowspan=\"1\"><em>Dark matter distribution in our Local Universe in two different simulations: a box with 160 Mpc\/h side length (big picture) and with 64 Mpc\/h side length (inset panel).<\/em><\/p>\n<p><em>See the\u00a0 <a href=\"https:\/\/www.clues-project.org\/cms\/images-and-movies\/\">Image Gallery<\/a> for more\u00a0 information and further images.<\/em><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n","protected":false},"excerpt":{"rendered":"<p>The Local Group and its environment is the most well observed region of the universe. Only in this unique environment can we study structure formation on scales as small as that of very low mass dwarf galaxies. The main goal of the CLUES-project is to provide constrained simulations of the local universe designed to be [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"open","template":"page-wide.php","meta":{"footnotes":""},"class_list":["post-6","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.clues-project.org\/cms\/wp-json\/wp\/v2\/pages\/6","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.clues-project.org\/cms\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.clues-project.org\/cms\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.clues-project.org\/cms\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.clues-project.org\/cms\/wp-json\/wp\/v2\/comments?post=6"}],"version-history":[{"count":39,"href":"https:\/\/www.clues-project.org\/cms\/wp-json\/wp\/v2\/pages\/6\/revisions"}],"predecessor-version":[{"id":726,"href":"https:\/\/www.clues-project.org\/cms\/wp-json\/wp\/v2\/pages\/6\/revisions\/726"}],"wp:attachment":[{"href":"https:\/\/www.clues-project.org\/cms\/wp-json\/wp\/v2\/media?parent=6"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}