{"id":4282,"date":"2024-05-17T10:23:38","date_gmt":"2024-05-17T13:23:38","guid":{"rendered":"https:\/\/iate.oac.uncor.edu\/?p=4282"},"modified":"2024-05-17T10:24:13","modified_gmt":"2024-05-17T13:24:13","slug":"nuevos-limites-para-la-espectroscopia-de-campo-integral","status":"publish","type":"post","link":"https:\/\/iate.oac.uncor.edu\/en\/2024\/05\/17\/nuevos-limites-para-la-espectroscopia-de-campo-integral\/","title":{"rendered":"Viernes 17\/05: Nuevos l\u00edmites para la espectroscopia de campo integral"},"content":{"rendered":"<p style=\"text-align: justify;\"><span style=\"font-size: 12pt;\"><strong>Expositor:<\/strong> Rafael Andr\u00e9s Pignata (OAC)<\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"font-size: 12pt;\"><strong>Date:<\/strong> viernes 17 de mayo, 11 hs.<\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"font-size: 12pt;\"><strong>Abstract:<\/strong> La espectroscopia de campo integral, una tecnolog\u00eda introducida hace poco m\u00e1s de 30 a\u00f1os, ha transformado la astronom\u00eda. Sin embargo, sus beneficios son limitados cuando se combina con herramientas que no aprovechan todo su potencial. Aunque los diagramas de diagn\u00f3stico resultan valiosos para evaluar las condiciones f\u00edsicas de las nebulosas planetarias, no se han adaptado a las nuevas capacidades de observaci\u00f3n y an\u00e1lisis. Utilizamos datos IFS de MUSE y t\u00e9cnicas de clustering para explorar nuevos diagramas de diagn\u00f3stico que ayuden a llenar este vac\u00edo. El objetivo no es realizar un an\u00e1lisis spaxel por spaxel para comparar directamente estos resultados con los diagramas de diagn\u00f3stico existentes, sino examinar la distribuci\u00f3n de conjuntos de spaxels que comparten propiedades comunes en un espacio de par\u00e1metros N-dimensional.<\/span><\/p>","protected":false},"excerpt":{"rendered":"<p>Expositor: Rafael Andr\u00e9s Pignata (OAC) Fecha: viernes 17 de mayo, 11 hs. Resumen: La espectroscopia de campo integral, una tecnolog\u00eda introducida hace poco m\u00e1s de 30 a\u00f1os, ha transformado la astronom\u00eda. Sin embargo, sus beneficios son limitados cuando se combina con herramientas que no aprovechan todo su potencial. Aunque los&hellip;<\/p>","protected":false},"author":1,"featured_media":4283,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[3,9],"tags":[],"class_list":["post-4282","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-novedades","category-seminarios"],"_links":{"self":[{"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/posts\/4282","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/comments?post=4282"}],"version-history":[{"count":0,"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/posts\/4282\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/media\/4283"}],"wp:attachment":[{"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/media?parent=4282"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/categories?post=4282"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iate.oac.uncor.edu\/en\/wp-json\/wp\/v2\/tags?post=4282"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}