{"id":73186,"date":"2005-12-03T00:00:00","date_gmt":"2005-12-03T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/x-gamma-ray-imaging-of-hmxrb-with-integral\/"},"modified":"2005-12-03T00:00:00","modified_gmt":"2005-12-03T00:00:00","slug":"x-gamma-ray-imaging-of-hmxrb-with-integral","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/ciencias-de-la-tierra-y-del-espacio\/x-gamma-ray-imaging-of-hmxrb-with-integral\/","title":{"rendered":"X-gamma ray imaging of hmxrb with integral"},"content":{"rendered":"<h2>Tesis doctoral de <strong> Silvia Martinez Nu\u00f1ez <\/strong><\/h2>\n<p>Esta tesis es el resultado de la participaci\u00f3n de la doctoranda en el desarrollo del software de an\u00e1lisis cient\u00edfico del monitor de rayos x (jem-x) a bordo de la misi\u00f3n integral (international gamma-ray astrophysics laboratory) y de la reducci\u00f3n y an\u00e1lisis de los datos proporcionados por los tres instrumentos de alta energ\u00eda del sat\u00e9lite.  integral es un telescopio de rayos gamma (15kev&#8211; 10 kev) con observaciones simult\u00e1neas en rayos x (4 &#8212; 35 kev) y en el \u00f3ptico (500 nm &#8211; 600 nm). los tres instrumentos de alta energ\u00eda son telescopios de m\u00e1scaras codificadas, por tanto la reducci\u00f3n de los datos es compleja, requiriendo un conocimiento profundo de los instrumentos y las herramientas para analizar los datos.  la tesis se divide en dos partes. En la primera parte se describe el software de an\u00e1lisis cient\u00edfico de jem-x.  El trabajo presentado en esta primera parte es consecuencia de un estudio del software de an\u00e1lisis del monitor, de su validaci\u00f3n cient\u00edfica durante las primeras fases de la misi\u00f3n y del desarrollo y  mantenimiento de los guiones (scripts) de an\u00e1lisis de jem-x.  en la segunda parte, se presentan los resultados de un estudio del enim\u00e1gtico sistema binario de rayos x cygnus x-3. Este sistema ha sido observado desde los comienzos de la astronom\u00eda de rayos x, pero su naturaleza es todav\u00eda desconocida. Esta tesis proporciona nuevas claves para resolver la misteriosa naturaleza de la fuente.  la  estructura de la tesis es la siguiente: la primera parte comienza con un resumen de la misi\u00f3n integral, sus instrumentos, la t\u00e9cnica de m\u00e1scaras codificadas, el programa de observaci\u00f3n y el segmento de tierra. En el cap\u00edtulo 2 se presentan los principales conceptos para la reducci\u00f3n de los datos de integral,  as\u00ed como una descripci\u00f3n detallada de cada uno de los niveles de an\u00e1lisis del monitor de rayos x.  Como ha evolucionado el software de jem-x desde el lanzamiento del sat\u00e9lite para adecuarse al com<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>X-gamma ray imaging of hmxrb with integral<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 X-gamma ray imaging of hmxrb with integral <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Silvia Martinez Nu\u00f1ez <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Universitat de val\u00e9ncia (estudi general)<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 12\/03\/2005<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n<h3>Direcci\u00f3n y tribunal<\/h3>\n<ul>\n<li><strong>Director de la tesis<\/strong>\n<ul>\n<li>Peter Krestschmar<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: \u00e1lvaro Gim\u00e9nez ca\u00f1ete <\/li>\n<li>pietro Ubertini (vocal)<\/li>\n<li>niels Lund (vocal)<\/li>\n<li>Jos\u00e9 Miguel Mas hesse (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Silvia Martinez Nu\u00f1ez Esta tesis es el resultado de la participaci\u00f3n de la doctoranda en el desarrollo [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center 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