{"id":116784,"date":"2014-09-12T00:00:00","date_gmt":"2014-09-12T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/recuperacion-de-informacion-astronomica-nuevas-perspectivas-de-analisis-de-la-cartografa%c2%ada-celeste-historica\/"},"modified":"2014-09-12T00:00:00","modified_gmt":"2014-09-12T00:00:00","slug":"recuperacion-de-informacion-astronomica-nuevas-perspectivas-de-analisis-de-la-cartografa%c2%ada-celeste-historica","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/historia\/recuperacion-de-informacion-astronomica-nuevas-perspectivas-de-analisis-de-la-cartografa%c2%ada-celeste-historica\/","title":{"rendered":"Recuperaci\u00f3n de informaci\u00f3n astron\u00f3mica: nuevas perspectivas de an\u00e1lisis de la cartograf\u00edaceleste hist\u00f3rica."},"content":{"rendered":"<h2>Tesis doctoral de <strong> Mar\u00eda  Pilar Alonso Lifante <\/strong><\/h2>\n<p>Resumen  la mejora de la descripci\u00f3n de contenidos de recursos especializados en general, y de astron\u00f3micos en particular, es todav\u00eda una asignatura pendiente de las ciencias de la documentaci\u00f3n. Actualmente existe gran cantidad de informaci\u00f3n astron\u00f3mica hist\u00f3rica de inter\u00e9s recogida en diversos tipos de documentos que se conservan en archivos y bibliotecas astron\u00f3micas de todo el mundo. Entre estos documentos se encuentran los denominados cat\u00e1logos y atlas de estrellas, as\u00ed como im\u00e1genes astrofotogr\u00e1ficas, todav\u00eda compilados en la actualidad aunque en formatos bien diferentes y con datos mucho m\u00e1s precisos. Sin embargo, las medidas procedentes de observaciones varios siglos atr\u00e1s siguen atrayendo a buena parte de la comunidad cient\u00edfica. No en vano, grandes descubrimientos en astronom\u00eda han sido posibles gracias a la comparaci\u00f3n de datos hist\u00f3ricos y contempor\u00e1neos.  actualmente existe una extensa lista de par\u00e1metros por los que los investigadores en astronom\u00eda y astrof\u00edsica suelen buscar en bases de datos especializadas, las cuales ofrecen un ampl\u00edsimo abanico de opciones de b\u00fasqueda posibilitando la recuperaci\u00f3n de casi cualquier dato que deseen entre todas las fuentes disponibles. El problema surge cuando estos investigadores quieren consultar el opac de la biblioteca de forma similar a como lo hacen en las bases de datos mencionadas. El principal obst\u00e1culo que encuentran es la propia interfaz de b\u00fasqueda, que no les permite realizar consultas especializadas. Esto sucede debido a que los est\u00e1ndares de catalogaci\u00f3n (marc 21, isbd, rda, etc.) Son muy generales y no permiten realizar descripciones suficientemente especializadas. Esto se traduce en que los fondos no pueden ser adecuadamente explotados por los investigadores.  por tanto, esta memoria persigue un doble objetivo: (1) la b\u00fasqueda de nuevos campos de descripci\u00f3n para cat\u00e1logos y atlas de estrellas as\u00ed como im\u00e1genes astrofotogr\u00e1ficas; y (2) mostrar la importancia de determinados campos presentes en las reglas de catalogaci\u00f3n que no est\u00e1n siendo ampliamente utilizados por parte de los catalogadores en las descripciones bibliogr\u00e1ficas.  Para ello, se ha llevado a cabo un estudio de una muestra de cat\u00e1logos y atlas de estrellas de los siglos xviii, xix y xx procedentes del real instituto y observatorio de la armada (san fernando), con el fin de conocer los datos cient\u00edficos m\u00e1s frecuentemente proporcionados. En el caso de las im\u00e1genes astrofotogr\u00e1ficas,  se ha analizado el software google sky y las bases de datos astron\u00f3micas a las que enlaza, con el fin de conocer los par\u00e1metros m\u00e1s consultados por los investigadores en la b\u00fasqueda de objetos celestes que pueden encontrarse en dichas im\u00e1genes.  como resultado del estudio, se ha extra\u00eddo un conjunto de par\u00e1metros de descripci\u00f3n que puede clasificarse en tres grupos: (1) par\u00e1metros que ya se encuentran presentes en los est\u00e1ndares empleados en archivos y bibliotecas; (2) nuevos par\u00e1metros que podr\u00edan ser registrados en algunos de los campos de dichas normativas; y (3) nuevos par\u00e1metros que s\u00f3lo podr\u00edan tener cabida en campos generales de notas, y que ser\u00edan susceptibles de convertirse en nuevos campos de los citados est\u00e1ndares. En esta memoria se analizan en detalle las limitaciones existentes en torno a la inclusi\u00f3n en las normas de los par\u00e1metros de los grupos 2 y 3, lo cual lleva a la propuesta de un modelo de datos para este tipo de recursos.  las conclusiones indican que los est\u00e1ndares de catalogaci\u00f3n no est\u00e1n preparados para abordar una adecuada descripci\u00f3n de los recursos astron\u00f3micos hist\u00f3ricos, a pesar de los grandes esfuerzos que se han venido realizando desde las agencias de normalizaci\u00f3n en los \u00faltimos a\u00f1os. Por tanto, esta propuesta de par\u00e1metros de descripci\u00f3n se presenta como una alternativa real para satisfacer las necesidades de informaci\u00f3n hist\u00f3rica de los investigadores.   abstract  the general improvement in the content description of specialised resources, astronomical in particular, is still a pending issue in the field of library and information science. There is currently a huge amount of useful historical astronomical information stored in different type of documents which are preserved in libraries and archives all over the world. Star catalogues and atlases are found among these documents, as well as astrophotography images, that are still collected nowadays, although using different formats and more accurate data. Nevertheless, measurements coming from observations carried out several centuries ago are still attractive to a large part of the scientific community. Indeed, most astronomical discoveries throughout history have been possible due to comparisons between old and contemporary data.  there is currently a long list of parameters by which astronomers and astrophysicists are used to querying their specialised databases, that offer a large amount of search options, thus making it possible a very satisfactory information retrieval among the available sources. However, serious difficulties arise when researchers want to query library opacs in a similar way as they do in the aforementioned databases. The main obstacle they find is the user graphical interface, which does not provide with tools for specialised queries. The reason is that cataloguing standards (marc 21, isbd, rda, etc.) Are too generic, hence specialised descriptions are not possible in many cases. As a consequence, researchers cannot exploit collections preserved in libraries and archives.  thus, the goal of this memoir is twofold: (1) searching for new description fields for star catalogues and atlases as well as celestial objects in astrophotography images; and (2) to show the importance of some existing fields which are not being widely used by cataloguers in bibliographic descriptions. To do this, a sample of historical star catalogues and atlases (18th, 19th and 20th centuries) from the royal institute and observatory of the spanish navy has been selected in order to identify the most frequently supplied scientific information. In the case of celestial objects with presence in astrophotography images, the software google sky and its linked databases have been analysed in order to know the most consulted parameters by researchers when searching for these celestial objects.  as a result of this analysis, a whole set of description parameters has been found, which can be classified in three groups: (1) parameters that can already be described by cataloguing standards; (2) new parameters that could be recorded in current description fields; and (3) new parameters that could be only recorded in general note fields. Furthermore, the existing limitations concerning the inclusion in the standards of the parameters from group 2 and 3 are also analysed in detail, which lead to the proposal of a data model for this type of resources.  conclusions show that cataloguing standards are still not ready to address adequate descriptions of historical astronomical resources, despite libraries and associations involved in the creation of these standards having made great efforts to describe, in general, the bibliographic universe during the last few years. Thus, this proposal of description parameters is presented as a real alternative to satisfy the historical information needs of researchers.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Recuperaci\u00f3n de informaci\u00f3n astron\u00f3mica: nuevas perspectivas de an\u00e1lisis de la cartograf\u00edaceleste hist\u00f3rica.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Recuperaci\u00f3n de informaci\u00f3n astron\u00f3mica: nuevas perspectivas de an\u00e1lisis de la cartograf\u00edaceleste hist\u00f3rica. <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Mar\u00eda  Pilar Alonso Lifante <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Murcia<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 09\/12\/2014<\/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>Juan  Jose Sanchez Baena<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Antonio Mu\u00f1oz ca\u00f1avate <\/li>\n<li>Marta Garcia garralon (vocal)<\/li>\n<li>Antonio Irigoyen lopez (vocal)<\/li>\n<li>eduardo Peis redondo (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Mar\u00eda Pilar Alonso Lifante Resumen la mejora de la descripci\u00f3n de contenidos de recursos especializados en general, [&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 center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""}},"footnotes":""},"categories":[1050,2264,5526,104,8235],"tags":[102982,177440,47401,8768,230413,162550],"class_list":["post-116784","post","type-post","status-publish","format-standard","hentry","category-astronomia-y-astrofisica","category-cartografia-geodesica","category-documentacion","category-historia","category-murcia","tag-antonio-irigoyen-lopez","tag-antonio-munoz-canavate","tag-eduardo-peis-redondo","tag-juan-jose-sanchez-baena","tag-maria-pilar-alonso-lifante","tag-marta-garcia-garralon"],"_links":{"self":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/posts\/116784","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/comments?post=116784"}],"version-history":[{"count":0,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/posts\/116784\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/media?parent=116784"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/categories?post=116784"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/tags?post=116784"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}