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<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/abstract>	"La cam\u00E9ra \u00E0 large champ 3 (Wide Field Camera 3, WFC3) est le dernier instrument du t\u00E9lescope spatial Hubble et le plus avanc\u00E9 sur le plan technologique pour prendre des images dans le spectre visible. Cette cam\u00E9ra est install\u00E9 en remplacement de la camera WFPC2 (Wide Field and Planetary Camera 2) lors de la premi\u00E8re sortie extrav\u00E9hiculaire de la mission STS-125 de la navette spatiale Atlantis le 14 mai 2009. En 2021, l'outil est toujours op\u00E9rationnel."@fr .
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<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/Prism_(optics)> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/NIRCam> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://www.w3.org/2000/01/rdf-schema#comment>	"La cam\u00E9ra \u00E0 large champ 3 (Wide Field Camera 3, WFC3) est le dernier instrument du t\u00E9lescope spatial Hubble et le plus avanc\u00E9 sur le plan technologique pour prendre des images dans le spectre visible. Cette cam\u00E9ra est install\u00E9 en remplacement de la camera WFPC2 (Wide Field and Planetary Camera 2) lors de la premi\u00E8re sortie extrav\u00E9hiculaire de la mission STS-125 de la navette spatiale Atlantis le 14 mai 2009. En 2021, l'outil est toujours op\u00E9rationnel."@fr .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/Space_Telescope_Imaging_Spectrograph> .
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<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://www.w3.org/2000/01/rdf-schema#comment>	"La C\u00E1mara de Gran Angular 3 (en ingl\u00E9s, Wide Field Camera 3 o WFC3) es una c\u00E1mara que fue montada en el telescopio espacial Hubble en la Misi\u00F3n de Servicio 4 (STS-125). Esta misi\u00F3n, programada para el 8 de octubre de 2008, fue pospuesta hasta el 22 de mayo de 2009 debido al fallo de un importante componente del telescopio que hizo que la NASA decidiera posponer la misi\u00F3n para poder preparar uno nuevo y entrenar a la tripulaci\u00F3n en su sustituci\u00F3n."@es .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://www.w3.org/2000/01/rdf-schema#comment>	"Wide Field Camera 3 (WFC3) \u2013 kamera CCD zainstalowana w Kosmicznym Teleskopie Hubble\u2019a. Zosta\u0142a zamontowana na miejsce kamery Wide Field and Planetary Camera 2 (WFPC2) 14 maja 2009 przez za\u0142og\u0119 misji STS-125 wahad\u0142owca Atlantis. Kamera WFC3 ma czujniki CCD pokrywaj\u0105ce zakres ultrafioletu (od 200 nm) i \u015Bwiat\u0142a widzialnego (ka\u017Cdy o rozdzielczo\u015Bci 2048 \u00D7 4096 pikseli) oraz jeden detektor podczerwieni (1024 \u00D7 1024 pikseli), kt\u00F3ry mo\u017Ce rejestrowa\u0107 promieniowanie o d\u0142ugo\u015Bci fali do 1700 nm."@pl .
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<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/Advanced_Camera_for_Surveys> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/Faint_Object_Camera> .
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<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/STS-61> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/Spitzer_Space_Telescope> .
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<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/Camera> .
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<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/Cosmic_Origins_Spectrograph> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageWikiLink>	<http://dbpedia.org/resource/Mystic_Mountain> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://www.w3.org/2000/01/rdf-schema#label>	"\u0428\u0438\u0440\u043E\u043A\u043E\u0443\u0433\u043E\u043B\u044C\u043D\u0430\u044F \u043A\u0430\u043C\u0435\u0440\u0430 3"@ru .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://xmlns.com/foaf/0.1/isPrimaryTopicOf>	<http://en.wikipedia.org/wiki/Wide_Field_Camera_3> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageExternalLink>	<http://www.stsci.edu/hst/wfc3> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/wikiPageExternalLink>	<http://www.stsci.edu/hst/wfc3/design/images/hst-detectors-sm4.html> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://www.w3.org/1999/02/22-rdf-syntax-ns#type>	<http://dbpedia.org/class/yago/Instrumentality103575240> .
<http://dbpedia.org/resource/Wide_Field_Camera_3>	<http://dbpedia.org/ontology/abstract>	"La C\u00E1mara de Gran Angular 3 (en ingl\u00E9s, Wide Field Camera 3 o WFC3) es una c\u00E1mara que fue montada en el telescopio espacial Hubble en la Misi\u00F3n de Servicio 4 (STS-125). Esta misi\u00F3n, programada para el 8 de octubre de 2008, fue pospuesta hasta el 22 de mayo de 2009 debido al fallo de un importante componente del telescopio que hizo que la NASA decidiera posponer la misi\u00F3n para poder preparar uno nuevo y entrenar a la tripulaci\u00F3n en su sustituci\u00F3n. Esta c\u00E1mara sustituy\u00F3 a la C\u00E1mara Planetaria y de Gran Angular 2 y es la \u00FAltima y m\u00E1s avanzada en tomar fotograf\u00EDas en el espectro visible en el telescopio Hubble. WFC3 cuenta con dos sensores CCD de detecci\u00F3n UV/visible, cada uno de 2048 \u00D7 4096 p\u00EDxeles, y un detector de IR separada de 1024 \u00D7 1024, capaces de recibir la radiaci\u00F3n infrarroja hasta 1700 nm."@es .
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