Current status of FRIDA, diffraction limited NIR Instrument for the GTC

FRIDA (inFRared Imager and Dissector for the Adaptive optics system of the Gran Telescopio Canarias) is designed as a diffraction limited instrument that will offer broad and narrow band imaging and integral field spectroscopy capabilities with low (R similar to 1,500), intermediate (R similar to 4,...

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Detalhes bibliográficos
Autores: Cardiel López, Nicolás, Eliche Moral, María del Carmen, Pascual, Sergio
Formato: artículo
Fecha de publicación:2012
País:España
Recursos:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/44431
Acesso em linha:https://hdl.handle.net/20.500.14352/44431
Access Level:acceso abierto
Palavra-chave:52
Infrared instrumentation - near infrared
Imaging
Integral field spectroscopy
IFU
GTC
Diffraction limited
Astrofísica
Astronomía (Física)
Física atmosférica
2501 Ciencias de la Atmósfera
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spelling Current status of FRIDA, diffraction limited NIR Instrument for the GTCCardiel López, NicolásEliche Moral, María del CarmenPascual, Sergio52Infrared instrumentation - near infraredImagingIntegral field spectroscopyIFUGTCDiffraction limitedAstrofísicaAstronomía (Física)Física atmosférica2501 Ciencias de la AtmósferaFRIDA (inFRared Imager and Dissector for the Adaptive optics system of the Gran Telescopio Canarias) is designed as a diffraction limited instrument that will offer broad and narrow band imaging and integral field spectroscopy capabilities with low (R similar to 1,500), intermediate (R similar to 4,500) and high (R similar to 30,000) spectral resolutions to operate in the wavelength range 0.9 - 2.5 mu m. The integral field unit is based on a monolithic image slicer. The imaging and IFS observing modes will use the same Teledyne 2K x 2K detector. FRIDA will be based at the Nasmyth B platform of GTC, behind the AO system. The key scientific objectives of the instrument include studies of solar system bodies, low mass objects, circumstellar outflow phenomena in advanced stages of stellar evolution, active galactic nuclei, high redshift galaxies, resolved stellar populations, semi-detached binary systems, young stellar objects and star forming environments. FRIDA is a collaborative project between the main GTC partners, namely, Spain, Mexico and Florida. In this paper, we present the status of the instrument design as it is currently being prepared for its manufacture, after an intensive prototypes' phase and design optimization. The CDR was held in September 2011.SPIE-Int Soc Optical EngineeringUniversidad Complutense de Madrid20122012-01-0120122012-01-01journal articlehttp://purl.org/coar/resource_type/c_6501info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/44431reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/444312026-06-02T12:44:21Z
dc.title.none.fl_str_mv Current status of FRIDA, diffraction limited NIR Instrument for the GTC
title Current status of FRIDA, diffraction limited NIR Instrument for the GTC
spellingShingle Current status of FRIDA, diffraction limited NIR Instrument for the GTC
Cardiel López, Nicolás
52
Infrared instrumentation - near infrared
Imaging
Integral field spectroscopy
IFU
GTC
Diffraction limited
Astrofísica
Astronomía (Física)
Física atmosférica
2501 Ciencias de la Atmósfera
title_short Current status of FRIDA, diffraction limited NIR Instrument for the GTC
title_full Current status of FRIDA, diffraction limited NIR Instrument for the GTC
title_fullStr Current status of FRIDA, diffraction limited NIR Instrument for the GTC
title_full_unstemmed Current status of FRIDA, diffraction limited NIR Instrument for the GTC
title_sort Current status of FRIDA, diffraction limited NIR Instrument for the GTC
dc.creator.none.fl_str_mv Cardiel López, Nicolás
Eliche Moral, María del Carmen
Pascual, Sergio
author Cardiel López, Nicolás
author_facet Cardiel López, Nicolás
Eliche Moral, María del Carmen
Pascual, Sergio
author_role author
author2 Eliche Moral, María del Carmen
Pascual, Sergio
author2_role author
author
dc.contributor.none.fl_str_mv Universidad Complutense de Madrid
dc.subject.none.fl_str_mv 52
Infrared instrumentation - near infrared
Imaging
Integral field spectroscopy
IFU
GTC
Diffraction limited
Astrofísica
Astronomía (Física)
Física atmosférica
2501 Ciencias de la Atmósfera
topic 52
Infrared instrumentation - near infrared
Imaging
Integral field spectroscopy
IFU
GTC
Diffraction limited
Astrofísica
Astronomía (Física)
Física atmosférica
2501 Ciencias de la Atmósfera
description FRIDA (inFRared Imager and Dissector for the Adaptive optics system of the Gran Telescopio Canarias) is designed as a diffraction limited instrument that will offer broad and narrow band imaging and integral field spectroscopy capabilities with low (R similar to 1,500), intermediate (R similar to 4,500) and high (R similar to 30,000) spectral resolutions to operate in the wavelength range 0.9 - 2.5 mu m. The integral field unit is based on a monolithic image slicer. The imaging and IFS observing modes will use the same Teledyne 2K x 2K detector. FRIDA will be based at the Nasmyth B platform of GTC, behind the AO system. The key scientific objectives of the instrument include studies of solar system bodies, low mass objects, circumstellar outflow phenomena in advanced stages of stellar evolution, active galactic nuclei, high redshift galaxies, resolved stellar populations, semi-detached binary systems, young stellar objects and star forming environments. FRIDA is a collaborative project between the main GTC partners, namely, Spain, Mexico and Florida. In this paper, we present the status of the instrument design as it is currently being prepared for its manufacture, after an intensive prototypes' phase and design optimization. The CDR was held in September 2011.
publishDate 2012
dc.date.none.fl_str_mv 2012
2012-01-01
2012
2012-01-01
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/20.500.14352/44431
url https://hdl.handle.net/20.500.14352/44431
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv SPIE-Int Soc Optical Engineering
publisher.none.fl_str_mv SPIE-Int Soc Optical Engineering
dc.source.none.fl_str_mv reponame:Docta Complutense
instname:Universidad Complutense de Madrid (UCM)
instname_str Universidad Complutense de Madrid (UCM)
reponame_str Docta Complutense
collection Docta Complutense
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15.301603

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