SAFARI optical system architecture and design concept

SpicA FAR infrared Instrument, SAFARI, is one of the instruments planned for the SPICA mission. The SPICA mission is the next great leap forward in space-based far-infrared astronomy and will study the evolution of galaxies, stars and planetary systems. SPICA will utilize a deeply cooled 2.5m-class...

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Detalles Bibliográficos
Autores: Pastor Sempere, Carmen, Jellema, Willem, Zuluaga Ramírez, Pablo, Arrazola, David, Fernández Rodríguez, M., Belenguer Dávila, Tomás, González Fernández, Luis M., Audley, Michael D., Evers, Jaap, Eggens, Martin, Torres Redondo, Josefina, Najarro, Francisco, Roelfsema, Peter
Tipo de recurso: capítulo de libro
Fecha de publicación:2016
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/24902
Acceso en línea:https://hdl.handle.net/20.500.14352/24902
Access Level:acceso abierto
Palabra clave:52-43
535
543.42
Far infrared
Grating spectrometer
Optical design
SPICA mission
Astrofísica
Óptica física, óptica cuántica
2209.19 Óptica física
id ES_b76e10ece59522b385bb8655ab19fbfa
oai_identifier_str oai:docta.ucm.es:20.500.14352/24902
network_acronym_str ES
network_name_str España
repository_id_str
spelling SAFARI optical system architecture and design conceptPastor Sempere, CarmenJellema, WillemZuluaga Ramírez, PabloArrazola, DavidFernández Rodríguez, M.Belenguer Dávila, TomásGonzález Fernández, Luis M.Audley, Michael D.Evers, JaapEggens, MartinTorres Redondo, JosefinaNajarro, FranciscoRoelfsema, Peter52-43535543.42Far infraredGrating spectrometerOptical designSPICA missionAstrofísicaÓptica física, óptica cuántica2209.19 Óptica físicaSpicA FAR infrared Instrument, SAFARI, is one of the instruments planned for the SPICA mission. The SPICA mission is the next great leap forward in space-based far-infrared astronomy and will study the evolution of galaxies, stars and planetary systems. SPICA will utilize a deeply cooled 2.5m-class telescope, provided by European industry, to realize zodiacal background limited performance, and high spatial resolution. The instrument SAFARI is a cryogenic grating-based point source spectrometer working in the wavelength domain 34 to 230 μm, providing spectral resolving power from 300 to at least 2000. The instrument shall provide low and high resolution spectroscopy in four spectral bands. Low Resolution mode is the native instrument mode, while the high Resolution mode is achieved by means of a Martin-Pupplet interferometer. The optical system is all-reflective and consists of three main modules; an input optics module, followed by the Band and Mode Distributing Optics and the grating Modules. The instrument utilizes Nyquist sampled filled linear arrays of very sensitive TES detectors. The work presented in this paper describes the optical design architecture and design concept compatible with the current instrument performance and volume design drivers.SPIEUniversidad Complutense de Madrid20162016-01-0120162016-01-01book parthttp://purl.org/coar/resource_type/c_3248info:eu-repo/semantics/bookPartapplication/pdfhttps://hdl.handle.net/20.500.14352/24902reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2Atribución-NoComercial-SinDerivadas 3.0 Españahttps://creativecommons.org/licenses/by-nc-nd/3.0/es/info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/249022026-06-02T12:44:21Z
dc.title.none.fl_str_mv SAFARI optical system architecture and design concept
title SAFARI optical system architecture and design concept
spellingShingle SAFARI optical system architecture and design concept
Pastor Sempere, Carmen
52-43
535
543.42
Far infrared
Grating spectrometer
Optical design
SPICA mission
Astrofísica
Óptica física, óptica cuántica
2209.19 Óptica física
title_short SAFARI optical system architecture and design concept
title_full SAFARI optical system architecture and design concept
title_fullStr SAFARI optical system architecture and design concept
title_full_unstemmed SAFARI optical system architecture and design concept
title_sort SAFARI optical system architecture and design concept
dc.creator.none.fl_str_mv Pastor Sempere, Carmen
Jellema, Willem
Zuluaga Ramírez, Pablo
Arrazola, David
Fernández Rodríguez, M.
Belenguer Dávila, Tomás
González Fernández, Luis M.
Audley, Michael D.
Evers, Jaap
Eggens, Martin
Torres Redondo, Josefina
Najarro, Francisco
Roelfsema, Peter
author Pastor Sempere, Carmen
author_facet Pastor Sempere, Carmen
Jellema, Willem
Zuluaga Ramírez, Pablo
Arrazola, David
Fernández Rodríguez, M.
Belenguer Dávila, Tomás
González Fernández, Luis M.
Audley, Michael D.
Evers, Jaap
Eggens, Martin
Torres Redondo, Josefina
Najarro, Francisco
Roelfsema, Peter
author_role author
author2 Jellema, Willem
Zuluaga Ramírez, Pablo
Arrazola, David
Fernández Rodríguez, M.
Belenguer Dávila, Tomás
González Fernández, Luis M.
Audley, Michael D.
Evers, Jaap
Eggens, Martin
Torres Redondo, Josefina
Najarro, Francisco
Roelfsema, Peter
author2_role author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Universidad Complutense de Madrid
dc.subject.none.fl_str_mv 52-43
535
543.42
Far infrared
Grating spectrometer
Optical design
SPICA mission
Astrofísica
Óptica física, óptica cuántica
2209.19 Óptica física
topic 52-43
535
543.42
Far infrared
Grating spectrometer
Optical design
SPICA mission
Astrofísica
Óptica física, óptica cuántica
2209.19 Óptica física
description SpicA FAR infrared Instrument, SAFARI, is one of the instruments planned for the SPICA mission. The SPICA mission is the next great leap forward in space-based far-infrared astronomy and will study the evolution of galaxies, stars and planetary systems. SPICA will utilize a deeply cooled 2.5m-class telescope, provided by European industry, to realize zodiacal background limited performance, and high spatial resolution. The instrument SAFARI is a cryogenic grating-based point source spectrometer working in the wavelength domain 34 to 230 μm, providing spectral resolving power from 300 to at least 2000. The instrument shall provide low and high resolution spectroscopy in four spectral bands. Low Resolution mode is the native instrument mode, while the high Resolution mode is achieved by means of a Martin-Pupplet interferometer. The optical system is all-reflective and consists of three main modules; an input optics module, followed by the Band and Mode Distributing Optics and the grating Modules. The instrument utilizes Nyquist sampled filled linear arrays of very sensitive TES detectors. The work presented in this paper describes the optical design architecture and design concept compatible with the current instrument performance and volume design drivers.
publishDate 2016
dc.date.none.fl_str_mv 2016
2016-01-01
2016
2016-01-01
dc.type.none.fl_str_mv book part
http://purl.org/coar/resource_type/c_3248
dc.type.openaire.fl_str_mv info:eu-repo/semantics/bookPart
format bookPart
dc.identifier.none.fl_str_mv https://hdl.handle.net/20.500.14352/24902
url https://hdl.handle.net/20.500.14352/24902
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
Atribución-NoComercial-SinDerivadas 3.0 España
https://creativecommons.org/licenses/by-nc-nd/3.0/es/
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
Atribución-NoComercial-SinDerivadas 3.0 España
https://creativecommons.org/licenses/by-nc-nd/3.0/es/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv SPIE
publisher.none.fl_str_mv SPIE
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 15,300724

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