Publication

SAFARI optical system architecture and design concept

Pastor, C., Jellema, W., Zuluaga-Ramírez, P., Arrazola, D., Fernández-Rodriguez, M., Belenguer, T., González Fernández, L. M., Audley, M. D., Evers, J., Eggens, M., Torres Redondo, J., Najarro, F. & Roelfsema, P., 2016, Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99043U (July 29, 2016). 99043U

Research output: Chapter in Book/Report/Conference proceedingConference contributionAcademic

APA

Pastor, C., Jellema, W., Zuluaga-Ramírez, P., Arrazola, D., Fernández-Rodriguez, M., Belenguer, T., ... Roelfsema, P. (2016). SAFARI optical system architecture and design concept. In Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99043U (July 29, 2016) [99043U] https://doi.org/10.1117/12.2232786

Author

Pastor, Carmen ; Jellema, Willem ; Zuluaga-Ramírez, Pablo ; Arrazola, David ; Fernández-Rodriguez, M. ; Belenguer, Tomás ; González Fernández, Luis M. ; Audley, Michael D. ; Evers, Jaap ; Eggens, Martin ; Torres Redondo, Josefina ; Najarro, Francisco ; Roelfsema, P. / SAFARI optical system architecture and design concept. Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99043U (July 29, 2016). 2016.

Harvard

Pastor, C, Jellema, W, Zuluaga-Ramírez, P, Arrazola, D, Fernández-Rodriguez, M, Belenguer, T, González Fernández, LM, Audley, MD, Evers, J, Eggens, M, Torres Redondo, J, Najarro, F & Roelfsema, P 2016, SAFARI optical system architecture and design concept. in Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99043U (July 29, 2016)., 99043U. https://doi.org/10.1117/12.2232786

Standard

SAFARI optical system architecture and design concept. / Pastor, Carmen; Jellema, Willem; Zuluaga-Ramírez, Pablo; Arrazola, David; Fernández-Rodriguez, M.; Belenguer, Tomás; González Fernández, Luis M.; Audley, Michael D.; Evers, Jaap; Eggens, Martin; Torres Redondo, Josefina; Najarro, Francisco; Roelfsema, P.

Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99043U (July 29, 2016). 2016. 99043U.

Research output: Chapter in Book/Report/Conference proceedingConference contributionAcademic

Vancouver

Pastor C, Jellema W, Zuluaga-Ramírez P, Arrazola D, Fernández-Rodriguez M, Belenguer T et al. SAFARI optical system architecture and design concept. In Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99043U (July 29, 2016). 2016. 99043U https://doi.org/10.1117/12.2232786


BibTeX

@inproceedings{a7f79e8ab87444119c286ad72b98da74,
title = "SAFARI optical system architecture and design concept",
abstract = "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.",
author = "Carmen Pastor and Willem Jellema and Pablo Zuluaga-Ram{\'i}rez and David Arrazola and M. Fern{\'a}ndez-Rodriguez and Tom{\'a}s Belenguer and {Gonz{\'a}lez Fern{\'a}ndez}, {Luis M.} and Audley, {Michael D.} and Jaap Evers and Martin Eggens and {Torres Redondo}, Josefina and Francisco Najarro and P. Roelfsema",
note = "M1 - Conference Proceedings",
year = "2016",
doi = "10.1117/12.2232786",
language = "English",
booktitle = "Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99043U (July 29, 2016)",

}

RIS

TY - GEN

T1 - SAFARI optical system architecture and design concept

AU - Pastor, Carmen

AU - Jellema, Willem

AU - Zuluaga-Ramírez, Pablo

AU - Arrazola, David

AU - Fernández-Rodriguez, M.

AU - Belenguer, Tomás

AU - González Fernández, Luis M.

AU - Audley, Michael D.

AU - Evers, Jaap

AU - Eggens, Martin

AU - Torres Redondo, Josefina

AU - Najarro, Francisco

AU - Roelfsema, P.

N1 - M1 - Conference Proceedings

PY - 2016

Y1 - 2016

N2 - 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.

AB - 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.

U2 - 10.1117/12.2232786

DO - 10.1117/12.2232786

M3 - Conference contribution

BT - Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99043U (July 29, 2016)

ER -

ID: 40916143