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Herschel-SPIRE: design, ground test results, and predicted performance

Authors :
Jean-Paul Baluteau
Edward Polehampton
Sunil Sidher
Walter Kieran Gear
Paolo Saraceno
Hien Nguyen
K. J. King
Marc Ferlet
Philippe André
L. Vigroux
Alberto Franceschini
G. J. Bendo
David J. Smith
Peter Charles Hargrave
Glenn Laurent
A. Abreu
Tanya Lim
Adam Woodcraft
Alain Abergel
Jason Glenn
Trevor Fulton
Gillian S. Wright
M. Rowan-Robinson
Locke D. Spencer
Alan Pearce
D. Rizzo
Seb Oliver
Bernhard Schulz
David A. Naylor
Kevin Xu
Nanyao Lu
Darren Dowell
Ivan Valtchanov
Maohai Huang
Bruce Swinyard
Emmanuel Lellouch
Lijun Zhang
Matthew Joseph Griffin
Peter A. R. Ade
Eric Sawyer
Göran Olofsson
Alan Dowell
Douglas Griffin
James J. Bock
Ismael Perez-Fournon
Mat Page
Annie Zavagno
Sarah Leeks
Service d'Astrophysique
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)
Institut d'astrophysique spatiale (IAS)
Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES)
Recherche en épidémiologie et biostatistique
Université Paris-Sud - Paris 11 (UP11)-Institut National de la Santé et de la Recherche Médicale (INSERM)
Observatoire Astronomique de Marseille Provence (OAMP)
Université de Provence - Aix-Marseille 1-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire d'Astrophysique de Marseille (LAM)
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Astronomy Centre, University of Sussex
Imperial College London
CEA Cadarache
Ton Duc Thang University [Hô-Chi-Minh-City]
University of Pisa - Università di Pisa
NASA Herschel Science Center
Infrared Processing and Analysis Center (IPAC)
California Institute of Technology (CALTECH)-California Institute of Technology (CALTECH)
Herschel Science Centre
Agence Spatiale Européenne = European Space Agency (ESA)
Department of Informatics and Mathematical Modelling [Lyngby] (IMM)
Danmarks Tekniske Universitet = Technical University of Denmark (DTU)
Oschmann
Jacobus M.
Jr. and de Graauw
Mattheus W.~M. and MacEwen
Howard A.
Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Department of Mathematics and Statistics, La Trobe University
Agro-Systèmes Territoires Ressources Mirecourt (ASTER Mirecourt)
Institut National de la Recherche Agronomique (INRA)
NASA-California Institute of Technology (CALTECH)
European Space Agency (ESA)
Technical University of Denmark [Lyngby] (DTU)
Source :
Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, 2008, Marseille, France. pp.701006, ⟨10.1117/12.788312⟩, SPIE Astronomical Telescopes + Instrumentation, SPIE Astronomical Telescopes + Instrumentation, 2009, Marseille, France. pp.701006, ⟨10.1117/12.788312⟩
Publication Year :
2008
Publisher :
SPIE, 2008.

Abstract

International audience; SPIRE, the Spectral and Photometric Imaging Receiver, is a submillimetre camera and spectrometer for Herschel. It comprises a three-band camera operating at 250, 350 and 500 Â\textmum, and an imaging Fourier Transform Spectrometer covering 194-672 \ensuremathμm. The photometer field of view is 4x8 arcmin., viewed simultaneously in the three bands. The FTS has an approximately circular field of view of 2.6 arcmin. diameter and spectral resolution adjustable between 0.04 and 2 cm^-1 ( \ensuremathλ/▵\ensuremathλ=20-1000 at 250 \ensuremathμm). Following successful testing in a dedicated facility designed to simulate the in-flight operational conditions, SPIRE has been integrated in the Herschel spacecraft and is now undergoing system-level testing prior to launch. The main design features of SPIRE are reviewed, the key results of instrument testing are outlined, and a summary of the predicted in-flight performance is given.

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter
Accession number :
edsair.doi.dedup.....a4cc4a4735c04b3b8c113902c35277e6
Full Text :
https://doi.org/10.1117/12.788312