Share Email Print

Proceedings Paper

Optical design for the 5-28um NGST infrared imager MIRI
Author(s): Didier Dubreuil; Alain Abergel; Jacques Baudrand; Slimane Bensammar; Jacky B. Cretolle; Pascal Dargent; Philippe Galdemard; Jean Gay; Francois Lacombe; Pierre-Olivier Lagage; Laurent Martin; Eric Prieto; Yves Rabbia; Jean-Michel Reess; Pierre Riaud; Daniel Rouan; Sophie Salasca; Alain Simeri; Gillian S. Wright; J. P. Mols
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

MIRI is the mid infrared instrument planned for the NGST. Working in the 5-28 μm band, it includes 3 units: a spectrograph, an imager and a calibration facility. We describe here the optical design of the MIRI imager channel as it is at teh end of the phase A study. The MIRI imager provides 3 observing modes: an imaging mode with a field of view of 1.3 arcmin x 1.7 arcmin and a Pixel Field of View of 0.1 arcsec/pixel, a coronagraphic mode and a low resolution spectroscopic mode for point sources, between 5 μm and 10 μm, with a spectral resolution R = λ/Δλ around 100.

Paper Details

Date Published: 5 March 2003
PDF: 10 pages
Proc. SPIE 4850, IR Space Telescopes and Instruments, (5 March 2003); doi: 10.1117/12.461509
Show Author Affiliations
Didier Dubreuil, CEA Saclay (France)
Alain Abergel, Institut d'Astrophysique Spatiale (France)
Jacques Baudrand, Observatoire de Paris-Meudon (France)
Slimane Bensammar, Observatoire de Paris-Meudon (France)
Jacky B. Cretolle, CEA Saclay (France)
Pascal Dargent, Lab. d'Astrophysique de Marseille (France)
Philippe Galdemard, CEA Saclay (France)
Jean Gay, Observatoire de la Cote d'Azur (France)
Francois Lacombe, Observatoire de Paris-Meudon (France)
Pierre-Olivier Lagage, CEA Saclay (France)
Laurent Martin, Lab. d'Astrophysique de Marseille (France)
Eric Prieto, Lab. d'Astrophysique de Marseille (France)
Yves Rabbia, Observatoire de la Cote d'Azur (France)
Jean-Michel Reess, Observatoire de Paris-Meudon (France)
Pierre Riaud, Observatoire de Paris-Meudon (France)
Daniel Rouan, Observatoire de Paris-Meudon (France)
Sophie Salasca, CEA Saclay (France)
Alain Simeri, Observatoire de Paris-Meudon (France)
Gillian S. Wright, UK Astronomy Technology Ctr. (United Kingdom)
J. P. Mols, CEA Saclay (France)

Published in SPIE Proceedings Vol. 4850:
IR Space Telescopes and Instruments
John C. Mather, Editor(s)

© SPIE. Terms of Use
Back to Top