
Proceedings Paper
The mid-infrared channel of the EChO missionFormat | Member Price | Non-Member Price |
---|---|---|
$17.00 | $21.00 |
Paper Abstract
The Exoplanet Characterisation Observatory, EChO, is a dedicated space mission to investigate the physics and chemistry of Exoplanet atmospheres. Using the differential spectroscopy by transit method, it provides simultaneously a complete spectrum in a wide wavelength range between 0.4μm and 16μm of the atmosphere of exoplanets. The payload is subdivided into 6 channels. The mid-infrared channel covers the spectral range between 5μm and 11μm. In order to optimize the instrument response and the science objectives, the bandpass is split in two using an internal dichroic. We present the opto-mechanical concept of the MWIR channel and the detector development that have driven the thermal and mechanical designs of the channel. The estimated end-to-end performance is also presented.
Paper Details
Date Published: 28 August 2014
PDF: 8 pages
Proc. SPIE 9143, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, 91432F (28 August 2014); doi: 10.1117/12.2054919
Published in SPIE Proceedings Vol. 9143:
Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Jacobus M. Oschmann Jr.; Mark Clampin; Giovanni G. Fazio; Howard A. MacEwen, Editor(s)
PDF: 8 pages
Proc. SPIE 9143, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, 91432F (28 August 2014); doi: 10.1117/12.2054919
Show Author Affiliations
J. M. Reess, LESIA, Observatoire de Paris, CNRS (France)
G. Tinetti, Univ. College London (United Kingdom)
J. P. Beaulieu, Institut d'Astrophysique de Paris (France)
P. Bernardi, LESIA, Observatoire de Paris, CNRS (France)
O. Boulade, Astrophysique Interactions Multi-échelles, CNRS, Univ. Paris Diderot (France)
C. Cara, Astrophysique Interactions Multi-échelles, CNRS, Univ. Paris Diderot (France)
V. Coudé de Foresto, LESIA, Observatoire de Paris, CNRS (France)
P. Drossart, LESIA, Observatoire de Paris, CNRS (France)
G. Tinetti, Univ. College London (United Kingdom)
J. P. Beaulieu, Institut d'Astrophysique de Paris (France)
P. Bernardi, LESIA, Observatoire de Paris, CNRS (France)
O. Boulade, Astrophysique Interactions Multi-échelles, CNRS, Univ. Paris Diderot (France)
C. Cara, Astrophysique Interactions Multi-échelles, CNRS, Univ. Paris Diderot (France)
V. Coudé de Foresto, LESIA, Observatoire de Paris, CNRS (France)
P. Drossart, LESIA, Observatoire de Paris, CNRS (France)
P. O. Lagage, Astrophysique Interactions Multi-échelles, CNRS, Univ. Paris Diderot (France)
G. Morinaud, Institut d'Astrophysique Spatiale, CNRS, Univ. Paris Sud 11 (France)
N. Nguyen-Tuong, LESIA, Observatoire de Paris, CNRS (France)
M. Ollivier, Institut d'Astrophysique Spatiale, CNRS, Univ. Paris Sud 11 (France)
F. Pinsard, Astrophysique Interactions Multi-échelles, CNRS, Univ. Paris Diderot (France)
J. Tanrin, LESIA, Observatoire de Paris, CNRS (France)
D. Zeganadin, LESIA, Observatoire de Paris, CNRS (France)
R. Cledassou, Ctr. National d'Études Spatiales (France)
G. Morinaud, Institut d'Astrophysique Spatiale, CNRS, Univ. Paris Sud 11 (France)
N. Nguyen-Tuong, LESIA, Observatoire de Paris, CNRS (France)
M. Ollivier, Institut d'Astrophysique Spatiale, CNRS, Univ. Paris Sud 11 (France)
F. Pinsard, Astrophysique Interactions Multi-échelles, CNRS, Univ. Paris Diderot (France)
J. Tanrin, LESIA, Observatoire de Paris, CNRS (France)
D. Zeganadin, LESIA, Observatoire de Paris, CNRS (France)
R. Cledassou, Ctr. National d'Études Spatiales (France)
Published in SPIE Proceedings Vol. 9143:
Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Jacobus M. Oschmann Jr.; Mark Clampin; Giovanni G. Fazio; Howard A. MacEwen, Editor(s)
© SPIE. Terms of Use
