Paper
5 August 2010 The E-NIS instrument on-board the ESA Euclid Dark Energy Mission: a general view after positive conclusion of the assessment phase
Author Affiliations +
Abstract
The Euclid Near-Infrared Spectrometer (E-NIS) Instrument was conceived as the spectroscopic probe on-board the ESA Dark Energy Mission Euclid. Together with the Euclid Imaging Channel (EIC) in its Visible (VIS) and Near Infrared (NIP) declinations, NIS formed part of the Euclid Mission Concept derived in assessment phase and submitted to the Cosmic Vision Down-selection process from which emerged selected and with extremely high ranking. The Definition phase, started a few months ago, is currently examining a substantial re-arrangement of the payload configuration due to technical and programmatic aspects. This paper presents the general lines of the assessment phase payload concept on which the positive down-selection judgments have been based.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
L. Valenziano, F. M. Zerbi, A. Cimatti, A. Bianco, C. Bonoli, F. Bortoletto, A. Bulgarelli, R. C. Butler, R. Content, L. Corcione, A. De Rosa, P. Franzetti, B. Garilli, F. Gianotti, E. Giro, R. Grange, P. Leutenegger, S. Ligori, L. Martin, N. Mandolesi, G. Morgante, L. Nicastro, M. Riva, M. Robberto, R. Sharples, P. Spanò, G. Talbot, M. Trifoglio, R. Wink, and F. Zamkotsian "The E-NIS instrument on-board the ESA Euclid Dark Energy Mission: a general view after positive conclusion of the assessment phase", Proc. SPIE 7731, Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave, 77311L (5 August 2010); https://doi.org/10.1117/12.857103
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Cited by 6 scholarly publications.
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KEYWORDS
Digital micromirror devices

Sensors

Spectrographs

Mirrors

Near infrared

Micromirrors

Galactic astronomy

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