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Proceedings Paper

Euclid near infrared spectrophotometer instrument concept and first test results at the end of phase B
Author(s): Thierry Maciaszek; Anne Ealet; Knud Jahnke; Eric Prieto; Rémi Barbier; Yannick Mellier; Anne Costille; Franck Ducret; Christophe Fabron; Jean-Luc Gimenez; Robert Grange; Laurent Martin; Christelle Rossin; Tony Pamplona; Pascal Vola; Jean Claude Clémens; Gérard Smadja; Jérome Amiaux; Jean Christophe Barrière; Michel Berthe; Adriano De Rosa; Enrico Franceschi; Gianluca Morgante; Massimo Trifoglio; Luca Valenziano; Carlotta Bonoli; Favio Bortoletto; Maurizio D'Alessandro; Leonardo Corcione; Sebastiano Ligori; Bianca Garilli; Marco Riva; Frank Grupp; Carolin Vogel; Felix Hormuth; Gregor Seidel; Stefanie Wachter; Jose Javier Diaz; Ferran Grañena; Cristobal Padilla; Rafael Toledo; Per B. Lilje; Bjarte G. B. Solheim; Corinne Toulouse-Aastrup; Michael Andersen; Warren Holmes; Ulf Israelsson; Michael Seiffert; Carissa Weber; Augustyn Waczynski; René J. Laureijs; Giuseppe Racca; Jean-Christophe Salvignol; Paolo Strada
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Paper Abstract

The Euclid mission objective is to understand why the expansion of the Universe is accelerating by mapping the geometry of the dark Universe by investigating the distance-redshift relationship and tracing the evolution of cosmic structures. The Euclid project is part of ESA's Cosmic Vision program with its launch planned for 2020. The NISP (Near Infrared Spectro-Photometer) is one of the two Euclid instruments and is operating in the near-IR spectral region (0.9-2μm) as a photometer and spectrometer. The instrument is composed of: - a cold (135K) optomechanical subsystem consisting of a SiC structure, an optical assembly (corrector and camera lens), a filter wheel mechanism, a grism wheel mechanism, a calibration unit and a thermal control system - a detection subsystem based on a mosaic of 16 Teledyne HAWAII2RG cooled to 95K with their front-end readout electronic cooled to 140K, integrated on a mechanical focal plane structure made with Molybdenum and Aluminum. The detection subsystem is mounted on the optomechanical subsystem structure - a warm electronic subsystem (280K) composed of a data processing / detector control unit and of an instrument control unit that interfaces with the spacecraft via a 1553 bus for command and control and via Spacewire links for science data This presentation describes the architecture of the instrument at the end of the phase B (Preliminary Design Review), the expected performance, the technological key challenges and preliminary test results obtained on a detection system demonstration model.

Paper Details

Date Published: 2 August 2014
PDF: 14 pages
Proc. SPIE 9143, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, 91430K (2 August 2014); doi: 10.1117/12.2056702
Show Author Affiliations
Thierry Maciaszek, Ctr. National d'Études Spatiales (France)
Observatoire Astronomique de Marseille-Provence (France)
Anne Ealet, Ctr. de Physique des Particules de Marseille (France)
Knud Jahnke, Max-Planck-Institut für Astronomie (Germany)
Eric Prieto, Observatoire Astronomique de Marseille-Provence (France)
Rémi Barbier, Institut de Physique Nucléaire de Lyon (France)
Yannick Mellier, Institut d'Astrophysique de Paris (France)
Commissariat à l'Énergie Atomique (France)
Anne Costille, Observatoire Astronomique de Marseille-Provence (France)
Franck Ducret, Observatoire Astronomique de Marseille-Provence (France)
Christophe Fabron, Observatoire Astronomique de Marseille-Provence (France)
Jean-Luc Gimenez, Observatoire Astronomique de Marseille-Provence (France)
Robert Grange, Observatoire Astronomique de Marseille-Provence (France)
Laurent Martin, Observatoire Astronomique de Marseille-Provence (France)
Christelle Rossin, Observatoire Astronomique de Marseille-Provence (France)
Tony Pamplona, Observatoire Astronomique de Marseille-Provence (France)
Pascal Vola, Observatoire Astronomique de Marseille-Provence (France)
Jean Claude Clémens, Ctr. de Physique des Particules de Marseille (France)
Gérard Smadja, Institut de Physique Nucléaire de Lyon (France)
Jérome Amiaux, Commissariat à l'Énergie Atomique (France)
Jean Christophe Barrière, Commissariat à l'Énergie Atomique (France)
Michel Berthe, Commissariat à l'Énergie Atomique (France)
Adriano De Rosa, INAF - IASF Bologna (Italy)
Enrico Franceschi, INAF - IASF Bologna (Italy)
Gianluca Morgante, INAF - IASF Bologna (Italy)
Massimo Trifoglio, INAF - IASF Bologna (Italy)
Luca Valenziano, INAF - IASF Bologna (Italy)
Carlotta Bonoli, INAF - Osservatorio Astronomico di Padova (Italy)
Favio Bortoletto, INAF - Osservatorio Astronomico di Padova (Italy)
Maurizio D'Alessandro, INAF - Osservatorio Astronomico di Padova (Italy)
Leonardo Corcione, INAF - Osservatorio Astronomico di Torino (Italy)
Sebastiano Ligori, INAF - Osservatorio Astronomico di Torino (Italy)
Bianca Garilli, INAF - IASF Milano (Italy)
Marco Riva, INAF - IASF Milano (Italy)
Frank Grupp, Max-Planck-Institut für extraterrestrische Physik (Germany)
Carolin Vogel, Max-Planck-Institut für extraterrestrische Physik (Germany)
Felix Hormuth, Max-Planck-Institut für Astronomie (Germany)
Gregor Seidel, Max-Planck-Institut für Astronomie (Germany)
Stefanie Wachter, Max-Planck-Institut für Astronomie (Germany)
Jose Javier Diaz, Instituto de Astrofísica de Canarias (Spain)
Ferran Grañena, Institut de Física d'Altes Energies (Spain)
Cristobal Padilla, Institut de Física d'Altes Energies (Spain)
Rafael Toledo, Univ. Politécnica de Cartagena (Spain)
Per B. Lilje, Univ. of Oslo (Norway)
Bjarte G. B. Solheim, CMR Prototech (Norway)
Corinne Toulouse-Aastrup, SSC (Denmark)
Michael Andersen, Technical Univ. of Denmark (Denmark)
Warren Holmes, NASA (United States)
Ulf Israelsson, NASA (United States)
Michael Seiffert, NASA (United States)
Carissa Weber, NASA (United States)
Augustyn Waczynski, NASA (United States)
René J. Laureijs, European Space Research and Technology Ctr. (Netherlands)
Giuseppe Racca, European Space Research and Technology Ctr. (Netherlands)
Jean-Christophe Salvignol, European Space Research and Technology Ctr. (Netherlands)
Paolo Strada, European Space Research and Technology Ctr. (Netherlands)


Published in SPIE Proceedings Vol. 9143:
Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Jacobus M. Oschmann; Mark Clampin; Giovanni G. Fazio; Howard A. MacEwen, Editor(s)

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