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• W2022170642 abstract "The Euclid mission objective is to understand why the expansion of the Universe is accelerating by mapping the geometry of the dark Universe byinvestigating the distance-redshift relationship and tracing the evolution of cosmic structures. The Euclid project is part of ESA's Cosmic Visionprogram 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 aphotometer 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, agrism 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 optomechanicalsubsystem structure- a warm electronic subsystem (280K) composed of a data processing / detector control unit and of an instrument control unit that interfaces with thespacecraft via a 1553 bus for command and control and via Spacewire links for science dataThis presentation describes the architecture of the instrument at the end of the phase B (Preliminary Design Review), the expected performance, thetechnological key challenges and preliminary test results obtained on a detection system demonstration model." @default.
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• W2022170642 date "2014-08-02" @default.
• W2022170642 modified "2023-10-11" @default.
• W2022170642 title "Euclid near infrared spectrophotometer instrument concept and first test results at the end of phase B" @default.
• W2022170642 cites W2034016787 @default.
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• W2022170642 doi "https://doi.org/10.1117/12.2056702" @default.
• W2022170642 hasPublicationYear "2014" @default.
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