EUCLID detector system demonstrator model: a first demonstration of the NISP detection system - CNRS - Centre national de la recherche scientifique Accéder directement au contenu
Communication Dans Un Congrès Année : 2015

EUCLID detector system demonstrator model: a first demonstration of the NISP detection system

Résumé

The detector system (DS) of Euclid NISP’s instrument (Near-Infrared Spectro-Photometer) is a matrix of 16 H2RG infrared detectors acquired simultaneously. After their characterization done at CPPM (Centre de Physique des Particules de Marseille), these detectors are integrated into a mechanical structure designed at LAM (Laboratoire d'Astronomie de Marseille) and called NI-FPA (Focal Plane Array) Before delivering the full instrument to ESA several test models have to demonstrate the performances of the detector system. The first test model, the Demonstrator Model (DM), has been integrated and tested in dedicated facilities at LAM. The aim was to validate both the integration process and the simultaneous acquisition of the detectors. Dark, noise, self-compatibility and EMC performances are presented in this paper.
Fichier non déposé

Dates et versions

hal-02144339 , version 1 (30-05-2019)

Identifiants

Citer

J.C. Clémens, B. Serra, M. Niclas, A. Ealet, W. Gillard, et al.. EUCLID detector system demonstrator model: a first demonstration of the NISP detection system. UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XIX, Aug 2015, San Diego, United States. pp.96020Y, ⟨10.1117/12.2188581⟩. ⟨hal-02144339⟩
40 Consultations
0 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More