Instrument workstation for the EGSE of the Near Infrared Spectro-Photometer instrument (NISP) of the EUCLID mission

M. Trifoglio; F. Gianotti; V. Conforti; E. Franceschi; J. B. Stephen; A. Bulgarelli; V. Fioretti; E. Maiorano; L. Nicastro; L. Valenziano; A. Zoli; N. Auricchio; A. Balestra; D. Bonino; C. Bonoli; F. Bortoletto; V. Capobianco; T. Chiarusi; L. Corcione; S. Debei; A. De Rosa; S. Dusini; F. Fornari; F. Giacomini; G. P. Guizzo; S. Ligori; A. Margiotta; N. Mauri; E. Medinaceli; G. Morgante; L. Patrizii; C. Sirignano; G. Sirri; F. Sortino; L. Stanco; M. Tenti

doi:10.1117/12.2234219

29 July 2016 Instrument workstation for the EGSE of the Near Infrared Spectro-Photometer instrument (NISP) of the EUCLID mission

M. Trifoglio, F. Gianotti, V. Conforti, E. Franceschi, J. B. Stephen, A. Bulgarelli, V. Fioretti, E. Maiorano, L. Nicastro, L. Valenziano, A. Zoli, N. Auricchio, A. Balestra, D. Bonino, C. Bonoli, F. Bortoletto, V. Capobianco, T. Chiarusi, L. Corcione, S. Debei, A. De Rosa, S. Dusini, F. Fornari, F. Giacomini, G. P. Guizzo, S. Ligori, A. Margiotta, N. Mauri, E. Medinaceli, G. Morgante, L. Patrizii, C. Sirignano, G. Sirri, F. Sortino, L. Stanco, M. Tenti

Author Affiliations +

Proceedings Volume 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave; 990460 (2016) https://doi.org/10.1117/12.2234219
Event: SPIE Astronomical Telescopes + Instrumentation, 2016, Edinburgh, United Kingdom

Abstract

The NISP instrument on board the Euclid ESA mission will be developed and tested at different levels of integration using various test equipment which shall be designed and procured through a collaborative and coordinated effort. The NISP Instrument Workstation (NI-IWS) will be part of the EGSE configuration that will support the NISP AIV/AIT activities from the NISP Warm Electronics level up to the launch of Euclid. One workstation is required for the NISP EQM/AVM, and a second one for the NISP FM. Each workstation will follow the respective NISP model after delivery to ESA for Payload and Satellite AIV/AIT and launch. At these levels the NI-IWS shall be configured as part of the Payload EGSE, the System EGSE, and the Launch EGSE, respectively. After launch, the NI-IWS will be also re-used in the Euclid Ground Segment in order to support the Commissioning and Performance Verification (CPV) phase, and for troubleshooting purposes during the operational phase. The NI-IWS is mainly aimed at the local storage in a suitable format of the NISP instrument data and metadata, at local retrieval, processing and display of the stored data for on-line instrument assessment, and at the remote retrieval of the stored data for off-line analysis on other computers. We describe the design of the IWS software that will create a suitable interface to the external systems in each of the various configurations envisaged at the different levels, and provide the capabilities required to monitor and verify the instrument functionalities and performance throughout all phases of the NISP lifetime.

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M. Trifoglio, F. Gianotti, V. Conforti, E. Franceschi, J. B. Stephen, A. Bulgarelli, V. Fioretti, E. Maiorano, L. Nicastro, L. Valenziano, A. Zoli, N. Auricchio, A. Balestra, D. Bonino, C. Bonoli, F. Bortoletto, V. Capobianco, T. Chiarusi, L. Corcione, S. Debei, A. De Rosa, S. Dusini, F. Fornari, F. Giacomini, G. P. Guizzo, S. Ligori, A. Margiotta, N. Mauri, E. Medinaceli, G. Morgante, L. Patrizii, C. Sirignano, G. Sirri, F. Sortino, L. Stanco, and M. Tenti "Instrument workstation for the EGSE of the Near Infrared Spectro-Photometer instrument (NISP) of the EUCLID mission", Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 990460 (29 July 2016); https://doi.org/10.1117/12.2234219

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