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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 3 CONTRIBUTI IN ATTI DI CONVEGNO (Proceedings)
  4. 3.01 Contributi in Atti di convegno
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/26307
Title: Instrument workstation for the EGSE of the Near Infrared Spectro-Photometer instrument (NISP) of the EUCLID mission
Authors: Trifoglio, M. 
Gianotti, F. 
CONFORTI, Vito 
FRANCESCHI, ENRICO 
STEPHEN, JOHN BUCHAN 
BULGARELLI, ANDREA 
FIORETTI, VALENTINA 
MAIORANO, Elisabetta 
NICASTRO, LUCIANO 
VALENZIANO, LUCA 
Zoli, A.
Auricchio, N. 
BALESTRA, Andrea 
BONINO, Donata 
Bonoli, C.
Bortoletto, F.
Capobianco, Vito 
Chiarusi, T.
CORCIONE, Leonardo 
Debei, S.
DE ROSA, ADRIANO GIUSEPPE 
Dusini, S.
Fornari, F.
Giacomini, F.
Guizzo, G. P.
LIGORI, Sebastiano 
Margiotta, A.
Mauri, N.
Medinaceli, E.
MORGANTE, GIANLUCA 
Patrizii, L.
Sirignano, C.
Sirri, G.
Sortino, F. 
Stanco, L.
Tenti, M.
Issue Date: 2016
Volume: Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave
Editors: MacEwen, Howard A.; Fazio, Giovanni G.; Lystrup, Makenzie; Batalha, Natalie; Siegler, Nicholas; Tong, Edward C.
Series: PROCEEDINGS OF SPIE 
Number: 9904
First Page: 990460
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.
Conference Name: Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave
Conference Place: Edinburgh, United Kingdom
Conference Date: 26 June - 1 July 2016
URI: http://hdl.handle.net/20.500.12386/26307
URL: https://www.spiedigitallibrary.org/conference-proceedings-of-spie/9904/1/Instrument-workstation-for-the-EGSE-of-the-Near-Infrared-Spectro/10.1117/12.2234219.full
ISSN: 0277-786X
ISBN: 9781510601871
DOI: 10.1117/12.2234219
Bibcode ADS: 2016SPIE.9904E..60T
Fulltext: open
Appears in Collections:3.01 Contributi in Atti di convegno

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