EUCLID's near infrared spectro-photometer ready for flight: review of final performances
- Medinaceli, E.
- Valenziano, L.
- Auricchio, N.
- Franceschi, E.
- Gianotti, F.
- Battaglia, P.
- Farinelli, R.
- Balestra, A.
- Dusini, S.
- Sirignano, C.
- Borsato, E.
- Stanco, L.
- Renzi, A.
- Troja, A.
- Gabarra, L.
- Ligori, S.
- Capobianco, V.
- Corcione, L.
- Bonino, D.
- Sirri, G.
- Patrizii, L.
- Tenti, M.
- Di Ferdinando, D.
- Valieri, C.
- Mauri, N.
- Giacomini, F.
- Le Mignant, D.
- Prieto, E.
- Carle, M.
- Ducret, F.
- Gillard, W.
- Secroun, A.
- Maciaszek, T.
- Ferriol, S.
- Barbier, R.
- Grupp, F.
- Holmes, W.
- Pniel, M.
- Waczynski, A.
- Prado, S.
- Seiffert, M.
- Jhabvala, M.
- Laureijs, R.
- Racca, G.
- Salvignol, J.C.
- Boenke, T.
- Strada, P.
DOIAbstract
International audienceSA’s mission Euclid while undertaking its final integration stage is fully qualified. Euclid will perform an extra galactic survey (0<z<2) using visible and near-infrared light. To detect the infrared radiation is equipped with the Near Infrared Spectro-Photometer (NISP) instrument with a sensitivity in the 0.9-2 μm range. We present an illustration of the NISP Data Processing Unit’s Application Software, highlighting the experimental process to obtain the final parametrization of the on-board processing of data produced by an array of 16 Teledyne’s HAWAII-2RG (HgCdTe) - each of 2048×2048 px2, 0.3 arcsec/px, 18 μm pixel pitch; using data from the latest test campaigns done with the flight configuration hardware - compl...
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