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. J.
- Racca G.
- Salvignol J. C.
- Boenke T.
- Strada P.
DOIAbstract
ESA's mission Euclid while undertaking its final integration stage is fully qualified. Euclid will perform an extra galactic survey (0<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 - complete optical system (Kor...
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