{"paper":{"title":"Euclid Near Infrared Spectrometer and Photometer instrument flight model presentation, performance and ground calibration results summary","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Balestra, A. Bonnefoi, A. Caillat, A. Costille, A. De Rosa, A. Ealet, A. Hornstrup, A. Margiotta, A. Secroun, A. S{\\o}rensen, A. Waczynski, B. Foulon, B. Kubik, C. Bonoli, C. Colodro-Conde, C. Fabron, C. Padilla, C. Sirignano, C. Thizy, D. Le Mignant, D. Liz\\'an, D. Penka, E. Borsato, E. Franceschi, E. Grassi, E. Medinaceli, E. Prieto, F. Bortoletto, F. Dal Corso, F. Ducret, F. Fornari, F. Giacomini, F. Grupp, F. Hormuth, F. Laudisio, F. Sortino, G. Morgante, G. Racca, G. Seidel, G. Sirri, I. Lloro, J. Andersen, J. C. Barri\\`ere, J. C. Cl\\'emens, J. C. Salvignol, J. Fontigne, J. Gomez, J. J. Diaz, J. L. Gimenez, J. Steinwagner, K. Jahnke, L. Caillat, L. Corcione, L. Martin, L. Pasqualini, L. Patrizii, L. Stanco, L. Valenziano, M. Berthe, M. Carle, M. D'Alessandro, M. I. Andersen, M. Jaquet, M. Jhabvala, M. Niclas, M. Pniel, M. Schirmer, M. Seiffert, M. Spurio, M. Tenti, M. Trifoglio, N. Auricchio, N. C. Jessen, N. Mauri, P. Battaglia, P. B. Lilje, P. Sanchez, P. Strada, R. Barbier, R. Casas, R. Farinelli, R. J. Laureijs, R. Toledo-Moreo, R. Travaglini, S. Dusini, S. Ferriol, S. Ligori, S. Pravdo, S. Ventura, T. Boenke, T. Chiarusi, T. Maciaszek, T. Pamplona, V. Capobianco, W. Bon, W. Gillard, W. Holmes, Y. Mellier (on behalf of the Euclid Consortium)","submitted_at":"2022-10-18T19:18:55Z","abstract_excerpt":"The NISP (Near Infrared Spectrometer and Photometer) is one of the two Euclid instruments. It operates in the near-IR spectral region (950-2020nm) as a photometer and spectrometer. The instrument is composed of: a cold (135 K) optomechanical subsystem consisting of a Silicon carbide structure, an optical assembly, a filter wheel mechanism, a grism wheel mechanism, a calibration unit, and a thermal control system, a detection system based on a mosaic of 16 H2RG with their front-end readout electronic, and a warm electronic system (290 K) composed of a data processing / detector control unit and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.10112","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2210.10112/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}