Euclid preparation: LXXVII. The NISP spectroscopy channel: Ground performance and calibration

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dc.contributor.authorSacquegna, S.
dc.contributor.authorSahlen, M.
dc.contributor.authorSanders, D. B.
dc.contributor.authorSarpa, E.
dc.contributor.authorSchneider, A.
dc.contributor.authorSciotti, D.
dc.contributor.authorSellentin, E.
dc.contributor.authorSmith, L. C.
dc.contributor.authorTanidis, K.
dc.contributor.authorTao, C.
dc.contributor.authorTestera, G.
dc.contributor.authorTeyssier, R.
dc.contributor.authorTosi, S.
dc.contributor.authorTroja, A.
dc.contributor.authorTucci, M.
dc.contributor.authorValieri, C.
dc.contributor.authorVenhola, A.
dc.contributor.authorVergani, D.
dc.contributor.authorVerza, G.
dc.contributor.authorWalton, N. A.
dc.contributor.authorZalesky, L.
dc.contributor.authorEuclid Collaboration
dc.contributor.organizationfi=Tuorlan observatorio|en=Tuorla Observatory|
dc.contributor.organization-code1.2.246.10.2458963.20.90670098848
dc.converis.publication-id523279629
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/523279629
dc.date.accessioned2026-05-13T20:11:19Z
dc.description.abstract<p>ESA’s <em>Euclid</em> cosmology mission relies on the very sensitive and accurately calibrated spectroscopy channel of the Near-Infrared Spectrometer and Photometer (NISP). With three operational grisms in two wavelength intervals, NISP provides diffraction-limited slitless spectroscopy over a field of 0.57 deg<sup>2</sup>. A blue grism, <em>BG</em><sub>E</sub>, covers the wavelength range 926–1366 nm at a spectral resolution (ℛ) of 440–900 for a 0.″5 diameter source with a dispersion of 1.24 nm px<sup>−1</sup>. Two red grisms, <em>RG</em><sub>E</sub>, span 1206 to 1892 nm at ℛ = 550–740 and a dispersion of 1.37 nm px<sup>−1</sup>. We describe the construction of the grisms as well as the ground testing of the flight model of the NISP instrument, where these properties were established.</p><p>Key words: instrumentation: spectrographs / space vehicles: instruments / techniques: imaging spectroscopy / techniques: spectroscopic / cosmology: observations</p><p><strong>Publisher note:</strong> The article number in this series contained a typo. The Roman numeral in the subtitle was corrected on 25 March 2026.</p>
dc.identifier.eissn1432-0746
dc.identifier.jour-issn0004-6361
dc.identifier.urihttps://www.utupub.fi/handle/11111/60642
dc.identifier.urlhttps://doi.org/10.1051/0004-6361/202555859
dc.identifier.urnURN:NBN:fi-fe2026051143084
dc.language.isoen
dc.okm.affiliatedauthorKajava, Jari
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherEDP Sciences
dc.publisher.countryFranceen_GB
dc.publisher.countryRanskafi_FI
dc.publisher.country-codeFR
dc.relation.articlenumberA227
dc.relation.doi10.1051/0004-6361/202555859
dc.relation.ispartofjournalAstronomy and Astrophysics
dc.relation.volume707
dc.titleEuclid preparation: LXXVII. The NISP spectroscopy channel: Ground performance and calibration
dc.year.issued2026

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