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

ESA's Euclid 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^2. A blue grism covers the wavelength range 926--1366,nm at a spectral resolution ( of $440--900$ for a 0 diameter source with a dispersion of 1.24,nm,px^-1. Two red grisms span 1206 to 1892,nm at mathcal R =550--$740$ and a dispersion of 1.37,nm,px^-1. 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.

Authors

Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2025-10-14
DOI
https://doi.org/10.1051/0004-6361/202555859/pdf
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

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

Diego Jm, J.-L Gimenez, Pn Appleton, D.Q. Lamb et al.
Springer Link (Chiba Institute of Technology)
Astronomy and Astrophysical Research
article

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

Diego Jm, J.-L Gimenez, Pn Appleton, D.Q. Lamb, W. Hartley, J.-G. Cuby, A.R. Cooray, I.M Hook, B.R. Granett, I.T Andika, H.I Teplitz, A.M. Di Giorgio, J.E. Kajava, G.F Lesci, T.I. Liaudat, F.M. Zerbi, P.B. Lilje, P. Simon, E. Maiorano, H. Hildebrandt, T. Vassallo, Q. Le Boulc'h, L. Valenziano, M. Tenti, E. Branchini, F. Dubath, S.V.H. Haugan, L. Gabarra, W.J. Percival, D. Di Ferdinando, R. Scaramella, S. Anselmi, M. Frailis, D. Potter, S. Bardelli, N. Fourmanoit, E. Jullo, A. Calabro, C. J.-J. Barriere, G. Verza, S. Cavuoti, L. Maurin, A.M.C. Le Brun, O. Marggraf, A. Díaz-Sánchez, Y. Q. Fang, J. Lesgourgues, S. Mei, C. Porciani, M. Seiffert, E. Medinaceli, B. Gillis, H. Degaudenzi, S. Camera, S. Bruton, S.-M. Niemi, J. Martín-Fleitas, A.G. Ferrari, K. George, J.A. Schewtschenko, S. Ferriol, M. Berthe, A. Blanchard, V. Allevato, H. Dole, C. Bonoli, S. Pires, Z. Sakr, F. Courbin, L. Legrand, A. Bonchi, N. Martinet, I. Risso, P. Hudelot, S. Davini, G. Morgante, J. Weller, G. Congedo, K. Tanidis, M. Scodeggio, A. Cimatti, A. Veropalumbo, R. Farinelli, S. Hemmati, H.J. McCracken, M. Fumana, J. García-Bellido, R. da Silva, C.J. Conselice, K. Jahnke, S. Quai, D. Vergani, C. Giocoli, S. Andreon, A. Renzi, J. Gracia-Carpio, E. Romelli, A. Enia, F. Cogato, A. Balestra, R. Toledo-Moreo, L. Pozzetti, S. Nadathur, A. Pisani, A. Mora, E. Zucca, J.W. Nightingale, G. Meylan, Y. N. Wang, G. Gozaliasl, A. Gregorio, W. Gillard, M. Sahlén, G. Castignani, C.J.R. McPartland, M. Meneghetti, G. Seidel, M. Miluzio, R. Chary, B. Sartoris, G. Verdoes Kleijn, A. Troja, V. Le Brun, F. Torradeflot, N.A. Walton, S. Marcin, G. Smadja, C. C. Kirkpatrick, M. Farina, L. Moscardini, R. Barbier, J. Valiviita, B. Altieri, D. Sciotti, H.M. Courtois, F. Pasian, S. Fotopoulou, R. Massey, K. Markovic, G.D. Racca, M.L. Brown, F. Raison, E. Sellentin, P. Fosalba, M. Castellano, C. Tao, S. Matthew, M. Kunz, F. Giacomini, J. Rhodes, C. Macabiau, E. Prieto, M. Wiesmann, P.-F. Rocci, X. Dupac, A. Bonnefoi, A.N. Taylor, D. Tavagnacco, L. Leuzzi, F. Lepori, I. Tutusaus, C. Baccigalupi, V. Scottez, A. Hornstrup, C. Mancini, L. Corcione, M. Melchior, A. Pezzotta, S. Escoffier, A. Secroun, M. Magliocchetti, R. Saglia, K. Pedersen, C. Carbone, E. Sefusatti, P. Casenove, S. Wachter, F. Marulli, M. Trifoglio, G. Polenta, B. Kubik, B. Camacho Quevedo, V. Pettorino, I. Lloro, K. Naidoo, E. Keihänen, M. Bethermin, K. Paterson, A. Hall, S. Kruk, S. Dusini, D. Sapone, A. Loureiro, F. Mannucci, E. Merlin, J. Steinwagner, G. Maggio, L.A. Popa, R. Cabanac, M. Schirmer, G. Sirri, A. Cappi, J. Le Graet, H. Cho, N.R. Stickley, R. Casas, E. Rossetti, K. Kiiveri, C.M. Gutierrez, M. Lembo, D. Bertacca, A. Montoro, S. Galeotta, A. Zacchei, L.C. Smith, A. Costille, D.B. Sanders, C. Neissner, J. Hjorth, Y. Kang, L. Blot, V. Kansal, A. Da Silva, F. Caro, R. Laureijs, S. Toft, D. Maino, S. Ligori, H. Aussel, M. Radovich, Y. Copin, J. Zoubian, C. Colodro-Conde, R. Teyssier, P. Dimauro, M. Tucci, V. Gautard, H. Kurki-Suonio, A. Finoguenov, S. Paltani, M. Fabricius, C. Burigana, D. Karagiannis, W. Bon, F. Passalacqua, P. Schneider, O. Cucciati, E. Gaztanaga, F. Gianotti, J. Macias-Perez, M. Viel, P.-A. Duc, A. Franco, C. Moretti, J. Hoar, D. Le Mignant, Y. Charles, G. Leroy, F. De Paolis, P. Monaco, L. Patrizii, E. Sarpa, J.A. Escartin Vigo, G. De Lucia, J. J. Diaz, J. Clemens, V. Capobianco, G. Desprez, S. Borgani, O. Mansutti, P. Franzetti, T. Gasparetto, A.G. Sánchez, R. Kohley, F. Ducret, A. Amara, G. Cañas-Herrera, L. Zalesky, P. Battaglia, P. Liebing, M. Guidi, G. Riccio, M. Poncet, J. Carretero, M. Martinelli, F. Grupp, A. Venhola, M. Carle, E. Bozzo, M. Sereno, M. Ballardini, M. Jhabvala, D. Vibert, A. Schneider, A. Biviano, I.A. Zinchenko, M. Moresco, C. Padilla, E. Franceschi, K.C. Chambers, R.B. Metcalf, M. Pöntinen, M. Archidiacono, V. Lindholm, A.M.N. Ferguson, R.C. Nichol, L. Conversi, S. Kermiche, A. Kiessling, S. Casas, R. Maoli, S. Sacquegna, I. Tereno, N. Mauri, M. Bolzonella, W. Holmes, R. Nakajima, Y. Akrami, M. Brescia, T. Auphan, L. Guzzo, G. Testera, M. Baldi, C.J.A.P. Martins, T. Maciaszek, S. Di Domizio, C. Valieri, R. Rebolo, P. Gómez-Alvarez, M. Douspis, M. Kümmel, S. Tosi, C. Sirignano, A. Navarro-Alsina, C. Boderndorf, Y. Mellier, M. Roncarelli, S. Maurogordato, G. Zamorani, S. Conseil, F. Atrio-Barandela, A. Grazian, K. Ganga, C.S. Carvalho, P.-Y. Chabaud, T. Schrabback, R. Bender, N. Aghanim, H. Hoekstra, N. Auricchio, P. Tallada-Crespí, L. Stanco, C. Hernández-Monteagudo, T. Castro, G. Mainetti, F. Hormuth, S.J. Liu, J. Brinchmann
article en

Abstract

ESA's Euclid 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^2. A blue grism covers the wavelength range 926--1366,nm at a spectral resolution ( of $440--900$ for a 0 diameter source with a dispersion of 1.24,nm,px^-1. Two red grisms span 1206 to 1892,nm at mathcal R =550--$740$ and a dispersion of 1.37,nm,px^-1. 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.

Springer Link (Chiba Institute of Technology)
Openalex Percentile: Top 30%
Astronomy and Astrophysical Research
DOISourceOpenAlex
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.