학술논문
Euclid. IV. The NISP Calibration Unit
Document Type
Working Paper
Author
Euclid Collaboration; Hormuth, F.; Jahnke, K.; Schirmer, M.; Lee, C. G. -Y.; Scott, T.; Barbier, R.; Ferriol, S.; Gillard, W.; Grupp, F.; Holmes, R.; Holmes, W.; Kubik, B.; Macias-Perez, J.; Laurent, M.; Marpaud, J.; Marton, M.; Medinaceli, E.; Morgante, G.; Toledo-Moreo, R.; Trifoglio, M.; Rix, Hans-Walter; Secroun, A.; Seiffert, M.; Stassi, P.; Wachter, S.; Gutierrez, C. M.; Vescovi, C.; Amara, A.; Andreon, S.; Auricchio, N.; Baldi, M.; Balestra, A.; Bardelli, S.; Battaglia, P.; Bender, R.; Bodendorf, C.; Bonino, D.; Branchini, E.; Brescia, M.; Brinchmann, J.; Camera, S.; Capobianco, V.; Carbone, C.; Cardone, V. F.; Carretero, J.; Casas, R.; Casas, S.; Castellano, M.; Cavuoti, S.; Cimatti, A.; Congedo, G.; Conselice, C. J.; Conversi, L.; Copin, Y.; Corcione, L.; Courbin, F.; Courtois, H. M.; Da Silva, A.; Degaudenzi, H.; Dinis, J.; Douspis, M.; Dubath, F.; Ducret, F.; Dupac, X.; Dusini, S.; Fabricius, M.; Farina, M.; Farrens, S.; Faustini, F.; Fotopoulou, S.; Fourmanoit, N.; Frailis, M.; Franceschi, E.; Franzetti, P.; Fumana, M.; Galeotta, S.; Garilli, B.; Gillis, B.; Giocoli, C.; Grazian, A.; Guzzo, L.; Haugan, S. V. H.; Hoekstra, H.; Hook, I.; Hornstrup, A.; Hudelot, P.; Jhabvala, M.; Keihänen, E.; Kermiche, S.; Kiessling, A.; Kilbinger, M.; Kitching, T.; Kohley, R.; Kümmel, M.; Kunz, M.; Kurki-Suonio, H.; Mignant, D. Le; Ligori, S.; Lilje, P. B.; Lindholm, V.; Lloro, I.; Maiorano, E.; Mansutti, O.; Marggraf, O.; Markovic, K.; Martinet, N.; Marulli, F.; Massey, R.; Maurogordato, S.; McCracken, H. J.; Mei, S.; Melchior, M.; Mellier, Y.; Meneghetti, M.; Merlin, E.; Meylan, G.; Mohr, J. J.; Moresco, M.; Moscardini, L.; Munari, E.; Nakajima, R.; Nichol, R. C.; Niemi, S. -M.; Nightingale, J. W.; Padilla, C.; Paech, K.; Paltani, S.; Pasian, F.; Pedersen, K.; Percival, W. J.; Pettorino, V.; Pires, S.; Polenta, G.; Poncet, M.; Popa, L. A.; Raison, F.; Rebolo, R.; Renzi, A.; Rhodes, J.; Riccio, G.; Romelli, E.; Roncarelli, M.; Rossetti, E.; Saglia, R.; Sapone, D.; Sartoris, B.; Sauvage, M.; Schneider, P.; Schrabback, T.; Seidel, G.; Serrano, S.; Sirignano, C.; Sirri, G.; Smadja, G.; Stanco, L.; Tallada-Crespí, P.; Tavagnacco, D.; Taylor, A. N.; Teplitz, H. I.; Tereno, I.; Torradeflot, F.; Tutusaus, I.; Valenziano, L.; Vassallo, T.; Veropalumbo, A.; Wang, Y.; Weller, J.; Zacchei, A.; Zamorani, G.; Zerbi, F. M.; Zucca, E.; Biviano, A.; Bolzonella, M.; Boucaud, A.; Bozzo, E.; Burigana, C.; Calabrese, M.; Colodro-Conde, C.; De Lucia, G.; Di Ferdinando, D.; Vigo, J. A. Escartin; Farinelli, R.; George, K.; Gracia-Carpio, J.; Kazandjian, M. V.; Mainetti, G.; Marcin, S.; Martinelli, M.; Mauri, N.; Morris, P. W.; Neissner, C.; Sakr, Z.; Scottez, V.; Tenti, M.; Viel, M.; Wiesmann, M.; Akrami, Y.; Allevato, V.; Anselmi, S.; Aubourg, E.; Baccigalupi, C.; Ballardini, M.; Bethermin, M.; Blanchard, A.; Blot, L.; Borgani, S.; Borlaff, A. S.; Borsato, E.; Bruton, S.; Cabanac, R.; Calabro, A.; Canas-Herrera, G.; Cappi, A.; Carvalho, C. S.; Casenove, P.; Castignani, G.; Castro, T.; Chambers, K. C.; Charles, Y.; Contarini, S.; Cooray, A. R.; Cucciati, O.; Davini, S.; De Caro, B.; de la Torre, S.; Desprez, G.; Díaz-Sánchez, A.; Diaz, J. J.; Di Domizio, S.; Dole, H.; Escoffier, S.; Ferrari, A. G.; Ferreira, P. G.; Ferrero, I.; Finelli, F.; Fontana, A.; Fornari, F.; Gabarra, L.; Ganga, K.; García-Bellido, J.; Gaztanaga, E.; Giacomini, F.; Gozaliasl, G.; Hall, A.; Hartley, W. G.; Hildebrandt, H.; Hjorth, J.; Huertas-Company, M.; Ilbert, O.; Jacobson, J.; Muñoz, A. Jimenez; Joudaki, S.; Kajava, J. J. E.; Kansal, V.; Karagiannis, D.; Kirkpatrick, C. C.; Laudisio, F.; Legrand, L.; Libet, G.; Loureiro, A.; Maggio, G.; Magliocchetti, M.; Mancini, C.; Mannucci, F.; Maoli, R.; Martins, C. J. A. P.; Matthew, S.; Maurin, L.; Metcalf, R. B.; Miluzio, M.; Moretti, C.; Nadathur, S.; Walton, Nicholas A.; Patrizii, L.; Pezzotta, A.; Pöntinen, M.; Popa, V.; Porciani, C.; Potter, D.; Risso, I.; Rocci, P. -F.; Rollins, R. P.; Rusholme, B.; Sahlén, M.; Sánchez, A. G.; Scarlata, C.; Schewtschenko, J. A.; Schneider, A.; Schultheis, M.; Sefusatti, E.; Sereno, M.; Shulevski, A.; Silvestri, A.; Simon, P.; Mancini, A. Spurio; Stadel, J.; Steinwagner, J.; Tao, C.; Testera, G.; Teyssier, R.; Toft, S.; Tosi, S.; Troja, A.; Tucci, M.; Valieri, C.; Valiviita, J.; Vergani, D.; Verza, G.; Zalesky, L.; Archidiacono, M.; Atrio-Barandela, F.; Bouvard, T.; Caro, F.; Dimauro, P.; Fang, Y.; Ferguson, A. M. N.; Finoguenov, A.; Gasparetto, T.; Brun, A. M. C. Le; Graet, J. Le; Liaudat, T. I.; Montoro, A.; Murray, C.; Oguri, M.; Pagano, L.; Paoletti, D.; Sarpa, E.; Tanidis, K.; Vernizzi, F.; Viitanen, A.; Kova{č}ić, I.; Lesgourgues, J.; Martín-Fleitas, J.; Mora, A.
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Abstract
The near-infrared calibration unit (NI-CU) onboard Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. Euclid is a mission in ESA's 'Cosmic Vision 2015-2025' framework, to explore the dark universe and provide a next-level characterisation of the nature of gravitation, dark matter, and dark energy. Calibrating photometric and spectrometric measurements of galaxies to better than 1.5% accuracy in a survey homogeneously mapping ~14000 deg^2 of extragalactic sky requires a very detailed characterisation of near-infrared (NIR) detector properties, as well their constant monitoring in flight. To cover two of the main contributions - relative pixel-to-pixel sensitivity and non-linearity characteristics - as well as support other calibration activities, NI-CU was designed to provide spatially approximately homogeneous (<12% variations) and temporally stable illumination (0.1%-0.2% over 1200s) over the NISP detector plane, with minimal power consumption and energy dissipation. NI-CU is covers the spectral range ~[900,1900] nm - at cryo-operating temperature - at 5 fixed independent wavelengths to capture wavelength-dependent behaviour of the detectors, with fluence over a dynamic range of >=100 from ~15 ph s^-1 pixel^-1 to >1500 ph s^-1 pixel^-1. For this functionality, NI-CU is based on LEDs. We describe the rationale behind the decision and design process, describe the challenges in sourcing the right LEDs, as well as the qualification process and lessons learned. We also provide a description of the completed NI-CU, its capabilities and performance as well as its limits. NI-CU has been integrated into NISP and the Euclid satellite, and since Euclid's launch in July 2023 has started supporting survey operations.
Comment: Paper submitted as part of the A&A special issue 'Euclid on Sky', which contains Euclid key reference papers and first results from the Euclid Early Release Observations
Comment: Paper submitted as part of the A&A special issue 'Euclid on Sky', which contains Euclid key reference papers and first results from the Euclid Early Release Observations