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Euclid preparation. LXXX. Overview of Euclid infrared detector performance from ground tests

  • B. Kubik*
  • , R. Barbier
  • , J. Clemens
  • , S. Ferriol
  • , A. Secroun
  • , G. Smadja
  • , W. Gillard
  • , N. Fourmanoit
  • , A. Ealet
  • , S. Conseil
  • , J. Zoubian
  • , R. Kohley
  • , J. C. Salvignol
  • , L. Conversi
  • , T. Maciaszek
  • , H. Cho
  • , W. Holmes
  • , M. Seiffert
  • , A. Waczynski
  • , S. Wachter
  • K. Jahnke, F. Grupp, C. Bonoli, L. Corcione, S. Dusini, E. Medinaceli, R. Laureijs, G. D. Racca, A. Bonnefoi, M. Carle, A. Costille, F. Ducret, J. L. Gimenez, D. Le Mignant, L. Martin, L. Caillat, L. Valenziano, N. Auricchio, P. Battaglia, A. Derosa, R. Farinelli, F. Cogato, G. Morgante, M. Trifoglio, V. Capobianco, S. Ligori, E. Borsato, C. Sirignano, L. Stanco, S. Ventura, R. Toledo-Moreo, L. Patrizii, Y. Copin, R. Foltz, E. Prieto, N. Aghanim, B. Altieri, S. Andreon, C. Baccigalupi, M. Baldi, A. Balestra, S. Bardelli, F. Bernardeau, A. Biviano, A. Bonchi, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, G. Cañas-Herrera, C. Carbone, J. Carretero, S. Casas, F. J. Castander, M. Castellano, G. Castignani, S. Cavuoti, K. C. Chambers, A. Cimatti, C. Colodro-Conde, G. Congedo, C. J. Conselice, F. Courbin, H. M. Courtois, A. Da Silva, R. Da Silva, H. Degaudenzi, G. De Lucia, A. M. Di Giorgio, H. Dole, M. Douspis, F. Dubath, C. A.J. Duncan, X. Dupac, S. Escoffier, M. Farina, F. Faustini, F. Finelli, S. Fotopoulou, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, B. Gillis, C. Giocoli, J. Gracia-Carpio, B. R. Granett, A. Grazian, L. Guzzo, S. V.H. Haugan, J. Hoar, H. Hoekstra, I. M. Hook, F. Hormuth, A. Hornstrup, P. Hudelot, M. Jhabvala, E. Keihänen, S. Kermiche, A. Kiessling, M. Kümmel, M. Kunz, H. Kurki-Suonio, Q. Le Boulc'h, A. M.C. Le Brun, P. Liebing, P. B. Lilje, V. Lindholm, I. Lloro, G. Mainetti, D. Maino, E. Maiorano, O. Mansutti, S. Marcin, O. Marggraf, M. Martinelli, N. Martinet, F. Marulli, R. Massey, S. Maurogordato, H. J. Mccracken, S. Mei, M. Melchior, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, A. Mora, M. Moresco, P. W. Morris, L. Moscardini, R. Nakajima, C. Neissner, R. C. Nichol, S. M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W. J. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. A. Popa, L. Pozzetti, F. Raison, R. Rebolo, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, R. Saglia, Z. Sakr, D. Sapone, B. Sartoris, J. A. Schewtschenko, M. Schirmer, P. Schneider, T. Schrabback, M. Scodeggio, E. Sefusatti, G. Seidel, S. Serrano, P. Simon, G. Sirri, J. Steinwagner, P. Tallada-Crespí, D. Tavagnacco, A. N. Taylor, H. I. Teplitz, I. Tereno, S. Toft, F. Torradeflot, A. Tsyganov, I. Tutusaus, J. Valiviita, T. Vassallo, G. Verdoes Kleijn, A. Veropalumbo, Y. Wang, J. Weller, A. Zacchei, G. Zamorani, F. M. Zerbi, E. Zucca, V. Allevato, M. Ballardini, M. Bolzonella, E. Bozzo, C. Burigana, R. Cabanac, A. Cappi, P. Casenove, D. Di Ferdinando, J. A. Escartin Vigo, L. Gabarra, W. G. Hartley, J. Martín-Fleitas, S. Matthew, N. Mauri, R. B. Metcalf, A. Pezzotta, M. Pöntinen, C. Porciani, I. Risso, V. Scottez, M. Sereno, M. Tenti, M. Viel, M. Wiesmann, Y. Akrami, I. T. Andika, S. Anselmi, M. Archidiacono, F. Atrio-Barandela, D. Bertacca, M. Bethermin, A. Blanchard, L. Blot, S. Borgani, M. L. Brown, S. Bruton, A. Calabro, B. Camacho Quevedo, F. Caro, C. S. Carvalho, T. Castro, Y. Charles, R. Chary, A. R. Cooray, O. Cucciati, S. Davini, F. De Paolis, G. Desprez, A. Díaz-Sánchez, S. Di Domizio, J. M. Diego, P. Dimauro, A. Enia, Y. Fang, A. M.N. Ferguson, A. G. Ferrari, A. Finoguenov, A. Fontana, A. Franco, K. Ganga, J. García-Bellido, T. Gasparetto, V. Gautard, E. Gaztanaga, F. Giacomini, F. Gianotti, G. Gozaliasl, M. Guidi, C. M. Gutierrez, A. Hall, H. Hildebrandt, J. Hjorth, J. J.E. Kajava, Y. Kang, V. Kansal, D. Karagiannis, K. Kiiveri, C. C. Kirkpatrick, S. Kruk, J. Le Graet, L. Legrand, M. Lembo, F. Lepori, G. Leroy, G. F. Lesci, J. Lesgourgues, L. Leuzzi, T. I. Liaudat, A. Loureiro, J. Macias-Perez, G. Maggio, M. Magliocchetti, C. Mancini, F. Mannucci, R. Maoli, C. J.A.P. Martins, L. Maurin, M. Miluzio, P. Monaco, A. Montoro, C. Moretti, C. Murray, S. Nadathur, K. Naidoo, A. Navarro-Alsina, F. Passalacqua, K. Paterson, A. Pisani, D. Potter, S. Quai, M. Radovich, P. F. Rocci, S. Sacquegna, M. Sahlén, D. B. Sanders, E. Sarpa, A. Schneider, D. Sciotti, E. Sellentin, G. Setnikar, L. C. Smith, K. Tanidis, C. Tao, G. Testera, R. Teyssier, S. Tosi, A. Troja, M. Tucci, C. Valieri, A. Venhola, D. Vergani, G. Verza, J. R. Weaver, L. Zalesky
*Corresponding author for this work
  • Universite Claude Bernard Lyon 1
  • CNRS
  • European Space Astronomy Centre
  • ESTEC
  • Centre national d'études spatiales
  • California Institute of Technology
  • NASA Goddard Space Flight Center
  • Carnegie Institution of Washington
  • Max Planck Institute for Astronomy
  • Ludwig Maximilian University of Munich
  • Astronomical Observatory of Padua
  • National Institute for Astrophysics
  • National Institute for Nuclear Physics
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Leiden University
  • University of Bologna
  • University of Padua
  • Technical University of Cartagena
  • Université Paris-Sud
  • Osservatorio Astronomico di Brera
  • University of Trieste
  • Institut d’Astrophysique de Paris
  • Osservatorio Astronomico di Trieste
  • Italian Space Agency
  • Osservatorio Astronomico di Capodimonte
  • University of Porto
  • Port d’Informació Científica
  • RWTH Aachen University
  • Institute of Space Studies of Catalonia
  • Osservatorio Astronomico Roma
  • University of Hawai'i at Mānoa
  • Instituto de Astrofísica de Canarias
  • University of Edinburgh
  • University of Manchester
  • ICREA
  • Institut national de physique nucléaire et de physique des particules
  • University of Lisbon
  • University of Geneva
  • University of Bristol
  • Max Planck Institute for Extraterrestrial Physics
  • University of Milan
  • University of Oslo
  • Lancaster University
  • Felix Hormuth Engineering
  • University of Helsinki
  • Observatoire de Paris
  • University College London
  • SKA Organisation
  • University of Applied Sciences Northwestern Switzerland
  • University of Bonn
  • Durham University
  • Université Côte d'Azur
  • Centre Pierre Binétruy
  • Swiss Federal Institute of Technology Lausanne
  • European Space Agency - ESA
  • Institute for High Energy Physics
  • University of Surrey
  • University of Copenhagen
  • University of Waterloo
  • French Alternative Energies and Atomic Energy Commission
  • Institute of Space Science
  • University of La Laguna
  • Heidelberg University 
  • Universidad de Chile
  • University of Innsbruck
  • CSIC - Institute of Space Sciences
  • Cosmic Dawn Center
  • CIEMAT
  • University of Groningen
  • Université de Toulouse
  • University of Ferrara
  • University of Oxford
  • Université catholique de Lille
  • Case Western Reserve University
  • Technical University of Munich
  • Universidad de Salamanca
  • Université de Strasbourg
  • ICSC - Centro Nazionale di Ricerca in High Performance Computing
  • University of California at Irvine
  • University of Salento
  • University of Genoa
  • CSIC-UC - Institute of Physics of Cantabria
  • Université Paris 7
  • CSIC-UAM - Institute of Theoretical Physics
  • Institut de recherche sur les lois fondamentales de l'Univers
  • University of Portsmouth
  • Ruhr University Bochum
  • University of Turku
  • Swinburne University of Technology
  • University of the Western Cape
  • University of Cambridge
  • University of Zurich
  • Université Paris-Saclay
  • Imperial College London
  • Université Grenoble Alpes
  • Osservatorio Astrofisico Di Arcetri, Florence
  • University of Rome La Sapienza
  • Uppsala University
  • Princeton University
  • University of Oulu
  • Simons Foundation
  • University of Massachusetts

Research output: Contribution to journal › Journal article › Research › peer-review

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Abstract

This paper describes the objectives, design, and findings of the pre-launch ground characterisation campaigns of the Euclid infrared detectors. The aim of the ground characterisations is to evaluate the performance of the detectors, to calibrate the pixel response, and to derive the pixel response correction methods. The detectors have been tested and characterised in the facilities set up for this purpose. The pixel properties, including baseline, bad pixels, quantum efficiency, inter pixel capacitance, quantum efficiency, dark current, readout noise, conversion gain, response non-linearity, and image persistence were measured and characterised for each pixel. We describe in detail the test flow definition that allows us to derive the pixel properties and we present the data acquisition and data quality check software implemented for this purpose. We also outline the measurement protocols of all the pixel properties presented and we provide a comprehensive overview of the performance of the Euclid infrared detectors as derived after tuning the operating parameters of the detectors. The main conclusion of this work is that the performance of the infrared detectors Euclid meets the requirements. Pixels classified as non-functioning accounted for less than 0.2% of all science pixels. The interpixel capacitance (IPC) coupling is minimal, the cross-talk between adjacent pixels is less than 1% between adjacent pixels, and 95% of the pixels show a quantum efficienty (QE) greater than 80% across the entire spectral range of the Euclid mission. The conversion gain is approximately 0.52 ADU/e-, with a variation of less than 1% between channels of the same detector. The reset noise is approximately equal to 23 ADU rms after reference pixel correction. The readout noise of a single frame is approximately 13 e- rms while the signal estimator noise is measured at 7 e- rms in photometric mode and 9 e- rms in spectroscopic acquisition mode. The deviation from linear response at signal levels up to 80 ke- is less than 5% for 95% of the pixels. Median persistence amplitudes are less than 0.3% of the signal, though persistence exhibits significant spatial variation and differences between detectors.

Original languageEnglish
Article numberA230
JournalAstronomy and Astrophysics
Volume707
Number of pages25
ISSN0004-6361
DOIs
Publication statusPublished - 2026

Keywords

  • Instrumentation: detectors
  • Methods: data analysis
  • Space vehicles: instruments

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