Euclid Near Infrared Spectrometer and Photometer instrument concept and first test results obtained for different breadboards models at the end of phase C

Thierry Maciaszek; Anne Ealet; Knud Jahnke; Eric Prieto; Yannick Mellier; William Bon; Anne Bonefoi; Michael Carle; Amandine Caillat; Anne Costille; Doriane Dormoy; Franck Ducret; Christophe Fabron; Aurélien Febvre; Benjamin Foulon; José Garrido Garcia; Jean Luc Gimenez; Emmanuel Grassi; David Le Mignant; Tony Pamplona; Patrice Sanchez; William Gillard; Mathieu Niclas; Aurélia Secroun; Bogna Kubik; Jérome Amiaux; Jean Christophe Barrière; Michel Berthe; Cyrille Rosset; Adriano De Rosa; Enrico Franceschi; Gianluca Morgante; Francesca Sortino; Massimo Trifoglio; Luca Valenziano; Laura Patrizii; F. Fornari; F. Giacomini; A. Margiotta; N. Mauri; L. Pasqualini; G. Sirri; M. Spurio; M. Tenti; R. Travaglini; Stefano Dusini; F. Dal Corso; C. Sirignano; Salvador Ventura; Carlotta Bonoli; Andrea Balestra; Eduardo Medina Celi; Ruben Farinelli; Leonardo Corcione; Sebastiano Ligori; Frank Grupp; Carolin Wimmer; Felix Hormuth; Gregor Seidel; Stefanie Wachter; Cristobal Padilla; Mikel Lamensans; Ricard Casas; Ivan Lloro; Rafael Toledo-Moreo; Jaime Gomez; Carlos Colodro-Conde; David Lizán; Jose Javier Diaz; Per B. Lilje; Michael I. Andersen; Anton N. Sørensen; Peter Jakobsen; Allan Hornstrup; Niels Christian Jessen; Cédric Thizy; Warren Holmes; Ulf Israelsson; Michael Seiffert; Augustyn Waczynski; René J. Laureijs; Giuseppe Racca; Jean Christophe Salvignol; Tobias Boenke; Paolo Strada

doi:10.1117/12.2232941

Euclid Near Infrared Spectrometer and Photometer instrument concept and first test results obtained for different breadboards models at the end of phase C

Thierry Maciaszek, Anne Ealet, Knud Jahnke, Eric Prieto, Yannick Mellier, William Bon, Anne Bonefoi, Michael Carle, Amandine Caillat, Anne Costille, Doriane Dormoy, Franck Ducret, Christophe Fabron, Aurélien Febvre, Benjamin Foulon, José Garrido Garcia, Jean Luc Gimenez, Emmanuel Grassi, David Le Mignant, Tony PamplonaPatrice Sanchez, William Gillard, Mathieu Niclas, Aurélia Secroun, Bogna Kubik, Jérome Amiaux, Jean Christophe Barrière, Michel Berthe, Cyrille Rosset, Adriano De Rosa, Enrico Franceschi, Gianluca Morgante, Francesca Sortino, Massimo Trifoglio, Luca Valenziano, Laura Patrizii, F. Fornari, F. Giacomini, A. Margiotta, N. Mauri, L. Pasqualini, G. Sirri, M. Spurio, M. Tenti, R. Travaglini, Stefano Dusini, F. Dal Corso, C. Sirignano, Salvador Ventura, Carlotta Bonoli, Andrea Balestra, Eduardo Medina Celi, Ruben Farinelli, Leonardo Corcione, Sebastiano Ligori, Frank Grupp, Carolin Wimmer, Felix Hormuth, Gregor Seidel, Stefanie Wachter, Cristobal Padilla, Mikel Lamensans, Ricard Casas, Ivan Lloro, Rafael Toledo-Moreo, Jaime Gomez, Carlos Colodro-Conde, David Lizán, Jose Javier Diaz, Per B. Lilje, Michael I. Andersen, Anton N. Sørensen, Peter Jakobsen, Allan Hornstrup, Niels Christian Jessen, Cédric Thizy, Warren Holmes, Ulf Israelsson, Michael Seiffert, Augustyn Waczynski, René J. Laureijs, Giuseppe Racca, Jean Christophe Salvignol, Tobias Boenke, Paolo Strada

17 Citations (Scopus)

Abstract

The Euclid mission objective is to understand why the expansion of the Universe is accelerating through by mapping the geometry of the dark Universe by investigating the distance-redshift relationship and tracing the evolution of cosmic structures. The Euclid project is part of ESA's Cosmic Vision program with its launch planned for 2020 (ref [1]). The NISP (Near Infrared Spectrometer and Photometer) is one of the two Euclid instruments and is operating in the near-IR spectral region (900- 2000nm) as a photometer and spectrometer. The instrument is composed of: - a cold (135K) optomechanical subsystem consisting of a Silicon carbide structure, an optical assembly (corrector and camera lens), a filter wheel mechanism, a grism wheel mechanism, a calibration unit and a thermal control system - a detection subsystem based on a mosaic of 16 HAWAII2RG cooled to 95K with their front-end readout electronic cooled to 140K, integrated on a mechanical focal plane structure made with molybdenum and aluminum. The detection subsystem is mounted on the optomechanical subsystem structure - a warm electronic subsystem (280K) composed of a data processing / detector control unit and of an instrument control unit that interfaces with the spacecraft via a 1553 bus for command and control and via Spacewire links for science data This presentation describes the architecture of the instrument at the end of the phase C (Detailed Design Review), the expected performance, the technological key challenges and preliminary test results obtained for different NISP subsystem breadboards and for the NISP Structural and Thermal model (STM).

Original language	English
Article number	UNSP 99040T
Journal	Proceedings of S P I E - International Society for Optical Engineering
Volume	9904
ISSN	0277-786X
DOIs	https://doi.org/10.1117/12.2232941
Publication status	Published - 26 Jun 2016

Keywords

Euclid
Infrared
Instrument
NISP
Photometry
Spectroscopy

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99040TFinal published version, 4.6 MB

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Maciaszek, T., Ealet, A., Jahnke, K., Prieto, E., Mellier, Y., Bon, W., Bonefoi, A., Carle, M., Caillat, A., Costille, A., Dormoy, D., Ducret, F., Fabron, C., Febvre, A., Foulon, B., Garcia, J. G., Gimenez, J. L., Grassi, E., Mignant, D. L., ... Strada, P. (2016). Euclid Near Infrared Spectrometer and Photometer instrument concept and first test results obtained for different breadboards models at the end of phase C. Proceedings of S P I E - International Society for Optical Engineering, 9904, Article UNSP 99040T. https://doi.org/10.1117/12.2232941

Euclid Near Infrared Spectrometer and Photometer instrument concept and first test results obtained for different breadboards models at the end of phase C. / Maciaszek, Thierry; Ealet, Anne; Jahnke, Knud et al.
In: Proceedings of S P I E - International Society for Optical Engineering, Vol. 9904, UNSP 99040T, 26.06.2016.

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

Maciaszek, T, Ealet, A, Jahnke, K, Prieto, E, Mellier, Y, Bon, W, Bonefoi, A, Carle, M, Caillat, A, Costille, A, Dormoy, D, Ducret, F, Fabron, C, Febvre, A, Foulon, B, Garcia, JG, Gimenez, JL, Grassi, E, Mignant, DL, Pamplona, T, Sanchez, P, Gillard, W, Niclas, M, Secroun, A, Kubik, B, Amiaux, J, Barrière, JC, Berthe, M, Rosset, C, De Rosa, A, Franceschi, E, Morgante, G, Sortino, F, Trifoglio, M, Valenziano, L, Patrizii, L, Fornari, F, Giacomini, F, Margiotta, A, Mauri, N, Pasqualini, L, Sirri, G, Spurio, M, Tenti, M, Travaglini, R, Dusini, S, Dal Corso, F, Sirignano, C, Ventura, S, Bonoli, C, Balestra, A, Celi, EM, Farinelli, R, Corcione, L, Ligori, S, Grupp, F, Wimmer, C, Hormuth, F, Seidel, G, Wachter, S, Padilla, C, Lamensans, M, Casas, R, Lloro, I, Toledo-Moreo, R, Gomez, J, Colodro-Conde, C, Lizán, D, Diaz, JJ, Lilje, PB, Andersen, MI , Sørensen, AN , Jakobsen, P, Hornstrup, A, Jessen, NC, Thizy, C, Holmes, W, Israelsson, U, Seiffert, M, Waczynski, A, Laureijs, RJ, Racca, G, Salvignol, JC, Boenke, T & Strada, P 2016, 'Euclid Near Infrared Spectrometer and Photometer instrument concept and first test results obtained for different breadboards models at the end of phase C', Proceedings of S P I E - International Society for Optical Engineering, vol. 9904, UNSP 99040T. https://doi.org/10.1117/12.2232941

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title = "Euclid Near Infrared Spectrometer and Photometer instrument concept and first test results obtained for different breadboards models at the end of phase C",

abstract = "The Euclid mission objective is to understand why the expansion of the Universe is accelerating through by mapping the geometry of the dark Universe by investigating the distance-redshift relationship and tracing the evolution of cosmic structures. The Euclid project is part of ESA's Cosmic Vision program with its launch planned for 2020 (ref [1]). The NISP (Near Infrared Spectrometer and Photometer) is one of the two Euclid instruments and is operating in the near-IR spectral region (900- 2000nm) as a photometer and spectrometer. The instrument is composed of: - a cold (135K) optomechanical subsystem consisting of a Silicon carbide structure, an optical assembly (corrector and camera lens), a filter wheel mechanism, a grism wheel mechanism, a calibration unit and a thermal control system - a detection subsystem based on a mosaic of 16 HAWAII2RG cooled to 95K with their front-end readout electronic cooled to 140K, integrated on a mechanical focal plane structure made with molybdenum and aluminum. The detection subsystem is mounted on the optomechanical subsystem structure - a warm electronic subsystem (280K) composed of a data processing / detector control unit and of an instrument control unit that interfaces with the spacecraft via a 1553 bus for command and control and via Spacewire links for science data This presentation describes the architecture of the instrument at the end of the phase C (Detailed Design Review), the expected performance, the technological key challenges and preliminary test results obtained for different NISP subsystem breadboards and for the NISP Structural and Thermal model (STM).",

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AU - Maciaszek, Thierry

AU - Ealet, Anne

AU - Jahnke, Knud

AU - Prieto, Eric

AU - Mellier, Yannick

AU - Bon, William

AU - Bonefoi, Anne

AU - Carle, Michael

AU - Caillat, Amandine

AU - Costille, Anne

AU - Dormoy, Doriane

AU - Ducret, Franck

AU - Fabron, Christophe

AU - Febvre, Aurélien

AU - Foulon, Benjamin

AU - Garcia, José Garrido

AU - Gimenez, Jean Luc

AU - Grassi, Emmanuel

AU - Mignant, David Le

AU - Pamplona, Tony

AU - Sanchez, Patrice

AU - Gillard, William

AU - Niclas, Mathieu

AU - Secroun, Aurélia

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AU - Amiaux, Jérome

AU - Barrière, Jean Christophe

AU - Berthe, Michel

AU - Rosset, Cyrille

AU - De Rosa, Adriano

AU - Franceschi, Enrico

AU - Morgante, Gianluca

AU - Sortino, Francesca

AU - Trifoglio, Massimo

AU - Valenziano, Luca

AU - Patrizii, Laura

AU - Fornari, F.

AU - Giacomini, F.

AU - Margiotta, A.

AU - Mauri, N.

AU - Pasqualini, L.

AU - Sirri, G.

AU - Spurio, M.

AU - Tenti, M.

AU - Travaglini, R.

AU - Dusini, Stefano

AU - Dal Corso, F.

AU - Sirignano, C.

AU - Ventura, Salvador

AU - Bonoli, Carlotta

AU - Balestra, Andrea

AU - Celi, Eduardo Medina

AU - Farinelli, Ruben

AU - Corcione, Leonardo

AU - Ligori, Sebastiano

AU - Grupp, Frank

AU - Wimmer, Carolin

AU - Hormuth, Felix

AU - Seidel, Gregor

AU - Wachter, Stefanie

AU - Padilla, Cristobal

AU - Lamensans, Mikel

AU - Casas, Ricard

AU - Lloro, Ivan

AU - Toledo-Moreo, Rafael

AU - Gomez, Jaime

AU - Colodro-Conde, Carlos

AU - Lizán, David

AU - Diaz, Jose Javier

AU - Lilje, Per B.

AU - Andersen, Michael I.

AU - Sørensen, Anton N.

AU - Jakobsen, Peter

AU - Hornstrup, Allan

AU - Jessen, Niels Christian

AU - Thizy, Cédric

AU - Holmes, Warren

AU - Israelsson, Ulf

AU - Seiffert, Michael

AU - Waczynski, Augustyn

AU - Laureijs, René J.

AU - Racca, Giuseppe

AU - Salvignol, Jean Christophe

AU - Boenke, Tobias

AU - Strada, Paolo

PY - 2016/6/26

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N2 - The Euclid mission objective is to understand why the expansion of the Universe is accelerating through by mapping the geometry of the dark Universe by investigating the distance-redshift relationship and tracing the evolution of cosmic structures. The Euclid project is part of ESA's Cosmic Vision program with its launch planned for 2020 (ref [1]). The NISP (Near Infrared Spectrometer and Photometer) is one of the two Euclid instruments and is operating in the near-IR spectral region (900- 2000nm) as a photometer and spectrometer. The instrument is composed of: - a cold (135K) optomechanical subsystem consisting of a Silicon carbide structure, an optical assembly (corrector and camera lens), a filter wheel mechanism, a grism wheel mechanism, a calibration unit and a thermal control system - a detection subsystem based on a mosaic of 16 HAWAII2RG cooled to 95K with their front-end readout electronic cooled to 140K, integrated on a mechanical focal plane structure made with molybdenum and aluminum. The detection subsystem is mounted on the optomechanical subsystem structure - a warm electronic subsystem (280K) composed of a data processing / detector control unit and of an instrument control unit that interfaces with the spacecraft via a 1553 bus for command and control and via Spacewire links for science data This presentation describes the architecture of the instrument at the end of the phase C (Detailed Design Review), the expected performance, the technological key challenges and preliminary test results obtained for different NISP subsystem breadboards and for the NISP Structural and Thermal model (STM).

AB - The Euclid mission objective is to understand why the expansion of the Universe is accelerating through by mapping the geometry of the dark Universe by investigating the distance-redshift relationship and tracing the evolution of cosmic structures. The Euclid project is part of ESA's Cosmic Vision program with its launch planned for 2020 (ref [1]). The NISP (Near Infrared Spectrometer and Photometer) is one of the two Euclid instruments and is operating in the near-IR spectral region (900- 2000nm) as a photometer and spectrometer. The instrument is composed of: - a cold (135K) optomechanical subsystem consisting of a Silicon carbide structure, an optical assembly (corrector and camera lens), a filter wheel mechanism, a grism wheel mechanism, a calibration unit and a thermal control system - a detection subsystem based on a mosaic of 16 HAWAII2RG cooled to 95K with their front-end readout electronic cooled to 140K, integrated on a mechanical focal plane structure made with molybdenum and aluminum. The detection subsystem is mounted on the optomechanical subsystem structure - a warm electronic subsystem (280K) composed of a data processing / detector control unit and of an instrument control unit that interfaces with the spacecraft via a 1553 bus for command and control and via Spacewire links for science data This presentation describes the architecture of the instrument at the end of the phase C (Detailed Design Review), the expected performance, the technological key challenges and preliminary test results obtained for different NISP subsystem breadboards and for the NISP Structural and Thermal model (STM).

KW - Euclid

KW - Infrared

KW - Instrument

KW - NISP

KW - Photometry

KW - Spectroscopy

U2 - 10.1117/12.2232941

DO - 10.1117/12.2232941

M3 - Conference article

AN - SCOPUS:84991316096

SN - 0277-786X

VL - 9904

JO - Proceedings of S P I E - International Society for Optical Engineering

JF - Proceedings of S P I E - International Society for Optical Engineering

M1 - UNSP 99040T

ER -

Euclid Near Infrared Spectrometer and Photometer instrument concept and first test results obtained for different breadboards models at the end of phase C

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