Ms. Nicoletta Mauri Profile

Nicoletta Mauri

at Univ degli Studi di Bologna

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Publications (3)

Proceedings Article | 27 August 2022 Presentation + Paper

Euclid near infrared spectrometer and photometer instrument flight model presentation, performance, and ground calibration results summary

T. Maciaszek, A. Ealet, W. Gillard, K. Jahnke, R. Barbier, E. Prieto, W. Bon, A. Bonnefoi, A. Caillat, M. Carle, A. Costille, F. Ducret, C. Fabron, B. Foulon, J.-L. Gimenez, E. Grassi, M. Jaquet, D. Le Mignant, L. Martin, T. Pamplona, P. Sanchez, J.-C. Clémens, L. Caillat, M. Niclas, A. Secroun, B. Kubik, S. Ferriol, M. Berthe, J.-C. Barrière, J. Fontignie, L. Valenziano, N. Auricchio, P. Battaglia, A. De Rosa, R. Farinelli, E. Franceschi, E. Medinaceli, G. Morgante, F. Sortino, M. Trifoglio, L. Corcione, V. Capobianco, S. Ligori, S. Dusini, E. Borsato, F. Dal Corso, F. Laudisio, C. Sirignano, L. Stanco, S. Ventura, L. Patrizii, T. Chiarusi, F. Fornari, F. Giacomini, A. Margiotta, N. Mauri, L. Pasqualini, G. Sirri, M. Spurio, M. Tenti, R. Travaglini, C. Bonoli, F. Bortoletto, A. Balestra, M. Dalessandro, F. Grupp, D. Penka, J. Steinwagner, F. Hormuth, M. Schirmer, G. Seidel, C. Padilla, R. Casas, Y. Lloro, R. Toledo-Moreo, J. Gomez, C. Colodro-Conde, D. Lizán, J.-J. Diaz, P. Lilje, M. Andersen, J. Andersen, A. Sørensen, A. Hornstrup, N. Jessen, C. Thizy, W. Holmes, M. Pniel, M. Jhabvala, S. Pravdo, M. Seiffert, A. Waczynski, R. Laureij, G. Racca, J.-C. Salvignol, T. Boenke, P. Strada, Y. Mellier

Proceedings Volume 12180, 121801K (2022) https://doi.org/10.1117/12.2630338

KEYWORDS: Sensors, Fermium, Frequency modulation, Calibration, Space operations, Data processing, Silicon carbide, Spectroscopy, Photometry, Performance modeling

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Proceedings Article | 27 August 2022 Paper

EUCLID's near infrared spectro-photometer ready for flight: review of final performances

E. Medinaceli, L. Valenziano, N. Auricchio, E. Franceschi, F. Gianotti, P. Battaglia, R. Farinelli, A. Balestra, S. Dusini, C. Sirignano, E. Borsato, L. Stanco, A. Renzi, A. Troja, L. Gabarra, S. Ligori, V. Capobianco, L. Corcione, D. Bonino, G. Sirri, L. Patrizii, M. Tenti, D. Di Ferdinando, C. Valieri, N. Mauri, F. Giacomini, D. Le Mignant, E. Prieto, M. Carle, F. Ducret, W. Gillard, A. Secroun, T. Maciaszek, S. Ferriol, R. Barbier, F. Grupp, W. Holmes, M. Pniel, A. Waczynski, S. Prado, M. Seiffert, M. Jhabvala, R. Laureijs, G. Racca, J. Salvignol, T. Boenke, P. Strada

Proceedings Volume 12180, 121801L (2022) https://doi.org/10.1117/12.2629843

KEYWORDS: Sensors, Spectroscopy, Point spread functions, Galactic astronomy, Electronics, Visible radiation, Telescopes, Staring arrays, Optical filters, Near infrared

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ESA’s mission Euclid while undertaking its final integration stage is fully qualified. Euclid will perform an extra galactic survey (0<z<2) using visible and near-infrared light. To detect the infrared radiation is equipped with the Near Infrared Spectro-Photometer (NISP) instrument with a sensitivity in the 0.9-2 μm range. We present an illustration of the NISP Data Processing Unit’s Application Software, highlighting the experimental process to obtain the final parametrization of the on-board processing of data produced by an array of 16 Teledyne’s HAWAII-2RG (HgCdTe) - each of 2048×2048 px², 0.3 arcsec/px, 18 μm pixel pitch; using data from the latest test campaigns done with the flight configuration hardware - complete optical system (Korsh anastigmat telescope), detectors array (0.56 deg² firld of view) and readout systems (16 Digital Control Units and Sidecar ASICs). Also, we show the outstanding Spectrometric (using a Blue and two Red Grisms) and Photometric (using Y_E 0.92-1.15μm, J_E 1.15-1.37μm, and H_E 1.37-2.0 μm filters) performances of the NISP detector derived from the end-to-end payload module test campaign at FOCAL 5 - CSL; among them the Photometric Point Spread Function (PSF) determination, and the Spectroscopic dispersion verification. Also the performances of the onboard processing are presented. Then, we describe the solution of a major issue found during this final test phase that put NISP in the critical path. We will describe how the problem was eventually understood and solved thanks to an intensive coordinated effort of an independent review team (tiger team lead by ESA) and a team of NISP experts from the Euclid Consortium. An extended PLM level campaign in ambient in Liege and a dedicated test campaign conducted in Marseille on the NISP EQM model, with both industrial and managerial support, finally confirmed the correctness of the diagnosis of the problem. Finally, the Euclid’s survey is presented (14000 deg² wide survey, and ∼40 deg² deep-survey) as well as the global statistics for a mission lifetime of 6 years (∼1.5 billion Galaxy’s shapes, and ∼50 million Galaxy’s spectra).

Proceedings Article | 6 July 2018 Paper

The application software of the instrument control unit of Euclid-NISP: ready for qualification tests

Sebastiano Ligori, Leonardo Corcione, Vito Capobianco, Donata Bonino, Gabriele Sirri, Claudia Valieri, Federico Fornari, Francesco Giacomini, Laura Patrizii, Riccardo Travaglini, Stefano Dusini, Fulvio Laudisio, Chiara Sirignano, Luca Valenziano, Natalia Auricchio, Enrico Franceschi, Andrea Balestra, Paola Maria Battaglia, Carlotta Bonoli, Enrico Borsato, Favio Bortoletto, Tommaso Chiarusi, Flavio Dal Corso, Donato Di Ferdinando, Ruben Farinelli, Anna Gregorio, Gian Paolo Guizzo, Elisabetta Maiorano, Annarita Margiotta, Nicoletta Mauri, Eduardo Medinaceli, Gianluca Morgante, Stefano Silvestri, Francesca Sortino, Maurizio Spurio, Luca Stanco, John Stephen, Matteo Tenti, Massimo Trifoglio, Sandro Ventura

Proceedings Volume 10698, 1069834 (2018) https://doi.org/10.1117/12.2313240

KEYWORDS: Sensors, Data processing, Space operations, Data acquisition, Signal detection, Electronics, Control systems, Interfaces, Software development

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