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PLATO flight model cameras TVAC focus calibration

Title: PLATO flight model cameras TVAC focus calibration
Authors: Pertenais, Martin; Eigmüller, Philipp; Cabrera Perez, Juan; Grießbach, Denis; van Kempen, Tim A.; Ferrari, Lorenza; Laauwen, Wouter; Appourchaux, Thierry; Dumesnil, Cydalise; Hervier, Véronique; Beraud, Nicolas; Guiot, Pierre; Hamm, Vincent; Condamin, Mathieu; Francois, Serge; Tamiatto, Catherine; Westphal, Pierre-Amaury; Ramos Zapata, Gonzalo; Montoro, Francisco; Borreguero, Elisa; Rodrigo, M. Teresa; Valverde, Ángel L.; Ángeles Sierra, M.; Espinosa, Lucía; Santiago, Amaia; Conde, Fernando; Gorius, Nicolas; Arena, Claudio; Borsa, Francesco; Aboudan, Alessio; Huygen, Rik; Regibo, Sara; Royer, Pierre; Vandenbussche, Bart; Hermans, Aline; Baeke, Ann; Mas-Hesse, Miguel; Rauer, Heike
Publisher Information: SPIE
Publication Year: 2025
Collection: German Aerospace Center: elib - DLR electronic library
Subject Terms: Weltrauminstrumente; Extrasolare Planeten und Atmosphären
Description: The PLAnetary Transits and Oscillations of stars (PLATO) mission aims at detecting and characterizing extrasolar planetary systems, including terrestrial exoplanets orbiting up to the habitable zone around bright solar-type stars1.2 The scientific payload of PLATO, developed and provided by the PLATO Mission Consortium (PMC) and ESA, is based on a multi-telescope configuration consisting of 24 Normal Cameras (N-CAM) and 2 Fast Cameras (F-CAM), so as to provide simultaneously a large field of view and a large collecting aperture. Each individual camera can be thermally re-focused in order to compensate for the accumulated integration errors between the Telescope Optical Unit (TOU) and the Focal Plane Assembly (FPA). It allows to operate each camera in-orbit at its optimum setpoint, minimizing the average PSF size of the stars on the focal plane. To achieve this, the camera itself is cold-biased on the spacecraft and its temperature is controlled by a Thermal Control System (TCS) that allows to reach a commanded stable temperature within the range [-90°C ; -70°C]. This work presents the preparation and results of the on-ground pre-launch calibration campaign of the cameras Flight Models (FM), scanning the complete temperature range and searching for the best focus temperature. A set of statistical data is presented, based on the assembly and testing of the first flight model cameras, confirming their high-quality and validating the processes defined for the serial production.
Document Type: conference object
File Description: application/pdf
Language: English
ISSN: 0277-786X
Relation: https://elib.dlr.de/217078/1/1369965.pdf; Pertenais, Martin und Eigmüller, Philipp und Cabrera Perez, Juan und Grießbach, Denis und van Kempen, Tim A. und Ferrari, Lorenza und Laauwen, Wouter und Appourchaux, Thierry und Dumesnil, Cydalise und Hervier, Véronique und Beraud, Nicolas und Guiot, Pierre und Hamm, Vincent und Condamin, Mathieu und Francois, Serge und Tamiatto, Catherine und Westphal, Pierre-Amaury und Ramos Zapata, Gonzalo und Montoro, Francisco und Borreguero, Elisa und Rodrigo, M. Teresa und Valverde, Ángel L. und Ángeles Sierra, M. und Espinosa, Lucía und Santiago, Amaia und Conde, Fernando und Gorius, Nicolas und Arena, Claudio und Borsa, Francesco und Aboudan, Alessio und Huygen, Rik und Regibo, Sara und Royer, Pierre und Vandenbussche, Bart und Hermans, Aline und Baeke, Ann und Mas-Hesse, Miguel und Rauer, Heike (2025) PLATO flight model cameras TVAC focus calibration. In: 2024 International Conference on Space Optics, ICSO 2024, 13699, Seite 1369965. SPIE. International Conference on Space Optics ICSO 2024, 2024-10-21, Antibes, Frankreich. doi:10.1117/12.3071286 . ISSN 0277-786X.
DOI: 10.1117/12.3071286.full
Availability: https://elib.dlr.de/217078/; https://elib.dlr.de/217078/1/1369965.pdf; https://www.spiedigitallibrary.org/conference-proceedings-of-spie/13699/3071286/PLATO-flight-model-cameras-TVAC-focus-calibration/10.1117/12.3071286.full
Accession Number: edsbas.67E34209
Database: BASE