Prototyping ARRAKIHS: accelerating and derisking instrument development for an ESA fast-class mission

Λεπτομέρειες βιβλιογραφικής εγγραφής
Τίτλος: Prototyping ARRAKIHS: accelerating and derisking instrument development for an ESA fast-class mission
Συγγραφείς: Prod'homme, Thibaut, Serrano, Santiago, Corral Van Damme, Carlos, Ruehl, Timo, Isaak, Kate, Sirianni, Marco, Loehring, Jens, Lucia, Massimo, Falcolini, Massimo, Halain, Jean-Philippe, Boucher, Luc, Verhoeve, Peter, Hernandez, Eloy, Soulat, Laurence, Broussely, Marc, Vaughan, Matthew, Kusumo Adi, Albertus, Escorial Olmos, Diego, Guzmán, Rafael, Kögl, Stefan, Kehl, Florian, Rodríguez-Senín, Antonio, Kögl, Paola, Ocerin, Eider, Mateo, David, Oñate, Juan, Ugalde, Eduardo, Ubierna, Marcos, Barrena, Aitor, Burgos, Laura, Truglio, Marco, Ojanguren, Iñigo, Torralbo, Ignacio, Benito, Leire, Tahiri, Yasin, Tye, Dan, Gröbelbauer, Hans-Peter, Wirz, Florian, Szekely, Gerhard, Vazquez Codesido, Eloi, Charuel, Clément, Lallemand, Etienne, Plesseria, Jean-Yves, Giono, Gabriel, Ottacher, Harald
Συνεισφορές: CSL - Centre Spatial de Liège - ULiège
Πηγή: Proceedings of SPIE: The International Society for Optical Engineering, 14152, 109 (2026-08-21); SPIE Astronomical Telescopes + Instrumentation, Copenhagen, Denmark [DK], 05-10/07/2026
Στοιχεία εκδότη: International Society for Optical Engineering, 2026.
Έτος έκδοσης: 2026
Θεματικοί όροι: ESA fast-class mission, ARRAKIHS, Prototyping instrument, straylight baffle, fold mirror, binocular telescope, optical bench, CMOS image sensor, Front-end electronics, data processing unit, thermal control unit, Engineering, computing & technology, Aerospace & aeronautics engineering, Ingénierie, informatique & technologie, Ingénierie aérospatiale
Περιγραφή: editorial reviewed
Fast-class missions in ESA’s science programme have as their main objective to nearly halve their development timecompared to medium or large-class missions; 8 years from selection to launch instead of 15. In the context of thisaccelerated scheme, the development of bespoke high-performing instruments for space missions with attractive scientificobjectives is a considerable challenge.Using the ARRAKIHS mission as an example we show how prototyping during the study phase helps accelerate and deriskthe development of such instruments. In this contribution, we first present the ARRAKIHS mission and the instrumentpreliminary design, we then provide a summary of the outcome of more than 10 different prototyping activities from opticsto detectors, from electronic boards to mechanical parts which took place during phase B. We conclude with our mainlessons learned.
Τύπος εγγράφου: conference paper
http://purl.org/coar/resource_type/c_5794
conferenceObject
editorial reviewed
Γλώσσα: English
Relation: urn:issn:0277-786X; urn:issn:1996-756X
DOI: 10.1117/12.3102872
Σύνδεσμος πρόσβασης: https://orbi.uliege.be/handle/2268/348139
Rights: open access
http://purl.org/coar/access_right/c_abf2
info:eu-repo/semantics/openAccess
Αριθμός Καταχώρησης: edsorb.348139
Βάση Δεδομένων: ORBi
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  Data: Proceedings of SPIE: The International Society for Optical Engineering, 14152, 109 (2026-08-21); SPIE Astronomical Telescopes + Instrumentation, Copenhagen, Denmark [DK], 05-10/07/2026
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  Data: editorial reviewed<br />Fast-class missions in ESA’s science programme have as their main objective to nearly halve their development timecompared to medium or large-class missions; 8 years from selection to launch instead of 15. In the context of thisaccelerated scheme, the development of bespoke high-performing instruments for space missions with attractive scientificobjectives is a considerable challenge.Using the ARRAKIHS mission as an example we show how prototyping during the study phase helps accelerate and deriskthe development of such instruments. In this contribution, we first present the ARRAKIHS mission and the instrumentpreliminary design, we then provide a summary of the outcome of more than 10 different prototyping activities from opticsto detectors, from electronic boards to mechanical parts which took place during phase B. We conclude with our mainlessons learned.
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