Romualdez, LJ;
Bernard, L;
Bocchieri, A;
Butler, N;
Changeat, Q;
D'Alessandro, A;
Edwards, B;
... Waldmann, I; + view all
(2024)
The EXoplanet Climate Infrared TElescope (EXCITE): Gondola Pointing & Stabilization Qualification.
In: Marshall, Heather K and Spyromilio, Jason and Usuda, Tomonori, (eds.)
Proceedings of SPIE - The International Society for Optical Engineering.
(pp. p. 136).
SPIE: Yokohama, Japan.
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Abstract
High precision sub-arcsecond pointing stability has become a capability widely utilized in the balloon-borne community, in particular for high resolution optical systems. However, many of these applications are also pushing the state-of-the-art with regards to detector technology, many forms of which require some level of cryogenic cooling and active dissipative cooling systems to achieve target performance specifications. Built on the success of the Super-pressure Balloon-borne Imaging Telescope (SuperBIT) experiment, we present the results of improved technologies and design methodologies applied to the EXoplanet Infrared TElescope (EXCITE), which uses active cryogenic systems to achieve detector performance while requiring pointing stability at the 100 milliarcsecond level. Results from EXCITE's recent balloon-borne campaign are presented within the context of Super-pressure Balloon (SPB) and Long Duration Balloon (LDB) applications.
Type: | Proceedings paper |
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Title: | The EXoplanet Climate Infrared TElescope (EXCITE): Gondola Pointing & Stabilization Qualification |
Event: | SPIE Astronomical Telescopes + Instrumentation |
Dates: | 16 Jun 2024 - 22 Jun 2024 |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1117/12.3018442 |
Publisher version: | http://dx.doi.org/10.1117/12.3018442 |
Language: | English |
Additional information: | This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions. |
Keywords: | Balloon-borne, sub-orbital, sub-arcsecond, stabilization, quali�cation, cryocooler, active fluid loop |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/10199881 |
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