Space-quality data from balloon-borne telescopes: The High Altitude Lensing Observatory (HALO)

Abstract : We present a method for attaining sub-arcsecond pointing stability during sub-orbital balloon flights, as designed for in the High Altitude Lensing Observatory (HALO) concept. The pointing method presented here has the potential to perform near-space quality optical astronomical imaging at similar to 1-2% of the cost of space-based missions. We also discuss an architecture that can achieve sufficient thermo-mechanical stability to match the pointing stability. This concept is motivated by advances in the development and testing of Ultra Long Duration Balloon (ULDB) flights which promise to allow observation campaigns lasting more than three months. The design incorporates a multi-stage pointing architecture comprising: a gondola coarse azimuth control system, a multi-axis nested gimbal frame structure with arcsecond stability, a telescope de-rotator to eliminate field rotation, and a fine guidance stage consisting of both a telescope mounted angular rate sensor and guide CCDs in the focal plane to drive a Fast-Steering Mirror. We discuss the results of pointing tests together with a preliminary thermo-mechanical analysis required for sub-arcsecond pointing at high altitude. Possible future applications in the areas of wide-field surveys and exoplanet searches are also discussed. (C) 2012 Elsevier B.V. All rights reserved.
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Astroparticle Physics, Elsevier, 2012, 38, pp.31--40. 〈10.1016/j.astropartphys.2012.05.015〉
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Soumis le : vendredi 20 janvier 2017 - 15:49:02
Dernière modification le : vendredi 15 mars 2019 - 14:28:06

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Jason Rhodes, Benjamin Dobke, Jeffrey Booth, Richard Massey, Kurt Liewer, et al.. Space-quality data from balloon-borne telescopes: The High Altitude Lensing Observatory (HALO). Astroparticle Physics, Elsevier, 2012, 38, pp.31--40. 〈10.1016/j.astropartphys.2012.05.015〉. 〈hal-01442397〉

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