Robust diffraction-limited NIR-to-NUV wide-field imaging from stratospheric balloon-borne platforms -- SuperBIT science telescope commissioning flight & performance
L. Javier Romualdez, Steven J. Benton, Anthony M. Brown, Paul Clark,, Christopher J. Damaren, Tim Eifler, Aurelien A. Fraisse, Mathew N. Galloway,, Ajay Gill, John W. Hartley, Bradley Holder, Eric M. Huff, Mathilde Jauzac,, William C. Jones, David Lagattuta, Jason S.-Y. Leung

TL;DR
SuperBIT is a balloon-borne telescope achieving space-like resolution and stability in the near-IR to near-UV, offering a cost-effective alternative to orbital missions for high-quality astronomical imaging.
Contribution
This paper reports the successful commissioning and performance of SuperBIT, a diffraction-limited, wide-field balloon telescope with advanced stabilization, surpassing many science requirements.
Findings
Achieved 48 milliarcseconds sky-fixed pointing stability
Demonstrated stable imaging over 1-hour observations
Surpassed science performance requirements
Abstract
At a fraction the total cost of an equivalent orbital mission, scientific balloon-borne platforms, operating above 99.7% of the Earth's atmosphere, offer attractive, competitive, and effective observational capabilities -- namely space-like resolution, transmission, and backgrounds -- that are well suited for modern astronomy and cosmology. SuperBIT is a diffraction-limited, wide-field, 0.5 m telescope capable of exploiting these observing conditions in order to provide exquisite imaging throughout the near-IR to near-UV. It utilizes a robust active stabilization system that has consistently demonstrated a 1 sigma sky-fixed pointing stability at 48 milliarcseconds over multiple 1 hour observations at float. This is achieved by actively tracking compound pendulations via a three-axis gimballed platform, which provides sky-fixed telescope stability at < 500 milliarcseconds and corrects…
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