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SuperBIT Superpressure Flight Instrument Overview and Performance: Near-diffraction-limited Astronomical Imaging from the Stratosphere

Gill, Ajay S.; Benton, Steven J.; Damaren, Christopher J.; Everett, Spencer W.; Fraisse, Aurelien A.; Hartley, John W.; Harvey, David; Holder, Bradley; Huff, Eric M.; Jones, William C.; Lagattuta, David; Leung, Jason S.-Y.; Jauzac, Mathilde; Li, Lun; Luu, Thuy Vy T.; Massey, Richard; McCleary, Jacqueline E.; Nagy, Johanna M.; Netterfield, C. Barth; Paracha, Emaad; Redmond, Susan F.; Rhodes, Jason D.; Robertson, Andrew; Romualdez, L. Javier; Schmoll, Jürgen; Shaaban, Mohamed M.; Sirks, Ellen L.; Vassilakis, Georgios N.; Vitorelli, André Z.

SuperBIT Superpressure Flight Instrument Overview and Performance: Near-diffraction-limited Astronomical Imaging from the Stratosphere Thumbnail


Authors

Ajay S. Gill

Steven J. Benton

Christopher J. Damaren

Spencer W. Everett

Aurelien A. Fraisse

John W. Hartley

David Harvey

Bradley Holder

Eric M. Huff

Jason S.-Y. Leung

Lun Li

Thuy Vy T. Luu

Jacqueline E. McCleary

Johanna M. Nagy

C. Barth Netterfield

Emaad Paracha

Susan F. Redmond

Jason D. Rhodes

L. Javier Romualdez

Mohamed M. Shaaban

Ellen L. Sirks

Georgios N. Vassilakis

André Z. Vitorelli



Abstract

SuperBIT was a 0.5 m near-UV to near-infrared wide-field telescope that launched on a NASA superpressure balloon into the stratosphere from New Zealand for a 45-night flight. SuperBIT acquired multiband images of galaxy clusters to study the properties of dark matter using weak gravitational lensing. We provide an overview of the instrument and its various subsystems. We then present the instrument performance from the flight, including the telescope and image stabilization system, the optical system, the power system, and the thermal system. SuperBIT successfully met the instrument’s technical requirements, achieving a telescope pointing stability of 0.″34 ± 0.″10, a focal plane image stability of 0.″055 ± 0.″027, and a point-spread function FWHM of ∼0.″35 over 5-minute exposures throughout the 45-night flight. The telescope achieved a near-diffraction-limited point-spread function in all three science bands (u, b, and g). SuperBIT served as a pathfinder to the GigaBIT observatory, which will be a 1.34 m near-UV to near-infrared balloon-borne telescope.

Citation

Gill, A. S., Benton, S. J., Damaren, C. J., Everett, S. W., Fraisse, A. A., Hartley, J. W., Harvey, D., Holder, B., Huff, E. M., Jones, W. C., Lagattuta, D., Leung, J. S.-Y., Jauzac, M., Li, L., Luu, T. V. T., Massey, R., McCleary, J. E., Nagy, J. M., Netterfield, C. B., Paracha, E., …Vitorelli, A. Z. (2024). SuperBIT Superpressure Flight Instrument Overview and Performance: Near-diffraction-limited Astronomical Imaging from the Stratosphere. Astronomical Journal, 168(2), Article 85. https://doi.org/10.3847/1538-3881/ad5840

Journal Article Type Article
Acceptance Date Jun 9, 2024
Online Publication Date Jul 22, 2024
Publication Date Aug 1, 2024
Deposit Date Jul 31, 2024
Publicly Available Date Jul 31, 2024
Journal Astronomical Journal
Print ISSN 0004-6256
Electronic ISSN 1538-3881
Publisher IOP Publishing
Peer Reviewed Peer Reviewed
Volume 168
Issue 2
Article Number 85
DOI https://doi.org/10.3847/1538-3881/ad5840
Keywords Space telescopes, Weak gravitational lensing, High altitude balloons, Astronomical instrumentation, Gravitational lensing, Galaxy clusters
Public URL https://durham-repository.worktribe.com/output/2617789

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