BibTex format
@inproceedings{Voyer:2024:10.1117/12.3017869,
author = {Voyer, P and Benton, SJ and Damaren, CJ and Everett, SW and Fraisse, AA and Gill, AS and Hartley, JW and Harvey, D and Henderson, M and Holder, B and Huff, EM and Jauzac, M and Jones, WC and Lagattuta, D and Leung, JSY and Li, L and Luu, TVT and Massey, R and McCleary, JE and Nagy, JM and Netterfield, CB and Paracha, E and Redmond, SF and Rhodes, JD and Robertson, A and Romualdez, LJ and Schmoll, J and Shaaban, MM and Sirks, EL and Vassilakis, GN and Vitorelli, AZ},
doi = {10.1117/12.3017869},
title = {From SuperBIT to GigaBIT: Informing next-generation balloon-borne telescope design with Fine Guidance System flight data},
url = {http://dx.doi.org/10.1117/12.3017869},
year = {2024}
}
RIS format (EndNote, RefMan)
TY - CPAPER
AB - The Super-pressure Balloon-borne Imaging Telescope (SuperBIT) is a near-diffraction-limited 0.5 m telescope that launched via NASA's super-pressure balloon technology on April 16, 2023. SuperBIT achieved precise pointing control through the use of three nested frames in conjunction with an optical Fine Guidance System (FGS), resulting in an average image stability of 0.055” over 300-second exposures. The SuperBIT FGS includes a tip-tilt fast-steering mirror that corrects for jitter on a pair of focal plane star cameras. In this paper, we leverage the empirical data from SuperBIT's successful 45-night stratospheric mission to inform the FGS design for the next-generation balloon-borne telescope. The Gigapixel Balloon-borne Imaging Telescope (GigaBIT) is designed to be a 1.35m wide-field, high resolution imaging telescope, with specifications to extend the scale and capabilities beyond those of its predecessor SuperBIT. A description and analysis of the SuperBIT FGS will be presented along with methodologies for extrapolating this data to enhance GigaBIT's FGS design and fine pointing control algorithm. We employ a systems engineering approach to outline and formalize the design constraints and specifications for GigaBIT's FGS. GigaBIT, building on the SuperBIT legacy, is set to enhance high-resolution astronomical imaging, marking a significant advancement in the field of balloon-borne telescopes.
AU - Voyer,P
AU - Benton,SJ
AU - Damaren,CJ
AU - Everett,SW
AU - Fraisse,AA
AU - Gill,AS
AU - Hartley,JW
AU - Harvey,D
AU - Henderson,M
AU - Holder,B
AU - Huff,EM
AU - Jauzac,M
AU - Jones,WC
AU - Lagattuta,D
AU - Leung,JSY
AU - Li,L
AU - Luu,TVT
AU - Massey,R
AU - McCleary,JE
AU - Nagy,JM
AU - Netterfield,CB
AU - Paracha,E
AU - Redmond,SF
AU - Rhodes,JD
AU - Robertson,A
AU - Romualdez,LJ
AU - Schmoll,J
AU - Shaaban,MM
AU - Sirks,EL
AU - Vassilakis,GN
AU - Vitorelli,AZ
DO - 10.1117/12.3017869
PY - 2024///
SN - 0277-786X
TI - From SuperBIT to GigaBIT: Informing next-generation balloon-borne telescope design with Fine Guidance System flight data
UR - http://dx.doi.org/10.1117/12.3017869
ER -