A high-resolution pointing system for fast scanning platforms: The EBEX example
Joy Didier, Daniel Chapman, Asad Aboobaker, Derek Araujo, Will, Grainger, Shaul Hanany, Kyle Helson, Seth Hillbrand, Andrei Korotkov, Michele, Limon, Amber Miller, Britt Reichborn-Kjennerud, Ilan Sagiv, Greg Tucker, Yuri, Vinokurov

TL;DR
This paper presents a high-resolution pointing system for the EBEX balloon-borne telescope, enabling precise attitude reconstruction during fast sky scans, validated with flight data to meet scientific accuracy requirements.
Contribution
The paper introduces a novel pointing system design and simulation pipeline tailored for high-speed balloon-borne telescopes like EBEX, achieving sub-10 arcsecond accuracy in the map domain.
Findings
Achieved RMS pointing error of 25" over 40-second intervals.
Validated system performance with flight data from EBEX 2012/2013.
Demonstrated systematic error control suitable for CMB polarization measurements.
Abstract
The E and B experiment (EBEX) is a balloon-borne telescope designed to measure the polarization of the cosmic microwave background with 8' resolution employing a gondola scanning with speeds of order degree per second. In January 2013, EBEX completed 11 days of observations in a flight over Antarctica covering 6000 square degrees of the sky. The payload is equipped with two redundant star cameras and two sets of three orthogonal gyroscopes to reconstruct the telescope attitude. The EBEX science goals require the pointing to be reconstructed to approximately 10" in the map domain, and in-flight attitude control requires the real time pointing to be accurate to 0.5 . The high velocity scan strategy of EBEX coupled to its float altitude only permits the star cameras to take images at scan turnarounds, every 40 seconds, and thus requires the development of a…
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