Effect of scan variability on vibrational heating and focal-plane stability
Investigate and quantify how telescope scan variability (including scan speed, accelerations, and turnarounds) modulates the Small Aperture Telescope Platform vibrational environment and determine the resulting impact on focal-plane array temperature stability at 100 mK in SAT-MF1 during routine operations, establishing whether PID temperature control fully compensates the induced fluctuations.
References
An analysis of the scan variability of the SATP vibrational environment and its predicted effect on FPA thermal stability is left for future investigations with the integrated SATP and SAT system.
— The Simons Observatory: Design, integration, and testing of the small aperture telescopes
(2405.05550 - Galitzki et al., 9 May 2024) in Section “Mechanical Resonance Heating” (Figure and discussion around vibrational tests)