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CACOFONI: Cosine Amplitude Calibration Organized in Frequency for On-sky Nimble Interaction-matrix. A Novel Method for Calibrating Adaptive Optics Systems II

  • Authors: Ruihan Zhang, 瑞涵 张, Olivier Lai, Mark Chun, Brianna Peck, Ellen Lee

Ruihan Zhang et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 10.

The frequency response function of the ASM system in the laboratory when the min(ν) data (Figure 9) was taken. The system was running at 434 Hz. The blue curve is the raw data, and the orange curve is the best-fit model to the blue curve. The model is used for the system frequency response function correction in this section.

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