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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 1.

Top left: the commands sent to the 36 actuators of the ASM, with even actuators increasing in frequency and odd actuators decreasing; actuator 1 is black, actuator 36 is red and the actuator number increases through the rainbow palette. The top right plot shows the same modulation (with the same color coding) as a function of (positive) frequency, but with an arbitrary constant offset for better visualization. The bottom plots show a modal frequency comb (left), projected onto the actuators (right); despite each actuator having a complex frequency content, the demodulation of the WFS signals in modal space allows us to measure the interaction matrix.

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