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The Simons Observatory (SO) is a set of cosmic microwave backgroundinstruments that will be deployed in the Atacama Desert in Chile. The keyscience goals include setting new constraints on cosmic inflation, measuringlarge scale structure with gravitational lensing, and constraining neutrinomasses. Meeting these science goals with SO requires high sensitivity andimproved calibration techniques. In this paper, we highlight a few of the mostimportant instrument calibrations, including spectral response, gain stability,and polarization angle calibrations. We present their requirements for SO andexperimental techniques that can be employed to reach those requirements.

Development of Calibration Strategies for the Simons Observatory