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Our understanding of stellar atmospheres and our ability to inferarchitectures of extrasolar planetary systems rely on understanding theemission of stars at submillimeter to centimeter wavelengths. In this chapterwe describe how unconstrained stellar emission can interfere with the accuratecharacterization of circumstellar debris. The ngVLA is the only facility withthe sensitivity that allows for the observations of a broad range of stellarspectral types in a feasible amount of time. The observations will enable thebuilding and testing of accurate models of stellar emission, which in turn arerequired for evaluating both the occurrence and abundance of debris over theproposed wavelength range of the ngVLA

Science with an ngVLA: Stellar Emission as a Source of Flux Bias in Debris Disks