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As a starting point, it is useful to consider the overall calibration philosophy used in AIPS++. The calibration system has been designed to meet several important goals: i) support for synthesis and single-dish radio-telescopes in a generic formalism which minimizes instrument-specific differences; ii) modeling of all relevant physical effects which may corrupt the observed data, in both the uv- and image-plane, such as propagation or instrumental response factors, in a unified framework; and iii) support for arbitrary parametrization of the individual calibration effects.