The Cycle 11 calibration plan closely follows the plans for previous Cycles. Supported modes continue to be monitored for sensitivity changes, flat-field evolution, dispersion solutions, and the evolution of charge transfer efficiency of the CCD detector. Existing monitor programs have been expanded to include routine sensitivity measurements at the E1 aperture positions, to include an annual
NUV-PRISM flux monitor observation, and to more thoroughly check the adopted STIS dispersion solutions. The frequency of some other monitors has been decreased, as our improved understanding of STIS allows us to predict future trends with greater confidence.