  Uncorrected wavefront errors create speckle noise in high-contrast
observations at small inner-working angles. These speckles can be sensed and
controlled by using coronagraph integrated wavefront sensors. Here, we will
present how the Phase Induced Amplitude Apodized Complex Mask Corongraph
(PIAACMC) can be integrated with both a Self-Coherent Camera (SCC) for focal
plane wavefront sensing and an extremely sensitivity high-order pupil plane
Zernike wavefront sensor (ZWFS). Non-common path aberrations can be completely
erased by integrating both sensors into the PIAACMC, which is of extremely high
importance in high-contrast imaging.
