Steps during the process to build a star spectrum from the spectral cube. The top left figure corresponds to one of our observations with HST WF2 in Baade’s window, the white square corresponds to the area covered by one of the VIMOS IFU images (top right). In the IFU field the first quadrant is enclosed, its respective convolved image produced during the deconvolution process to check the detection of stars in the first quadrant appear at the bottom right. Finally some examples of the spectra extracted by this process are shown at the bottom left.