A new approach to the design of holographic concave gratings is presented, in which a grating is treated as if it were composed of many small plane gratings, i .e . of local elementary gratings . A wavefront of the diffracted wave is constructed from the waves diffracted from the local elementary gratings . The expression of the focal curves is represented by the loci of centres of principal curvature of the wavefront . The aberration functions are defined as the differences between the direction cosines of the normal to the diffracted wave and those of the reference spherical wave . Blanks are assumed to be toric . The gratings are designed for use with Seya-Namioka monochromators and grazing incidence monochromators, and their theoretical performances are investigated by means of spot diagrams .