“…From the purely geometrical point of view, this approach makes use of Grimm's curved superspace geometry [4], which is perfectly suitable to describe N = 2 conformal supergravity and has a simple relation to Howe's superspace formulation [5]. Kinematically, matter fields in [1] are described in terms of covariant projective supermultiplets which are curved-space versions of the superconformal projective multiplets [6] living in rigid projective superspace [7,8]. In addition to the local N = 2 superspace coordinates z M = (x m , θ µ i ,θ iμ ), where m = 0, 1, · · · , 3, µ = 1, 2,μ = 1, 2 and i = 1, 2, such a supermultiplet, Q (n) (z, u + ), depends on auxiliary isotwistor variables u + i ∈ C 2 \ {0}, with respect to which Q (n) is holomorphic and homogeneous, Q (n) (c u + ) = c n Q (n) (u + ), on an open domain of C 2 \ {0} (the integer parameter n is called the weight of Q (n) ).…”