“…Enforcing the chiral projection of the Rarita-Schwinger equation ε µνρκ σν ∇ ρ χ gen ∆,J;κ = 0 as well as the gauge conditions ∇ µ χ gen ∆,J;µ = 0 , X µ χ gen ∆,J;µ = 0 , σµ χ gen ∆,J;µ = 0 , (2.15) yields the radiative conformal primary wavefunctions (2.9) and their shadows (2.11) for generic ∆ ∈ C and J = ± 3 2 , as well as a discrete set of solutions ∆ = 5 2 and J = ± 1 2 which we will come back to in section 4. 2 We have chosen the normalization conventions of [37] which differ from those of [4,50] by an overall sign in the s = 1 2 shadow wavefunctions.…”