 However it seems that, at least in the first instance, Wright has a relatively quick response to this point at his disposal. Waiving the point that in any case the width of cosmological role constraint applies to classes of properties and facts, he can point out that in the example constructed by Rosen the narrowness of Q’s cosmological role is an a posteriori matter. Whereas what we want is that the narrowness of cosmological role is an a priori matter: one does not need to conduct an empirical investigation to convince oneself that facts about the funny fail to have wide cosmological role.