Perhaps it is not completely superfluous to remind that Clauser-Horne
factorability, introduced in [1], is only necessary when \lambda, the hidden
variable (HV), is sufficiently deterministic: for {M_i} a set of possible
measurements (isolated or not by space-like intervals) on a given system, the
most general sufficient condition for factorability on \lambda\ is obtained by
finding a set of expressions M_i=M_i(\lambda,\xi_i), with {\xi_i} a set of
HV’s, all independent from one another and from \lambda. Otherwise,
factorability can be recovered on \gamma = \lambda\ \oplus\ \mu, with \mu
another additional HV, so that a description M_i=M_i(\gamma,\xi_i) is again
found: conceptually, this is always possible; experimentally, it may not: \mu
may be unaccessible or even its existence unknown (and so, too, from the point
of view of a phenomenological theory). Results here may help clarify our recent
post in [6].

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