We here present extra details for the results published in arxiv:1711.09893 ("A general theory of linear cosmological
perturbations: stability conditions, the quasistatic limit and dynamics"), that were omitted in the paper for brevity. Specifically we give results for the special vector-tensor case with
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In the file "StabilityConditionsVTII.pdf", we give the coefficients of the mass matrix and antisymmetric kinetic-mass mixing terms required to explicitly compute the stability conditions for this model.
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In the file "QuasistaticParametersVTII.pdf", we give the modified gravity parameters
$\mu$ and$\Gamma$ , which come out of the quasi-static analysis for this model.