Including parameter dependence in the data and covariance for
  cosmological inference
  The final step of most large-scale structure analyses involves the comparison
of power spectra or correlation functions to theoretical models. It is clear
that the theoretical models have parameter dependence, but frequently the
measurements and the covariance matrix depend upon some of the parameters as
well. We show that a very simple interpolation scheme from an unstructured mesh
allows for an efficient way to include this parameter dependence
self-consistently in the analysis at modest computational expense. We describe
two schemes for covariance matrices. The scheme which uses the geometric
structure of such matrices performs roughly twice as well as the simplest
scheme, though both perform very well.
