Cosmological large-scale structure analyses based on two-point correlation functions often assume a Gaussian likelihood function with a fixed covariance matrix. We study the impact on cosmological parameter estimation of ignoring the parameter dependence of this covariance matrix. focusing on the particular case of joint weak-lensing and galaxy clustering analyses. Using a Fisher matr... https://smokeysmountainfurnitureoutlets.shop/product-category/youth-bedroom-set/