Cosmography with the Sunyaev-Zeldovich effect and X-ray data
  Cosmography provides a direct method to map the expansion history of the
Universe in a model-independent way. Recently, different kinds of observations
have been used in cosmographic analyses, such as SNe Ia and gamma ray bursts
measurements, weak and strong lensing, cosmic microwave background
anisotropies, etc. In this work we examine the prospects for constraining
cosmographic parameters from current and future measurements of galaxy clusters
distances based on their Sunyaev-Zeldovich effect (SZE) and X-ray observations.
By assuming the current observational error distribution, we perform Monte
Carlo simulations based on a well-behaved parameterization for the deceleration
parameter to generate samples with different characteristics and study the
improvement on the determination of the cosmographic parameters from upcoming
data. The influence of galaxy clusters (GC) morphologies on the $H_0- q_0$
plane is also investigated.
