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Angular Diameter Distance





d_A= rac{x}{ heta}


The angular diameter distance depends on the assumed Cosmology of the universe. The angular diameter distance to an object at Redshift , z , is expressed in terms of the Comoving Distance , \chi as:


d_A = rac{r(\chi)}{1+z}


Where r(\chi) is defined as:

r(\chi) = \begin{cases}