The Fisher gAlaxy suRvey cOde ($\texttt{FARO}$)
  The Fisher gAlaxy suRvey cOde ($\texttt{FARO}$) is a new public Python code
that computes the Fisher matrix for galaxy surveys observables. The observables
considered are the linear multitracer 3D galaxy power spectrum, the linear
convergence power spectrum for weak lensing, and the linear multitracer power
spectrum for the correlation between galaxy distribution and convergence. The
code allows for tomographic and model-independent analysis in which, for
scale-independent growth, the following functions of redshift $A_a (z) \equiv
\sigma_{8}(z) \, b_a (z)$, $R(z) \equiv \sigma_{8}(z) \, f(z)$, $L(z) \equiv
\Omega_{m} \, \sigma_{8}(z) \, \Sigma (z)$ and $E(z) \equiv H(z)/H_0$, together
with the function of scale $\hat{P}(k)$, are taken as free parameters in each
redshift and scale bins respectively. In addition, a module for change of
variables is provided to project the Fisher matrix on any particular set of
parameters required. The code is built to be as fast as possible and
user-friendly. As an application example, we forecast the sensitivity of future
galaxy surveys like DESI, Euclid, J-PAS and LSST and compare their performance
on different redshift and scale ranges.
