  This thesis investigates algorithms regarding their applicability for highly
nonlinear model fitting on big datasets. Various mathematical methods are
presented with which a model fit using the least squares criterion is possible.
Special requirements regarding the processing of large data sets as a basis for
such a model fit are discussed.
  The specific example of the search for gravitational wave signals in
simulated data of the ESA satellite mission Gaia is used to demonstrate how a
model fit is possible, even with complex models and large amount of data. For
this purpose, a highly parallel prototype of a future search software is
implemented. The resulting prototype uses a hybrid algorithm which utilizes a
linear search, an evolutionary algorithm and a classical iterative Gauss-Newton
fit. The performance and behavior of its components are investigated in detail.
  With the help of software presented in this work it has been possible for the
first time to detect gravitational wave signals in simulated astrometric data,
and to determine their parameters. Furthermore, it can be concluded from the
runtime behavior of the software that such a search is also possible in real
data of the Gaia mission.
