  Using the cosmological data sets, accelerating cosmological models are
obtained in this paper by constraining the free parameters in symmetric
teleparallel gravity. Using the best-fit values of free parameters, we
determine the present values of geometrical parameters and the late-time
behaviour of the universe. We also consider two $f(Q)$ models ($Q$ being the
non-metricity scalar): one that contains the term of higher power of
non-metricity scalar and the other with the inverse. From the constrained free
parameters, the present values of the geometrical parameters are obtained and
that of the effective equation of state parameter for both models.
Interestingly, we found that all the values lie within the range prescribed by
the cosmological observations. Further, the models exhibit the $\Lambda{CDM}$
behaviour at the late time of the evolution.

General Relativity and Quantum Cosmology;High Energy Physics - Theory