  We have studied neutrino phenomenology in the supersymmetric type-I seesaw
model endowed with the $\Gamma_2 \simeq S_3$ modular symmetry. We have
identified different realizations of the $S_3$ modular symmetry, referred to as
models A, B, C, and D. The 4 models are compatible with neutrino mass being
inverted ordering (IO). Moreover, models A, B, and D can also accommodate
normal ordering (NO) neutrino masses. We identify parameter space for each
model compatible with neutrino oscillation at the 2-$\sigma$ level. We then
proceed to study the neutrino phenomenology of each model. We find that the
lightest neutrino mass can be as light as 0.64 meV in the case of NO in model A
and 50 meV in the case of IO in model D. The smallest effective electron
neutrino mass attainable in our analysis is 8.8 meV in the case of NO (model
A), and 50 meV for IO (model D). Finally, we note that the effective Majorana
mass can be as small as 0.33 meV in the case of NO (model A) and 22 meV for IO
(model D).
