  Of late, a number of instances of neutrino flux anomalies observed at
short-baselines have given traction to the hypothesis of adding new neutrino
flavours to our Standard Model set, albeit ones not associated with a partnered
lepton. Anomalies observed at LSND, MiniBooNE and at short distances from
nuclear reactors have suggested the existence of sterile mass states with
masses on the scale of $\sim1\text{eV}$, prompting further investigations.
Subsequently, Fermilab is set to host a Short-Baseline Neutrino (SBN)
oscillation program which will cross-check each of these anomalies by deploying
three state-of-the-art liquid argon detectors along the Booster Neutrino
Beamline. Through an event-by-event Monte Carlo simulation study, this document
presents short-baseline oscillation sensitivity predictions for SBN on a purely
statistical basis in the scope of a 3+1 sterile neutrino model approximated
with a two flavour mixing basis. As a world's first, sensitivities in parameter
space to 3+1 mixing angles $\theta_{14}$ and $\theta_{24}$ are presented, in
addition to the sensitivities gained by combining $\nu_\mu$ disappearance and
$\nu_e$ appearance channel data. Provided also are energy spectra and 3+1
oscillation parameter sensitivity predictions for these two individual
channels. The results agreed with parameter space sensitivity predictions
already conceived by Fermilab to a satisfactory degree.
