  Recent observations from the Interface Region Imaging Spectrograph (IRIS)
appear to show impulsive brightenings in high temperature lines, which when
combined with simultaneous ground based observations in H$\alpha$, appear
co-spatial to Ellerman Bombs (EBs). We use the RADYN 1-dimensional radiative
transfer code in an attempt to try and reproduce the observed line profiles and
simulate the atmospheric conditions of these events. Combined with the MULTI/RH
line synthesis codes, we compute the H$\alpha$, Ca II 8542~\AA, and Mg II h \&
k lines for these simulated events and compare them to previous observations.
Our findings hint that the presence of superheated regions in the photosphere
($>$10,000 K) is not a plausible explanation for the production of EB
signatures. While we are able to recreate EB-like line profiles in H$\alpha$,
Ca II 8542~\AA, and Mg II h \& k, we cannot achieve agreement with all of these
simultaneously.
