  Recent photometric detections of extreme $(z>10)$ redshift galaxies from the
JWST have been shown to be in strong tension with existing simulation models
for galaxy formation, and in the most acute case, in tension with $\Lambda CDM$
itself. These results, however, all rest on the confirmation of these distances
by spectroscopy. Recently, the JADES survey has detected the most distant
galaxies with spectroscopically confirmed redshifts, with four galaxies found
with redshifts between $z=10.38$ and $z=13.2$. In this paper, we compare
simulation predictions from four large cosmological volumes and two zoom-in
protoclusters with the JADES observations to determine whether these
spectroscopically confirmed galaxy detections are in tension with existing
models for galaxy formation, or with $\Lambda CDM$ more broadly. We find that
existing models for cosmological galaxy formation can generally reproduce the
observations for JADES, in terms of galaxy stellar masses, star formation
rates, and the number density of galaxies at $z>10$.
