  The $James \ Webb \ Space \ Telescope \ (JWST)$ recently reported a large
population of UV luminous galaxies at high redshifts, $ z > 10$, as well as
Lyman-$\alpha$ emitting (LAE) galaxies out to $z \sim 11$. We use the observed
UV luminosities along with a data-driven approach at lower redshifts to place
constraints on the observability of the intergalactic Lyman-$\alpha$ intensity,
scattered in the form of Loeb-Rybicki haloes, during the pre-reionization and
reionization epochs ($z \sim 9-16$). We forecast the sensitivity and resolution
required to detect these intergalactic haloes, finding that individual haloes
with LAE luminosities $> 10^{43}$ ergs/s are detectable at a few sigma level at
$z \lesssim 11$, while stacking of $\sim 10$ haloes is expected to result in
detections out to $z \sim 16$. Finding these haloes is expected to shed light
on the neutral intergalactic hydrogen during cosmic reionization.
