  We present a deep, narrow J-band search for proto--galactic Lyman Alpha
emission at redshifts z~9. We combine an exceptionally deep image of the Hubble
Deep Field South, obtained using a narrow band filter centred on the wavelength
1.187 microns using the VLT/ISAAC facility, with existing deep, broad band
images covering optical to near infrared wavelengths. We search for z~9 Lyman
Alpha emitting galaxies displaying a significant narrow band excess relative to
the Js-band that are undetected at optical wavelengths. We detect no sources
consistent with this criterion to the 90% point source flux limit of the NB
image, F_{NB} = 3.28 x 10^{-18} ergs/s/cm2. The survey selection function
indicates that we have sampled a volume of approximately 340 h^{-3} Mpc^3 to a
Lyman Alpha emission luminosity of 10^{43} h^{-2} ergs/s. We conclude by
considering the potential implications for the physics of the high--redshift
universe.
