The Grism Lens-Amplified Survey from Space (GLASS). III. A census of Ly\alpha\ Emission at $z\gtrsim$7 from HST Spectroscopy

[abbreviated] We present a census of Ly\alpha\ emission at $z\gtrsim 7$ utilizing deep near infrared HST grism spectroscopy from the first six completed clusters of the Grism Lens-Amplified Survey from Space (GLASS). In 24/159 photometrically selected galaxies we detect emission lines consistent with Ly\alpha\ in the GLASS spectra. Based on the distribution of signal-to-noise ratios and on simulations we expect the completeness and the purity of the sample to be 40-100% and 60-90%, respectively. For the objects without detected emission lines we show that the observed (not corrected for lensing magnification) 1$\sigma$ flux limits reaches $5\times {10}^{-18}$erg/s/cm${}^2$ per position angle over the full wavelength range of GLASS (0.8-1.7$\mu$m). Based on the conditional probability of Ly\alpha\ emission measured from the ground at $z\sim 7$ we would have expected 12-18 Ly\alpha\ emitters. This is consistent with the number of detections, within the uncertainties, confirming the drop in Ly\alpha\ emission with respect to $z\sim 6$. These candidates include a promising source at $z=8.1$. The spatial extent of Ly\alpha\ in a deep stack of the most convincing Ly\alpha\ emitters with $⟨z⟩=7.2$ is consistent with that of the rest-frame UV continuum. Extended Ly$\alpha$ emission, if present, has a surface brightness below our detection limit, consistent with the properties of lower redshift comparison samples. From the stack we estimate upper limits on rest-frame UV emission line ratios and find $f_$\text{CIV}$ / f_$\text{Ly}\alpha$ \lesssim 0.32$and$f_$\text{CIII]}$ / f_$\text{Ly}\alpha$ \lesssim 0.23$ in good agreement with other values published in the literature.