Validating z > 7.5 Lyman Break Galaxy candidates in the COSMOS field with JWST/PASSAGE

We analyze spectroscopy from one NIRISS pointing in the JWST-PASSAGE program for seven candidate $z\gtrsim 7.5$ photometrically-selected COSMOS-Web sources. We spectroscopically confirm one out of seven sources as a Lyman break galaxy (LBG) at $z=7.962_{-0.006}^{+0.003}$, with $m_{F150W}=25.9$ (AB). The remaining sources are too faint in the continuum (i.e., $m_{F150W}\gtrsim 26$ AB) to provide a redshift measurement from the Lyman break, and do not show emission lines in their spectra. Although this study contains only one spectroscopically confirmed source, the confirmation of a luminous $z\sim 8$ galaxy within this $\sim 4.8$ arcmin${}^2$ field implies a surface density of $\sim 0.21_{-0.17}^{+0.59}$ arcmin${}^{-2}$, $\approx 10\times$ higher than inferred from wide-area photometric surveys, suggesting a potential overdensity at $z\sim 8$ in the COSMOS field.