Publication
We present JWST/NIRSpec prism spectroscopy of seven galaxies selected from Cosmic Evolution Early Release Science (CEERS) survey NIRCam imaging with photometric redshifts z(phot) > 8. We measure emission line redshifts of z = 7.65 and 8.64 for two galaxies. For two other sources without securely detected emission lines we measure = z 9.77(-0.29)(+0.37) and 10.01 (+0.14)(-0.19) by fitting model spectral templates to the prism data, from which we detect continuum breaks consistent with Ly alpha opacity from a mostly neutral intergalactic medium. The presence of strong breaks and the absence of strong emission lines give high confidence that these two galaxies have redshifts z > 9.6, but the redshift values derived from the breaks alone have large uncertainties given the low spectral resolution and relatively low S/N of the CEERS NIRSpec prism data. The two z similar to 10 sources observed are relatively luminous (MUV < -20), with blue continua (-2.3 less than or similar to ss less than or similar to -1.9) and low dust attenuation ( A similar or equal to 0.15(- 0.1)(+ 0.3)); and at least one of them has a high stellar mass for a galaxy at that redshift ( log M-* M-circle dot similar or equal to 9.3(-0.30)(+0.2) ). Considered together with spectroscopic observations of other CEERS NIRCam-selected high-z galaxy candidates in the literature, we find a high rate of redshift confirmation and low rate of confirmed interlopers (8%). Ten out of 35 z > 8 candidates with CEERS NIRSpec spectroscopy do not have secure redshifts, but the absence of emission lines in their spectra is consistent with redshifts z > 9.6. We find that z > 8 photometric redshifts are generally in agreement (within their uncertainties) with the spectroscopic values, but also that the photometric redshifts tend to be slightly overestimated ( = 0.45 +/- 0.11), suggesting that current templates do not fully describe the spectra of veryhigh-z sources. Overall, the spectroscopy solidifies photometric redshift evidence for a high spatial density of bright galaxies at z > 8 compared to theoretical model predictions, and further disfavors an accelerated decline in the integrated UV luminosity density at z > 8.