2019ApJ...883...99S

We present 16 new ultrabright H_AB <= 25 galaxy candidates at z ∼ 8 identified over the COSMOS/UltraVISTA field. The new search takes advantage of the deepest-available ground-based optical and near-infrared observations, including the DR3 release of UltraVISTA and full-depth Spitzer/IRAC observations from the SMUVS and SPLASH programs. Candidates are selected using Lyman-break color criteria, combined with strict optical non-detection and SED-fitting criteria, designed to minimize contamination by low-redshift galaxies and low-mass stars. HST/WFC3 coverage from the DASH program reveals that one source evident in our ground-based near-IR data has significant substructure and may actually correspond to 3 separate z ∼ 8 objects, resulting in a total sample of 18 galaxies, 10 of which seem to be fairly robust (with a >97% probability of being at z > 7). The UV-continuum slope β for the bright z ∼ 8 sample is β = -2.2 ± 0.6, bluer but still consistent with that of similarly bright galaxies at z ∼ 6 (β = -1.55 ± 0.17) and z ∼ 7 (β = -1.75 ± 0.18). Their typical stellar masses are 10^9.1-0.4^+0.5M_☉, with the SFRs of 32_–32⁺⁴⁴M_☉ yr^–1, specific SFR of 4_–4⁺⁸ Gyr^–1, stellar ages of ∼22_–22⁺⁶⁹ Myr, and low dust content A_V=0.15_–0.15^+0.30 mag. Using this sample we constrain the bright end of the z ∼ 8 UV luminosity function. When combined with recent empty field luminosity function estimates at similar redshifts, the resulting z ∼ 8 luminosity function can be equally well represented by either a Schechter or a double-power-law form. Assuming a Schechter parameterization, the best-fit characteristic magnitude is M^* =-20.95_–0.35^+0.30 mag with a very steep faint-end slope α=-2.15_–0.19^+0.20. These new candidates include some of the brightest objects found at these redshifts, 0.5-1.0 magnitude brighter than those found over CANDELS, and providing excellent targets for spectroscopic and longer-wavelength follow-up studies.