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We present a full analysis of galaxy major merger pair fractions, merger rates, and mass accretion rates, thus uncovering the role of mergers in galaxy formation at the earliest previously unexplored epoch of 4. 5<z<11. 5. We target galaxies with masses ₁₀ (M_*/M_) = 8. 0 - 10. 0, utilizing data from eight JWST Cycle-1 fields (CEERS, JADES GOODS-S, NEP-TDF, NGDEEP, GLASS, El-Gordo, SMACS-0723, MACS-0416), covering an unmasked area of 189. 36 arcmin². We develop a new probabilistic pair-counting methodology that integrates full photometric redshift posteriors and corrects for detection incompleteness to quantify close pairs with physical projected separations between 20 and 50 kpc. Our analysis reveals an increase in pair fractions up to z = 8, reaching 0. 211 0. 065, followed by a statistically flat evolution to z = 11. 5. We find that the galaxy merger rate increases from the local Universe up to z = 6 and then stabilizes at a value of 6 Gyr^-1 up to z = 11. 5. We fit both a power-law and a power-law + exponential model to our pair fraction and merger rate redshift evolution, finding that the latter model describes the trends more accurately, particularly at z = 8. 0 - 11. 5. In addition, we measure that the average galaxy increases its stellar mass due to mergers by a factor of 2. 77 0. 99 from redshift z = 10. 5 to z = 5. 0. Lastly, we investigate the impact of mergers on galaxy stellar mass growth, revealing that mergers contribute 71 25\% as much to galaxy stellar mass increases as star formation from gas. This indicates that mergers drive about half of galaxy assembly at high redshift.
Duan et al. (2024) studied this question.