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We study the evolution of the low-order moments of the galaxy overdensitydistribution over the redshift interval 0.7<z<1.5. We find that the varianceand the normalized skewness evolve over this redshift interval in a way that isremarkably consistent with predictions of first- and second-order perturbationtheory. This finding confirms the standard gravitational instability paradigmover nearly 9 Gyrs of cosmic time and demonstrates the importance of accountingfor the non-linear component of galaxy biasing to avoid disagreement betweentheory and observations.

Testing gravity on large scales. The skewness of the galaxy distribution at z~1