Temporal Aliasing in high-z Galaxies Applying the 1.085 Metric to MOM-z14

This research addresses the cosmological discrepancy presented by the high-redshift galaxy MOM-z14 ($z \approx 14$), whose observed stellar mass challenges standard Lambda-CDM models by appearing anomalous for its epoch. Rather than relying on unverified hypotheses such as Early Dark Energy, this paper applies the 1.085 Scaling Constant derived from the Gross-Observer Effect to resolve the anomaly as a case of Temporal Aliasing. The perceived mass excess is shown to be an artifact of an 8.5% synchronization lag between causal timelines. Applying this synchronization anchor adjusts the calculated baryonic mass into alignment with standard early-universe star-formation expectations, establishing the 1.085 metric as a universal calibration anchor for high-redshift datasets.