Metric-background dependence of inferred galaxy properties at z ≃ 14: A bounded GCFT benchmark remapping of MoM-z14 and PAN-z14-1

This publication presents a reproducible metric-background remapping of the spectroscopically confirmed high-redshift galaxies MoM-z14 at z=14.44z=14.44z=14.44 and PAN-z14-1 at z=13.53z=13.53z=13.53. Detector-level observables—including angular morphology, observed flux density, and sealed redshift coordinates—are held fixed, while inferred physical radius and monochromatic luminosity density are recalculated using the bounded GCFT background and an independently reproduced Lambda-CDM control. Under the GCFT conversion, the central MoM-z14 radius estimates transfer from 74 to 142.3 pc and from 147 to 282.7 pc. The corresponding PAN-z14-1 radius definitions transfer from 233 to 456.6 pc and from 443 to 868.1 pc. For the source-authoritative MoM-z14 NIRCam photometry, eighteen positive-flux luminosity transfers are supported, with a central GCFT-to-control monochromatic-luminosity ratio of 3.720877. The associated −1.4266-1.4266−1.4266 mag distance-modulus shift is reported only as a conditional fixed-semantics identity. Under the shared metric-redshift and distance-duality contract, the pure distance factor in Lν/R2L_ν/R^2Lν/R2 cancels to numerical unity. The analysis deliberately withholds PAN luminosity remapping, numerical remapping of the source-reported MoM MUVMUVMUV, absolute GCFT cosmic age, and all stellar-population, halo-abundance, survey-population, model-selection, or GCFT-preference claims for which the required authority is absent. Scientific values remain governed by the sealed predecessor records; this CDN-567 / GCFT-0567-R5 Art Edition is an additive presentation and release derivative. It is an independent Aporion Dynamics preprint, distributed under CC BY 4.0, and has not been peer reviewed.