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The SPARC sample consists of 175 nearby galaxies with modern surfacephotometry at $3.6\,\mu m$ and high quality rotation curves. The sample hasbeen constructed to span very wide ranges in surface brightness, luminosity,rotation velocity and Hubble type, thereby forming a representative sample ongalaxies in the nearby Universe. To date, the SPARC sample is the largestcollection of galaxies with both high-quality rotation curves and NIR surfacephotometry.  The neo-MOND model used here to analyse the SPARC sample recognizablyconforms to the general pattern of the classical MOND algorithm, with theprimary difference that, whereas the classical MOND model is purelyphenomonological, the neo-MOND model is a special case of a general theorymotivated by the ideas of Leibniz and Mach (not discussed here). The consequentmain results can be broadly summarized as follows:  (1) neo-MOND provides the basis for the derivation of a complete theory ofthe baryonic Tully-Fisher relation; (2) the details of the derivation provide ameans of setting absolute distance scales for disc galaxies independently ofstandard candles and the photometric method; (3) subsequent determinations ofdynamical mass (computed directly from neo-MOND fits to SPARC rotation curves)track photometric mass (estimated from SPARC surface photometry) across thewhole SPARC sample in a statistically perfect way.  To summarize, if the input to neo-MOND is disk dynamical data, then theoutput is whole-disk mass data together with absolute distance scales.

Modelling the SPARC galaxies using neo-MOND scaling relationships: the determination of distance scales and masses purely from disk dynamical data