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tokens: quality factors. A selection of these factors from the original sources is summarized below. 4.1. Selected Galaxy Information When measuring rotation curve data, there are many systematic issues that affect the accuracy of the information. In Oh et al. ( 2015 ), the authors gave a comprehensive discussion of each of the galaxies in the entire sample. Although both CG and MOND capture the essence of the rotation curves across the sample well, there are occurrences where it is useful to have the relevant information about the galaxy to understand why a fit may not be as precise. We have compiled some of the relevant information below for convenience. CVN (UGCA 292) is a gas rich dwarf galaxy in the Canes Venatici constellation. This galaxy has been shown to have a high gas mass fraction and low metallicity suggesting that it is highly unevolved with an extremely LSB (van Zee 2000 ). From a fitting point of view, this galaxy is unique with its extremely low rotational measured velocities. The models shown, however, provide a sufficient fit despite this property. DDO 133 (UGC 7698) is a large, faint galaxy in the Canes Venatici cloud whose extremely LSB shows high stellar evolution (Zhang et al. 2012 ). Due to its lack of tidal motions, this galaxy is assumed to be an isolated system, which is typically beneficial for obtaining a rotation curve. However, this rotation curve was studied by one of us in the past, and can be shown to have a lower than quoted inclination (O’Brien 2012 ). Hence, we use the inclination that was previously studied and published to alleviate any discrepancies. DDO 154 (UGC 8024) is an asymmetrical dwarf galaxy and is a member of the Coma Benenices star constellation. It has been proposed that it is a physical companion of the M64 group. The galaxy is very dim, presenting a low star formation rate and contains a very large amount of atomic hydrogen (Drexler 2006 ). The galaxy is also hypothesized to have a large dark matter to baryon ratio and hence is extremely important to this work. This galaxy has been studied in CG (Mannheim O’Brien 2012 ) after the initial THINGS survey was completed by Walter et al. ( 2008 ). It can be seen in this most recent survey that the alternative gravity models can circumvent the need for the quoted high dark matter to baryon ratio. DDO 168 (UGC 8320) is a galaxy in the Canes Venatici group and is a probable pair with UGC 8308 and sometimes included in the M51 group (Karachentsev et al. 2003 ). The galaxy has a large number of dispersed H ii regions, resulting in an unusual shape to the rotation curve. The essence of the rotation curve is captured in the fits, but due to the overall structure, one cannot expect a high-resolution fit. DDO 210 is located in the Aquarius star constellation. It was one of the original galaxies discovered by van den Bergh ( 1959 ) of the David Dunlap Observatory catalog (DDO) survey. This aquarius dwarf is extremely faint, and has a very LSB, though it contains