$\mu$m flux in Janskys, d is the distance in parsecs, and 179.7 is the zero point flux in Janksys for the 4.5 $\mu$m IRAC band [@reach05]. Distances are taken from the literature, as described in Table \[tbl1\], and assumed to have $10\%$ uncertainty where none were provided. IRAC calibration uncertainties are $5-10\%$ for the 4.5 $\mu$m data. Later, in Section \[sec:M-Z\], we use these $M_{[4.5]}$ magnitudes to analyze the NIR luminosity-metallicity relationship. Similarly, $M_{K_S}$ values were determined by @dale09 from 2MASS imaging, where 666.7 is the zero point flux in Janksys for the 2MASS $K_S$ band. Although 2MASS $F_{K_S}$ values are available for those objects which [@dale09] don’t provide $K_S$ magnitudes, we choose not to use them. The small apertures used in the 2MASS extraction produce unexpectedly faint magnitudes for smaller galaxies when compared to similar extractions from IRAC 3.6 and 4.5 $\mu$m data , and so may not be terribly accurate for our sample. The $K_S$ magnitudes were used to determine stellar masses in Section \[sec:M-Z\].

Finally, *V*-band magnitudes were needed to calculate $B-V$ colors (see Table \[tbl1\]). When available, $M_{V}$ values were provided by @vanzee12, using the LVL elliptical aperture. In other cases, values are taken from [@devaucouleurs91] 