Light curve photometry for a typical Cepheid from our sample. The average magnitude and its error are calculated using the GLOESS fits, shown in this plot as the continuous lines. In cases where the data were not well sampled, J, H, or Ks magnitudes are not plotted and were calculated by finding the average value of the data points (see Table 2). The FourStar data, plotted as stars, agree well with those of F12, as discussed in Section 2.4. In all cases, the J, H, and Ks fits are dominated by the F12 data. Error bars have been omitted for clarity; they are listed in Table 1.