We measured phosphorus abundances in 22 FGK dwarfs and giants that span ‑0.55 < [Fe/H] < 0.2 using spectra obtained with the Phoenix high-resolution infrared spectrometer on the Kitt Peak National Observatory Mayall 4 m telescope, the Gemini South Telescope, and the Arcturus spectral atlas. We fit synthetic spectra to the P i feature at 10581 Å to determine abundances for our sample. Our results are consistent with previously measured phosphorus abundances; the average [P/Fe] ratio measured in [Fe/H] bins of 0.2 dex for our stars are within ∼1σ compared to averages from other IR phosphorus studies. Our study provides more evidence that models of chemical evolution using the results of theoretical yields are underproducing phosphorus compared to the observed abundances. Our data better fit a chemical evolution model with phosphorus yields increased by a factor of 2.75 compared to models with unadjusted yields. We also found average [P/Si] = 0.02 ± 0.07 and [P/S] = 0.15 ± 0.15 for our sample, showing no significant deviations from the solar ratios for [P/Si] and [P/S] ratios.