  We report experimental oscillator strengths for 28 infrared Fe I transitions,
for which no previous experimental values exist. These transitions were
selected to address an urgent need for oscillator strengths of lines in the
H-band (between 1.4 um and 1.7 um) required for the analysis of spectra
obtained from the Sloan Digital Sky Survey (SDSS-III) Apache Point Galactic
Evolution Experiment (APOGEE). Upper limits have been placed on the oscillator
strengths of an additional 7 transitions, predicted to be significant by
published semi-empirical calculations, but not observed to be so.
