  We present our on-going work on the determination of elemental abundances of
giants in the Galactic Bulge by means of infrared spectroscopy. We show a
preliminarily reduced spectrum and a synthetic spectrum fit of the Bulge giant
Arp 4203 recorded with the near-infrared, high-resolution Crires spectrograph
mounted on the VLT during its science verification run in August 2006.
Abundances derived from this spectrum are discussed.
