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The bulge is one of the oldest, yet very metal-rich Galactic components suggesting that it experienced early, rapid chemical enrichment. Yet, the first, metal-poor stars to have formed in the Universe are predicted to be found in this central region of the Milky Way. I will present results from our endeavour to detect and characterize signatures from such stars. The chemical abundances of our candidates (at [Fe/H] of -1.5 to -2.6 dex) vastly overlap with those of halo stars and our sample also contains one CEMP-s and a CH-star - the first detections of such objects in the bulge. While we do not see any evidence of Population III enrichment in our sample, the chemical abundance patterns still give a deep insight into the dominant enrichment mechanisms in the early phases of galaxy assembly. This can be contrasted to observations of other, most metal-poor stellar systems such as globular clusters. |
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