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Galactic Pal eontology:abundance analysis of the disrupted globular cluster Palomar 5

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Figure

Fig. 1. CMD using SDSS photometry of stars within two half-light radii.Blue squares indicate foreground stars, open red symbols are AGB can-didates, while our RGB targets are shown as solid stars
Table 2. Properties of the target stars
Table 3. Linelist
Table 4. Abundance results from co-added spectra. Abundance ratios for ionized species are given relative to FeThe line-to-line scatter ii
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