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The discovery, abundances and [Fe/H]NB392 distributions of metal poor stars in the halo of the Milky Way

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Figure

Figure 1. An image of the observatory housing the Isaac NewtonTelescope which was used as the source for the catalogue of dataused in this study.
Figure 2. A demonstration of the variation in CaHK absorption within a G-type star’s spectra with changes in metallicity, [Fe/H]
Figure 3. A sample of galaxies and stars, selected from an NB392separated by a cut on a graph of the magnitude differencesagainstfilter catalogue of 123,505 sources using spectroscopic redshiftsof zspec = 0 for stars and 0.5 < zspec < 7.0 for galaxies, best U − J J − K.
Figure 5. A histogram of the error in the magnitude differenceg −i for the whole catalogue
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