Searching for stars ejected from the Galactic Centre in DESI

Open Access

Fig. 5

Relative contributions of Splash, GSE, and GC ejecta for stars with |L_Z| < 500 kpc km s⁻¹ as a function of metallicity. The rows show the number of stars and fraction in each population, while the columns show dwarfs and giants. The horizontal error bars correspond to the bin size in [Fe/H], and the vertical error bars are from the 16th and 84th percentiles of the posterior.

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