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Fig. 7


The combined XLFs of LMXBs in different environments plotted in the cumulative form. LX is the unabsorbed X-ray luminosity in 0.5–8 keV. The contribution of CXB sources was subtracted and the incompleteness correction was applied. The field XLF (solid) is normalized to the stellar mass of 1010 M. The normalizations of GC (dashed) and M 31 nucleus (dash-dotted) XLFs are arbitrary. The shaded areas around the curves show 1σ statistical uncertainty.

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