Image Details
Caption: Figure 2.
﹩{L}_{\mathrm{HX}}﹩/SFR depends on gas-phase metallicity, as predicted by XRB population synthesis models (thick black line; Fragos et al. 2013a). This figure is modified from Basu-Zych et al. (2013b) to show the galaxies discussed in this paper, which appear as labeled encircled points.
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