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EXPLORING THE OVERABUNDANCE OF ULXs IN METAL- AND DUST-POOR LOCAL LYMAN BREAK ANALOGS

  • Authors: Antara R. Basu-Zych, Bret Lehmer, Tassos Fragos, Ann Hornschemeier, Mihoko Yukita, Andreas Zezas, and Andy Ptak

2016 The Astrophysical Journal 818 140.

  • Provider: AAS Journals

Caption: Figure 6.

As in Figure 5, the black points show the observed XLF and the thicker gray line shows the input standard XLF (without source blending effects) in both panels. The simulated XLFs are displayed in different colors and line styles to show the effects of varying normalizations and bright-end slopes, respectively. Table 4 provides the parameter values that correspond to the models. Model #1 refers to the standard star-forming galaxy XLF.

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