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A DEEPER LOOK AT LEO IV: STAR FORMATION HISTORY AND EXTENDED STRUCTURE

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Figure

Figure 1. Left: CMD of Leo IV within r h = 2.85 arcmin. We note several regions marking off particular stellar populations
Table 1 Leo IV Photometry
Figure 3. Stellar profile of Leo IV. The data points are the binned star counts for all stars within the CMD selection box shown in Figure 2
Figure 4. Smoothed contour plots of Leo IV, showing the 3σ , 4σ, 5σ , 6σ , 7σ , 10σ , and 15σ levels
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