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Population parameters of intermediate age star clusters in the Large Magellanic Cloud, I NGC 1846 and its wide main sequence turnoff

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Figure

Figure 1. Difference in normalized instrumental F435W magnitude ( −2.5 log (e − s −1 )) derived from short vs
Figure 4. CMDs of stars in regions in color–magnitude space that have less than 10% of the field star contamination (see the text in Section 3.3)
Figure 8. Radial surface number density distributions of stars in different regions of the CMD, as depicted in Figure 7 with red solid lines
Figure 9. Dependence of three distance- and reddening-independent parameters involving fiducial points on the m F435W vs
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