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Globular Cluster Populations: First Results from S4G Early-type Galaxies

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Figure

Figure 1. Demonstration of the model subtraction for NGC 1553. We selected this galaxy as an example of a fairly luminous, extended galaxy in our sample
Figure 2. Demonstration of the model subtraction near the core of NGC 1553. The quality of the model subtraction is highly variable within a few kiloparsecs of the galaxy center.
Figure 5. Histogram of the apparent magnitude distribution for the combined source distribution of NGC 584 and NGC 1047
Figure 6. Surface-number-density radial profiles of candidate globular cluster populations
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