Fig. C.7.
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Comparison of derived mean stellar population properties between GIST and NGIST for galaxy IC 1711. The left column shows GIST output for age (top) and metallicity [M/H] (bottom), whereas the right column shows the results from NGIST. For both the GIST and NGIST runs, cubes were binned to S/N = 100 (using the binning maps created by NGIST), and all other input parameters were kept identical.
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