Figure 6 from The Panchromatic Hubble Andromeda Treasury. III. Measuring Ages and Masses of Partially Resolved Stellar Clusters

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The Panchromatic Hubble Andromeda Treasury. III. Measuring Ages and Masses of Partially Resolved Stellar Clusters

Authors: Lori C. Beerman, L. Clifton Johnson, Morgan Fouesneau, Julianne J. Dalcanton, Daniel R. Weisz, Anil C. Seth, Ben F. Williams, Eric F. Bell, Luciana C. Bianchi, Nelson Caldwell, Andrew E. Dolphin, Dimitrios A. Gouliermis, Jason S. Kalirai, Søren S. Larsen, Jason L. Melbourne, Hans-Walter Rix, and Evan D. Skillman

Beerman et al. 2012 The Astrophysical Journal 760 104.

Provider: AAS Journals

Caption: Figure 6.

Recovered vs. input age of the simulated test clusters, color coded by the difference in recovered vs. input extinction, for four values of M _lim in the F814W filter. To clearly see the distribution of recovered values, Gaussian noise with a dispersion of σ = 0.05 dex in each direction was added in the upper panels. The bottom panels show the median for the residuals in log( t) for all clusters at each input age, along with the 16th and 84th percentile of the residuals.

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