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Spatially Resolved Star Formation History of Sextans dSph

  • Authors: Andrés E. Piatti

Andrés E. Piatti 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 3.

Diagnostic CMD-fitting results for the Sextans dSph for one of the bootstrapping realizations. The top left panel shows the luminosity distribution (g0), comparing the observed data (red) and synthetic model (blue). The top right panel displays the significance of the residuals, defined as ﹩({\rm{o}}{\rm{b}}{\rm{s}}{\rm{e}}{\rm{r}}{\rm{v}}{\rm{e}}{\rm{d}}-{\rm{m}}{\rm{o}}{\rm{d}}{\rm{e}}{\rm{l}})/\sqrt{{\rm{m}}{\rm{o}}{\rm{d}}{\rm{e}}{\rm{l}}}﹩. The bottom panels provide the residuals distribution (left) and the color distribution (g − r)0 (right) comparing the data (red) and model (blue).

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