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Semiresolved Stellar Populations as Distance Indicators

  • Authors: Ignacio Martín-Navarro, Patricia Iglesias Navarro, Francesco La Barbera, Alexandre Vazdekis, Michael A. Beasley, Marc Huertas-Company, ChangHoon Hahn, Luis Peralta de Arriba, Isaac Alonso Asensio, Eirini Angeloudi, Miguel Cerviño, Katja Fahrion, Tereza Jerabkova, Jesús Falcón-Barroso, Sebastián F. Sánchez, Prashin Jethwa

Ignacio Martín-Navarro et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 2.

(Top) The I-band brightness profile is shown in blue, with the regions corresponding to the spectra selected for the analysis marked with purple symbols. (Bottom) Some examples of different OSIRIS spectra, color-coded by their r-band magnitude. The bottom panel shows the smoothed (wide lines) and raw (thin lines) residuals with respect to the mean spectrum.

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