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Tracing M22’s Origins: Spatial and Chemical Constraints on Its Formation History

  • Authors: Emanuele Dondoglio, Antonino P. Milone, Randa Asa'd, Anna F. Marino, Alessandra Mastrobuono-Battisti, Fabrizio Muratore, Tuila Ziliotto, Emanuele Bortolan, Giacomo Cordoni, Maria Vittoria Legnardi, Edoardo P. Lagioia, Marco Tailo

Emanuele Dondoglio et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 1.

Panel (a): chip #79 reduced OmegaCAM image of M22. Panel (b): qFIT vs. uSDSS of sources measured in chip#79, with the orange lines separating the stellar (black) from the excluded (gray). Panel (c): chip #81 and #89 footprints, colored in gray and teal, respectively. Panel (d): zoomed-in view of their coordinates (gray dots and teal crosses) in the overlapping area. Panel (e): chip #81 and #89 magnitude difference against uSDSS of chip #81. Gray and red lines indicate the zero-difference and the observed offset, respectively.

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