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3D CMZ. V. A New Orbital Model of Our Galaxy’s Center, Informed by Data Across the Electromagnetic Spectrum

  • Authors: Dani R. Lipman, Cara Battersby, Daniel Walker, Maïca Clavel, B.L. DuBois, Adam Ginsburg, Jonathan D. Henshaw, Ralf S. Klessen, Elisabeth A.C. Mills, Francisco Nogueras-Lara, Mattia C. Sormani, Robin G. Tress

Dani R. Lipman et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure B1.

Prior and posterior PPDFs for all cloud masks in the catalog. Each panel shows priors for different methods as colored lines, and the posterior is indicated by a black solid line. We report the location of the peak (μ, vertical gray dashed–dotted line), the relative probability peak (A), and the 68% confidence interval (CI68, horizontal solid gray line), which are used to obtain a posterior PPDF distribution used for the orbital fitting procedure in Section 3.2.

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