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Revealing the Structure and Internal Rotation of the Sagittarius Dwarf Spheroidal Galaxy with Gaia and Machine Learning

  • Authors: Andrés del Pino, Mark A. Fardal, Roeland P. van der Marel, Ewa L. Łokas, Cecilia Mateu, and Sangmo Tony Sohn

2021 The Astrophysical Journal 908 244.

  • Provider: AAS Journals

Caption: Figure 5.

Calibrated CMD of Sgr. Black dots are Sgr selected members. Stars screened out as contaminants are shown in gray. The RR Lyrae and spectroscopically observed stars selected as Sgr members are shown in blue and red, respectively. Two isochrones from the PARSEC stellar evolution library have been drawn over the CMD: [Fe/H] = −3.3, 13.5 Gyr (orange) and [Fe/H] = −0.4, 5 Gyr (light blue).

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