Image Details
Caption: Figure 12.
Absolute V-band magnitude MV, half-light radius rh, and pericenter radius rp for GALACTICUS analogs of Segue 1, Tri II, and Tuc V. The left-hand panel shows the distribution of MV for analogs selected by rh and rp; the middle panel shows the distribution of rh for analogs selected by MV and rp; and the right-hand panel shows the distribution of rp for analogs selected by MV and rh. For comparison, the dotted curves show the uncertainty distributions of the observationally inferred values (which can exhibit minor discontinuity due to how we model asymmetric uncertainties).
© 2026. The Author(s). Published by the American Astronomical Society.