Image Details

Choose export citation format:

Testing Warm Dark Matter with Kinematics of the Smallest Galaxies

  • Authors: M. Sten Delos, Niusha Ahvazi, Andrew Benson

M. Sten Delos et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

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).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse