Image Details
Caption: Figure 9.
MZR for the CECILIA Faint sample when including all galaxies (purple solid line) and when excluding the two lowest-mass systems (blue dashed line and shaded region). The relations are compared to the K. Nakajima et al. (2022) O3-based calculated KBSS MZR.
© 2026. The Author(s). Published by the American Astronomical Society.