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CECILIA: The Mass–Metallicity Relation of Low-mass Galaxies at Cosmic Noon

  • Authors: Menelaos Raptis, Gwen C. Rudie, Ryan F. Trainor, Noah S. J. Rogers, Allison L. Strom, Nathalie A. Korhonen Cuestas, Caroline von Raesfeld, Ye Lin, Ojima Ojodomo Abraham, Christopher Chapman, Charles C. Steidel, Michael V. Maseda

Menelaos Raptis et al 2026 The Astrophysical Journal Letters 1004 .

  • Provider: AAS Journals

Caption: Figure 8.

Dynamical vs. stellar masses for the CECILIA Faint sample (pink squares) with the 1:1 line (black dashed). Dynamical masses are computed using the geometric mean of the spatial-profile-based and spectral-resolution-based size estimates to determine the effective radius of each object, as described in the text. Overall, the galaxies show good agreement between their dynamical and stellar masses.

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