Image Details
Caption: Figure 5.
The effective radius as a function of stellar luminosity for the ERQs in comparison with inactive galaxy samples (A. van der Wel et al. 2014). The blue (red) line represents the relation for early-type (late-type) galaxies at z ∼ 2.25. The 1σ errors of the relations are marked with color-shaded regions. The error bars on the half-light radii also include a 0.1 dex (1σ) systematic uncertainty.
© 2026. The Author(s). Published by the American Astronomical Society.