Image Details
Caption: Figure 3.
Radio flux densities for AGNs observed in CEERS, JADES, and UNCOVER for α = 0.3 with detection limits for ngVLA (left column) and SKA (right column). The dotted, dashed, and dotted–dashed red and brown lines are H II region and SN flux densities for SFRs of 1, 3, and 10 M ⊙ yr−1, respectively. The black solid, dashed, and dotted horizontal bars show ngVLA and SKA limits for integration times of 1, 10, and 100 hr, respectively.
© 2024. The Author(s). Published by the American Astronomical Society.