Image Details
Caption: Figure 8.
A histogram of the distribution of masses for the subset of 186 embedded cluster candidates with an F150W peak pixel S/N > 5. There are two sources with mass estimates below 102 M⊙ not shown. The maroon error bars show the 1σ standard deviations from Monte Carlo simulations for each bin with at least one embedded cluster candidate.
© 2025. The Author(s). Published by the American Astronomical Society.