Image Details
Caption: Figure 4.
Stellar population synthesis modeling with Bagpipes. The left panel shows the observed galaxy SED and spectrum (black, showing only JWST photometry) after the application of the polynomial calibration with 1σ errors (assuming an error floor of 5%) and the median model (red). Additionally, the median model is shown at the full resolution (gold), highlighting the predicted emission features that are washed out by the instrumental resolution. In the right panel, we show the covariant posteriors for a number of key measured parameters after accounting for the magnification of the source.
© 2023. The Author(s). Published by the American Astronomical Society.