Image Details
Caption: Figure 7.
Posterior distributions of three SFE parameters for the best-fit UV LFs presented in Figure 3. The results are displayed in blue and red, differentiating between cases with and without consideration of dust attenuation. The contours are at the 68%, 95%, and 99% credible level. The values correspond to the 68% credible level.
© 2023. The Author(s). Published by the American Astronomical Society.