Image Details
Caption: Figure 5.
Joint posteriors of the constrained parameters after fitting a broken power law to the model-agnostic normalized variances estimates. Because the amplitude is well constrained within the range of baseline lengths for which good estimates of the variability exist, we set the normalization at ∣ u ∣ = 4 Gλ, denoted as a 4. Contours show the enclosed 50th, 90th, and 99th percentiles. The purple bands indicate the ranges used as priors during the full-track modeling, associated with the interquartile ranges.
© 2022. The Author(s). Published by the American Astronomical Society.