Image Details
Caption: Figure 5.
Best-fit τ and ﹩\dot{\tau }﹩ (with error bars) inferred from Gaussian fits to the 2.4 ms feature across three frequency bands on MJD 58245. The contours mark the 1σ widths of the Gaussians. The center and widths for a fit for the total intensity on MJD 58298 are shown for comparison.
© 2023. The Author(s). Published by the American Astronomical Society.