Image Details
Caption: Figure 4.
Total intensity of the wavefields in the two observations (with the wavefield intensities of the 19 subbands aligned using ﹩(\tau ,\dot{\tau })﹩ coordinates before summing). The color scale corresponds to ﹩{\mathrm{log}}_{10}| W(\tau ,\dot{\tau }){| }^{2}﹩ in arbitrary units. A plus sign denotes the measured center of the 2.4 ms feature in both panels. The excess noise around τ = 0, 1.6, and 3.2 ms (as well as, more faintly, at 0.8 and 2.4 ms) is due to the regular pulse emission. An interactive version of this figure, which shows the ﹩(\tau ,\dot{\tau })﹩ wavefields for each frequency band, is available on the Journal website.
(An interactive version of this figure is available.)
An interactive version of this figure is available in the online journal.
© 2023. The Author(s). Published by the American Astronomical Society.