Image Details
Caption: Figure 8.
Visualizations of 14 interesting candidate groups. These candidates were initially identified based on ETI signal characteristics and subsequently passed visual inspection, a process that confirms they do not exhibit obvious RFI features. These 14 groups are part of 33 such candidates selected in this work and are equal to those previously found by Y.-C. Wang et al. (2023).
© 2026. The Author(s). Published by the American Astronomical Society.