![Grad-CAM autopsy at an amplitude of 4.0. (a) Q2_bright_hit: D1-3 S-shaped, detected. (b) Q2c_bright_mis: D1-1 extreme drift, missed. Columns: input, Grad-CAM map, and CAM difference (injected minus clean). Inputs are shown as the detector sees them: the three ON panels side by side, with frequency running vertically; white lines mark panel boundaries and the green line the injection’s starting channel. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Missed-Detections.png?resize=1200%2C720&ssl=1)
[astro-ph.IM] Radio technosignature searches rely on machine learning detectors to shrink the candidate pool before a human looks at it.
radio technosignature
![The on-sky geometry of the Anti-Solar Point (ASP), the ecliptic, and the synthesized beams of the ATA-ASP campaign. See the pilot paper by Sheikh and Hort et al. 2026 for full detail [1]. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/A-Technosignature.png?resize=1200%2C719&ssl=1)
Posted inSETI & Technosignatures
A Technosignature Survey Of The Anti-Solar Point: The SETI Institute’s Largest-Ever Campaign With The Allen Telescope Array
[astro-ph.IM] The ATA-ASP campaign is a radio technosignature survey of the Anti-Solar Point as a “Schelling point”, using the Allen Telescope Array (ATA) in the Search for Extraterrestrial Intelligence (SETI).