No periodic radio technosignature above 0.146 W detected from 3I/ATLAS using FAST L-band observations and canonical polyadic decomposition analysis.
L., Rohlfs, K., & Hüttemeister, S
3 Pith papers cite this work. Polarity classification is still indexing.
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2026 3verdicts
UNVERDICTED 3representative citing papers
A CNN trained on AREPO simulations and synthetic observations reverts edge-on 13CO spectral data to top-down views of the CMZ as a proof-of-concept for supervised reversion.
Cryogenic phased array feed achieves 21-25 K system temperature over efficiency and 3D SVD noise reduction improves compact and extended HI source detection over traditional 2D methods.
citing papers explorer
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Periodic Radio Technosignature Search toward 3I/ATLAS with FAST
No periodic radio technosignature above 0.146 W detected from 3I/ATLAS using FAST L-band observations and canonical polyadic decomposition analysis.
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IRIS: Deciphering Spectral-Line Imagery of the Galactic Center by Machine-Learning on Simulations
A CNN trained on AREPO simulations and synthetic observations reverts edge-on 13CO spectral data to top-down views of the CMZ as a proof-of-concept for supervised reversion.
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Murriyang cryogenic phased array feed: spectral-line results and noise-reduction methods
Cryogenic phased array feed achieves 21-25 K system temperature over efficiency and 3D SVD noise reduction improves compact and extended HI source detection over traditional 2D methods.