ALMA Identifies Ancient Starburst Galaxy as Likely Source of IceCube High-Energy Neutrino
Summary
Astronomers using ALMA have identified a compact, intensely star-forming galaxy from 11 billion years ago as the most likely source of a high-energy neutrino detected by IceCube. Gravitational lensing allowed detailed study of this dust-obscured galaxy, which is the strongest electromagnetic counterpart candidate linked to an IceCube neutrino event. The discovery helps bridge multi-messenger astronomy, connecting neutrino detections with their cosmic origins.
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Key quotes
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Located in the same patch of sky as a high-energy neutrino detected by the IceCube Neutrino Observatory, the galaxy is the most plausible electromagnetic counterpart candidate.
Gravitational lensing allowed astronomers to study a compact, dust-obscured galaxy from 11 billion years ago that is the most plausible counterpart candidate to an IceCube neutrino event.
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