No kilonova detected from sub-solar GW candidate S251112cm, but coincident IIb supernova SN 2025adtq yields suggestive evidence for the superkilonova channel, though inconclusive after accounting for chance coincidence.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 2verdicts
UNVERDICTED 2representative citing papers
A broad-mass-function population of primordial black holes formed at the QCD epoch predicts a merger rate of 0.8 per year that matches the S251112cm candidate, implying f_PBH > 0.04 if confirmed.
citing papers explorer
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Electromagnetic Follow-up of the Sub-Solar Mass Gravitational Wave Candidate S251112cm: Kilonova Constraints and a Coincident IIb Supernova
No kilonova detected from sub-solar GW candidate S251112cm, but coincident IIb supernova SN 2025adtq yields suggestive evidence for the superkilonova channel, though inconclusive after accounting for chance coincidence.
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Implications for Primordial Black Hole Dark Matter from a Single Subsolar Mass Gravitational-wave Detection in LVK O1--O4
A broad-mass-function population of primordial black holes formed at the QCD epoch predicts a merger rate of 0.8 per year that matches the S251112cm candidate, implying f_PBH > 0.04 if confirmed.