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Utsumi, Y · 2017 · DOI 10.1093/pasj/psx118

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Heavy element dust explains the late-time spectra of kilonovae

astro-ph.HE · 2026-07-01 · unverdicted · novelty 6.0

Dust from refractory r-process elements forms efficiently in kilonova ejecta and explains the observed late-time infrared spectra.

Electromagnetic Follow-up of the Sub-Solar Mass Gravitational Wave Candidate S251112cm: Kilonova Constraints and a Coincident IIb Supernova

astro-ph.HE · 2026-05-11 · unverdicted · novelty 5.0

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.

Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy

astro-ph.HE · 2026-04-16

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Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy astro-ph.HE · 2026-04-16 · unreviewed · ref 71

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