Substituting Daya Bay's measured antineutrino spectra for the Huber-Müller model in a KamLAND global fit lowers best-fit Δm²₂₁ to 7.50 × 10^{-5} eV² and trends tan²θ₁₂ downward, improving agreement with JUNO.
Measurement of the Electron Antineu- trino Oscillation with 1958 Days of Operation at Daya Bay
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Global Fit of KamLAND Data and the Daya Bay Antineutrino Energy Spectrum
Substituting Daya Bay's measured antineutrino spectra for the Huber-Müller model in a KamLAND global fit lowers best-fit Δm²₂₁ to 7.50 × 10^{-5} eV² and trends tan²θ₁₂ downward, improving agreement with JUNO.