SNO combined three-phase analysis: polynomial P_ee fit, covariance and sensitivity tables

SNO combined analysis (2013): ⁸B flux, P_ee polynomial with covariance, S(Eν) sensitivities

Data sets SNO Solar Oscillation parameters Flux modelling Curated

The parameterised result of the SNO combined three-phase analysis (Phys. Rev. C 88, 025501): ⁸B flux and day/night survival-probability polynomial coefficients with their covariance (Tables XXIV, XXV), and the CC/ES day/night sensitivity functions S(Eν) (Appendix B, Table XXVI) needed to use the result in fits (Sec. VI B).

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https://doi.org/10.1103/PhysRevC.88.025501 primaryJournal supplementPDF (tables in document)
transcription in Newtrinos.jl mirrorGitHubCSV / TSV

Metadata

CreatorsSNO Collaboration
Published2013
LicenceNo licence stated
AccessOpen
Experiments SNO
ChannelsCharged current (CC), Neutral current (NC), Elastic scattering on electrons (ES)
Detector technologyHeavy-water Cherenkov
Data levelsSummary values, Detector response, Systematics model
Covariance / systematics / MCyes / /
Result ofdoi:10.1103/PhysRevC.88.025501

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StatusCurated (candidate: harvested, not reviewed · curated: reviewed metadata · verified: resource downloaded and checked against its paper)
Added2026-10-23

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