Super-K solar day/night amplitude A_DN vs Δm²21, extracted from PRD 109, 092001
Super-K SK-IV and SK-I–IV day/night amplitude-fit curves A_DN(Δm²21), vector-extracted
The day/night asymmetry from SK's amplitude fit as a function of Δm²21 for SK-IV and for SK-I–IV combined; the amplitude fit is what drives the solar–KamLAND Δm²21 comparison. Digitised / vector-extracted by the Newtrinos developers from published figures; scripts alongside the data.
Data card 3/11 sections
| Provenance | Extracted from the two A_DN(Δm²21) figures of PRD 109, 092001 with the scripts in the same folder (vector paths where available). |
|---|---|
| Validation | Checked against the published numbers / curves in the verification entries listed above. |
| Known limitations | Digitisation, not an official release; precision limited by the figure. Smoothed in the module with a ±0.5e-5 eV² running mean. |
Get it
| Location | Role | Host | Formats | Size |
|---|---|---|---|---|
| Newtrinos.jl repository | primary | GitHub | CSV / TSV |
Metadata
| Creators | Newtrinos developers |
|---|---|
| Owner | Newtrinos-org |
| Published | 2026 |
| Licence | MIT as part of Newtrinos.jl; the underlying figures belong to the collaborations / publishers |
| Access | Open |
| Experiments | Super-Kamiokande |
| Data levels | Digitised from figures, Binned observed data |
Used by
- Newtrinos Newtrinos.jl — modules
sk_solar_dn; verified in 10.1103_PhysRevD.109.092001
Know of another paper or code that uses this, or an input it depends on? Tell us.
Papers
- A_DN vs Δm²21 figures · doi:10.1103/PhysRevD.109.092001 · arXiv:2312.12907 (uses)
Related
- derived from doi:10.1103/PhysRevD.109.092001
Curation
| Status | Curated (candidate: harvested, not reviewed · curated: reviewed metadata · verified: resource downloaded and checked against its paper) |
|---|---|
| Added | 2026-10-23 |