Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Complementarity of $B\to K^{(*)} \mu \bar \mu$ and $B\to K^{(*)} + \mathrm{inv}$ for searches of GeV-scale Higgs-like scalars
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2306.09508.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T08:16:58.012221Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 76c2ebd5-fcfc-420e-9146-b551a64296f8 · inbound
Radiative generation of chiral vector operators in $b\to s \nu\bar{\nu}$ transition cites this paper.
Radiative generation of chiral vector operators in $b\to s \nu\bar{\nu}$ transition Complementarity of $B\to K^{(*)} \mu \bar \mu$ and $B\to K^{(*)} + \mathrm{inv}$ for searches of GeV-scale Higgs-like scalars
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T08:16:58.012221Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cdbc9a51-da99-475f-8e5b-5665270e60c1 · inbound
A Unified Dark Matter Explanation for $\boldsymbol{B^+ \!\to K^+\nu\bar{\nu}}$ and the Super-Kamiokande Antineutrino Excess cites this paper.
A Unified Dark Matter Explanation for $\boldsymbol{B^+ \!\to K^+\nu\bar{\nu}}$ and the Super-Kamiokande Antineutrino Excess Complementarity of $B\to K^{(*)} \mu \bar \mu$ and $B\to K^{(*)} + \mathrm{inv}$ for searches of GeV-scale Higgs-like scalars
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T04:08:44.112644Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.