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Paper Citation Record · LEDGER

Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0906.0766.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
0906.0766 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

184
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 523dd0e6-6471-4f5f-a22f-56c4ee0f0411 · inbound

Oscillations of red giant stars with magnetic damping in the core. II. Mixed mode visibilities on the red-giant branch cites this paper.

Oscillations of red giant stars with magnetic damping in the core. II. Mixed mode visibilities on the red-giant branch Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission

Reference 11

Resolution
verified exact
local_arxiv, observed 2026-06-28T03:31:30.923038Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:afd11648e0299cbcf131baba7580efb739c771655c31b5c069365c0c8bff0bbe

Observation 9476527b-4c4d-4dd2-ae5d-cfd2a7e30a82 · inbound

Unveiling the nature of barium stars. I. Asteroseismic masses and the evolutionary link between Ba dwarfs and giants cites this paper.

Unveiling the nature of barium stars. I. Asteroseismic masses and the evolutionary link between Ba dwarfs and giants Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-06-25T19:48:18.179395Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a1c7adc1639fc9e780c29b5e650a9f0517f5e9d91bd9ea6c285494b73bda9a33