Pith. sign in

Paper Citation Record · LEDGER

Predicting the detectability of oscillations in solar-type stars observed by Kepler

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1103.0702.

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

pith.paper-citation-record.v1
1103.0702 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 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-25T14:15:55.326188Z

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 b768506d-999f-4f33-bf07-559e5c257778 · inbound

Asteroseismology of solar-type stars cites this paper.

Asteroseismology of solar-type stars Predicting the detectability of oscillations in solar-type stars observed by Kepler

Reference 115

Resolution
metadata mismatch
local_arxiv, observed 2026-05-25T14:15:55.329403Z

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=sha256:3042b4cfac90b4a5562584c439950cb9cbd29ef500987291f31c4558afa3e737

Observation b0429a88-f912-48b6-a02c-c3e3ba6e7e99 · inbound

Ensemble asteroseismology: An ensemble approach to detecting signatures of solar-like oscillations in K-dwarfs cites this paper.

Ensemble asteroseismology: An ensemble approach to detecting signatures of solar-like oscillations in K-dwarfs Predicting the detectability of oscillations in solar-type stars observed by Kepler

Reference 1

Resolution
verified exact
local_arxiv, observed 2026-05-25T03:05:15.470334Z

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:e0f6a47338b2c7e34982039e2351269bd77344ac08152df0c925ac272ccd5417