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Paper Citation Record · LEDGER

On the usefulness of existing Solar-wind models for pulsar timing corrections

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1905.02989.

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

pith.paper-citation-record.v1
1905.02989 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:42:21.440622Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T05:42:21.989378Z

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 20d67a10-6691-4037-bae4-1a96ebe5d758 · inbound

Unlocking the hidden potential of pulsar astronomy cites this paper.

Unlocking the hidden potential of pulsar astronomy On the usefulness of existing Solar-wind models for pulsar timing corrections

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-08-07T05:42:21.992220Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-07T05:42:21.440622Z digest=sha256:d0cfa70f86f6b076aff4204266e359033b2104828b532c21b1baf03c0ccf7c5e

Observation 59c05d7f-58d3-4ab2-a1a1-6796b4e62417 · inbound

PSRDISP: A novel approach to modeling dispersive processes in single-pulsar noise analysis using epoch-wise dispersion measures cites this paper.

PSRDISP: A novel approach to modeling dispersive processes in single-pulsar noise analysis using epoch-wise dispersion measures On the usefulness of existing Solar-wind models for pulsar timing corrections

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-02T06:30:42.824794Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T06:30:42.824794Z digest=sha256:f7b39c3581851dbe5831c4cbfee40b762a7ce5aed3cff1630aa2fce6564e4824

Observation 795f45c6-63e6-4090-868e-875d774c35be · inbound

PSRDISP: A novel approach to modeling dispersive processes in single-pulsar noise analysis using epoch-wise dispersion measures cites this paper.

PSRDISP: A novel approach to modeling dispersive processes in single-pulsar noise analysis using epoch-wise dispersion measures On the usefulness of existing Solar-wind models for pulsar timing corrections

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-03T02:03:27.570501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T02:03:27.570501Z digest=sha256:3dd4a3091546d2c5d557533c2c3907262fa4654222b2871308a68da4dd978cc2