Paper Citation Record · LEDGER

Origin of the Soft Excess in X-ray Pulsars

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0407115.

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

pith.paper-citation-record.v1
astro-ph/0407115 v2

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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T17:48:13.859010Z

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

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

188
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 1ea5e206-c10b-4a70-b519-ec9c3ef62a78 · inbound

Iron line diagnostics of the stellar wind in X1908+075 cites this paper.

Iron line diagnostics of the stellar wind in X1908+075 Origin of the Soft Excess in X-ray Pulsars

Reference 87

Resolution: verified exact; local_arxiv, observed 2026-05-20T09:28:09.975624Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation bb22189f-f14e-4f12-ba5f-063198536764 · inbound

A multi-epoch spectral and photometric study to understand the nature of the interesting Be star candidate HD 249179 cites this paper.

A multi-epoch spectral and photometric study to understand the nature of the interesting Be star candidate HD 249179 Origin of the Soft Excess in X-ray Pulsars

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-04T17:48:13.859010Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.