Pith. sign in

Paper Citation Record · LEDGER

Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the Small Magellanic Cloud

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1311.4343.

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

pith.paper-citation-record.v1
1311.4343 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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T05:41:08.776975Z

measured 0 of 1 external citation measurements

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 54eef3b7-cd8c-487f-a6c4-b7aaeaae998c · inbound

X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries cites this paper.

X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the Small Magellanic Cloud

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-11T05:41:08.776975Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T05:41:08.776975Z digest=sha256:5fa4a1787c315f5d569fc220996f9bad35e42883c086a298deaccdecaafa8751

Observation 69e7ac8e-cbb5-49a8-b047-b1376d9ec7e6 · 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 Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the Small Magellanic Cloud

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-04T17:48:13.967042Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T17:48:13.967042Z digest=sha256:faffa5e9e4a434016c913bd38830d441c6581967d84575108959c296e8072024