Pith. sign in

Paper Citation Record · LEDGER

Glitching pulsars as gravitational wave sources

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2311.04586.

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

pith.paper-citation-record.v1
2311.04586 v2

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 2026-08-15T06:32:42.880941+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T11:42:10.875798Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T00:55:12.022859Z

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 9f24025e-223f-4102-a709-53ef37d85f54 · inbound

Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model cites this paper.

Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model Glitching pulsars as gravitational wave sources

Reference 119

Resolution
unresolved
no resolver link, observed 2026-08-05T11:42:10.875798Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T11:42:10.875798Z digest=sha256:ce6e9b71810bce463bd4b6e922acc3281c7fef762ea3f5a395b750c46ae32613

Observation 44bab0d8-1de7-4ad5-add3-b5379f303495 · inbound

Axial $w$-modes of anisotropic neutron stars cites this paper.

Axial $w$-modes of anisotropic neutron stars Glitching pulsars as gravitational wave sources

Reference 13

Resolution
verified exact
arxiv_id, observed 2026-05-11T16:21:08.290123Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-09T17:21:00.568089Z digest=sha256:64b5cfcb505c0d3d247e000377c4823aafe4372b6be786524fa9ec6b836ecba6

Observation 933d9e17-fef2-4b53-bd90-47109c4d801e · inbound

Axial $w$-modes of anisotropic neutron stars cites this paper.

Axial $w$-modes of anisotropic neutron stars Glitching pulsars as gravitational wave sources

Reference 13

Resolution
verified exact
arxiv_id, observed 2026-07-01T00:55:12.024583Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-07-01T00:50:25.466659Z digest=sha256:2d21a16c8e297017eb9909f0a59bc959b23f7bb660a765c2c2d39c2c2c0ae7e5