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Paper Citation Record · LEDGER

A unified model of the magnetar and radio pulsar bursting phenomenology

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1101.1098.

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

pith.paper-citation-record.v1
1101.1098 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 2026-08-01T08:25:14.445941Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T20:19:55.597518Z

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 6a00e395-1d12-4546-969c-e94c6c6be97d · inbound

A Log-Uniform Initial Magnetic Field Distribution Explains Pulsar and Magnetar Populations through Magnetic Inclination Alignment cites this paper.

A Log-Uniform Initial Magnetic Field Distribution Explains Pulsar and Magnetar Populations through Magnetic Inclination Alignment A unified model of the magnetar and radio pulsar bursting phenomenology

Reference 237

Resolution
verified exact
local_arxiv, observed 2026-06-26T20:19:55.598874Z

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=2026-07-11T11:50:26.030339Z digest=sha256:2c874d21f9241566b18899834c5f0b26720bcadcb148966269f57764bba091e1

Observation 58706a4c-f12e-4ec0-9958-10a14bbb4ec4 · inbound

Tidal deformation and strain accumulation of solid compact stars cites this paper.

Tidal deformation and strain accumulation of solid compact stars A unified model of the magnetar and radio pulsar bursting phenomenology

Reference 72

Resolution
unresolved
no resolver link, observed 2026-07-14T03:15:05.552524Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T03:15:05.552524Z digest=sha256:c88433c8db7b728ec2d15b3fa69fe518143adf45377b731abedb7e6eaf07f017

Observation 7289ad25-f57c-4824-a591-e378493c8073 · inbound

Fast Inference on Astronomical Time Series with Trans-Dimensional Flow Matching Posterior Estimation cites this paper.

Fast Inference on Astronomical Time Series with Trans-Dimensional Flow Matching Posterior Estimation A unified model of the magnetar and radio pulsar bursting phenomenology

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-01T08:25:14.445941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T08:25:14.445941Z digest=sha256:2bfe77352a4ddf7ffa7b05ef1ad799f72b9427639a020dd715338be7b3b3422a