Paper Citation Record · LEDGER

Properties of non-rotating and rapidly rotating protoneutron stars

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9908132.

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

pith.paper-citation-record.v1
astro-ph/9908132 v1

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

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:16:20.828270Z

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

21
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation ed3a2a15-f03f-4518-b832-22679d3ddf71 · inbound

The Properties of a Black Hole-Neutron Star Merger Candidate cites this paper.

The Properties of a Black Hole-Neutron Star Merger Candidate Properties of non-rotating and rapidly rotating protoneutron stars

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-14T14:16:20.828270Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ec563ddb-2d3a-4e16-857e-734d37eded2e · inbound

Optical Super-orbital Modulation of SMC X-1: Disk Precession and a Revised Pulsar Mass cites this paper.

Optical Super-orbital Modulation of SMC X-1: Disk Precession and a Revised Pulsar Mass Properties of non-rotating and rapidly rotating protoneutron stars

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-05-21T04:03:56.575662Z

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.