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Paper Citation Record · LEDGER

The internal composition of proto-neutron stars under strong magnetic fields

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1606.04843.

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

pith.paper-citation-record.v1
1606.04843 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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:28:08.126519Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T14:28:13.270028Z

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 8b54076f-42dc-4398-9b3b-5994fdf851e0 · inbound

Constraints on maximum neutron star mass from proto-neutron star evolution cites this paper.

Constraints on maximum neutron star mass from proto-neutron star evolution The internal composition of proto-neutron stars under strong magnetic fields

Reference 26

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:28:13.327819Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-08-07T14:28:08.126519Z digest=sha256:529c98004619b2663e53c9b13523412451e8c3c490e89f33fcc78efc0e9dde6e

Observation 19b72db2-ce70-45db-9c29-b91db2ace0d6 · inbound

Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach cites this paper.

Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach The internal composition of proto-neutron stars under strong magnetic fields

Reference 56

Resolution
unresolved
no resolver link, observed 2026-07-13T05:17:12.889672Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T05:17:12.889672Z digest=sha256:45abf81cfaa3e990dac67ffb732e26b0bfa83df3adb33e76d182eb969a05ec25