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Paper Citation Record · LEDGER

What a Two Solar Mass Neutron Star Really Means

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1012.3208.

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

pith.paper-citation-record.v1
1012.3208 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 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:29:49.053779Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T10:51:56.091762Z

Reference resolution

0 of 0 outbound references displayed

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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 1b7acc7d-c6aa-4bf7-b12a-ffcd77cfab81 · inbound

A unified binary neutron star merger magnetar model for the Chandra X-ray transients CDF-S XT1 and XT2 cites this paper.

A unified binary neutron star merger magnetar model for the Chandra X-ray transients CDF-S XT1 and XT2 What a Two Solar Mass Neutron Star Really Means

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-14T15:29:49.053779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T15:29:49.053779Z digest=sha256:d18507bd268dad4509fae3e8364400d95377f5817e8117f753d8b74a79156b6a

Observation e12e0ecb-d1a1-4ec7-8232-cdb84c96b420 · inbound

Cold quark matter with heavy quarks and the stability of charm stars cites this paper.

Cold quark matter with heavy quarks and the stability of charm stars What a Two Solar Mass Neutron Star Really Means

Reference 3

Resolution
verified exact
local_arxiv, observed 2026-08-14T10:51:56.096327Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-14T10:51:55.838508Z digest=sha256:6af7adf1102ca6673e0e1bac770ad1f9f952c247db3e9cfb2b624e85eb3ceae2

Observation e60019b9-653d-4aa1-ab36-a1de9920586b · inbound

Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations cites this paper.

Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations What a Two Solar Mass Neutron Star Really Means

Reference 236

Resolution
unresolved
no resolver link, observed 2026-08-09T23:06:18.302547Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T23:06:18.302547Z digest=sha256:200b8c944ebb64ed49fb565ae7f3b70d5dcb657947efbaacf36175593c60b2db