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Paper Citation Record · LEDGER

Quasiuniversal properties of neutron star mergers

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1402.6244.

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

pith.paper-citation-record.v1
1402.6244 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:18:07.040169Z

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

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External citation measurements

128
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation e4de3d3c-2762-42c9-be12-695a4d3f0b04 · inbound

Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data cites this paper.

Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data Quasiuniversal properties of neutron star mergers

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-14T13:18:07.040169Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:18:07.040169Z digest=sha256:f965c32270591389058fdd3f46aacc7cde46e2005825b744410e945cb2ddfede

Observation 6db60bec-725b-4d5b-b0db-b0ae9d932326 · inbound

kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter cites this paper.

kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter Quasiuniversal properties of neutron star mergers

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-14T10:20:11.418025Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:20:11.418025Z digest=sha256:debf1375eddfe5c1610a20ffc16a13cbac7c31a7671901b9827ca76f6f64966e

Observation a8d80832-9a5d-4f67-85ec-64fc6286e90c · inbound

Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars cites this paper.

Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars Quasiuniversal properties of neutron star mergers

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-11T18:36:01.107230Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T18:36:01.107230Z digest=sha256:b626bcf0ced29a8b2fe48d9e98c297cef3c9f44ef4de489dee5c6112662a05e1

Observation 32f9bbbc-6052-4c1e-8db6-4a211ee20f8a · inbound

Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter cites this paper.

Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter Quasiuniversal properties of neutron star mergers

Reference 101

Resolution
verified exact
local_arxiv, observed 2026-05-19T03:47:01.857214Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-19T03:44:07.472458Z digest=sha256:50a0295e17877f11ed10006d89ff99941adaf167704e802c32caa5e56f7fcd0f

Observation bd92a297-a518-46ac-886b-38309c66a4da · inbound

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers cites this paper.

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers Quasiuniversal properties of neutron star mergers

Reference 160

Resolution
verified exact
local_arxiv, observed 2026-07-09T20:06:29.541911Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ba77fab2e4688afd0533ff1df34642974647e06b0da8cb818fbfab23fe17cd27

Observation 3d77f522-b020-464e-b8ce-95c8ee8dff2c · inbound

High-Density Sound Speed and Post-Merger Dynamics cites this paper.

High-Density Sound Speed and Post-Merger Dynamics Quasiuniversal properties of neutron star mergers

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-01T22:58:58.628640Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T22:58:58.628640Z digest=sha256:31b5b1d26ffe6428e804549878e85eb2f0ce057813fca003cccdb0c8695d5a08

Observation 4cd239e5-2ff9-4c9d-9c37-c33246142237 · inbound

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope cites this paper.

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope Quasiuniversal properties of neutron star mergers

Reference 184

Resolution
unresolved
no resolver link, observed 2026-08-01T09:39:03.161942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T09:39:03.161942Z digest=sha256:cd4d762a35b65c78424e9672faf4d49ea7f3715adcdcdcf43d308e50a7c02f5e