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Paper Citation Record · LEDGER

GW190814's secondary component with mass $(2.50-2.67)$ M$_{\odot}$ as a super-fast pulsar

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2007.02513.

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

pith.paper-citation-record.v1
2007.02513 v2

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 2026-08-16T06:30:59.297886+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:38:46.954357Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-15T15:58:54.575035Z

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 7575fbd4-9f82-48dc-9671-5841f83aaf71 · inbound

Bayesian inferences on covariant density functionals from multimessenger astrophysical data: The impacts of likelihood functions of low density matter constraints cites this paper.

Bayesian inferences on covariant density functionals from multimessenger astrophysical data: The impacts of likelihood functions of low density matter constraints GW190814's secondary component with mass $(2.50-2.67)$ M$_{\odot}$ as a super-fast pulsar

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-16T04:38:46.954357Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:38:46.954357Z digest=sha256:e23ca4f775a00b3b8a316cf81afa49941c653b144be41d3e107049de3fb1089c

Observation 50699409-aa04-446b-add7-4784aaa9df43 · inbound

Testing the nature of compact objects in the lower mass gap using gravitational wave observations cites this paper.

Testing the nature of compact objects in the lower mass gap using gravitational wave observations GW190814's secondary component with mass $(2.50-2.67)$ M$_{\odot}$ as a super-fast pulsar

Reference 87

Resolution
verified exact
local_arxiv, observed 2026-08-15T15:58:54.588334Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-08-15T15:58:53.841699Z digest=sha256:b36ad474039adaa9d9db0d6b8f5eda10f0b76cb71490a83d66fecaf69d5816f5

Observation 911a7b46-f40a-4726-b136-1d815e7e5dd2 · inbound

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition cites this paper.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition GW190814's secondary component with mass $(2.50-2.67)$ M$_{\odot}$ as a super-fast pulsar

Reference 143

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:07.067617Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:07.067617Z digest=sha256:9224acbbae3e1203e0e5075a86b9896d2f413ed50219690099bdf7a6feefd4b3