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Paper Citation Record · LEDGER

Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2007.01372.

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

pith.paper-citation-record.v1
2007.01372 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T02:15:27.549426Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T09:26:51.415042Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 66782265-9846-4746-957e-d3c589d7c903 · 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 Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass

Reference 59

Resolution
verified exact
arxiv_id, observed 2026-05-19T03:47:02.345854Z

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=2026-05-19T03:44:07.472458Z digest=sha256:2ec2ba21620a985cafb4367e658efdc9e20c1c76a4bd5622e514efc86802f7e8

Observation 678fd79b-a667-4e0c-9c9c-0ca10714e02c · inbound

Gravitational-wave astronomy requires population-informed parameter estimation cites this paper.

Gravitational-wave astronomy requires population-informed parameter estimation Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass

Reference 45

Resolution
verified exact
arxiv_id, observed 2026-05-10T08:22:37.254935Z

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=2026-05-10T08:19:46.145955Z digest=sha256:b903006364d6bab342bfc396d3c094ed59032cf29dfc690b14e426f00a994e43

Observation 2584af9d-2b98-4319-96d1-262d7f3c16cc · inbound

Gravitational-wave astronomy requires population-informed parameter estimation cites this paper.

Gravitational-wave astronomy requires population-informed parameter estimation Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-02T16:12:01.358739Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T16:12:01.358739Z digest=sha256:9d2fd210ed607396021ee9a436f4f65bf2182963d1a7b51bbab0b3e0c627ecab

Observation 772d15f0-4c61-4b36-b3a4-791316aa6a29 · inbound

Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.

Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass

Reference 14

Resolution
verified exact
arxiv_id, observed 2026-07-02T09:26:51.416415Z

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=2026-06-28T05:31:01.574505Z digest=sha256:d7536cda9809e10c15f7d96dba2356f78227e92d01c433b3f6995123fa895d07

Observation 1255d310-9e3f-40eb-90e3-140b7c0ac35a · inbound

Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.

Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Discriminating between Neutron Stars and Black Holes with Imperfect Knowledge of the Maximum Neutron Star Mass

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-03T02:15:27.549426Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T02:15:27.549426Z digest=sha256:c4699d6ea0f9cfdd5f4bcee0c4c23ec68458a8a44d185e4446bac20f06ae684a