Paper Citation Record · LEDGER

Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1509.00512.

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

pith.paper-citation-record.v1
1509.00512 v1

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 9 of 9 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 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:58:53.903748Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T09:26:51.290599Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 75569314-2469-4081-bc09-417ec1ebaea1 · inbound

Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties cites this paper.

Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-14T11:35:56.195075Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e37acb4-5159-488d-8f3d-845b31d600aa · inbound

Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia cites this paper.

Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-06T22:29:59.440960Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 55d74e2b-5a25-44f8-a164-b43b9f0e9e94 · inbound

Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity cites this paper.

Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-06T21:32:50.544798Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 84cb1307-99a2-4444-a93e-1627c5032299 · inbound

Primordial black holes versus their impersonators at gravitational wave observatories cites this paper.

Primordial black holes versus their impersonators at gravitational wave observatories Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

Reference 96

Resolution: verified exact; local_arxiv, observed 2026-05-21T22:15:42.066281Z

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.

Observation 9fe9fb22-edf1-4f7a-8f88-22a39821f455 · 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 Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-15T15:58:53.903748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95c8bda4-8812-449d-820a-b3dd7f47afa7 · 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 Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

Reference 81

Resolution: verified exact; local_arxiv, observed 2026-07-02T09:26:51.291808Z

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.

Observation 8f5b0010-8af4-403a-9bb4-9f5805c2b313 · 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 Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-03T02:15:35.934622Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3ebbccd8-4a77-4529-bffc-99449d1be16e · inbound

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures cites this paper.

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-01T09:55:45.286465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 161bf264-dfb4-424e-abe4-b0819a8e4ef0 · inbound

A story about a tipsy kangaroo: Reversible jump MCMC for model selection in the analysis of gravitational-wave signals from the coalescence of compact objects cites this paper.

A story about a tipsy kangaroo: Reversible jump MCMC for model selection in the analysis of gravitational-wave signals from the coalescence of compact objects Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-01T07:26:22.596653Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.