Pith. sign in

Paper Citation Record · LEDGER

New gravitational waveform model for precessing binary neutron stars with double-spin effects

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2311.15978.

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

pith.paper-citation-record.v1
2311.15978 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T12:28:44.164542Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-23T23:58:38.822605Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 5f7b67eb-32f5-41e7-a31b-e22d57309b08 · inbound

Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object cites this paper.

Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object New gravitational waveform model for precessing binary neutron stars with double-spin effects

Reference 84

Resolution
verified exact
arxiv_id, observed 2026-05-23T23:58:38.825554Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-23T23:58:10.771496Z digest=sha256:e8f8edc27cf04b668da532249bf0657a33ea4124ccc1a42e3b46280cb141f8ca

Observation a5e62349-e668-4e45-8939-4989e6bce9e7 · inbound

Tidal contributions to the full gravitational waveform to the second-and-a-half post-Newtonian order cites this paper.

Tidal contributions to the full gravitational waveform to the second-and-a-half post-Newtonian order New gravitational waveform model for precessing binary neutron stars with double-spin effects

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-11T12:28:44.164542Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T12:28:44.164542Z digest=sha256:06aa5a21edd64af39f12dd04b2a4232740a02cff9643dc2a082aeab40dc592f2

Observation a3d91f20-7acd-4c4b-aa20-282dbfbb08b0 · inbound

Fast frequency-domain gravitational waveforms for precessing binaries with a new twist cites this paper.

Fast frequency-domain gravitational waveforms for precessing binaries with a new twist New gravitational waveform model for precessing binary neutron stars with double-spin effects

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-11T10:24:53.475976Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T10:24:53.475976Z digest=sha256:202c524ce66b9a6dc75d038df3c9b1010dd8d1b293c1bc30806fa15306801438

Observation e91c65fa-4706-4b8d-ab66-ae983f8eae08 · inbound

Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries cites this paper.

Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries New gravitational waveform model for precessing binary neutron stars with double-spin effects

Reference 115

Resolution
unresolved
no resolver link, observed 2026-08-09T00:23:46.967453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T00:23:46.967453Z digest=sha256:e87e9976ecfbf0795bc33de0283e71a2d4bf57fe43c746031c98dca5c5ac809e

Observation 876eb93b-7afd-4119-b2fc-8422f99a91d7 · inbound

A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences cites this paper.

A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences New gravitational waveform model for precessing binary neutron stars with double-spin effects

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-06T22:15:37.363005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T22:15:37.363005Z digest=sha256:518c7c0266eb7c67258e8ff8cdf3cef7c04636e402085b2587a617c135acd29a

Observation fc1b8fb1-2bd3-46d1-9394-5c88d2567985 · inbound

Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run cites this paper.

Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run New gravitational waveform model for precessing binary neutron stars with double-spin effects

Reference 179

Resolution
unresolved
no resolver link, observed 2026-08-05T14:59:58.280316Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T14:59:58.280316Z digest=sha256:47b49631bb86e42102827a4ed7e67df3dea2d62a10893a12673d6d350f24aa57

Observation 4a55467a-f948-4ae1-9c0c-dd2d9cff2ba1 · inbound

Agnostically decoding gravitational wave model deficiencies in GWTC-3 cites this paper.

Agnostically decoding gravitational wave model deficiencies in GWTC-3 New gravitational waveform model for precessing binary neutron stars with double-spin effects

Reference 63

Resolution
verified exact
arxiv_id, observed 2026-05-12T09:31:26.719467Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-07T10:37:26.702450Z digest=sha256:655129eecc219862000c78a351758cebfdb5622062483b08917d881677fe2e1a

Observation a055d57f-c26e-449f-b1d4-dc5a28b3962a · inbound

Cosmological constraints and standard sirens forecasts for non-dynamical dark energy in Horndeski gravity cites this paper.

Cosmological constraints and standard sirens forecasts for non-dynamical dark energy in Horndeski gravity New gravitational waveform model for precessing binary neutron stars with double-spin effects

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-08T00:42:49.889777Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T00:42:49.889777Z digest=sha256:ad2f840026cc55f1f8a317f8392f80de5b83bd418bbfd699fa25959c44b650e8