Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:gr-qc/0007074.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T06:36:36.270122Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-04T06:59:37.463311Z
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 55ef09a3-89b3-4325-b593-96b98dafb674 · inbound
Waveform Modelling for the Laser Interferometer Space Antenna cites this paper.
Waveform Modelling for the Laser Interferometer Space Antenna Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
Reference 70
- Resolution
- verified exact
- local_arxiv, observed 2026-05-24T05:23:57.466853Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 99412d1c-1173-43be-94c7-d8c8dd1722ba · inbound
Artificial Precision Timing Array: bridging the decihertz gravitational-wave sensitivity gap with clock satellites cites this paper.
Artificial Precision Timing Array: bridging the decihertz gravitational-wave sensitivity gap with clock satellites Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
Reference 77
- Resolution
- verified exact
- local_arxiv, observed 2026-05-24T05:13:56.180579Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 2d5ff124-06a9-4e87-888a-601feac06cab · inbound
Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals cites this paper.
Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
Reference 81
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T06:36:36.270122Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d09562fd-9d0e-4b62-b894-f91a74e8f72e · inbound
Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals cites this paper.
Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
Reference 17
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T18:21:07.955725Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation a79ce35e-3bc1-4899-906c-4bb0cbe0e0c0 · inbound
Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals cites this paper.
Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
Reference 17
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T04:36:00.065514Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ecb14a35-5c7e-469c-b8a7-1f60a7fc5c5f · inbound
Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals cites this paper.
Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
Reference 18
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T13:25:45.695055Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation aca077a2-c07f-45cd-aba1-9235b94506e6 · inbound
Rational Orbits and Gravitational Waves in Static Spherical Spacetimes: An Open-Source Numerical Framework cites this paper.
Rational Orbits and Gravitational Waves in Static Spherical Spacetimes: An Open-Source Numerical Framework Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
Reference 72
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T06:59:37.464768Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 000d52da-40be-4547-9566-db723e1a6e3a · inbound
Rational Orbits and Gravitational Waves in Static Spherical Spacetimes: An Open-Source Numerical Framework cites this paper.
Rational Orbits and Gravitational Waves in Static Spherical Spacetimes: An Open-Source Numerical Framework Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T10:46:55.180066Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4aa467d3-ce25-430e-98cb-8d8357755443 · inbound
Synergies Between Pulsar Timing Array and Astrometry cites this paper.
Synergies Between Pulsar Timing Array and Astrometry Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA
Reference 78
- Resolution
- verified exact
- local_arxiv, observed 2026-06-25T22:48:38.220441Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.