Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1305.7197.
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 2026-08-11T14:29:01.341045Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-12T00:41:18.988335Z
Reference resolution
0 of 0 outbound references displayed
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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 8de087fe-aa71-45e3-9e9c-f5d17b44372a · inbound
Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons cites this paper.
Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state
Reference 110
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T14:29:01.341045Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c708d623-c6d7-4a94-8e74-a44b66f6b6ad · inbound
Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides cites this paper.
Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T16:33:19.613606Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 45ddba0e-fe89-42e4-b34c-9b86396459d5 · inbound
Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model cites this paper.
Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state
Reference 121
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T11:42:10.888512Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 80e62f4f-e9ff-4b25-8e7f-000be39574cf · inbound
Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field cites this paper.
Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T18:11:08.778273Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d3fb37a0-9d8c-4252-a55c-c7b9e422576a · inbound
Non-radial pulsations of gravitationally coupled two-fluid neutron stars in general relativity cites this paper.
Non-radial pulsations of gravitationally coupled two-fluid neutron stars in general relativity Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state
Reference 49
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T18:38:38.724744Z
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.