Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-07T23:28:59.338294Z
Paper Citation Record · LEDGER
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State?
As of 9 August 2026, this Paper Citation Record lists 35 of 35 outbound references and 0 inbound Pith citation observations for arXiv:2608.05794.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
35 of 35 outbound references displayed
- verified exact3
- verified fuzzy5
- unresolved27
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 847a20e1-6e66-4b0a-be26-5a4e9771cf61 · outbound
This paper cites Matter effects on binary neutron star waveforms.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Matter effects on binary neutron star waveforms
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.201656Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bbb0578a-92cc-4043-83ae-7149020bcb86 · outbound
This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.206325Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 557925ab-1ae7-4a11-9234-a9106b9e0dd2 · outbound
This paper cites Punturoet al., Class.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Punturoet al., Class
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.210661Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a4b42298-26f4-4e8d-a9e5-de9f646b5de0 · outbound
This paper cites Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.214976Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d17a5392-28f5-4df6-bfdc-e9b90de5e843 · outbound
This paper cites Measuring tidal effects with the Einstein Telescope: A design study.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Measuring tidal effects with the Einstein Telescope: A design study
Reference 5
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T23:28:59.695712Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 139f45c8-ff76-42dc-a6d6-34b86d68d22f · outbound
This paper cites an unresolved cited work.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Unresolved cited work
Reference 6
- Resolution
- unresolved
- raw_fallback, observed 2026-08-07T23:28:59.849305Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation d481d37a-2a75-446b-bf20-bf93c24cedcf · outbound
This paper cites an unresolved cited work.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Unresolved cited work
Reference 7
- Resolution
- unresolved
- raw_fallback, observed 2026-08-07T23:28:59.838225Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 0ff32805-b7b6-4cd8-bfe0-2532bd77c8ef · outbound
This paper cites Kashyap, I.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Kashyap, I
Reference 8
- Resolution
- verified exact
- raw_fallback, observed 2026-08-07T23:28:59.677996Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 22bb30af-577e-44bd-b125-552c88d8b582 · outbound
This paper cites A Bayesian investigation of the neutron star equation-of-state vs. gravity degeneracy.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? A Bayesian investigation of the neutron star equation-of-state vs. gravity degeneracy
Reference 9
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T23:28:59.605856Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 900cf5a4-d3fa-4544-b6f3-4055997e9732 · outbound
This paper cites Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.240925Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 606c7c47-1a0e-4df3-bdb6-989415c7576d · outbound
This paper cites Model Waveform Accuracy Standards for Gravitational Wave Data Analysis.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Model Waveform Accuracy Standards for Gravitational Wave Data Analysis
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.245354Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9d964be9-a846-4d34-ab78-aa0d995ae0c9 · outbound
This paper cites ripple: Differentiable and Hardware-Accelerated Waveforms for Gravitational Wave Data Analysis.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? ripple: Differentiable and Hardware-Accelerated Waveforms for Gravitational Wave Data Analysis
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.249603Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bfd7b786-8454-4727-bedc-7d2901a4983a · outbound
This paper cites Fast gravitational wave parameter estimation without compromises.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Fast gravitational wave parameter estimation without compromises
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.253721Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ee166c5a-c592-40cd-9f6d-57a073758832 · outbound
This paper cites Wouters, P.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Wouters, P
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.257680Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation aaa6d644-4254-4cce-af3f-6d7389ac77e4 · outbound
This paper cites Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Closed-form tidal approximants for binary neutron star gravitational waveforms constructed from high-resolution numerical relativity simulations
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.261537Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f5a33156-6f63-47ae-bcad-6c95b830fb1f · outbound
This paper cites Improving the NRTidal model for binary neutron star systems.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Improving the NRTidal model for binary neutron star systems
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.265501Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5924b22b-9d3f-4616-8f44-4f0c56d31a2e · outbound
This paper cites an unresolved cited work.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Unresolved cited work
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.269425Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a2a87a02-c1eb-4d30-90ea-46d9ba943739 · outbound
This paper cites an unresolved cited work.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Unresolved cited work
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.273378Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9d223eaf-d97e-47af-a79a-78f2266af38a · outbound
This paper cites an unresolved cited work.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Unresolved cited work
Reference 19
- Resolution
- unresolved
- raw_fallback, observed 2026-08-07T23:28:59.813395Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 3800c0e0-150e-49d0-b812-19b027999ee3 · outbound
This paper cites Typel, G.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Typel, G
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.280980Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 60ab7a67-909f-460e-b4a1-6e0ec46079e0 · outbound
This paper cites Multi-messenger Observations of a Binary Neutron Star Merger.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Multi-messenger Observations of a Binary Neutron Star Merger
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.284779Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 18efcd14-fc9f-4931-97aa-50cae5c3d893 · outbound
This paper cites A Hubble constant measurement from superluminal motion of the jet in GW170817.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? A Hubble constant measurement from superluminal motion of the jet in GW170817
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.288832Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2851b35d-d698-4515-9810-0e496c8d5b6c · outbound
This paper cites Jeffreys,Theory of Probability, 3rd ed.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Jeffreys,Theory of Probability, 3rd ed
Reference 23
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-07T23:28:59.794295Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 7239793c-48f5-4eff-8822-0de4731af26d · outbound
This paper cites Chabanat, P.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Chabanat, P
Reference 24
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-07T23:28:59.783147Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 66546818-a14b-4f08-bdf0-e40073cfe10a · outbound
This paper cites Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.300353Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation be5af378-31d4-4873-83b5-6bccff4531be · outbound
This paper cites Tidal Deformability Doppelgangers: Implications of a low-density phase transition in the neutron star equation of state.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Tidal Deformability Doppelgangers: Implications of a low-density phase transition in the neutron star equation of state
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.304316Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f22f5861-6e67-4eee-ac31-1f558322d7a3 · outbound
This paper cites how loud must a neutron-star merger be to reveal its equation of state?.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? how loud must a neutron-star merger be to reveal its equation of state?
Reference 27
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-07T23:28:59.772509Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 0787e555-989f-472d-9818-4113c811d817 · outbound
This paper cites how loud must a neutron-star merger be to reveal its equation of state?.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? how loud must a neutron-star merger be to reveal its equation of state?
Reference 28
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-07T23:28:59.762008Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 6c9cd1fe-d479-49c3-a279-dcd2021d36a7 · outbound
This paper cites $\texttt{GWFAST}$: a Fisher information matrix Python code for third-generation gravitational-wave detectors.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? $\texttt{GWFAST}$: a Fisher information matrix Python code for third-generation gravitational-wave detectors
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.315961Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6f637b88-1fc1-4355-9028-652f622eb667 · outbound
This paper cites Science-Driven Tunable Design of Cosmic Explorer Detectors.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Science-Driven Tunable Design of Cosmic Explorer Detectors
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.319722Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2f99b05c-6cb9-4b64-a007-4e536aa98b7e · outbound
This paper cites Branchesiet al., Journal of Cosmology and Astroparticle Physics2023(07), 068.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Branchesiet al., Journal of Cosmology and Astroparticle Physics2023(07), 068
Reference 31
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-07T23:28:59.751086Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation cc0cea6d-1288-416c-a333-6408c4226fba · outbound
This paper cites Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.327311Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 49a691a4-ef86-46f1-a3b2-7c1321528fc7 · outbound
This paper cites an unresolved cited work.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Unresolved cited work
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.331160Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fa1f13ce-755c-4edd-8835-39e4fb20f8f8 · outbound
This paper cites Chen and J.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Chen and J
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.334519Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 87865cbd-610e-4ce6-a6e2-70283b62ec80 · outbound
This paper cites A New Parameterization for the Lagrangian Density of Relativistic Mean Field Theory.
How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? A New Parameterization for the Lagrangian Density of Relativistic Mean Field Theory
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:28:59.338294Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
No inbound Pith citation observations are available.