Paper Citation Record · LEDGER

How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State?

As of 17 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.

pith.paper-citation-record.v1
2608.05794 v2

Coverage vector

measured 35 of 35 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-11T04:21:33.152456Z

measured 35 of 35 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

35 of 35 outbound references displayed

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External citation measurements

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Outbound references

Observation 98cfbb60-1d50-435d-b23a-022bca374229 · 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 2026-08-11T04:21:32.845474Z

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Unavailable: canonical work link unavailable.

Observation 7a99695f-e11f-42ee-9a75-56d3fdbf50b6 · 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 2026-08-11T04:21:32.857447Z

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Observation c92ade23-eead-4f4f-9b70-0bf2472364af · 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 2026-08-11T04:21:32.864894Z

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Observation 1ec614ea-823b-48bd-81c0-48bef8bdd13a · 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 2026-08-11T04:21:32.875423Z

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Observation 045a56fc-5e66-4ad8-8471-d17a8f53dc9a · 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: unresolved; no resolver link, observed 2026-08-11T04:21:32.882286Z

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Observation 07a4b1c7-a815-4d8d-9540-281e3e459133 · 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; no resolver link, observed 2026-08-11T04:21:32.888385Z

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Observation 4e837716-ab55-4f4f-b7e2-07a9da809928 · 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; no resolver link, observed 2026-08-11T04:21:32.896774Z

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Observation c77dd5ff-a3a8-4877-b92c-92419c135540 · 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: unresolved; no resolver link, observed 2026-08-11T04:21:32.903907Z

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Observation 1e1e854a-2c33-4b16-a918-16c5eb7447c1 · 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: unresolved; no resolver link, observed 2026-08-11T04:21:32.912846Z

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Observation 6a98c0b6-71bd-4cbe-a392-3b293762e146 · 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 2026-08-11T04:21:32.921056Z

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Observation 847756e8-5572-4f14-9352-bd246d3bdf57 · 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 2026-08-11T04:21:32.935146Z

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Observation 7dd93f54-9261-4387-8800-1245bec97c7c · 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 2026-08-11T04:21:32.946679Z

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Observation 45dd2add-ee3f-486b-be7b-ab5862286aba · 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 2026-08-11T04:21:32.957452Z

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Observation de555e8a-bce0-4b4f-a9d5-875afa721630 · 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 2026-08-11T04:21:32.965737Z

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Observation e68441f4-8177-4c27-8060-b48a4fe7520a · 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 2026-08-11T04:21:32.971745Z

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Observation ec4cf037-2eed-40f9-89ce-f6a88a7526ce · 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 2026-08-11T04:21:32.978550Z

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Observation 5237d142-885c-44df-bd27-53f5130b109a · 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 2026-08-11T04:21:32.985624Z

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Observation e9fd93c6-681d-44ed-8a17-94d8b94f759f · 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 2026-08-11T04:21:32.996946Z

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Observation aefc5ac2-a001-4c1a-bce9-d504d975a510 · 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; no resolver link, observed 2026-08-11T04:21:33.006679Z

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Observation 7480e6cb-974f-421c-95f5-0642a759baf5 · 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 2026-08-11T04:21:33.016411Z

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Unavailable: canonical work link unavailable.

Observation b1788e9c-47a5-4911-9871-b03833f8d902 · 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 2026-08-11T04:21:33.025076Z

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Observation 9a18e248-4511-4a52-a83b-84cb12164b62 · 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 2026-08-11T04:21:33.035162Z

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Observation 697f62f9-3ced-477d-bfc4-6bbcba1ca65b · 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 2026-08-11T04:21:34.250685Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation b7e40927-3905-4b96-9831-fa719b5be239 · 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: unresolved; no resolver link, observed 2026-08-11T04:21:33.049934Z

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Unavailable: canonical work link unavailable.

Observation f9848189-373f-4307-8077-01d652507479 · 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 2026-08-11T04:21:33.061008Z

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Unavailable: canonical work link unavailable.

Observation 9bedbb07-e2a2-45ae-8fc4-fcce7f1942d2 · 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 2026-08-11T04:21:33.069185Z

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Observation 43aea225-4deb-4a16-abea-e6f7d05872d6 · 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: unresolved; no resolver link, observed 2026-08-11T04:21:33.076487Z

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Observation c9b7c087-d796-4d27-8cfd-7f26a6501433 · 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 2026-08-11T04:21:34.180972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 22968c32-7160-48e7-97fb-02561676177e · 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 2026-08-11T04:21:33.103941Z

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Observation cdfeca01-ca75-4292-a407-a50ecebfd5c9 · 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 2026-08-11T04:21:33.110054Z

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Observation d0aaf0a5-95a7-41f8-b8d0-3d12f1391eed · outbound

This paper cites Branchesiet al., Journal of Cosmology and Astropar- ticle Physics2023(07), 068.

How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State? Branchesiet al., Journal of Cosmology and Astropar- ticle Physics2023(07), 068

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:21:34.146268Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 414f922a-dade-4a81-ba72-16926cea3193 · 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 2026-08-11T04:21:33.127173Z

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Unavailable: canonical work link unavailable.

Observation 9431f9fa-8a46-42e6-9b95-6e61d9b4ccd1 · 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 2026-08-11T04:21:33.135460Z

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Observation 9896af71-335e-4dd2-a800-6563674e0f14 · 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 2026-08-11T04:21:33.145156Z

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Observation 1973740f-f855-4bda-95e3-88a8d74ffdae · 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: malformed identifier; no resolver link, observed 2026-08-11T04:21:33.152456Z

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Pith citing papers

No inbound Pith citation observations are available.