Paper Citation Record · LEDGER

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression

As of 19 August 2026, this Paper Citation Record lists 60 of 60 outbound references and 1 inbound Pith citation observation for arXiv:2504.19962.

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pith.paper-citation-record.v1
2504.19962 v3

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Outbound references

Observation 7baf4264-65bf-4d6a-bbc0-e29cd6af5684 · outbound

This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 1

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This paper cites Advanced LIGO.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Advanced LIGO

Reference 2

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This paper cites mass limit 50 % 90 % LVC This work LVC This work 8 9 10 11 12 13 14 15 R, R [km] 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 Parametrized EOS, no max.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression mass limit 50 % 90 % LVC This work LVC This work 8 9 10 11 12 13 14 15 R, R [km] 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 Parametrized EOS, no max

Reference 3

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Observation a6b069e1-d320-465e-acf1-e0923e7e6c29 · outbound

This paper cites Multi-messenger Observations of a Binary Neutron Star Merger.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Multi-messenger Observations of a Binary Neutron Star Merger

Reference 4

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Observation 459a313b-8ab3-41dd-a4c3-3025c1825899 · outbound

This paper cites Haensel, A.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Haensel, A

Reference 5

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Observation b099c4ae-d407-4b7c-b2f3-7de20197be81 · outbound

This paper cites Advanced Virgo: a 2nd generation interferometric gravitational wave detector.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Advanced Virgo: a 2nd generation interferometric gravitational wave detector

Reference 6

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Observation 55914e04-9de5-4c8d-a396-10fa86f12579 · outbound

This paper cites The Radius of PSR J0740+6620 from NICER and XMM-Newton Data.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression The Radius of PSR J0740+6620 from NICER and XMM-Newton Data

Reference 7

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Unresolved cited work

Reference 8

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Observation 8fb66ba6-d6e5-4183-9cc8-ad47fd2f046d · outbound

This paper cites Andersson,Gravitational-Wave Astronomy: Explor- ing the Dark Side of the Universe(Oxford University Press, 2019).

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Andersson,Gravitational-Wave Astronomy: Explor- ing the Dark Side of the Universe(Oxford University Press, 2019)

Reference 9

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Observation 98bbaf20-cd53-401a-b872-ba92d561a726 · outbound

This paper cites Tidal deformability from GW170817 as a direct probe of the neutron star radius.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Tidal deformability from GW170817 as a direct probe of the neutron star radius

Reference 10

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Unresolved cited work

Reference 11

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Unresolved cited work

Reference 12

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Observation d116d36f-a6d5-4093-ad43-445e92bde8cd · outbound

This paper cites I-Love-Q Relations in Neutron Stars and their Applications to Astrophysics, Gravitational Waves and Fundamental Physics.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression I-Love-Q Relations in Neutron Stars and their Applications to Astrophysics, Gravitational Waves and Fundamental Physics

Reference 13

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This paper cites Measuring the neutron star tidal deformability with equation-of-state-independent relations and gravitational waves.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Measuring the neutron star tidal deformability with equation-of-state-independent relations and gravitational waves

Reference 14

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Observation 972f4aa6-2068-4c00-ac42-ef86f2a624f3 · outbound

This paper cites Neutron star tidal deformability and equation of state constraints.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Neutron star tidal deformability and equation of state constraints

Reference 15

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Observation 9674b223-ce7d-42d9-94ed-27821f98927b · outbound

This paper cites Fujimoto, K.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Fujimoto, K

Reference 16

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Observation 34705a73-2d91-4ce2-a1a3-f66e2b403e5e · outbound

This paper cites Neural networks reconstruction of the dense-matter equation of state from neutron-star parameters.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Neural networks reconstruction of the dense-matter equation of state from neutron-star parameters

Reference 17

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Observation 5cbd6ffe-a309-43ff-be03-7e6a75f1bdc9 · outbound

This paper cites Inferring neutron star properties from GW170817 with universal relations.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Inferring neutron star properties from GW170817 with universal relations

Reference 18

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Observation 057053c7-a4ab-49e4-b07f-f70c2b104a0a · outbound

This paper cites Deducing Neutron Star Equation of State from Telescope Spectra with Machine-learning-derived Likelihoods.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Deducing Neutron Star Equation of State from Telescope Spectra with Machine-learning-derived Likelihoods

Reference 19

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Observation b6bd956a-c7c4-45a8-8ca9-978d2250a4eb · outbound

This paper cites Insights into neutron star equation of state by machine learning.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Insights into neutron star equation of state by machine learning

Reference 20

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Observation 93738a17-fc34-4191-b199-eea9f420fc10 · outbound

This paper cites Ferreira, V.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Ferreira, V

Reference 21

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Observation 77d5ce0b-92e0-4aaa-b9aa-49f8156c561c · outbound

This paper cites Enhancing Gravitational-Wave Science with Machine Learning.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Enhancing Gravitational-Wave Science with Machine Learning

Reference 22

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This paper cites Machine Learning Applications in Gravitational Wave Astronomy.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Machine Learning Applications in Gravitational Wave Astronomy

Reference 23

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Ferreira and M

Reference 24

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This paper cites Angelis, F.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Angelis, F

Reference 25

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Tenachi, R

Reference 26

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This paper cites Applications of machine learning in gravitational wave research with current interferometric detectors.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Applications of machine learning in gravitational wave research with current interferometric detectors

Reference 27

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Automated discovery of interpretable gravitational-wave population models

Reference 28

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Saeed and C

Reference 30

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This paper cites Inferring the Equation of State from Neutron Star Observables via Machine Learning.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Inferring the Equation of State from Neutron Star Observables via Machine Learning

Reference 31

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Calibrating global behaviour of equation of state by combining nuclear and astrophysics inputs in a machine learning approach

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This paper cites Machine Learning-Based Analytical Expressions for Gray-Body Factors and Application to Primordial Black Holes.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Machine Learning-Based Analytical Expressions for Gray-Body Factors and Application to Primordial Black Holes

Reference 33

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This paper cites Upper limit set by causality on the tidal deformability of a neutron star.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Upper limit set by causality on the tidal deformability of a neutron star

Reference 37

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Constraining neutron star tidal Love numbers with gravitational wave detectors

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Bezanson, A

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Interpretable Machine Learning for Science with PySR and SymbolicRegression.jl

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression A unified equation of state of dense matter and neutron star structure

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Akmal, V

Reference 46

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Experimental Nuclear Masses and the Ground State of Cold Dense Matter

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This paper cites Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter

Reference 50

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Hyperons in neutron-star cores and two-solar-mass pulsar

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This paper cites 3 presented the recovered radii for both BNS components, using various assumptions about the EOS; see LIGO-P1800115 for the data behind the figure.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression 3 presented the recovered radii for both BNS components, using various assumptions about the EOS; see LIGO-P1800115 for the data behind the figure

Reference 52

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Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Existence of hyperons in the pulsar PSRJ1614-2230

Reference 53

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Reference 54

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Observation 469d610b-79b7-461f-9544-d1d5c2494972 · outbound

This paper cites GW170817: Measurements of Neutron Star Radii and Equation of State.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression GW170817: Measurements of Neutron Star Radii and Equation of State

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-16T05:44:03.667992Z

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Unavailable: canonical work link unavailable.

Observation 7e138319-be85-4c3a-8400-96022daab632 · outbound

This paper cites an unresolved cited work.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Unresolved cited work

Reference 56

Resolution: unresolved; raw_fallback, observed 2026-08-16T05:44:04.711521Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 3060d140-83f6-4b57-9fb9-98bd600e22b8 · outbound

This paper cites Virtanen, R.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Virtanen, R

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-16T05:44:03.679037Z

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Unavailable: canonical work link unavailable.

Observation 2f5cab51-e461-4814-8b8f-e6fd90b33f7b · outbound

This paper cites an unresolved cited work.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Unresolved cited work

Reference 58

Resolution: unresolved; raw_fallback, observed 2026-08-16T05:44:04.675132Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 79fec894-86f8-4877-9561-21e97e83b036 · outbound

This paper cites Akiba, S.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Akiba, S

Reference 59

Resolution: verified fuzzy; raw_fallback, observed 2026-08-16T05:44:04.655913Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8fb73563-9a3b-4f30-975d-78f1b0dcfd5a · outbound

This paper cites an unresolved cited work.

Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression Unresolved cited work

Reference 60

Resolution: unresolved; raw_fallback, observed 2026-08-16T05:44:04.635325Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Pith citing papers

Observation 881db6aa-6970-491a-99ae-e561c18cf812 · inbound

Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.

Predicting intermediate-mass black hole formation in star clusters with machine learning Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression

Reference 99

Resolution: verified exact; arxiv_id, observed 2026-05-22T09:21:20.874418Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.