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Paper Citation Record · LEDGER

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring

As of 19 August 2026, this Paper Citation Record lists 65 of 65 outbound references and 1 inbound Pith citation observation for arXiv:2508.11872.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2508.11872 v3

Coverage vector

measured 65 of 65 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-05T19:46:32.625871Z

measured 66 of 66 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

65 of 65 outbound references displayed

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External citation measurements

72
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation 336aaa44-5110-4c12-87c7-41746a02492f · outbound

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

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 1

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Observation 0ea9fdfb-4564-4de2-b6fd-49f4d78c91ce · outbound

This paper cites Properties of the binary neutron star merger GW170817.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Properties of the binary neutron star merger GW170817

Reference 2

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Observation f24e0a8a-3f8e-4b9f-91f9-126119fada99 · outbound

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

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring GW170817: Measurements of Neutron Star Radii and Equation of State

Reference 3

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Observation 51a68c50-c8d0-42f9-86a4-5c18ad8ad5e2 · outbound

This paper cites Gravitational-wave constraints on the neutron-star-matter Equation of State.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Gravitational-wave constraints on the neutron-star-matter Equation of State

Reference 4

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Observation f5ed294a-adc4-418f-bf6e-87070dc6934f · outbound

This paper cites Improving the NRTidal model for binary neutron star systems.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Improving the NRTidal model for binary neutron star systems

Reference 5

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Observation fa199b82-7280-4fbc-a4c4-a1f19ce0a06e · outbound

This paper cites Punturo, M.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Punturo, M

Reference 6

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Observation 2640fa57-8301-419d-bda1-dd964b465455 · outbound

This paper cites Scientific Objectives of Einstein Telescope.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Scientific Objectives of Einstein Telescope

Reference 7

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Observation 4fd53bcc-0237-4786-b4cf-9a44d7f2bd7a · outbound

This paper cites Science Case for the Einstein Telescope.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Science Case for the Einstein Telescope

Reference 8

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Observation a678b95e-7d79-4a08-9ab7-03c67fab345b · outbound

This paper cites Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO

Reference 9

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Observation bbab2132-baf2-4eb7-b6d8-9181a5cd0f48 · outbound

This paper cites Determining the equation of state of neutron stars with Einstein Telescope using tidal effects and r-mode excitations from a population of binary inspirals.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Determining the equation of state of neutron stars with Einstein Telescope using tidal effects and r-mode excitations from a population of binary inspirals

Reference 10

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Observation 039c24db-e9db-4e5d-a988-0f7d6d2c3797 · outbound

This paper cites Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars

Reference 11

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local_arxiv, observed 2026-08-05T19:46:34.197820Z

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Observation 45121db9-95fd-4d93-988c-385b60b40dd9 · outbound

This paper cites Walker, R.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Walker, R

Reference 12

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Observation 17998d54-69c0-4672-9188-4dc131a671bf · outbound

This paper cites PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

Reference 13

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Observation 281e15b3-0aff-4d77-81d1-d890ad7c4ad9 · outbound

This paper cites A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation

Reference 14

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Observation 81ba84d4-30a2-4267-8518-5b3e44954506 · outbound

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

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring The Radius of PSR J0740+6620 from NICER and XMM-Newton Data

Reference 15

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Observation a0dd3f22-0359-42f4-825d-e2e5312a5ef3 · outbound

This paper cites A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy

Reference 16

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Observation be747a99-d29a-49a7-9b8c-56051bdd9056 · outbound

This paper cites Constraining the dense matter equation-of-state with radio pulsars.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Constraining the dense matter equation-of-state with radio pulsars

Reference 17

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Observation 64bcc813-c70a-48e2-bdb6-fa205c7af6cd · outbound

This paper cites Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620

Reference 18

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Observation 277d2410-62c7-4897-8b5f-c0254137e72a · outbound

This paper cites Kramer, I.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Kramer, I

Reference 19

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Observation 8d35eaa3-e182-4bf6-ba2c-823a380af910 · outbound

This paper cites Accurate Determination of the Neutron Skin Thickness of $^{208}$Pb through Parity-Violation in Electron Scattering.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Accurate Determination of the Neutron Skin Thickness of $^{208}$Pb through Parity-Violation in Electron Scattering

Reference 20

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Observation 493329d1-ea2a-447e-a2f0-07b4cce6bf7d · outbound

This paper cites Precision Determination of the Neutral Weak Form Factor of $^{48}$Ca.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Precision Determination of the Neutral Weak Form Factor of $^{48}$Ca

Reference 21

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Observation 93aa21d5-681b-4e5a-85ac-c89cee1b4b33 · outbound

This paper cites an unresolved cited work.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Unresolved cited work

Reference 22

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Observation 9b392041-22d0-4a54-a5ac-caf03b7d1cde · outbound

This paper cites Relativistic Equation of State of Nuclear Matter for Supernova and Neutron Star.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Relativistic Equation of State of Nuclear Matter for Supernova and Neutron Star

Reference 23

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Observation 5eabdb4b-d3f6-404e-9c69-69388be41a49 · outbound

This paper cites Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions

Reference 24

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Observation 823e8ca0-5e21-413d-b42f-d6de827fbb6a · outbound

This paper cites Relativistic mean-field theories for neutron-star physics based on chiral effective field theory.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Relativistic mean-field theories for neutron-star physics based on chiral effective field theory

Reference 25

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Observation dc8ba493-d241-4fdd-a14a-7649614141b6 · outbound

This paper cites Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase

Reference 26

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Observation 8cb70489-eb0f-462e-b92c-1589b2946c17 · outbound

This paper cites Core-collapse supernova equations of state based on neutron star observations.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Core-collapse supernova equations of state based on neutron star observations

Reference 27

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Observation 3ee94483-98b1-4039-a17a-26daf8594b26 · outbound

This paper cites Fully general-relativistic simulations of isolated and binary strange quark stars.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Fully general-relativistic simulations of isolated and binary strange quark stars

Reference 28

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Observation e35e7975-0309-4169-bf9b-4dd12d14c3cc · outbound

This paper cites Realistic Finite-Temperature Effects in Neutron Star Merger Simulations.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Realistic Finite-Temperature Effects in Neutron Star Merger Simulations

Reference 29

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local_arxiv, observed 2026-08-05T19:46:33.651381Z

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

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Observation 3b0b2fa3-e432-40e4-a93d-5228dba2f007 · outbound

This paper cites Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects

Reference 30

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local_arxiv, observed 2026-08-05T19:46:33.639224Z

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

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Observation f717a0cd-38b2-4df1-ac38-e6da7cbe7587 · outbound

This paper cites Hydrodynamic Simulations of Electron-capture Supernovae: Progenitor and Dimension Dependence.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Hydrodynamic Simulations of Electron-capture Supernovae: Progenitor and Dimension Dependence

Reference 31

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local_arxiv, observed 2026-08-05T19:46:33.626474Z

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

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Observation 0861147c-f50b-49e9-ae19-2d73ce20519b · outbound

This paper cites an unresolved cited work.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Unresolved cited work

Reference 32

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Observation 9e54c110-a527-496b-806f-66393cc2d372 · outbound

This paper cites Nucleon radius effects on neutron stars in quark mean field model.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Nucleon radius effects on neutron stars in quark mean field model

Reference 33

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local_arxiv, observed 2026-08-05T19:46:33.410883Z

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Observation 48e2ddb9-6870-4410-bfca-add055d8620a · outbound

This paper cites Neutron star equation of state from the quark level in the light of GW170817.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Neutron star equation of state from the quark level in the light of GW170817

Reference 34

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local_arxiv, observed 2026-08-05T19:46:33.398045Z

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

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Observation 2ddc9522-8e67-4351-b3e4-622c7ce1edda · outbound

This paper cites Equation of state of nuclear matter and neutron stars: Quark mean-field model versus relativistic mean-field model.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Equation of state of nuclear matter and neutron stars: Quark mean-field model versus relativistic mean-field model

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Observation 2d3ca6e8-fb96-497b-85b3-08dafc096928 · outbound

This paper cites Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models using Astrophysical Measurements.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models using Astrophysical Measurements

Reference 36

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Observation 3ce3ac58-3644-41db-8c0d-630b3b361646 · outbound

This paper cites A Bayesian inference of relativistic mean-field model for neutron star matter from observation of NICER and GW170817/AT2017gfo.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring A Bayesian inference of relativistic mean-field model for neutron star matter from observation of NICER and GW170817/AT2017gfo

Reference 37

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Observation a48f9426-80cb-4907-8125-75794caf175a · outbound

This paper cites Legred, L.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Legred, L

Reference 38

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Observation c6f2c775-8586-45b2-802c-984cfc6dc73d · outbound

This paper cites an unresolved cited work.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Unresolved cited work

Reference 39

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Observation a95c7bfd-d79c-4fac-b230-305200221245 · outbound

This paper cites Chabanov and L.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Chabanov and L

Reference 40

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verified fuzzy
raw_fallback, observed 2026-08-05T19:46:34.309507Z

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

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Observation 11a630fb-0132-4fb5-81e8-656e6300cc7a · outbound

This paper cites Impact of bulk viscosity on the post-merger gravitational-wave signal from merging neutron stars.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Impact of bulk viscosity on the post-merger gravitational-wave signal from merging neutron stars

Reference 41

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Observation 7157d6b6-f504-4702-bf4f-8f5f8c786cc7 · outbound

This paper cites Finite-temperature extension for cold neutron star equations of state.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Finite-temperature extension for cold neutron star equations of state

Reference 42

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local_arxiv, observed 2026-08-05T19:46:32.993454Z

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

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Observation ecb52178-ef66-4258-9191-a1d18c89b705 · outbound

This paper cites Combined Constraints on the Equation of State of Dense Neutron-Rich Matter from Terrestrial Experiments and Observations of Neutron Stars.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Combined Constraints on the Equation of State of Dense Neutron-Rich Matter from Terrestrial Experiments and Observations of Neutron Stars

Reference 43

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Observation 0f6ed6d5-4fe5-4be3-9cc9-14a1f8a68879 · outbound

This paper cites Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

Reference 44

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Observation 01cc85ec-a1dc-4cf0-b5fc-2b46fcc5b81d · outbound

This paper cites Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library

Reference 45

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Observation 5dfb9010-0ed6-4134-a0ae-75329d1326f3 · outbound

This paper cites Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue

Reference 46

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source=pdf_text observed=2026-08-05T19:46:32.570033Z digest=sha256:1ee96afcfdbd284724cff850ad35fe14b34d0b92b9942d78a9872cfe5c5b7ab6

Observation e25df382-5987-45c3-84d9-01b8a9cc3a51 · outbound

This paper cites Expanding RIFT: Improving performance for GW parameter inference.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Expanding RIFT: Improving performance for GW parameter inference

Reference 47

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source=pdf_text observed=2026-08-05T19:46:32.573061Z digest=sha256:348a19d2afdbcaf6b0a0fecd6eb6d16b9ee5ad4b54b5de373ceb31c3ed86ccc3

Observation 45ae7d08-74bf-49ae-9100-d9c326787cc7 · outbound

This paper cites Rapid and accurate parameter inference for coalescing, precessing compact binaries.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Rapid and accurate parameter inference for coalescing, precessing compact binaries

Reference 48

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Observation df09b648-0564-4b85-9310-5410262ed324 · outbound

This paper cites Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?

Reference 49

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source=pdf_text observed=2026-08-05T19:46:32.578807Z digest=sha256:6169201e79561ee5aacb7c2380143611adcd527adb527ba8ce99d6b42dd8b03e

Observation 1044b2b9-7af7-4a6e-8e87-1045cdc6be68 · outbound

This paper cites Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms

Reference 50

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Observation d6c4158d-058c-4205-be8b-a851be424e99 · outbound

This paper cites Gravitational waves from BH-NS binaries: Effective Fisher matrices and parameter estimation using higher harmonics.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Gravitational waves from BH-NS binaries: Effective Fisher matrices and parameter estimation using higher harmonics

Reference 51

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Observation 765f6433-c4af-4d30-be59-34da150a8655 · outbound

This paper cites Parameter Estimation of Gravitational Waves from Nonprecessing BH-NS Inspirals with higher harmonics: Comparing MCMC posteriors to an Effective Fisher Matrix.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Parameter Estimation of Gravitational Waves from Nonprecessing BH-NS Inspirals with higher harmonics: Comparing MCMC posteriors to an Effective Fisher Matrix

Reference 52

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source=pdf_text observed=2026-08-05T19:46:32.586908Z digest=sha256:5074de355a8ca37a844c0086e64be7c9011aadf05bd5b0b8b855b6e36a0f45b8

Observation ea13fc7b-3552-4dd2-a213-37330fbe4c8e · outbound

This paper cites Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology

Reference 53

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source=pdf_text observed=2026-08-05T19:46:32.590010Z digest=sha256:afaae9dcced368e84f5169052dabce61d3e3ac343afcc86ac649d5ebda063942

Observation 83502f9a-8111-4681-90bf-fb2236679e66 · outbound

This paper cites $\texttt{GWFAST}$: a Fisher information matrix Python code for third-generation gravitational-wave detectors.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring $\texttt{GWFAST}$: a Fisher information matrix Python code for third-generation gravitational-wave detectors

Reference 54

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source=pdf_text observed=2026-08-05T19:46:32.593134Z digest=sha256:415f858782f9ef58b3e3ab8fcc1c967b94eed0ea743ecaff9d456fef89488cd3

Observation d8f1c1e3-3678-47c3-bda7-cf87086368bb · outbound

This paper cites Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\texttt{GWFAST}$.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\texttt{GWFAST}$

Reference 55

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Observation 2a50b33d-8b22-46ec-b15d-148b2347d096 · outbound

This paper cites The Accuracy of Neutron Star Radius Measurement with the Next Generation of Terrestrial Gravitational-Wave Observatories.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring The Accuracy of Neutron Star Radius Measurement with the Next Generation of Terrestrial Gravitational-Wave Observatories

Reference 56

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source=pdf_text observed=2026-08-05T19:46:32.598751Z digest=sha256:7801f72a2eefe5dcf885ea99669b1909fd2b35b99faee9139548064aeb9482ae

Observation 7c04d25d-54da-48cc-be36-30f3c82f1df2 · outbound

This paper cites The population of merging compact binaries inferred using gravitational waves through GWTC-3.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring The population of merging compact binaries inferred using gravitational waves through GWTC-3

Reference 57

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Observation 84605643-6abf-4df8-be80-a0d788bf22be · outbound

This paper cites an unresolved cited work.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Unresolved cited work

Reference 58

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

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Observation 2071593b-becc-4724-a0e8-ab439c19f92c · outbound

This paper cites Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era

Reference 59

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Observation 56bf135a-beab-45ee-816a-21486af9268b · outbound

This paper cites Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state

Reference 60

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Observation 27f350c3-120f-43aa-8f4b-026a55861e29 · outbound

This paper cites Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral

Reference 61

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Observation 9b42472f-1ab5-4afb-b5c7-c947e23887ff · outbound

This paper cites Tidal deformability and gravitational-wave phase evolution of magnetised compact-star binaries.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Tidal deformability and gravitational-wave phase evolution of magnetised compact-star binaries

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local_arxiv, observed 2026-08-05T19:46:32.820544Z

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

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Observation ddebaef4-588d-44c1-8e9e-ff853f74c089 · outbound

This paper cites Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis

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Observation 25dfbe6f-5a55-42a8-94a8-3a686737f2c6 · outbound

This paper cites Lindblom, Astrophys.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Lindblom, Astrophys

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Observation 0fbf4826-790c-40ca-81df-5ce51a46696b · outbound

This paper cites Lindblom, Phys.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Lindblom, Phys

Reference 65

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Pith citing papers

Observation fca87619-421b-4d5f-9659-51d377d65144 · inbound

Talking Slide Avatars: Open-Source Multimodal Communication Approach for Teaching cites this paper.

Talking Slide Avatars: Open-Source Multimodal Communication Approach for Teaching Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring

Reference 2

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metadata mismatch
local_arxiv, observed 2026-07-01T09:15:41.849820Z

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