Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-06T16:49:31.607142Z
Paper Citation Record · LEDGER
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State
As of 8 August 2026, this Paper Citation Record lists 57 of 57 outbound references and 1 inbound Pith citation observation for arXiv:2507.12540.
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, observed 2026-05-21T22:56:05.224146Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-21T23:00:43.807823Z
Reference resolution
57 of 57 outbound references displayed
- verified exact0
- verified fuzzy9
- unresolved46
- parse uncertain0
- malformed identifier2
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External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 3a207786-cdea-477a-a530-62d1d526cbb4 · outbound
This paper cites [34]), J0740+6620, and J0437+4715, along with 70 well-vetted radio pulsar mass measurements.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State [34]), J0740+6620, and J0437+4715, along with 70 well-vetted radio pulsar mass measurements
Reference 1
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T16:49:35.020564Z
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 4c20f727-915a-4dfc-a603-3e3b67e39c06 · outbound
This paper cites an unresolved cited work.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Unresolved cited work
Reference 2
- Resolution
- unresolved
- raw_fallback, observed 2026-08-06T16:49:34.741458Z
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 46378000-62ba-4a3f-930f-266200edbd36 · outbound
This paper cites [34], which assumes more complex hot spot geometries.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State [34], which assumes more complex hot spot geometries
Reference 3
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T16:49:34.538050Z
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 02fde21a-8067-48f0-969c-173d48fa6cb8 · outbound
This paper cites an unresolved cited work.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Unresolved cited work
Reference 4
- Resolution
- malformed identifier
- raw_fallback, observed 2026-08-06T16:49:34.278383Z
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 d84bd420-7ee3-4c9d-b792-0c7ad8c23c05 · outbound
This paper cites The equa- tion of state of hot, dense matter and neutron stars,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State The equa- tion of state of hot, dense matter and neutron stars,
Reference 5
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T16:49:34.018732Z
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 0c53e7fd-a21c-4071-9217-2ffb53ba14d7 · outbound
This paper cites Equa- tions of state for supernovae and compact stars,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Equa- tions of state for supernovae and compact stars,
Reference 6
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-06T16:49:24.690017Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7256ff53-d33c-4029-b3f5-a6ffd782621c · outbound
This paper cites From hadrons to quarks in neutron stars: a review,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State From hadrons to quarks in neutron stars: a review,
Reference 7
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T16:49:33.759566Z
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 5d94fc59-6e1c-4023-a8db-01a54b453a08 · outbound
This paper cites A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:24.998426Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 265c8d1f-5906-414e-9410-f0b2ecca7cff · outbound
This paper cites PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:25.146397Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 005c021f-f9af-4903-a332-cd403112bee7 · outbound
This paper cites A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:25.312809Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a2fa3518-dfb7-48d1-aca2-544233f17fd8 · outbound
This paper cites The Radius of PSR J0740+6620 from NICER and XMM-Newton Data.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:25.430053Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cd6c3f81-3496-4e01-b20e-dc6fac28129b · outbound
This paper cites A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:25.551118Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4771358f-fb34-4083-a452-8f79eb4f5fa2 · outbound
This paper cites The Neutron star Interior Composition Ex- plorer (NICER): design and development,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State The Neutron star Interior Composition Ex- plorer (NICER): design and development,
Reference 13
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T16:49:33.536888Z
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 3041eb7d-aec5-4b9b-8814-3f697526e0a7 · outbound
This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:25.805522Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ac44f174-21b6-4ca9-baca-77af8d3eb509 · outbound
This paper cites Properties of the binary neutron star merger GW170817.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Properties of the binary neutron star merger GW170817
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:25.945511Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1908a19f-d0f7-4ada-8972-de3e9e854550 · outbound
This paper cites GW170817: Measurements of Neutron Star Radii and Equation of State.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State GW170817: Measurements of Neutron Star Radii and Equation of State
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:26.052613Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 092f87b4-7e60-4494-971d-c2ffd7ac0bc0 · outbound
This paper cites Advanced LIGO.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Advanced LIGO
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:26.274789Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cbb47f1e-5565-47f5-a974-65a8e1188e8a · outbound
This paper cites Advanced Virgo: a 2nd generation interferometric gravitational wave detector.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Advanced Virgo: a 2nd generation interferometric gravitational wave detector
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:26.421320Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8c403de6-06b2-4e65-adec-635c4b6b7b01 · outbound
This paper cites Modern Theory of Nuclear Forces.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Modern Theory of Nuclear Forces
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:26.527939Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 358ad354-ffec-49cb-bd9f-353845bbf60f · outbound
This paper cites Chiral effective field theory and nuclear forces.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Chiral effective field theory and nuclear forces
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:26.662063Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7ac19213-a38f-4a53-8789-871153a20ab5 · outbound
This paper cites Three-body forces: From cold atoms to nuclei.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Three-body forces: From cold atoms to nuclei
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:26.782232Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e7b85c76-0cc4-49ce-8982-3a370139b7a8 · outbound
This paper cites Three-Nucleon Forces: Implementation and Applications to Atomic Nuclei and Dense Matter.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Three-Nucleon Forces: Implementation and Applications to Atomic Nuclei and Dense Matter
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:26.901241Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e134aff3-ffde-4ae4-ae5f-65da335f1b5e · outbound
This paper cites Chiral Effective Field Theory and the High-Density Nuclear Equation of State.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Chiral Effective Field Theory and the High-Density Nuclear Equation of State
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:27.026937Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1af1904c-02d6-43f1-a2b3-495b2bcbf5f5 · outbound
This paper cites How perturbative QCD constrains the Equation of State at Neutron-Star densities.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State How perturbative QCD constrains the Equation of State at Neutron-Star densities
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:27.210285Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 953adc7d-6487-4bbd-8429-0113354ba25c · outbound
This paper cites Accurate Determination of the Neutron Skin Thickness of $^{208}$Pb through Parity-Violation in Electron Scattering.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Accurate Determination of the Neutron Skin Thickness of $^{208}$Pb through Parity-Violation in Electron Scattering
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:27.335739Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a2f7165b-517b-442a-a3af-94017309eba4 · outbound
This paper cites Precision Determination of the Neutral Weak Form Factor of $^{48}$Ca.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Precision Determination of the Neutral Weak Form Factor of $^{48}$Ca
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:27.456148Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 66674eda-8388-4e50-81d6-bd2713e25546 · outbound
This paper cites Simultaneously Constraining the Neutron Star Equation of State and Mass Distribution through Multimessenger Observations and Nuclear Benchmarks.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Simultaneously Constraining the Neutron Star Equation of State and Mass Distribution through Multimessenger Observations and Nuclear Benchmarks
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:27.594077Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0ca1ac21-56d3-4f81-9f8e-e789a5a825a4 · outbound
This paper cites Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:27.700484Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5253b333-4060-442c-aecc-454b4b68ab3f · outbound
This paper cites GW190814: On the properties of the secondary component of the binary.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State GW190814: On the properties of the secondary component of the binary
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:27.818594Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b142e481-cd53-452a-a5a5-bd5e63ac8623 · outbound
This paper cites Impact of PREX-II and combined Radio/NICER/XMM-Newton's mass-radius measurement of PSRJ0740+6620 on the dense matter equation of state.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Impact of PREX-II and combined Radio/NICER/XMM-Newton's mass-radius measurement of PSRJ0740+6620 on the dense matter equation of state
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:27.994267Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 542e91e8-0cfb-449d-aa6f-a0cae5cc8d6f · outbound
This paper cites Asymmetric nuclear mat- ter equation of state,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Asymmetric nuclear mat- ter equation of state,
Reference 32
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T16:49:33.316785Z
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 d5ae009f-1da7-4267-ac37-dadc487198dc · outbound
This paper cites Haensel, A.
Reference 33
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T16:49:33.111076Z
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 4d7b288b-36c9-4456-bc66-930fc324dfc0 · outbound
This paper cites The Nuclear Symmetry Energy.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State The Nuclear Symmetry Energy
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:28.398224Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e98f1594-f095-46be-bfdf-ee42636f48d3 · outbound
This paper cites The equation of state for dense nucleonic matter from a metamodeling. I. Foundational aspects.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State The equation of state for dense nucleonic matter from a metamodeling. I. Foundational aspects
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:28.525089Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3f688dc3-677e-48f5-b3c0-db1fd8372188 · outbound
This paper cites Constraints on a phenomenologically parameterized neutron-star equation of state.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Constraints on a phenomenologically parameterized neutron-star equation of state
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:28.647577Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a760adc9-4a97-45ba-8632-1f0de0186fe1 · outbound
This paper cites Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:28.778866Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 41693507-1fc3-435e-9208-63baad01e556 · outbound
This paper cites An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:28.917824Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 553c8080-7619-4ea4-ae4a-7f511ec485f7 · outbound
This paper cites An updated mass-radius anal- ysis of the 2017-2018 nicer data set of psr j0030+0451,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State An updated mass-radius anal- ysis of the 2017-2018 nicer data set of psr j0030+0451,
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:29.139490Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 135daed2-3651-46ae-ac73-0ab7d18180fd · outbound
This paper cites A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614–3329,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614–3329,
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:29.251103Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e999de3e-7d4e-4778-be88-b6aaa835d46d · outbound
This paper cites A unified equation of state of dense matter and neutron star structure.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State A unified equation of state of dense matter and neutron star structure
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:29.359495Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 28268e0c-6d7e-4dcb-9cf8-84c688247e0a · outbound
This paper cites The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:29.478552Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bef8db28-d77f-4099-8c00-77fd8d5a8cd8 · outbound
This paper cites Data and software for: ’the radius of the high- mass pulsar psr j0740+6620 with 3.6 yr of nicer data’,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Data and software for: ’the radius of the high- mass pulsar psr j0740+6620 with 3.6 yr of nicer data’,
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:29.655519Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f5ed9c40-252d-4b6d-b70e-d4e5ac5f5184 · outbound
This paper cites Reproduction package for: ’a nicer view of the nearest and brightest millisecond pulsar: Psr j0437–4715’,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Reproduction package for: ’a nicer view of the nearest and brightest millisecond pulsar: Psr j0437–4715’,
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:29.779394Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d5fce33d-0063-4acc-b25d-c0acf42e2252 · outbound
This paper cites GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:29.899487Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8ce277cf-bbbb-4216-85a4-cacddc8b5688 · outbound
This paper cites Buqeye software repository,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Buqeye software repository,
Reference 46
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T16:49:32.919050Z
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 c975b150-a6ce-4555-9def-4ce5b1756d9d · outbound
This paper cites How well do we know the neutron-matter equation of state at the densities inside neutron stars? A Bayesian approach with correlated uncertainties.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State How well do we know the neutron-matter equation of state at the densities inside neutron stars? A Bayesian approach with correlated uncertainties
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:30.138219Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 70b1649a-94b8-423e-a0cd-2ab063c1043d · outbound
This paper cites Soft interactions in cold quark matter.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Soft interactions in cold quark matter
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:30.337552Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e7724c08-3113-478a-8270-6a0633eec01b · outbound
This paper cites Ab-initio QCD calculations impact the inference of the neutron-star-matter equation of state.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Ab-initio QCD calculations impact the inference of the neutron-star-matter equation of state
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:30.404662Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 47a49baf-f60c-411a-a6bc-6de31c495605 · outbound
This paper cites Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:30.530694Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 99eae5dc-5b65-47f9-8b24-98c51d7d79c1 · outbound
This paper cites Bayesian constraints on covariant density functional equations of state of compact stars with new NICER mass-radius measurements.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Bayesian constraints on covariant density functional equations of state of compact stars with new NICER mass-radius measurements
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:30.766274Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8c9e61ca-d2ac-47c8-b5a5-caf5899029e5 · outbound
This paper cites Bayesian inferences on covariant density functionals from multi- messenger astrophysical data: Nucleonic models,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Bayesian inferences on covariant density functionals from multi- messenger astrophysical data: Nucleonic models,
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:30.906092Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 29525091-9f8b-4c06-aa14-a2b5facbb1ee · outbound
This paper cites A NICER View of PSR J1231$-$1411: A Complex Case.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State A NICER View of PSR J1231$-$1411: A Complex Case
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:31.021204Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 09c4e80e-909f-4b3a-a29d-77eec4b8eaab · outbound
This paper cites X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:31.178770Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d3559ee0-a5b3-4beb-89ea-79ad57beca28 · outbound
This paper cites Bayes Factors,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Bayes Factors,
Reference 55
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-06T16:49:32.698917Z
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 c9f9afea-42ba-4252-987b-a8d65c1a27d6 · outbound
This paper cites Constraining the dense matter equation of state with new NICER mass-radius measurements and new chiral effective field theory inputs.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Constraining the dense matter equation of state with new NICER mass-radius measurements and new chiral effective field theory inputs
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:31.458564Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d01933d7-0b97-4c25-9c76-57cf4be4a116 · outbound
This paper cites Relativistic mean-field predictions for dense matter equation of state and application to neutron stars.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Relativistic mean-field predictions for dense matter equation of state and application to neutron stars
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:31.555882Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fecc22fc-fbf6-43a2-8d22-82a980a7b69c · outbound
This paper cites Infer- ring the neutron star equation of state with nuclear- physics informed semiparametric models,.
Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Infer- ring the neutron star equation of state with nuclear- physics informed semiparametric models,
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:31.607142Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
Observation 8c758a56-6f81-4072-93e3-5e3de02bde79 · inbound
Equation of State Extrapolation Systematics: Parametric vs. Nonparametric Inference of Neutron Star Structure cites this paper.
Equation of State Extrapolation Systematics: Parametric vs. Nonparametric Inference of Neutron Star Structure Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State
Reference 36
- Resolution
- verified exact
- arxiv_id, observed 2026-05-21T23:00:43.810126Z
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.