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Paper Citation Record · LEDGER

A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 45 inbound Pith citation observations for arXiv:2407.06789.

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

pith.paper-citation-record.v1
2407.06789 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 45 of 45 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 45 of 45 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T06:03:01.263251Z

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

0 of 0 outbound references displayed

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External citation measurements

1
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation bc087344-b5fb-4405-91b1-1df76aaa522d · inbound

Strongly Interacting Dark Matter admixed Neutron Stars cites this paper.

Strongly Interacting Dark Matter admixed Neutron Stars A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 98

Resolution
metadata mismatch
arxiv_id, observed 2026-05-22T22:47:13.211848Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-22T22:45:48.648963Z digest=sha256:c0efc99ad738c4f9cf5bbd33cc0e8ab9b98e92478183415d9a6756d053e5f9b2

Observation 22911948-e33b-4b27-8aa6-e887a03127f1 · inbound

Properties of the neutron star crust informed by nuclear structure data cites this paper.

Properties of the neutron star crust informed by nuclear structure data A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 28

Resolution
verified exact
arxiv_id, observed 2026-05-22T01:40:54.215445Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-22T01:36:22.187463Z digest=sha256:ade9648b3a5551b389c5e108d6a12d39872982051bbc4bb3f4b850cc72c5653e

Observation c2c4abae-cb6e-4353-becd-79e62c5d0fe9 · inbound

Representing Equations of State With Strong First-Order Phase Transitions cites this paper.

Representing Equations of State With Strong First-Order Phase Transitions A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-07T06:03:01.263251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T06:03:01.263251Z digest=sha256:2ae21aa6b44cb44559a10b1f712cd70018f86c4416a89d5f7a08cf6b1096d6aa

Observation cd6c3f81-3496-4e01-b20e-dc6fac28129b · inbound

Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State cites this paper.

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.

source=pdf_text observed=2026-08-06T16:49:25.551118Z digest=sha256:fe8a37920275221b9cd37aed624b0f7ca9457348d27610442ff111d69a38c447

Observation c17ade8a-4fc1-4472-b413-643a63a0d188 · inbound

Subsurface Vacancy Engineering Enables Atomically Clean and Oxidation-Resistant Copper Interfaces for Anode-Free Lithium Metal Batteries cites this paper.

Subsurface Vacancy Engineering Enables Atomically Clean and Oxidation-Resistant Copper Interfaces for Anode-Free Lithium Metal Batteries A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-06T10:19:23.434158Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T10:19:23.434158Z digest=sha256:1bcc9f28aec81e64d077da20619c9765579131cc945703ed789282b9493e593e

Observation 2ded9d1a-7702-430d-8687-ea53fb29ad1d · inbound

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta cites this paper.

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-05T15:52:56.394845Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T15:52:56.394845Z digest=sha256:b7c39b679adcbf2657578babbb7ec6ca07e51c46806d360547e4beeeb7306cb8

Observation c645a350-751a-4180-8600-dcf5ea3f13d7 · inbound

Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model cites this paper.

Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-05T11:42:10.291614Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T11:42:10.291614Z digest=sha256:ee07968f9defc7cfd647ad4969067aa0a9f0db58168119b3cde3a945e208aca5

Observation 6f81d010-a35d-432c-b379-33bc9363232c · inbound

Origin of nucleon mass in the light of PSR J0614-3329 with quark-hadron crossover cites this paper.

Origin of nucleon mass in the light of PSR J0614-3329 with quark-hadron crossover A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-05T11:21:41.562008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T11:21:41.562008Z digest=sha256:f4425f9d596196c0b339f0676c53d1e9c768fe2c2f9c4891d2af116815252c81

Observation cd60754f-525d-474d-93e4-e4ea0efb07b0 · 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 A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 9

Resolution
metadata mismatch
arxiv_id, observed 2026-05-21T23:00:43.720072Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-21T22:56:05.224146Z digest=sha256:1a522e6bd988408694547226d4fd171d9c9b52abcba5770a1306e2d9a27e1637

Observation 6f65cae7-4fb6-42a6-925f-1b8e9824e041 · inbound

Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach cites this paper.

Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 81

Resolution
verified exact
arxiv_id, observed 2026-05-17T23:12:12.119716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-17T23:10:30.793407Z digest=sha256:8933a915f8c8fe4749f038a6b6f8b44cc43db066608e8ade9bd3dd73c2fb313e

Observation c669214e-1110-4932-b3fc-d22509ba0e9c · inbound

Tracing the Trace Anomaly of Dense Matter inside Neutron Stars cites this paper.

Tracing the Trace Anomaly of Dense Matter inside Neutron Stars A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 63

Resolution
verified exact
arxiv_id, observed 2026-05-17T06:24:09.882994Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-17T06:22:00.471748Z digest=sha256:79da7defcfadb3c7c5f7b79a24a316d51e5000c176a035bfcb85c215361b8db6

Observation 217d9051-9639-4662-907f-10605cb00ebe · inbound

Quarkyonic Quark-Meson Coupling Model for Nuclear and Neutron Matter cites this paper.

Quarkyonic Quark-Meson Coupling Model for Nuclear and Neutron Matter A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-03T18:37:51.762177Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T18:37:51.762177Z digest=sha256:35364e7ab4ef635a045a2625519aaefa4b1b27f896d84dac55efff691b2501c2

Observation 1d01329d-8309-4b11-a5c4-d34abd5c8521 · inbound

Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement cites this paper.

Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-03T17:54:34.680339Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T17:54:34.680339Z digest=sha256:51da26529d1ceb09d9476d184b4c4493092f0ce4349fab263de3c71a6373803f

Observation 064ae173-e264-4b46-9520-7ad5c0001006 · inbound

Constraining Hamiltonians from chiral effective field theory with neutron-star data cites this paper.

Constraining Hamiltonians from chiral effective field theory with neutron-star data A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-04T00:40:09.793223Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T00:40:09.793223Z digest=sha256:0c3128c60ea11fcd764e6844170204000d62b3182db66f869e359a570558ee4f

Observation 79e2ac16-5a50-4404-8d72-8b33d32a3206 · inbound

Neutron star with dark matter using vector portal cites this paper.

Neutron star with dark matter using vector portal A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 61

Resolution
metadata mismatch
arxiv_id, observed 2026-05-10T22:50:48.599232Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-10T19:33:30.024439Z digest=sha256:47784e72c302329cd4f40671493f6579e0814f29530131f2858f9e495c618d4d

Observation f9f19c17-60fd-4ae6-ac6f-43c109d480a7 · inbound

Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models cites this paper.

Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 27

Resolution
verified exact
arxiv_id, observed 2026-05-11T08:30:57.626875Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-10T16:35:52.640568Z digest=sha256:6f54733a282102e43afe7fd5eaebedbd5c45b4d00f4dadc0564945f34d6a1503

Observation 1beb6df0-1a5c-450f-b1a2-0fb2af781a6e · inbound

Emulator-Assisted Nuclear DFT Inference and Its Consequences for the Structure of Neutron Stars cites this paper.

Emulator-Assisted Nuclear DFT Inference and Its Consequences for the Structure of Neutron Stars A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 46

Resolution
verified exact
arxiv_id, observed 2026-05-11T09:21:01.501303Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-10T16:04:50.609515Z digest=sha256:3a687b8dbc3a393f887fe68c568c47b209794d125a3427848c46bcec4dbaee90

Observation a84f8e00-6dfa-4336-a584-f3cc5df68c8e · inbound

Combining the Mass--Radius Posteriors of J0030+0451 Allowing for Unknown Model Systematics cites this paper.

Combining the Mass--Radius Posteriors of J0030+0451 Allowing for Unknown Model Systematics A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 12

Resolution
metadata mismatch
arxiv_id, observed 2026-05-10T15:20:32.083518Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-10T15:17:40.011178Z digest=sha256:032d8fe2f1323dbd46bae9b7cbe6f7024a97b126cf71ab3ee874a4714867cae2

Observation 112935ab-89be-4eb1-bff3-7ec3d6423240 · inbound

A Poincar\'e-covariant study of strange quark stars cites this paper.

A Poincar\'e-covariant study of strange quark stars A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 47

Resolution
verified exact
arxiv_id, observed 2026-05-11T14:01:07.260958Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-09T23:41:53.852948Z digest=sha256:6768e4a3c5ba73b5de3f3ed083bb98dd5609047e30008104b88a623a1b5e76d0

Observation 82e1c090-079a-44ed-b9a3-5af00ceb3e1a · inbound

A Physics Informed Bayesian Neural Network for the Neutron Star Equation of State cites this paper.

A Physics Informed Bayesian Neural Network for the Neutron Star Equation of State A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 16

Resolution
metadata mismatch
arxiv_id, observed 2026-05-11T23:06:17.945897Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-08T01:41:01.971187Z digest=sha256:9058a9a2d93c6e4198e2ca2f28b50b09fa3b928f60c54fceab5126650470a229

Observation a48324bd-67ca-4d5f-9243-f749b961b596 · inbound

Characterizing the quark-hadron mixed phase in compact star cores : sensitivity to nuclear saturation and quark-model parameters at finite-temperature cites this paper.

Characterizing the quark-hadron mixed phase in compact star cores : sensitivity to nuclear saturation and quark-model parameters at finite-temperature A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 48

Resolution
verified exact
arxiv_id, observed 2026-05-11T18:21:10.229941Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-08T16:07:31.198921Z digest=sha256:05e9d400ec8f672162e9c3cbcee04843981a71e4e3e4ef2bdf78a1f0d7de2a19

Observation 2ddbf3d3-1bb4-4642-be79-1a86ce3a88f5 · inbound

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover cites this paper.

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 9

Resolution
verified exact
arxiv_id, observed 2026-05-12T08:21:25.728626Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-12T01:12:43.979451Z digest=sha256:fd6bbacea7c3ed4299b6c05eca8f120764b23483c43777991cb75fd1d95e7891

Observation 0114d9ef-aef3-4238-a498-6946e3a1b7f8 · inbound

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover cites this paper.

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 11

Resolution
verified exact
arxiv_id, observed 2026-07-01T13:15:46.568540Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-30T23:36:07.718605Z digest=sha256:5791d566e7aa7e9b17b7fc4c65244cef8d96449abbba218ed538ce94f9ded14b

Observation a2d32b9e-fbe2-4c59-b3e4-1600b3d853d5 · inbound

Bayesian analysis of density profile of light dark matter elucidating the properties of dark matter admixed neutron stars in the presence of hyperons cites this paper.

Bayesian analysis of density profile of light dark matter elucidating the properties of dark matter admixed neutron stars in the presence of hyperons A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 39

Resolution
verified exact
arxiv_id, observed 2026-05-15T01:48:28.162406Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-15T01:47:28.438537Z digest=sha256:94e77c7c521bcb25d119efb3740b55e27254f8be4bb19bb2d8790340f0bcf3b6

Observation 6b8b18c5-77a3-40f0-927e-5129b733e68f · inbound

Magnetic field dynamics in isolated neutron stars with an external dipole field cites this paper.

Magnetic field dynamics in isolated neutron stars with an external dipole field A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 10

Resolution
verified exact
arxiv_id, observed 2026-05-25T05:40:25.163482Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-25T05:30:35.222684Z digest=sha256:6e3efbf23f436308ede5aa593e7108e75be7e8892faaeefdb01cd1c6e6e95fb4

Observation 2c009eed-10fd-4d49-aac7-936dff9a89bf · inbound

Magnetic field dynamics in isolated neutron stars with an external dipole field cites this paper.

Magnetic field dynamics in isolated neutron stars with an external dipole field A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 9

Resolution
unresolved
no resolver link, observed 2026-07-12T16:13:25.334553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T16:13:25.334553Z digest=sha256:a5f3daf765f04f65456e0d9d9a59c313a0de36eea6f6702832d8129aa7581185

Observation 9c3374a9-5670-4336-93e6-1d27de13b8cb · inbound

Impact of hyperon mixing on neutron star structure based on Skyrme-type equations of state: Systematic analysis of $\Lambda NN$ and $\Lambda\Lambda N$ three-body forces with Bayesisan inference cites this paper.

Impact of hyperon mixing on neutron star structure based on Skyrme-type equations of state: Systematic analysis of $\Lambda NN$ and $\Lambda\Lambda N$ three-body forces with Bayesisan inference A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 8

Resolution
verified exact
arxiv_id, observed 2026-06-29T13:53:29.636393Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-29T09:23:20.507275Z digest=sha256:80a80aefbde35faa7047ee9df4f4657a37bd361524f5ca2a65308c36bbe8c623

Observation e771b13b-4138-4e65-bf31-5e24b4de63be · inbound

Hybrid Stars with Post-Merger Rotation Profiles cites this paper.

Hybrid Stars with Post-Merger Rotation Profiles A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 52

Resolution
verified exact
arxiv_id, observed 2026-07-03T22:08:58.806342Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-26T23:50:12.361235Z digest=sha256:a48463159f71771088d6b020af7f430308cbbab1b6389ed255f92a31d705d0e2

Observation a9edb64d-b194-46fa-b6bd-95f8e3e89969 · inbound

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis cites this paper.

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-07-04T07:49:39.054932Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-26T12:50:53.032717Z digest=sha256:501739e78413d92838bb44cde8e3883e7f190390d2abae71e5332a7208a362ef

Observation 7a09ce02-7bab-43b7-bf90-182175919a9b · inbound

Hyperonic equation of state for neutron stars: A systematic Bayesian comparison of density-dependent and non-linear relativistic mean-field models cites this paper.

Hyperonic equation of state for neutron stars: A systematic Bayesian comparison of density-dependent and non-linear relativistic mean-field models A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 34

Resolution
metadata mismatch
arxiv_id, observed 2026-07-04T07:49:39.959134Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-26T12:34:28.137843Z digest=sha256:ae6a543a4480f83cb4db1dde10a9a9c3fa7bf401c1cc9374e687033129d16a32

Observation 8fe573a1-c23c-49d4-82a9-150d1b1a4299 · inbound

Causality alone bounds the maximum radius difference between different-mass neutron stars cites this paper.

Causality alone bounds the maximum radius difference between different-mass neutron stars A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 12

Resolution
verified exact
arxiv_id, observed 2026-07-04T19:00:04.505576Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-25T22:16:36.441357Z digest=sha256:39b4f7c0cf83ae7ce525dcda84503bdb6adbb5ffe4782b1e99ad1a005d43ff83

Observation 52535858-7b00-48e7-a648-5af0e0ae113e · inbound

Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study cites this paper.

Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 72

Resolution
metadata mismatch
arxiv_id, observed 2026-06-30T02:24:13.147133Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-30T02:21:35.299781Z digest=sha256:c3d4aaaf1703a02453e800c7f6a003b180d41a99094479e9456683e1081adf09

Observation d66342eb-ce5a-4ac7-ae3d-2c130c63e613 · inbound

Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD cites this paper.

Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 80

Resolution
metadata mismatch
arxiv_id, observed 2026-06-30T03:04:14.865025Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-30T01:49:38.961950Z digest=sha256:f64af50d194acb6c750d54938502f20d1c963cabdf0351aca1a5b8af5cdb0b96

Observation a3595b48-45b0-4dcb-bdd8-ac8eb1ac9132 · inbound

Systematic study of the morphology and length of slow stable hybrid star branches cites this paper.

Systematic study of the morphology and length of slow stable hybrid star branches A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 14

Resolution
metadata mismatch
arxiv_id, observed 2026-06-30T15:04:46.631093Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-30T05:13:51.085511Z digest=sha256:d7e3fc31687186d2d729fe4f92a2ca429bd9b4c8a965122a576cb3b4512b1814

Observation f6e42863-77ff-4ded-b0d6-ab89e4ab9d6a · inbound

Systematic study of the morphology and length of slow stable hybrid star branches cites this paper.

Systematic study of the morphology and length of slow stable hybrid star branches A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-04T04:38:43.682144Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T04:38:43.682144Z digest=sha256:8ea1d1d99ddf184f6e7825c86f201e977bd0eb6362169368a91b4acf7697898c

Observation 5bafdcec-53e1-4c3b-9b43-24b920f58b89 · inbound

Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO cites this paper.

Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 74

Resolution
unresolved
no resolver link, observed 2026-07-12T09:19:35.429829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T09:19:35.429829Z digest=sha256:fb70b1681968e3decfffada869be34053ffebbcbca791c7dd3e79a1690893061

Observation 6e810779-8359-4172-8c80-b3d6c584fa5f · inbound

nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors cites this paper.

nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 48

Resolution
unresolved
no resolver link, observed 2026-07-12T05:14:58.841553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T05:14:58.841553Z digest=sha256:20c212099443611ced0989b39492a5ec494938794ef2b0bae410580ee72d4b3b

Observation 2178eef0-603d-4c9f-9360-30a3b00b63e8 · inbound

A NICER view of the millisecond pulsar PSR J2124$-$3358: evidence for a helium atmosphere cites this paper.

A NICER view of the millisecond pulsar PSR J2124$-$3358: evidence for a helium atmosphere A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 30

Resolution
unresolved
no resolver link, observed 2026-07-12T00:24:01.284884Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T00:24:01.284884Z digest=sha256:2173fd50b7015686708756dc4b19cbbe1c22a63256ab3a766d1aacdf162ba8ed

Observation c1aef06a-9754-465d-a5c7-be4bc7370be9 · inbound

Can average speed of sound and thermodynamic response functions signal the exotic phases in neutron star cores? cites this paper.

Can average speed of sound and thermodynamic response functions signal the exotic phases in neutron star cores? A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 58

Resolution
unresolved
no resolver link, observed 2026-07-11T05:52:28.674753Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-11T05:52:28.674753Z digest=sha256:c3a5806d5188a8085d912cc6e89b7dad2a771615e293f15ccf851acaf742c2dd

Observation b7701f05-0376-4565-a9cf-80303d7494d6 · inbound

Slowly rotating condensate dark stars beyond the mean-field approximation cites this paper.

Slowly rotating condensate dark stars beyond the mean-field approximation A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 17

Resolution
metadata mismatch
local_arxiv, observed 2026-07-09T23:36:37.319831Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-07-09T23:31:14.212701Z digest=sha256:23eec0ca194ad84cb3a83000c6330fc12bc3f37e266e614e8343918a5a666b33

Observation a21a6216-d56f-4520-9082-dd5beebff3bb · inbound

NNStar: An end-to-end AI agent for nuclear matter and neutron star physics cites this paper.

NNStar: An end-to-end AI agent for nuclear matter and neutron star physics A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-02T03:23:34.079693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T03:23:34.079693Z digest=sha256:58f7aca6fc2aba332becf1304fddb9328bf8b23c55511a69c776044cdf85b9e8

Observation 3b05e0f5-9dc7-4399-bd3b-b8d910d79edf · inbound

The equation of state for neutron stars cites this paper.

The equation of state for neutron stars A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 216

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:26.184249Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:26.184249Z digest=sha256:ad477fc03d3d808c12b8e5b54ad7df846b36e3053359c79df619532441b1f9b2

Observation 4959c469-d4a8-4d1e-8ec5-118049942a7b · inbound

Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars cites this paper.

Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 136

Resolution
unresolved
no resolver link, observed 2026-08-01T16:06:33.871846Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T16:06:33.871846Z digest=sha256:69f74f0bdc0b498b7dc1973318a16ca6e0691056ef73adcb5a3cf4cfc6f9af28

Observation 08ce429d-ccc5-498a-9cdb-45d8e5079ae6 · inbound

Holographic Soliton Crystals for Dense Nuclear Matter and Neutron Stars cites this paper.

Holographic Soliton Crystals for Dense Nuclear Matter and Neutron Stars A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-01T13:29:49.355284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T13:29:49.355284Z digest=sha256:cf1385908ba40645534eeba008f0e239fe1998b3cfa4beaf2515d0f74ff1937b

Observation eeca81a4-b3d0-49d9-b9f1-7db0ec9d5fbe · inbound

Quarkyonic Stars with Strangeness cites this paper.

Quarkyonic Stars with Strangeness A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-01T13:16:47.582823Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T13:16:47.582823Z digest=sha256:19aefb4e4955f12d8e7226cdc57034388b5eb337a608a9066e2598dbae3ff2ad