Paper Citation Record · LEDGER

Constraint on the maximum mass of neutron stars using GW170817 event

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:1905.03656.

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

pith.paper-citation-record.v1
1905.03656 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:34:20.969227Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T07:49:39.067518Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation cfb170a1-6ba3-410a-baf4-a75518a8d0bd · inbound

Thermal evolution of neo-neutron stars. I: envelopes, Eddington luminosity phase and implications for GW170817 cites this paper.

Thermal evolution of neo-neutron stars. I: envelopes, Eddington luminosity phase and implications for GW170817 Constraint on the maximum mass of neutron stars using GW170817 event

Reference 110

Resolution: unresolved; no resolver link, observed 2026-08-14T13:34:20.969227Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 510b4ceb-594e-4acb-87f3-c2a36ad8134d · inbound

Diversity of kilonova light curves cites this paper.

Diversity of kilonova light curves Constraint on the maximum mass of neutron stars using GW170817 event

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-14T13:07:34.133891Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e32584c-8460-4c06-8be7-93d7af4a884d · inbound

Close-in Exoplanets as Candidates of Strange Quark Matter Objects cites this paper.

Close-in Exoplanets as Candidates of Strange Quark Matter Objects Constraint on the maximum mass of neutron stars using GW170817 event

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-14T10:31:03.035143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1fbd4b86-e079-4bc3-8888-5d7b059387f3 · inbound

Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars cites this paper.

Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars Constraint on the maximum mass of neutron stars using GW170817 event

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T18:36:00.699152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 24895af9-3e97-4a37-a22e-9f42ecb3cddb · inbound

The error budget of binary neutron star merger simulations for configurations with high spin cites this paper.

The error budget of binary neutron star merger simulations for configurations with high spin Constraint on the maximum mass of neutron stars using GW170817 event

Reference 131

Resolution: unresolved; no resolver link, observed 2026-08-07T11:40:59.219844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9ec99a8c-e481-41c4-b4cf-ab03bc3f7f0e · inbound

A magnetar formation in binary neutron star merger cites this paper.

A magnetar formation in binary neutron star merger Constraint on the maximum mass of neutron stars using GW170817 event

Reference 118

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:37:44.695352Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 02a0b20d-d43b-4415-bbe2-e174d2d39630 · 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 Constraint on the maximum mass of neutron stars using GW170817 event

Reference 129

Resolution: verified exact; arxiv_id, observed 2026-07-04T07:49:39.069006Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 19939578-7690-4eb9-a90e-f27c9cb0e3f1 · 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 Constraint on the maximum mass of neutron stars using GW170817 event

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-06-30T15:04:46.691078Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation e86d7914-e29e-4ae7-a79d-3eebe2d47096 · 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 Constraint on the maximum mass of neutron stars using GW170817 event

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-04T04:38:43.944468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c4a5d9f0-9030-4988-b964-b45abd7a00f9 · inbound

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures cites this paper.

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures Constraint on the maximum mass of neutron stars using GW170817 event

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T09:55:38.091097Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.