Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraint on the maximum mass of neutron stars using GW170817 event
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1905.03656.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T18:36:00.699152Z
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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- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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 2026-08-12T06:34:41.77262+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.