Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Are small radii of compact stars ruled out by GW170817/AT2017gfo?
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1803.09696.
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 2026-08-06T12:12:25.461139Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T07:49:39.075755Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- 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 4a3f234a-50e1-4ff5-ad6d-bb9b96aa135f · inbound
On the formation of strange quark stars from supernova in compact binaries cites this paper.
On the formation of strange quark stars from supernova in compact binaries Are small radii of compact stars ruled out by GW170817/AT2017gfo?
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T12:12:25.461139Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 242b4312-f7a8-4b8e-b6eb-2a925cde8788 · 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 Are small radii of compact stars ruled out by GW170817/AT2017gfo?
Reference 51
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T07:49:39.077312Z
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 6243469b-7500-4550-9ab9-9201ea3348c9 · 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 Are small radii of compact stars ruled out by GW170817/AT2017gfo?
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:55:37.843596Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.