Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Tight multi-messenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light curve synthesis
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2102.02229.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T04:20:55.957840Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-14T04:20:57.684591Z
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 dadfe894-d111-41d8-b21b-c8a94c1a1709 · inbound
Toward a Unified Understanding of the Dense Matter Equation of State cites this paper.
Toward a Unified Understanding of the Dense Matter Equation of State Tight multi-messenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light curve synthesis
Reference 266
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-03T20:20:20.164489Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 93f208c8-94a9-482e-8165-fe8a8056b1f7 · inbound
Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology cites this paper.
Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology Tight multi-messenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light curve synthesis
Reference 191
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T07:22:45.980256Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 03f12d27-912f-4b10-96cf-ed51246aed86 · inbound
3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves cites this paper.
3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Tight multi-messenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light curve synthesis
Reference 61
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T04:20:57.690625Z
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.