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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 4 inbound Pith citation observations for arXiv:2102.02229.

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

pith.paper-citation-record.v1
2102.02229 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T18:52:44.122263Z

measured 0 of 1 external citation measurements

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

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  • verified fuzzy0
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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 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.

source=pdf_text observed=2026-08-03T20:20:20.164489Z digest=sha256:244ba323a696b5d87437fac9b9ba844f381f8f3aabd6c803c188bd15f44de9ea

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.

source=arxiv_source observed=2026-07-31T07:22:45.980256Z digest=sha256:d02d94539ac4795624eeeca0c35f5927df00dc5a8bac99319d798be330f1621f

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:20:55.957840Z digest=sha256:f56f921efb7e6ae576450798446a43147be1a4e4040ac6d983fd04cf71679fda

Observation c112a115-a110-462d-b58f-d74ffc856c1d · inbound

AT 2024qfm: a luminous fast blue optical transient at a redshift of z = 0.2267 identified by Lasair-ZTF cites this paper.

AT 2024qfm: a luminous fast blue optical transient at a redshift of z = 0.2267 identified by Lasair-ZTF Tight multi-messenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light curve synthesis

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-15T18:52:44.122263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T18:52:44.122263Z digest=sha256:0af6b825467fdebc5d621dcca2b099378f5394310793b86226640cf8398164d7