Paper Citation Record · LEDGER

A kilonova as the electromagnetic counterpart to a gravitational-wave source

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1710.05841.

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

pith.paper-citation-record.v1
1710.05841 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T09:55:36.979397Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T07:37:45.109106Z

Reference resolution

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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 71405b21-23af-4ab7-90be-da926e59b632 · inbound

Science Case for the Einstein Telescope cites this paper.

Science Case for the Einstein Telescope A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 13

Resolution: verified exact; local_arxiv, observed 2026-05-16T00:13:18.354090Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation dfa17487-8bb8-4693-8a74-e284d6b89344 · inbound

Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers cites this paper.

Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 11

Resolution: verified exact; arxiv_id, observed 2026-05-12T08:41:25.452782Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 1c53dbfe-a75b-4bc9-a3f6-eb25367e0bd7 · inbound

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

A magnetar formation in binary neutron star merger A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 116

Resolution: verified exact; local_arxiv, observed 2026-07-03T07:37:45.113087Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 0669f842-8160-463a-bf8a-437f2477a467 · inbound

SKAO and Gamma-Ray Synergies cites this paper.

SKAO and Gamma-Ray Synergies A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 157

Resolution: verified exact; local_arxiv, observed 2026-06-29T03:03:03.574891Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation eaeabb74-b69a-468f-bf3f-5c6c7d63454c · inbound

Beta-Particle Transport and Thermalization in Kilonova Ejecta with Detailed Atomic Microphysics cites this paper.

Beta-Particle Transport and Thermalization in Kilonova Ejecta with Detailed Atomic Microphysics A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 191

Resolution: verified exact; local_arxiv, observed 2026-07-02T07:16:44.043903Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 679eab32-5d7f-4a7b-b63f-3d2fbff2fe28 · inbound

Late-time emission-line profiles from kilonova models cites this paper.

Late-time emission-line profiles from kilonova models A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 11

Resolution: unresolved; no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a114626-9e84-4520-9d1a-3545cfd5137f · 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 A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-01T09:55:36.979397Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a319bdb1-384b-4150-9451-c1e955f32036 · 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 A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 246

Resolution: unresolved; no resolver link, observed 2026-07-31T07:22:46.156998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.