Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A kilonova as the electromagnetic counterpart to a gravitational-wave source
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1710.05841.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T18:41:11.226270Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T07:37:45.109106Z
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 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 2026-08-06T06:34:29.942622+00:00.
Observation 3696cfbd-3818-4696-99fc-92e790696ccb · inbound
Calibrated Lanthanide Atomic Data for Kilonova Radiative Transfer. I. Atomic Structure and Opacities cites this paper.
Calibrated Lanthanide Atomic Data for Kilonova Radiative Transfer. I. Atomic Structure and Opacities A kilonova as the electromagnetic counterpart to a gravitational-wave source
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:41:11.226270Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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 2026-08-06T06:34:29.942622+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 2026-08-06T06:34:29.942622+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 2026-08-06T06:34:29.942622+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 2026-08-06T06:34:29.942622+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.