Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
What is the Most Promising Electromagnetic Counterpart of a Neutron Star Binary Merger?
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1108.6056.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T23:40:05.556659Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T20:06:29.475873Z
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 ccb481b3-6969-4ead-bc0b-c7878e3d8b31 · inbound
Resonant Axion-Photon Conversion in the Early Inspiral of Neutron Star Binaries cites this paper.
Resonant Axion-Photon Conversion in the Early Inspiral of Neutron Star Binaries What is the Most Promising Electromagnetic Counterpart of a Neutron Star Binary Merger?
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T23:40:05.556659Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 86e49e13-eab9-4b46-a385-2e99e870051d · inbound
Black Hole Ringdown Seen in Photon Polarization Swings cites this paper.
Black Hole Ringdown Seen in Photon Polarization Swings What is the Most Promising Electromagnetic Counterpart of a Neutron Star Binary Merger?
Reference 21
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T19:49:59.169285Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation acc04626-14e3-421b-bb88-30e64ac7dedd · inbound
Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers cites this paper.
Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers What is the Most Promising Electromagnetic Counterpart of a Neutron Star Binary Merger?
Reference 129
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T20:06:29.477301Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation fb36be3e-4252-4077-bcd8-0f18322d9870 · inbound
The road towards precision measurements of $H_0$ with bright sirens in the Einstein Telescope era cites this paper.
The road towards precision measurements of $H_0$ with bright sirens in the Einstein Telescope era What is the Most Promising Electromagnetic Counterpart of a Neutron Star Binary Merger?
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:56:40.791723Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 715c0dcb-0118-4eba-9b8f-9fe6aa5dd607 · inbound
Gamma-ray burst progenitors revisited cites this paper.
Gamma-ray burst progenitors revisited What is the Most Promising Electromagnetic Counterpart of a Neutron Star Binary Merger?
Reference 184
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:44:27.905990Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.