Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2204.00737.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T23:49:10.314351Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T07:37:44.846408Z
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 6826e5d4-aa06-4f84-b0a8-edf50dfd5f33 · inbound
3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae cites this paper.
3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer
Reference 231
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T23:49:10.314351Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c076382e-86b7-4e5a-b9c3-1a3d7a5db328 · inbound
A magnetar formation in binary neutron star merger cites this paper.
A magnetar formation in binary neutron star merger Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer
Reference 54
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T07:37:44.848187Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 2eae86b6-b696-4ac6-87d1-3da67be080c2 · inbound
nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors cites this paper.
nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T05:14:58.841553Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 74576fd8-f259-4f9f-9b39-3c10d8a01b68 · inbound
Late-time emission-line profiles from kilonova models cites this paper.
Late-time emission-line profiles from kilonova models Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer
Reference 10
- 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 e2a8aafa-74ed-4c8d-b198-96c5441302ea · inbound
Luminous Red Novae as shock-powered transients I: Electron-scattering wings and deviations from Case B cites this paper.
Luminous Red Novae as shock-powered transients I: Electron-scattering wings and deviations from Case B Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:34:10.166185Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.