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Paper Citation Record · LEDGER

Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1402.4803.

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

pith.paper-citation-record.v1
1402.4803 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:41:12.335664Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T03:25:57.940946Z

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 f1bd649a-6b4a-48dd-89c5-3eafb87a09bd · 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 Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-06T18:41:12.335664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:41:12.335664Z digest=sha256:3fcc1faf7f4082ab4c7bca61bf4af00c3ef91f3ad6c8d32717e01446826c4a57

Observation fdaac0b0-43ef-4c76-8f69-212b6cccf282 · inbound

Subsolar-mass binary mergers of strange stars and neutron stars: gravitational waves and ejecta cites this paper.

Subsolar-mass binary mergers of strange stars and neutron stars: gravitational waves and ejecta Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-07-09T03:25:57.942175Z

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.

source=pdf_text observed=2026-07-09T03:17:52.224143Z digest=sha256:1f2aacf2f68b1d25620f4c19f1e2c6990107f9a2808478c5aa6810095a5f91f4

Observation 1839438c-e1af-4458-aa32-15fd7239e851 · inbound

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

Late-time emission-line profiles from kilonova models Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

Reference 68

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:004cbf86e70aa59bdbaddaa9f3e196bc521517cee387312cf6614e4fd6f9c6e9