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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 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 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 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:31:55.518262Z

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 e804c17d-b26f-4642-953b-9c4e380f4059 · inbound

Thermodynamics conditions of matter in the neutrino decoupling region during neutron star mergers cites this paper.

Thermodynamics conditions of matter in the neutrino decoupling region during neutron star mergers Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-14T13:31:55.518262Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:31:55.518262Z digest=sha256:5a76f6d60bdfaed3be22ddda160b7a34273e7984d3ab05ec5126c6f86a1b9093

Observation f303d7c9-0ff4-48fd-8083-e929623d1657 · inbound

Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties cites this paper.

Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-14T11:35:56.576992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T11:35:56.576992Z digest=sha256:60241c1f0e3b14c2e45e67e0b02b8383eb7f7d6e32d628012f25ca2c4fd5d448

Observation 4b6c61c5-762c-4c72-8c88-68d3c18dfad5 · inbound

A Galaxy-Targeted Search for the Optical Counterpart of the Candidate NS-BH Merger S190814bv with Magellan cites this paper.

A Galaxy-Targeted Search for the Optical Counterpart of the Candidate NS-BH Merger S190814bv with Magellan Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-14T11:30:52.365677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:30:52.365677Z digest=sha256:856b023b2381ffed3a4677beb4e3f23984223d3320a23dc6caefa41218648afe

Observation 1f619e21-b14d-4af5-87f1-248ecc0cde6b · inbound

Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers cites this paper.

Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-11T21:29:52.436242Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T21:29:52.436242Z digest=sha256:4ff31c7c8271d4c5fa2064ca33ca92e6c91fd9efd0c62c097a31f1ca1cefb4f4

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:a2132abf241a1c2a600661cbf424460cdae5de8ddbc7333c5a356c19a2e157ec

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 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-07-09T03:17:52.224143Z digest=sha256:6b098bb06db3a1a4657179800ac58cb0ea928b2387c8edf3f42561bd0383bbd8

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:cbdc5a4580299635c583b6259367dbfbd65827c046266dc00233da3dbbe6c6ba