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Paper Citation Record · LEDGER

Element formation in radiation-hydrodynamics simulations of kilonovae

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2403.13883.

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

pith.paper-citation-record.v1
2403.13883 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T09:02:10.553457Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-12T08:41:25.581313Z

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 75eb88a7-14e8-4ec1-8f45-ca11beeed9b8 · 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 Element formation in radiation-hydrodynamics simulations of kilonovae

Reference 85

Resolution
verified exact
arxiv_id, observed 2026-05-12T08:41:25.582757Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-07T14:05:21.961266Z digest=sha256:fdcf1f57f6bcb1b41843952a40c21496d824852c54fc55e526403491241f353b

Observation 433a93bf-c34f-40d3-b41c-6e700d28bffe · inbound

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

Late-time emission-line profiles from kilonova models Element formation in radiation-hydrodynamics simulations of kilonovae

Reference 52

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:e751cd1cc3b00357ed07b430091d96358cfa84a8a197fc8cb1b5a48f12a4f95f