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Paper Citation Record · LEDGER

Radiation hydrodynamics modeling of kilonovae with SNEC

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2111.06870.

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

pith.paper-citation-record.v1
2111.06870 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 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:20:56.012920Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-15T13:15:49.691234Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 6c679283-5f3b-473d-a7f7-4bc0199ff75a · inbound

Gamma-ray Signatures of r-Process Radioactivity from the Collapse of Magnetized White Dwarfs cites this paper.

Gamma-ray Signatures of r-Process Radioactivity from the Collapse of Magnetized White Dwarfs Radiation hydrodynamics modeling of kilonovae with SNEC

Reference 48

Resolution
verified exact
arxiv_id, observed 2026-05-15T13:15:49.692710Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-05-15T13:14:50.500932Z digest=sha256:b8ada65c14d0b3dcc4c9c22f5bee5d5b7ba2124b2572504fb635392a69039089

Observation 020ccf33-54ea-4209-aea7-92d1a2032f59 · inbound

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves cites this paper.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Radiation hydrodynamics modeling of kilonovae with SNEC

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.012920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.012920Z digest=sha256:62d36596ecd7ad60ea2b5330a71235a6961d2beef423950b49df7bfa9540bed0