Pith. sign in

Paper Citation Record · LEDGER

A publicly available simulation of an enhanced network region of the Sun

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1510.07581.

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

pith.paper-citation-record.v1
1510.07581 v1

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 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T10:57:04.628183Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 f5257970-aa7f-4763-9a77-7ea4116e2139 · inbound

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations cites this paper.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations A publicly available simulation of an enhanced network region of the Sun

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-05T10:57:04.628183Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T10:57:04.628183Z digest=sha256:e0e6008264ec0179a79dcdfc87e9816974127e3a73549a279767faaaff0bf197

Observation bafb5f5e-a4e6-4279-bc37-3413b16a47ed · 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 A publicly available simulation of an enhanced network region of the Sun

Reference 110

Resolution
unresolved
no resolver link, observed 2026-08-03T23:48:56.719829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T23:48:56.719829Z digest=sha256:114c4727d6b52866c1764465c283fbef2df021500b6014fe737b4de6d381a3e0