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Paper Citation Record · LEDGER

Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2006.14322.

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

pith.paper-citation-record.v1
2006.14322 v3

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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T17:19:39.930647Z

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

Reference 234

Resolution
unresolved
no resolver link, observed 2026-08-06T18:16:14.828007Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T18:16:14.828007Z digest=sha256:92463b94b0e730a08f4018a2987ccba68c6a7283f6f857285b1a984047cc1488

Observation 5f569694-dbf6-48ee-a670-7747e0627854 · inbound

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-10T17:19:39.930647Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T17:19:39.930647Z digest=sha256:6a975a4715a2c10cfdbd597562e15b283b121051bbe2af6f19fe7bc6600053ed