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Paper Citation Record · LEDGER

A new galaxy spectral energy distribution model consistent with the evolution of dust

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2205.07591.

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

pith.paper-citation-record.v1
2205.07591 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 2026-08-20T06:33:59.587034+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T00:39:29.459918Z

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 9d522e22-2373-4417-89bd-d2f37879e12b · inbound

The influence of dust destruction on gas cooling cites this paper.

The influence of dust destruction on gas cooling A new galaxy spectral energy distribution model consistent with the evolution of dust

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-01T01:08:38.879756Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T01:08:38.879756Z digest=sha256:ceb5b725ffca7e83e4ff8de182204888bd15ca5dd4f3aa75de06b436e9f42b45

Observation 4ba4181c-34d6-4962-aaa2-f3fd4ac0540c · inbound

Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.15 cites this paper.

Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.15 A new galaxy spectral energy distribution model consistent with the evolution of dust

Reference 120

Resolution
unresolved
no resolver link, observed 2026-08-12T00:39:29.459918Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T00:39:29.459918Z digest=sha256:57220897ce352734cf90647625a83935fd48f60f3b318a4260c7377ea4e3cf48