Pith. sign in

Paper Citation Record · LEDGER

Population III Supernovae as a dust factory I --- molecule formation and mixing/fallback in ejecta

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2504.17506.

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

pith.paper-citation-record.v1
2504.17506 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T11:23:58.826602Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3f29217c-4c1d-45c4-9e21-6d57ab7bcdae · inbound

Confined Circumstellar Material as a Dust Formation Site in Type II Supernovae cites this paper.

Confined Circumstellar Material as a Dust Formation Site in Type II Supernovae Population III Supernovae as a dust factory I --- molecule formation and mixing/fallback in ejecta

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-06T11:23:58.826602Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T11:23:58.826602Z digest=sha256:b8443bb6e54f573f2b722154e2e4b904183ea439ce87d7c411b3435f2a8296ac

Observation f12a8bb8-53a2-4d88-a3a4-fc0ea042d1a6 · inbound

How can we finally see the first light? Status and perspective in the search for Population III stars cites this paper.

How can we finally see the first light? Status and perspective in the search for Population III stars Population III Supernovae as a dust factory I --- molecule formation and mixing/fallback in ejecta

Reference 56

Resolution
verified exact
arxiv_id, observed 2026-07-02T18:37:15.785637Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-07-02T17:57:57.440482Z digest=sha256:bea6f88b65876cad6bcba7bba424336d6f21c9a3247ab90935b18cd41e8fb906

Observation 03b0b2f3-ccc6-4fe4-b7c4-9ad6faf7b90d · inbound

Determining Total Infrared Luminosities from Submm Measurements of High Redshift Galaxies cites this paper.

Determining Total Infrared Luminosities from Submm Measurements of High Redshift Galaxies Population III Supernovae as a dust factory I --- molecule formation and mixing/fallback in ejecta

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-03T01:31:19.389288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T01:31:19.389288Z digest=sha256:94d6739455e83d4738240cc40ff84f4b87ee8c0f5f2f4f69dd2b010d8d3e7909