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Paper Citation Record · LEDGER

Fragmentation in Massive Star Formation

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0402501.

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

pith.paper-citation-record.v1
astro-ph/0402501 v2

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 2026-08-15T06:32:42.880941+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T07:32:04.795396Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

83
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7b6dc496-be4a-4172-8315-1cdd79b30cde · inbound

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI Fragmentation in Massive Star Formation

Reference 254

Resolution
metadata mismatch
local_arxiv, observed 2026-06-26T18:09:41.455524Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ae56789ccc9b1c325aa391e821e8a07ee03d5e85d1b1d51e03728831fe3187c6

Observation b920cee6-6b91-4142-ac98-885b7009afef · inbound

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Fragmentation in Massive Star Formation

Reference 69

Resolution
unresolved
no resolver link, observed 2026-07-14T15:02:03.459139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T15:02:03.459139Z digest=sha256:cd3d5c96c77ab78365d2e7c495fbec1d9f20f73a5d9e29f941a78d911a214b4a

Observation deeec0f9-c232-4c7e-a597-a5cee589b2b5 · inbound

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Fragmentation in Massive Star Formation

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-02T07:32:04.795396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T07:32:04.795396Z digest=sha256:61c416701cedfe82406f0762a36391185e026cf192b7173ae1cf138933a4de37