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Paper Citation Record · LEDGER

Star formation in clusters: a survey of compact mm-wave sources in the Serpens core

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/9809323.

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

pith.paper-citation-record.v1
astro-ph/9809323 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 2026-08-16T06:30:59.297886+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T07:31:57.260780Z

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

349
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b9ed7c30-d839-4a68-87f2-925ac86dce72 · inbound

Emergence of high-mass stars in complex fiber networks (EMERGE) VI. Turbulence dissipation and the formation of dense fibers cites this paper.

Emergence of high-mass stars in complex fiber networks (EMERGE) VI. Turbulence dissipation and the formation of dense fibers Star formation in clusters: a survey of compact mm-wave sources in the Serpens core

Reference 164

Resolution
verified exact
local_arxiv, observed 2026-07-11T07:57:53.261003Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-07-11T07:55:39.166465Z digest=sha256:6228f5cc34203159d9ed8885943470a3db4573d78293d750748fad7aec8c413a

Observation 275709e1-a64a-474f-a087-722d8d0d33f3 · 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 Star formation in clusters: a survey of compact mm-wave sources in the Serpens core

Reference 10

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:bcd8076288816ea08d86bd2d915216565f9c50259d5469b49a783c631ee67562

Observation 6a7b8a02-70a4-4cf2-a532-e79b2f7e4cb3 · 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 Star formation in clusters: a survey of compact mm-wave sources in the Serpens core

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-02T07:31:57.260780Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T07:31:57.260780Z digest=sha256:a9c52146bd64fbfe3ec0bdf1a4790e0f965d9387304ae3ee8bfb2c9f3977ea57