Pith. sign in

Paper Citation Record · LEDGER

Quiescent and coherent cores from gravoturbulent fragmentation

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0306055.

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

pith.paper-citation-record.v1
astro-ph/0306055 v2

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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T12:59:58.251850Z

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

142
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation c55dda88-bcd7-4f1e-95c6-d886a1b87a8b · inbound

ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 cites this paper.

ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 Quiescent and coherent cores from gravoturbulent fragmentation

Reference 160

Resolution
unresolved
no resolver link, observed 2026-07-11T12:59:58.251850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T12:59:58.251850Z digest=sha256:68de15442d0dbd414f03b5b1ae2ce97b0a5e35a403f7d30c1fb16806eb237af5

Observation 7e3765f0-b1ab-4a24-a21a-f630a73aa121 · 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 Quiescent and coherent cores from gravoturbulent fragmentation

Reference 78

Resolution
verified exact
local_arxiv, observed 2026-07-11T07:57:53.340457Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-07-11T07:55:39.166465Z digest=sha256:a1631e0ecb89c9dbd1646238fdedfc1fc16f30fe54f62f262552b63cf8f8c9e8