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Paper Citation Record · LEDGER

An ALMA study of the Orion Integral Filament: I. Evidence for narrow fibers in a massive cloud

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1801.01500.

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

pith.paper-citation-record.v1
1801.01500 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 2026-08-20T06:33:59.587034+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:17:25.875173Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-22T08:11:17.060945Z

Reference resolution

0 of 0 outbound references displayed

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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 289835cc-d4db-49e9-9bab-a037ef0d72c0 · inbound

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas cites this paper.

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas An ALMA study of the Orion Integral Filament: I. Evidence for narrow fibers in a massive cloud

Reference 50

Resolution
verified exact
local_arxiv, observed 2026-05-22T08:11:17.064265Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-05-22T08:10:11.145849Z digest=sha256:bcc710dcb2b851b86ed9ae8b00ad5e3aff46092735b6fb739bd70b3b138727f4

Observation 2484d8ef-b738-451c-ab1e-3c9190dbec18 · 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 An ALMA study of the Orion Integral Filament: I. Evidence for narrow fibers in a massive cloud

Reference 59

Resolution
unresolved
no resolver link, observed 2026-07-11T07:55:39.166465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T07:55:39.166465Z digest=sha256:be4f25848063e05ca870484a2702a309bd85f0070fd1a2080e4f5f6d6d60ecff

Observation d6ff73e9-1a14-440d-909a-a4e6ca6dc137 · inbound

Does IRS13 require an intermediate-mass black hole? cites this paper.

Does IRS13 require an intermediate-mass black hole? An ALMA study of the Orion Integral Filament: I. Evidence for narrow fibers in a massive cloud

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.875173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.875173Z digest=sha256:31823445b029e5653d7d66b0af1815f9275910b9603469ea8bc1d91504dd9d5d