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Paper Citation Record · LEDGER

Quantifying Observational Projection Effects Using Molecular Cloud Simulations

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1310.1929.

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

pith.paper-citation-record.v1
1310.1929 v1

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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:23:50.226539Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-11T07:57:53.207932Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
  • metadata mismatch0

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 ec8e16b3-09ce-4a92-9a32-e4bb5352abb6 · 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 Quantifying Observational Projection Effects Using Molecular Cloud Simulations

Reference 15

Resolution
verified exact
local_arxiv, observed 2026-07-11T07:57:53.209858Z

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=sha256:484930b05adaadf8fc2b19164edd4bcf9c62341021b86c5617b746325ba73c97

Observation bb630839-240a-4c45-9823-b9644739b4b3 · inbound

Hub-filament systems and the growth of massive stars: episodic accretion, clustered environments, and projection effects cites this paper.

Hub-filament systems and the growth of massive stars: episodic accretion, clustered environments, and projection effects Quantifying Observational Projection Effects Using Molecular Cloud Simulations

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-15T15:23:50.226539Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:23:50.226539Z digest=sha256:37d6dd5131005fec127b8ce10b182b1e279aa89107b5bb121a37508c34df1a34