Paper Citation Record · LEDGER

Fibers in the NGC1333 proto-cluster

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1703.07029.

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

pith.paper-citation-record.v1
1703.07029 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:17:25.869448Z

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
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External citation measurements

109
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b6e28189-edab-4b5c-a41e-232a25d97e40 · inbound

Systematic underestimation of polarisation angle dispersion and its consequences for magnetic field strength estimates in star-forming regions cites this paper.

Systematic underestimation of polarisation angle dispersion and its consequences for magnetic field strength estimates in star-forming regions Fibers in the NGC1333 proto-cluster

Reference 13

Resolution: metadata mismatch; arxiv_id, observed 2026-05-12T11:01:30.396544Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 4fa51ebe-cd85-41c5-88de-d7d390352ef7 · inbound

Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions cites this paper.

Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions Fibers in the NGC1333 proto-cluster

Reference 213

Resolution: verified exact; local_arxiv, observed 2026-05-21T03:59:32.046242Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 8d904da6-8aef-4ecb-baae-5f73984a5d18 · 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 Fibers in the NGC1333 proto-cluster

Reference 57

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ffd8a8ba-a895-4e65-99a5-4b8aa21a9408 · inbound

Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds cites this paper.

Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds Fibers in the NGC1333 proto-cluster

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-02T02:36:21.311704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a553c6ab-7b3b-4c9b-89a8-f8926b19f59b · inbound

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

Does IRS13 require an intermediate-mass black hole? Fibers in the NGC1333 proto-cluster

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-14T04:17:25.869448Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.