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Paper Citation Record · LEDGER

On the relation between the column density structures and the magnetic field orientation in the Vela C molecular complex

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1702.03853.

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

pith.paper-citation-record.v1
1702.03853 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T01:20:20.725491Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • 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 83824741-2a82-4393-88b5-6d3af8f4bf62 · 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 On the relation between the column density structures and the magnetic field orientation in the Vela C molecular complex

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-05-21T03:59:32.297439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:06e08cb5f52b2fbd7bfb977c483b1c9eb258793439cd57d612e07c256c479242

Observation 6b036580-98ec-4742-88ac-201133b8193f · inbound

B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12 cites this paper.

B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12 On the relation between the column density structures and the magnetic field orientation in the Vela C molecular complex

Reference 58

Resolution
verified exact
local_arxiv, observed 2026-05-21T03:29:28.731751Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:442c2168ea8cb9f39fc5aa60b072fb66592b8bbb4b184b05ce72caf2b6e3cf69

Observation 82e0f742-8920-4134-9d88-23776c896f41 · 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 On the relation between the column density structures and the magnetic field orientation in the Vela C molecular complex

Reference 287

Resolution
metadata mismatch
local_arxiv, observed 2026-05-22T08:11:16.179187Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9634138a5822cab4cac896cdddd211206c9bafdbea15796556b810fafa9b66b3

Observation abdc8688-4ffa-4160-be9e-791005af5fe5 · inbound

Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds cites this paper.

Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds On the relation between the column density structures and the magnetic field orientation in the Vela C molecular complex

Reference 244

Resolution
verified exact
local_arxiv, observed 2026-06-27T01:20:20.726767Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:723e27d89b82cad883b6335a25aae99b24405a0b013fe68579e62f9499ef118c