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Paper Citation Record · LEDGER

Gravity, Magnetic Field, and Turbulence: Relative Importance and Impact on Fragmentation in the Infrared Dark Cloud G34.43+00.24

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1903.12397.

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

pith.paper-citation-record.v1
1903.12397 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 2026-08-23T06:30:58.430688+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T06:50:40.250555Z

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 a34ce22e-4d75-4171-b9c0-ad8b53e50fb8 · inbound

Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps cites this paper.

Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps Gravity, Magnetic Field, and Turbulence: Relative Importance and Impact on Fragmentation in the Infrared Dark Cloud G34.43+00.24

Reference 62

Resolution
metadata mismatch
local_arxiv, observed 2026-05-14T20:57:58.433895Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:05b9a6403343cddf4467e6f830d794e03b0ca784ab5accf74ce634978e5d6b8e

Observation c06e921b-87aa-45fc-9261-85c371de9746 · inbound

Grain alignment and dust evolution physics with polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra cites this paper.

Grain alignment and dust evolution physics with polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra Gravity, Magnetic Field, and Turbulence: Relative Importance and Impact on Fragmentation in the Infrared Dark Cloud G34.43+00.24

Reference 129

Resolution
verified exact
local_arxiv, observed 2026-06-27T06:50:40.251738Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a04a300a7ea40125ed2edf8b77e40dba49c833267251a0b1ff5f35aba153e10e

Observation 9c7138ea-ce0b-4349-affd-c993743181db · inbound

Characterising magnetic fields at the onset of star cluster formation: From giant molecular clouds to infrared dark clumps cites this paper.

Characterising magnetic fields at the onset of star cluster formation: From giant molecular clouds to infrared dark clumps Gravity, Magnetic Field, and Turbulence: Relative Importance and Impact on Fragmentation in the Infrared Dark Cloud G34.43+00.24

Reference 32

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:49:08.327948Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:dd8175d388f3a5c18e4edc80e42d95e4af5ae6e0665955f19315a5c1d8696388