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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 22 July 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 2026-07-22T06:31:00.163083+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 2026-07-22T06:31:00.163083+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:dd9f12e0df0d7628156d5b82cb622b3a82556c83124f5433d65662f518a5b0f1

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 2026-07-22T06:31:00.163083+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8547b492514245b4e86307cd44b054de517ab2f1ebd0807cfd2ec798251625db

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 2026-07-22T06:31:00.163083+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:09e0c40db1c0567cb78bdfbc2073e680968b315fdb53cf08c6c1e8cc4ece3f29