Pith. sign in

Paper Citation Record · LEDGER

Giant Molecular Filaments in the Milky Way

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1403.1450.

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

pith.paper-citation-record.v1
1403.1450 v2

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 2026-08-15T15:23:50.069397Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-19T20:17:45.217599Z

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 edbdf84b-cd66-42c4-a05e-8ce164653dc9 · inbound

The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud cites this paper.

The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud Giant Molecular Filaments in the Milky Way

Reference 205

Resolution
verified exact
local_arxiv, observed 2026-05-19T20:17:45.218967Z

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=2026-07-11T11:50:26.030339Z digest=sha256:430c2a7c7b5fc2687cc78b99555b58b1f2c409099cebd84ebc11a64cc093d5d0

Observation d600b34f-f2cf-4cd3-b7bb-58f65df72012 · 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 Giant Molecular Filaments in the Milky Way

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-15T15:23:50.069397Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:23:50.069397Z digest=sha256:9dbdf925aa4ee73a7ebc0e65ca7f5276b26855f7f2c21656142034ff1eed73ae