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Paper Citation Record · LEDGER

CO-dark gas and molecular filaments in Milky Way type galaxies

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1403.1589.

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

pith.paper-citation-record.v1
1403.1589 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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

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
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

204
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 8e5898ca-655f-43bc-8856-463c82d7418f · inbound

PMO Polaris CO survey. II. Where is the dust? cites this paper.

PMO Polaris CO survey. II. Where is the dust? CO-dark gas and molecular filaments in Milky Way type galaxies

Reference 60

Resolution
verified exact
local_arxiv, observed 2026-06-26T17:19:35.856176Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6797e48e279d6a14f13dede82237afa5a8086b557fed1dcf6a206ce45bbf9df1

Observation c50c7598-8860-4d78-b117-f4c027b6852f · inbound

Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds cites this paper.

Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds CO-dark gas and molecular filaments in Milky Way type galaxies

Reference 239

Resolution
unresolved
no resolver link, observed 2026-07-11T06:21:15.541076Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:21:15.541076Z digest=sha256:ad7ffb6b73821425976444ff1ff9d1bf3ca78ee2e9a7eead29b868ef8a9c5bcc