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Paper Citation Record · LEDGER

Atomic and molecular gas as traced by [C II] emission

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2410.14284.

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

pith.paper-citation-record.v1
2410.14284 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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:54:56.724842Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T12:16:16.480190Z

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 9b2c377e-06d9-48c0-b51c-c74d457247fa · inbound

Pushing ALMA to the limit: 140 pc resolution observations of a z=6.6 quasar-galaxy merger resolve strikingly different morphologies of dust continuum and [CII] 158 um emission cites this paper.

Pushing ALMA to the limit: 140 pc resolution observations of a z=6.6 quasar-galaxy merger resolve strikingly different morphologies of dust continuum and [CII] 158 um emission Atomic and molecular gas as traced by [C II] emission

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-11T18:54:56.724842Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T18:54:56.724842Z digest=sha256:c4ffd02e0bbb82770f9d5d17bb326d68ca45f5a492a4a529c77d0988d3e9eb13

Observation 3f05a655-7a89-4981-afdb-84e3338daf7a · inbound

The effects of different cooling and heating function models on a simulated analog of NGC300 cites this paper.

The effects of different cooling and heating function models on a simulated analog of NGC300 Atomic and molecular gas as traced by [C II] emission

Reference 20

Resolution
metadata mismatch
local_arxiv, observed 2026-08-11T11:37:18.754459Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.558346Z digest=sha256:7b721575bb08301c29d9651cc1aeb91d785dbd2a9c61619d4f2134b2a77e531a