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Paper Citation Record · LEDGER

Is the dust-to-gas ratio constant in molecular clouds?

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1706.05107.

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

pith.paper-citation-record.v1
1706.05107 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T10:57:05.026264Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T07:37:45.492707Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
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  • 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 a67840af-29ed-426b-8897-7a4c6cbd3371 · inbound

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations cites this paper.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Is the dust-to-gas ratio constant in molecular clouds?

Reference 168

Resolution
unresolved
no resolver link, observed 2026-08-05T10:57:05.026264Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T10:57:05.026264Z digest=sha256:1d40fcbad2cc8406c7369be6e032ce6056cd4d90b6f24d26e48d568ac92ba65a

Observation 5e83b132-3dd0-4252-a9ac-41d3bf0e6dfd · inbound

Full one-fluid dusty gas with multiple grain species in SPH cites this paper.

Full one-fluid dusty gas with multiple grain species in SPH Is the dust-to-gas ratio constant in molecular clouds?

Reference 73

Resolution
verified exact
local_arxiv, observed 2026-07-03T07:37:45.493967Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-06-27T11:57:05.509752Z digest=sha256:3bcedec374320486157ee00f215ae60c416aade124132b1cd83b85e01ab9866f

Observation cfe87c4f-2291-457c-a9e8-3eb929c0849b · inbound

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster cites this paper.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Is the dust-to-gas ratio constant in molecular clouds?

Reference 290

Resolution
unresolved
no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T05:32:07.775931Z digest=sha256:9096993ac07b43b31bf97ef4f13aa062a7882b8158771a1cae9633955b00019c

Observation af127434-a9fd-4775-b30e-2175438b2370 · inbound

Using Scattered Near-Infrared Light to Map Water Ice in Prestellar Cores with SPHEREx cites this paper.

Using Scattered Near-Infrared Light to Map Water Ice in Prestellar Cores with SPHEREx Is the dust-to-gas ratio constant in molecular clouds?

Reference 3

Resolution
unresolved
no resolver link, observed 2026-07-31T05:35:50.378505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T05:35:50.378505Z digest=sha256:b537cea8271e65c5bf7bff0e1f78b3bb2dda57d0834335c746dd80e10d39e4ba