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Paper Citation Record · LEDGER

Physical Properties and Galactic Distribution of Molecular Clouds identified in the Galactic Ring Survey

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1010.2798.

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

pith.paper-citation-record.v1
1010.2798 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T06:06:17.085491Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T07:49:08.277834Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 f9b619a4-22de-4e2d-982c-747450e28c1b · inbound

Analytic Modeling of CO Surface-Density Profiles in the M31 Molecular Clouds cites this paper.

Analytic Modeling of CO Surface-Density Profiles in the M31 Molecular Clouds Physical Properties and Galactic Distribution of Molecular Clouds identified in the Galactic Ring Survey

Reference 492

Resolution
unresolved
no resolver link, observed 2026-08-07T06:06:17.085491Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T06:06:17.085491Z digest=sha256:a8db9b44467939789c17efbf4d9eeffb14fc73ca638d521dc3a5596ecdf3a8b1

Observation e330cb8d-3f71-4a43-9c48-9e36f9a9f0ee · inbound

Sub-kpc scale gas density histograms of the nearby barred spiral galaxy M83: Multi-component molecular gas structure reflecting the galactic environment cites this paper.

Sub-kpc scale gas density histograms of the nearby barred spiral galaxy M83: Multi-component molecular gas structure reflecting the galactic environment Physical Properties and Galactic Distribution of Molecular Clouds identified in the Galactic Ring Survey

Reference 94

Resolution
verified exact
local_arxiv, observed 2026-05-20T17:33:36.354017Z

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:d24006b4ed2c35a2d19cf483e5045b7e6ce65f9bb4cd82162a5c52fce4b03508

Observation c28108cb-11ee-4fe6-92f6-44bf62ead52b · inbound

B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12 cites this paper.

B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12 Physical Properties and Galactic Distribution of Molecular Clouds identified in the Galactic Ring Survey

Reference 135

Resolution
verified exact
local_arxiv, observed 2026-05-21T03:29:28.708722Z

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=sha256:994ee09b5ab49d55c58ece7bf6ec7c61d1b2fc8c54d17958322819f01f58fdb1

Observation 7f3e45d5-ae8c-4ae8-88ec-96ed211a73ed · inbound

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas cites this paper.

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas Physical Properties and Galactic Distribution of Molecular Clouds identified in the Galactic Ring Survey

Reference 91

Resolution
metadata mismatch
local_arxiv, observed 2026-05-22T08:11:16.612954Z

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=sha256:041c1fb6244e007b517d40093b4cbdc22cde0334f8660fe52d68b42369f3a22d

Observation f1ddb205-0f06-4a74-960b-90d4d280cc63 · 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 Physical Properties and Galactic Distribution of Molecular Clouds identified in the Galactic Ring Survey

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:49:08.279431Z

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=sha256:760279ca00b1908a4f274672ef6c8b81993b3105f65b11a6bd9246a1c5644387