Pith. sign in

Paper Citation Record · LEDGER

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

As of 20 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 2026-08-20T06:33:59.587034+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

  • 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 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=sha256:46c501751af9bcc65061e079bfbcd6b4a3cfc34670b4188b7d5278faae398e8a

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c0b495276425ca327c26deec06130c6f4b0b1b1ffbba8fe4a75a54e3ac236e88

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:1fd73317260ec1da861958c96caf636e31ee1451ce2ff503e02ea268db1b461e

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:93b7a43822b7fe64e524141e5a17e82deda97ea75d06439cd1e5f8d11a16a56c

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 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5af434e24eef4583e3cb2d1a36cbd138a371d0ca6d610524e9d58f44c4e8013c