Paper Citation Record · LEDGER

Physical properties of molecular clouds for the entire Milky Way disk

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1610.05918.

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

pith.paper-citation-record.v1
1610.05918 v2

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 2026-08-10T06:31:04.303077+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T10:26:52.956061Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-21T03:29:28.604533Z

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 6d5f6c22-29eb-4366-af56-22e9ffb29f87 · inbound

The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud cites this paper.

The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud Physical properties of molecular clouds for the entire Milky Way disk

Reference 182

Resolution: verified exact; local_arxiv, observed 2026-05-19T20:17:44.958037Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 8d506f60-aec3-4788-93b0-72f9002c9b49 · 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 of molecular clouds for the entire Milky Way disk

Reference 136

Resolution: verified exact; local_arxiv, observed 2026-05-21T03:29:28.606256Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation d5682b9e-6d07-430c-83e5-0d77ecbd68c8 · inbound

Characterising the Kinematics and Evolution of Young Stellar Groups within 1 kpc of the Sun Using Gaia DR3 cites this paper.

Characterising the Kinematics and Evolution of Young Stellar Groups within 1 kpc of the Sun Using Gaia DR3 Physical properties of molecular clouds for the entire Milky Way disk

Reference 78

Resolution: unresolved; no resolver link, observed 2026-07-13T02:50:38.049062Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7036ff47-4ee7-4cc8-94cd-205b0ed59c99 · inbound

CO Structures with Narrow Lines in Nearby Quiescent Regions cites this paper.

CO Structures with Narrow Lines in Nearby Quiescent Regions Physical properties of molecular clouds for the entire Milky Way disk

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-10T10:26:52.956061Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.