Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A Bayesian Approach to the Vertical Structure of the Disk of the Milky Way
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2003.05757.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T20:44:14.847510Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
15
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 28d7bf77-04fd-4000-b9cf-a87daf482578 · inbound
Vertical Structure and Dynamics of a Galactic Disk cites this paper.
Vertical Structure and Dynamics of a Galactic Disk A Bayesian Approach to the Vertical Structure of the Disk of the Milky Way
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T20:44:14.847510Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 56b80876-4bf9-47be-8e59-59d114a42d34 · inbound
The Milky Way is a less massive galaxy--new estimates of the Milky Way's local and global stellar masses cites this paper.
The Milky Way is a less massive galaxy--new estimates of the Milky Way's local and global stellar masses A Bayesian Approach to the Vertical Structure of the Disk of the Milky Way
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T19:03:23.710164Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d1aace9e-4dfe-4d83-9428-c49414b4d46e · inbound
Mapping the Milky Way with Gaia Bp/Rp spectra-IV: the broken and asymmetric density profile of the stellar disk traced by a large sample of red clumps cites this paper.
Mapping the Milky Way with Gaia Bp/Rp spectra-IV: the broken and asymmetric density profile of the stellar disk traced by a large sample of red clumps A Bayesian Approach to the Vertical Structure of the Disk of the Milky Way
Reference 41
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T00:44:27.786323Z
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.