Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
NGC5846-UDG1: A galaxy formed mostly by star formation in massive, extremely dense clumps of gas
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2111.14851.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T13:20:41.134969Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-22T21:55:10.735544Z
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 9c212d4b-330c-404c-bb11-a5783667cc14 · inbound
The Formation of Globular Clusters cites this paper.
The Formation of Globular Clusters NGC5846-UDG1: A galaxy formed mostly by star formation in massive, extremely dense clumps of gas
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T13:20:41.134969Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 215855f8-8680-4d9f-a909-ea20b769c149 · inbound
Globular cluster distributions as a dynamical probe of dark matter cites this paper.
Globular cluster distributions as a dynamical probe of dark matter NGC5846-UDG1: A galaxy formed mostly by star formation in massive, extremely dense clumps of gas
Reference 33
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T21:55:10.739679Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation abaf4ad2-7a82-4fa9-9d61-b88ee0591b02 · inbound
Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.
Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins NGC5846-UDG1: A galaxy formed mostly by star formation in massive, extremely dense clumps of gas
Reference 123
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:51:42.465920Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.