Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Observational constraints on stellar feedback in dwarf galaxies
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2205.06825.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:13.079572Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 5d412953-8c82-4093-b949-3656ee1ae742 · inbound
The multiple classes of ultra-diffuse galaxies: Can we tell them apart? cites this paper.
The multiple classes of ultra-diffuse galaxies: Can we tell them apart? Observational constraints on stellar feedback in dwarf galaxies
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T00:56:18.807252Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 46753b0b-ffae-4489-92c4-0cfa8b8fe579 · inbound
The satellite galaxies of the Milky Way and Andromeda cites this paper.
The satellite galaxies of the Milky Way and Andromeda Observational constraints on stellar feedback in dwarf galaxies
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T14:18:30.545995Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a8656a00-afd0-444a-8a6b-4afebfd5b4a3 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry Observational constraints on stellar feedback in dwarf galaxies
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:56.949571Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 100f3d3b-e490-4d99-8a28-2cd99b000d30 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry Observational constraints on stellar feedback in dwarf galaxies
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:13.079572Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.