Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Blowing out the Candle: How to Quench Galaxies at High Redshift -- an Ensemble of Rapid Starbursts, AGN Feedback and Environment
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2310.16085.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T17:55:46.163671Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-12T00:16:22.474752Z
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 38c9f99d-66e8-4db0-8594-ecd62c66ba85 · inbound
COALAS III: The ATCA CO(1-0) look at the growth and death of H$\alpha$ emitters in the Spiderweb protocluster at z=2.16 cites this paper.
COALAS III: The ATCA CO(1-0) look at the growth and death of H$\alpha$ emitters in the Spiderweb protocluster at z=2.16 Blowing out the Candle: How to Quench Galaxies at High Redshift -- an Ensemble of Rapid Starbursts, AGN Feedback and Environment
Reference 108
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:55:46.163671Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1f478705-3ac8-4a44-8254-7fc0011f636c · inbound
Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? cites this paper.
Why do some Ultra Diffuse Galaxies have Rich Globular Cluster Systems? Blowing out the Candle: How to Quench Galaxies at High Redshift -- an Ensemble of Rapid Starbursts, AGN Feedback and Environment
Reference 61
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-11T20:03:51.894027Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.