Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Strength in Numbers: Red Galaxies Bolster the Cosmic Star Formation Rate Density at z > 3
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2508.05740.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T23:16:38.404342Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T12:15:01.137692Z
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 84455c61-cf6d-4dad-a38a-1c503ba5bf51 · inbound
CLAPP: The CLASS LLM Agent for Pair Programming cites this paper.
CLAPP: The CLASS LLM Agent for Pair Programming Strength in Numbers: Red Galaxies Bolster the Cosmic Star Formation Rate Density at z > 3
Reference 1
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-05T23:16:38.404342Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation be9d1bcc-13e4-465d-9baa-f8375024b0cf · inbound
A Redshift-based Red Selection of Dusty Star-forming Galaxies cites this paper.
A Redshift-based Red Selection of Dusty Star-forming Galaxies Strength in Numbers: Red Galaxies Bolster the Cosmic Star Formation Rate Density at z > 3
Reference 1
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-30T14:44:45.259016Z
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 41126d53-62c9-42fe-975f-06c00551a73d · inbound
A Population of Red Galaxies with Very Strong Emission Lines at $z > 5$ Revealed by the NIRCam Medium Bands: ''Classic'' LRDs, Dusty Star-Forming Galaxies, and a Missing Population of LRDs cites this paper.
A Population of Red Galaxies with Very Strong Emission Lines at $z > 5$ Revealed by the NIRCam Medium Bands: ''Classic'' LRDs, Dusty Star-Forming Galaxies, and a Missing Population of LRDs Strength in Numbers: Red Galaxies Bolster the Cosmic Star Formation Rate Density at z > 3
Reference 33
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T01:41:30.223554Z
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.