Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Origin of Star Formation Gradients in Rich Galaxy Clusters
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0004078.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T00:44:52.557544Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T09:57:55.396147Z
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 cf5bc246-af92-4546-aaa8-1683483868bf · inbound
Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation cites this paper.
Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation The Origin of Star Formation Gradients in Rich Galaxy Clusters
Reference 40
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T16:11:02.261561Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 9c1c01cb-586c-4069-a4b5-cffb73e0f125 · inbound
A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations cites this paper.
A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations The Origin of Star Formation Gradients in Rich Galaxy Clusters
Reference 34
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T09:40:47.938727Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 6d580396-dd82-44e1-9136-05f51dc66b03 · inbound
No hidden monsters: Probing recently-quenched galaxies for obscured AGN with JWST-PRIMER MIRI and NIRCam cites this paper.
No hidden monsters: Probing recently-quenched galaxies for obscured AGN with JWST-PRIMER MIRI and NIRCam The Origin of Star Formation Gradients in Rich Galaxy Clusters
Reference 29
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T16:39:35.544299Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation a5a2ef44-2ebb-45dd-8095-8db107bceab7 · inbound
Resolved HI and Environmental Dynamics cites this paper.
Resolved HI and Environmental Dynamics The Origin of Star Formation Gradients in Rich Galaxy Clusters
Reference 7
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T09:57:55.397797Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation becd80a9-f2bd-4257-a15c-cd95f01fc2df · inbound
Identifying backsplash galaxies using machine learning cites this paper.
Identifying backsplash galaxies using machine learning The Origin of Star Formation Gradients in Rich Galaxy Clusters
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:44:52.557544Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.