Paper Citation Record · LEDGER

Why z > 1 radio-loud galaxies are commonly located in proto-clusters

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1409.1218.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1409.1218 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T19:42:49.258432Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-06-26T07:59:08.746048Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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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 1c4d321c-eb87-4bd8-a701-4f2f79ecb71e · inbound

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters cites this paper.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Why z > 1 radio-loud galaxies are commonly located in proto-clusters

Reference 114

Resolution: verified exact; local_arxiv, observed 2026-06-26T07:59:08.747170Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation fcff1889-9d08-45c7-aff1-15492ba059d0 · inbound

The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters cites this paper.

The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters Why z > 1 radio-loud galaxies are commonly located in proto-clusters

Reference 48

Resolution: unresolved; no resolver link, observed 2026-07-12T07:56:00.734481Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a0205374-9f17-4ed8-ae0f-e54074f9b6d0 · inbound

Tracing the Cosmic web across Cosmic time through SKA observations of radio galaxies cites this paper.

Tracing the Cosmic web across Cosmic time through SKA observations of radio galaxies Why z > 1 radio-loud galaxies are commonly located in proto-clusters

Reference 145

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:49.322884Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7ac0a7aa-3644-4178-964b-bd153dd8127f · inbound

MIGHTEE-HI: Environmental effects of cosmic filaments on extragalactic HI detections in the COSMOS and XMM-LSS fields cites this paper.

MIGHTEE-HI: Environmental effects of cosmic filaments on extragalactic HI detections in the COSMOS and XMM-LSS fields Why z > 1 radio-loud galaxies are commonly located in proto-clusters

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-06T19:42:49.258432Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.