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Paper Citation Record · LEDGER

Lower AGN Abundance in Galaxy Clusters at z < 0.5

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1912.10342.

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

pith.paper-citation-record.v1
1912.10342 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:26:31.485389Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T10:26:32.183924Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 e2611b12-a3be-416c-a745-1ff278015de1 · inbound

Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation cites this paper.

Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation Lower AGN Abundance in Galaxy Clusters at z < 0.5

Reference 64

Resolution
verified exact
local_arxiv, observed 2026-08-07T10:26:32.187847Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-08-07T10:26:31.485389Z digest=sha256:c4481841ae32fcfb548ecaae3e6c70e3423aabd2206358e79114284bb3b54d1a

Observation 9a4347f6-4c3a-492e-a73a-648568771f68 · inbound

Fuelling the central region of galaxies with misaligned gas accretion cites this paper.

Fuelling the central region of galaxies with misaligned gas accretion Lower AGN Abundance in Galaxy Clusters at z < 0.5

Reference 192

Resolution
unresolved
no resolver link, observed 2026-08-02T01:00:44.369781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T01:00:44.369781Z digest=sha256:ccb980e5806becff5675de52add94f8bedce33f64df5fde19aeaccbf6cf5bc0d

Observation 1355d3dd-84a9-4647-856d-de0e60f2760c · inbound

Too many quiescent late-type galaxies or a matter of misclassification? cites this paper.

Too many quiescent late-type galaxies or a matter of misclassification? Lower AGN Abundance in Galaxy Clusters at z < 0.5

Reference 192

Resolution
unresolved
no resolver link, observed 2026-07-31T08:31:42.028733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T08:31:42.028733Z digest=sha256:bbffb3f56b17bcee74b9794128faf4203cee5ddac6bdbdf1782cbde0561bd24f