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Paper Citation Record · LEDGER

The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2312.08277.

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

pith.paper-citation-record.v1
2312.08277 v2

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 2026-08-06T06:34:29.942622+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T14:37:45.897820Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-20T16:13:34.353109Z

Reference resolution

0 of 0 outbound references displayed

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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 0920328e-051d-478a-9091-fdf8a736e062 · inbound

How does feedback affect the star formation histories of galaxies? cites this paper.

How does feedback affect the star formation histories of galaxies? The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-05T14:37:45.897820Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T14:37:45.897820Z digest=sha256:9b7507f7151bd3bcc1cf71c55fef185bd575d28e4f575b7cc1017ec47d9bb90e

Observation e5edfd68-9fbe-4283-9e36-513baeb455f5 · inbound

The limits of feedback from active galactic nuclei cites this paper.

The limits of feedback from active galactic nuclei The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations

Reference 47

Resolution
verified exact
arxiv_id, observed 2026-05-20T16:13:34.356973Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-20T16:13:17.171905Z digest=sha256:981414338b5d044aeafbf9088c855a3ce08bd2e9b929fa7266f6bc930546f71c

Observation 6d9ebff5-c91f-4078-9188-af970ddcf630 · inbound

S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups cites this paper.

S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations

Reference 37

Resolution
unresolved
no resolver link, observed 2026-07-12T07:35:44.141755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T07:35:44.141755Z digest=sha256:b0e7c4f2ae1e9c8276c34444496ec3c129e0700237261523ce84c1ff8304301e

Observation b92c952a-7a69-482c-8e49-732acdcd1317 · inbound

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba cites this paper.

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-01T08:26:03.264135Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T08:26:03.264135Z digest=sha256:210c3174f7d40506901e6d20187e989c5082cdf1177bad1486250508ed0997a6