Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2312.08277.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T17:19:39.963208Z
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
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Pith citing papers
Observation bfda29c3-cdcd-4394-ab72-6739834e58e7 · inbound
The Power Spectrum of the Thermal Sunyaev-Zeldovich Effect cites this paper.
The Power Spectrum of the Thermal Sunyaev-Zeldovich Effect The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T18:59:00.935501Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 86336a46-f365-4235-ada9-ec43c9591d52 · inbound
Unified weak lensing constraints on the evolution of the mass -- X-ray luminosity relation for galaxy clusters cites this paper.
Unified weak lensing constraints on the evolution of the mass -- X-ray luminosity relation for galaxy clusters The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T13:32:05.522400Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 91c9d9f8-4de7-46c8-b422-fee98378569f · inbound
Baryonification II: Constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations cites this paper.
Baryonification II: Constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:36:06.228617Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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.
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
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
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.
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.
Observation 77173d9b-eee8-4c94-a9c0-3957c44dd219 · inbound
Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations cites this paper.
Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T04:15:20.655817Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 89ffc935-df89-41a8-b560-97919fd56b2c · inbound
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations
Reference 93
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T17:19:39.963208Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.