Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulations
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2312.05126.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T04:15:20.614968Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-20T16:13:34.016324Z
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 97e941b6-f9ca-4603-8f16-693d3ed2df60 · inbound
The limits of feedback from active galactic nuclei cites this paper.
The limits of feedback from active galactic nuclei Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulations
Reference 68
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T16:13:34.018802Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation b3a9e518-5eaa-4997-a5f2-2ec7e32ab503 · 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 Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulations
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T04:15:20.614968Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.