Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Hydrostatic mass bias for galaxy groups and clusters in the FLAMINGO simulations
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2409.07849.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T20:08:19.048178Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-16T12:16:17.039197Z
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 c42a636b-bd20-4bcc-b8fc-00fd77849a2d · inbound
Jet outbursts, non-thermal pressure and the AGN jet duty cycle cites this paper.
Jet outbursts, non-thermal pressure and the AGN jet duty cycle Hydrostatic mass bias for galaxy groups and clusters in the FLAMINGO simulations
Reference 8
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-15T20:08:19.576740Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 5394f197-3588-4de4-8b20-1601848b7cc1 · inbound
Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations cites this paper.
Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations Hydrostatic mass bias for galaxy groups and clusters in the FLAMINGO simulations
Reference 115
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T06:10:49.488503Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.