Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Accretion Shocks in Clusters of Galaxies and their SZ Signature from Cosmological Simulations
As of 24 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0902.3323.
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 2026-08-14T15:11:32.697889Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-12T07:58:38.628514Z
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 c7a411f8-17f8-4036-948e-0532b55ef517 · inbound
Voyage through the Hidden Physics of the Cosmic Web cites this paper.
Voyage through the Hidden Physics of the Cosmic Web Accretion Shocks in Clusters of Galaxies and their SZ Signature from Cosmological Simulations
Reference 1803
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T15:11:32.697889Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8eaf0dc6-379b-4470-95a0-0df33e892809 · inbound
The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters cites this paper.
The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters Accretion Shocks in Clusters of Galaxies and their SZ Signature from Cosmological Simulations
Reference 63
- Resolution
- verified exact
- local_arxiv, observed 2026-07-12T07:58:38.630259Z
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.