Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Mass modeling of galaxy clusters: quantifying hydrostatic bias and contribution from non-thermal pressure
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1608.04388.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T18:16:45.129137Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
11
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation c4328e41-5c14-4777-ac4e-bff90abe0c76 · inbound
SLICE: SPT-CL J0546-5345 -- A prominent strong-lensing cluster at $z=1.07$ cites this paper.
SLICE: SPT-CL J0546-5345 -- A prominent strong-lensing cluster at $z=1.07$ Mass modeling of galaxy clusters: quantifying hydrostatic bias and contribution from non-thermal pressure
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:16:45.129137Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e1a5b007-e7fb-4244-91b1-e22b05ef6657 · inbound
Correcting the hydrostatic mass for non-thermal gas motions: a comparison of two approaches cites this paper.
Correcting the hydrostatic mass for non-thermal gas motions: a comparison of two approaches Mass modeling of galaxy clusters: quantifying hydrostatic bias and contribution from non-thermal pressure
Reference 249
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-02T07:26:44.995461Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.