Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1306.3993.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T23:42:37.950621Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-02T07:26:45.130410Z
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 a24a3207-4305-4ac9-bb01-aa7101f30299 · inbound
Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster cites this paper.
Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias
Reference 12
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T05:01:39.372326Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 7eb251db-e991-4a90-bae4-e240398de79b · 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 Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias
Reference 239
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T07:26:45.131786Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 8712b96c-9b7f-4ddc-a828-96c9b30d8a29 · inbound
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy cites this paper.
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy Weighing Galaxy Clusters with Gas. I. On the Methods of Computing Hydrostatic Mass Bias
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:42:37.950621Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.