Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Why are some galaxy clusters underluminous? The very low concentration of the CL2015 mass profile
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1909.11491.
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 2026-08-02T02:52:00.075316Z
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
4
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation ad5435ad-b628-4030-bc27-6a4c94f2c371 · inbound
The Treble Clef radio phoenix and its old nonthermal filaments cites this paper.
The Treble Clef radio phoenix and its old nonthermal filaments Why are some galaxy clusters underluminous? The very low concentration of the CL2015 mass profile
Reference 130
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T23:57:46.375969Z
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 bc32407b-ee98-4cd2-8c98-792da6e2313e · inbound
The topology of the magnetic field in Abell 2255 out to its virial radius. Results from the LOFAR Galaxy Cluster Ultra-Deep Field cites this paper.
The topology of the magnetic field in Abell 2255 out to its virial radius. Results from the LOFAR Galaxy Cluster Ultra-Deep Field Why are some galaxy clusters underluminous? The very low concentration of the CL2015 mass profile
Reference 130
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T02:52:00.075316Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.