Pith. sign in

Paper Citation Record · LEDGER

The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1906.02339.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1906.02339 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:52:14.006843Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-10T23:57:46.322495Z

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 ac12e1e1-f862-4b79-ab23-d1c04b73ddcb · inbound

The Treble Clef radio phoenix and its old nonthermal filaments cites this paper.

The Treble Clef radio phoenix and its old nonthermal filaments The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state

Reference 264

Resolution
metadata mismatch
local_arxiv, observed 2026-07-10T23:57:46.345071Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:880d499b373ff3160fc1c40060b485212cd491017e5f4f0c024fb78aaf8c323e

Observation e2932d51-995f-4360-9fa5-9f34587ac278 · 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 The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state

Reference 264

Resolution
unresolved
no resolver link, observed 2026-08-02T02:52:14.006843Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:52:14.006843Z digest=sha256:efafe50f5f1eee3a6cf5488a433f7a2b8b0dd39fb0518b02e20a3c1e8b5fe768