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Paper Citation Record · LEDGER

The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1209.1391.

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

pith.paper-citation-record.v1
1209.1391 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 2026-08-04T06:05:13.498867Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-21T19:50:33.482724Z

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 ea80935f-f415-4974-9929-8e499a162439 · inbound

Self-Interaction of Super-Resonant Dark Matter cites this paper.

Self-Interaction of Super-Resonant Dark Matter The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-05-21T19:50:33.485958Z

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=pdf_text observed=2026-05-21T19:49:36.832677Z digest=sha256:5d551155d3bb53d0b39ff1eb6040c4fe415efcc18c61bb45c3f820484ac2aa02

Observation 886c9df2-bab8-41fe-85de-5b13a42bbe19 · inbound

Exploring Non-minimal coupling using ultra-diffuse galaxies cites this paper.

Exploring Non-minimal coupling using ultra-diffuse galaxies The Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-04T06:05:13.498867Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T06:05:13.498867Z digest=sha256:0af2c345158d112dbef15f142f8d168027524fe7d76ee8e51d05706b786f5392