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Paper Citation Record · LEDGER

Weighing simulated galaxy clusters using lensing and X-ray

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0912.1343.

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

pith.paper-citation-record.v1
0912.1343 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:15:20.895913Z

measured 1 of 1 external citation measurements

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

302
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b5e0559d-cba2-46b1-9075-af330fe70dbb · inbound

Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era cites this paper.

Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era Weighing simulated galaxy clusters using lensing and X-ray

Reference 180

Resolution
verified exact
local_arxiv, observed 2026-06-25T21:28:28.353364Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:94c2953110867d0b5cd690dc2b30c6829e9be0179bc17c8b34573c00c435927c

Observation 40609710-20db-4ffc-a798-9a85e8c5e88a · 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 simulated galaxy clusters using lensing and X-ray

Reference 229

Resolution
verified exact
local_arxiv, observed 2026-07-02T07:26:45.057721Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:33ccae7907409a8b72ce292414f6fce298a8e58cd4fb99c2212732161957ff04

Observation 665810cc-8a74-4c59-a780-dc8ad6afca8b · inbound

Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations cites this paper.

Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations Weighing simulated galaxy clusters using lensing and X-ray

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-10T04:15:20.895913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T04:15:20.895913Z digest=sha256:bef1ee14749cefcef0b5c3bd903230bd12494f5250f67815de49eeebada31c50