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Paper Citation Record · LEDGER

Simulations of X-ray Clusters

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9408069.

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

pith.paper-citation-record.v1
astro-ph/9408069 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 2026-08-15T06:32:42.880941+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T00:06:27.226367Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-19T20:22:45.109125Z

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 6516f6a1-05d4-49bc-aafa-9612d6d5f1cb · inbound

Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison cites this paper.

Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison Simulations of X-ray Clusters

Reference 88

Resolution
verified exact
local_arxiv, observed 2026-05-19T20:22:45.110515Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e715d36d2fa4f55fe9b727c956d282beff8f93adfb09e9459db3bf5c99f9670e

Observation 44d0807d-49b9-4061-9ab7-ce5f77e59573 · inbound

Eccentricity-Modulated Phase Degeneracy and Distinguishability between Dark Matter and Accretion Disk Environmental Effects in EMRIs cites this paper.

Eccentricity-Modulated Phase Degeneracy and Distinguishability between Dark Matter and Accretion Disk Environmental Effects in EMRIs Simulations of X-ray Clusters

Reference 58

Resolution
unresolved
no resolver link, observed 2026-07-13T04:38:50.936878Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T04:38:50.936878Z digest=sha256:854c3307b75c412adf85ead39ce6367e7cbe511acb7154490c541490f232819a

Observation dec36e73-b8a1-437b-b563-444a6186cfa7 · inbound

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies cites this paper.

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies Simulations of X-ray Clusters

Reference 173

Resolution
unresolved
no resolver link, observed 2026-08-06T00:06:27.226367Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T00:06:27.226367Z digest=sha256:a2ca31260b358e9c7b94f8ff5963751aff3367573d3a0b6a5bd89248dbcb0d05