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Paper Citation Record · LEDGER

A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2207.05834.

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

pith.paper-citation-record.v1
2207.05834 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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:15:20.763608Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T04:15:22.639395Z

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 c7a037e5-fbfd-4cf6-a17d-5dff9a8f3e79 · inbound

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models cites this paper.

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups

Reference 70

Resolution
unresolved
no resolver link, observed 2026-07-31T05:29:29.890769Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T05:29:29.890769Z digest=sha256:b87bd6e499c9adb3798db0ebe3d8ae39bd1018404492128b4ffb8c94d4483c85

Observation 42d8debd-24ec-41e0-a94c-c29f807ccead · 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 A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-08-10T04:15:22.644649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-08-10T04:15:20.763608Z digest=sha256:053c1776df8770c891e57a3bd5e548a3551f862bb6b97adc6cccbbe7048c58f6