Pith. sign in

Paper Citation Record · LEDGER

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

As of 21 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 2026-08-21T06:32:19.484+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=sha256:3dd38b8b821c89770defa8e564b3c4f8f21ea1f6415312eae1c5b4bab4c6c68f

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-08-10T04:15:20.763608Z digest=sha256:c7287f3357a78c70e8b6e66840e68c1fbfab889af5b907772588af49c6e18294