Pith. sign in

Paper Citation Record · LEDGER

Evolution of the cluster X-ray scaling relations since z>0.4

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0207445.

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

pith.paper-citation-record.v1
astro-ph/0207445 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 2026-08-20T06:33:59.587034+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:15:20.712795Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-16T02:27:10.034634Z

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 cde61be0-28aa-40a5-b2a2-6a88bcbc6c1a · inbound

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method cites this paper.

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method Evolution of the cluster X-ray scaling relations since z>0.4

Reference 173

Resolution
verified exact
local_arxiv, observed 2026-05-16T02:27:10.037953Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-16T02:22:49.920780Z digest=sha256:6abfb6516d22584a6e7f60b76466d89f9ded582137fe8c23d63aa84313c90b2b

Observation 698b496c-8be5-48e0-abea-125a43184224 · inbound

Probing cosmic anisotropy with galaxy clusters and supernovae cites this paper.

Probing cosmic anisotropy with galaxy clusters and supernovae Evolution of the cluster X-ray scaling relations since z>0.4

Reference 75

Resolution
verified exact
arxiv_id, observed 2026-05-10T22:00:49.791677Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-05-10T20:19:11.159342Z digest=sha256:dce82d7b4c40a3bfb5fdd8140d91b2d2639add26d41439e23926d52cff503c8f

Observation 3ed32ed6-28c4-46a5-9e44-64f61b9b7a08 · 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 Evolution of the cluster X-ray scaling relations since z>0.4

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-10T04:15:20.712795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T04:15:20.712795Z digest=sha256:40a91f625f157b0a61ab4759af95b9a7402c93dbed58e618ad6424342b7c6e79