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Paper Citation Record · LEDGER

Predicting Single-Temperature Fit to Multi-Component Thermal Plasma Spectra

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0504098.

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

pith.paper-citation-record.v1
astro-ph/0504098 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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:15:20.743469Z

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

142
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 8d736096-fabd-4f37-a7a9-0765f0b7a848 · inbound

Beyond Self-Similarity: Reconciling X-Ray Scaling Relations in Galaxy Clusters and Groups cites this paper.

Beyond Self-Similarity: Reconciling X-Ray Scaling Relations in Galaxy Clusters and Groups Predicting Single-Temperature Fit to Multi-Component Thermal Plasma Spectra

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-06-28T12:52:10.298055Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b4cc88e6e898ffeb7a837ed7a6b6c676195331212f55c4f38201defd6ecb594b

Observation 809ae623-8b48-4494-ac5e-865aeb42ddf4 · 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 Predicting Single-Temperature Fit to Multi-Component Thermal Plasma Spectra

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-10T04:15:20.743469Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T04:15:20.743469Z digest=sha256:554070b5e582aafba9b6a38648c13e374dd76b94f2e7a1aa89ca77c24769bdae