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Paper Citation Record · LEDGER

X-ray scaling relations for a representative sample of Planck selected clusters observed with XMM-Newton

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2002.11740.

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

pith.paper-citation-record.v1
2002.11740 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 2026-08-06T06:34:29.942622+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T06:10:12.400726Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-12T07:38:36.853933Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 2022a8d5-8e24-4734-bf66-6ce23f7e838e · inbound

S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups cites this paper.

S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups X-ray scaling relations for a representative sample of Planck selected clusters observed with XMM-Newton

Reference 29

Resolution
verified exact
local_arxiv, observed 2026-07-12T07:38:36.856002Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-12T07:35:44.141755Z digest=sha256:5ea6155ef31d30540626a61168355a987e00094d7d946ceb20fe6021af646568

Observation f1c96c84-1172-4fd9-bc49-4f45e4972359 · inbound

Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations cites this paper.

Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations X-ray scaling relations for a representative sample of Planck selected clusters observed with XMM-Newton

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-02T06:10:12.400726Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T06:10:12.400726Z digest=sha256:019c113460db58664aae78f28ecfabd8205fa6773f52ae616e7c45226d85283a

Observation c6a13693-cafc-4f3e-ae23-c5f7adaf2dcd · inbound

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba cites this paper.

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba X-ray scaling relations for a representative sample of Planck selected clusters observed with XMM-Newton

Reference 114

Resolution
unresolved
no resolver link, observed 2026-08-01T08:26:08.694844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T08:26:08.694844Z digest=sha256:aff1bbd5408f352a16df0ab4645948268a9cf562ef00747085945abd36d4fbe1