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Paper Citation Record · LEDGER

Semi-analytic predictions for statistical properties of X-ray clusters of galaxies in cold dark matter universes

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9604141.

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

pith.paper-citation-record.v1
astro-ph/9604141 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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T04:48:07.755651Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T16:04:53.397885Z

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 35dfd65c-f2cf-410f-bb5a-af5f36926b2d · inbound

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation cites this paper.

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation Semi-analytic predictions for statistical properties of X-ray clusters of galaxies in cold dark matter universes

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-07T04:48:07.755651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T04:48:07.755651Z digest=sha256:edb35d972d641a36e19c3f106c89986230d7ae5fd7aa326acd02f810576818bf

Observation 742902bd-fc80-40ab-86c0-b9ff84907ec5 · inbound

Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference cites this paper.

Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference Semi-analytic predictions for statistical properties of X-ray clusters of galaxies in cold dark matter universes

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-06-30T16:04:53.399524Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-30T04:52:09.974573Z digest=sha256:95391ae3a322f4f80ffaffaf1d15671da081fe219bd26efd83f976adbb3ee02e