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Paper Citation Record · LEDGER

Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2007.11583.

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

pith.paper-citation-record.v1
2007.11583 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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-31T05:29:29.901862Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-20T16:13:34.074191Z

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 203b6d99-2e8c-46bf-a0eb-3aa9e8f81118 · inbound

The limits of feedback from active galactic nuclei cites this paper.

The limits of feedback from active galactic nuclei Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect

Reference 76

Resolution
verified exact
arxiv_id, observed 2026-05-20T16:13:34.077043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-20T16:13:17.171905Z digest=sha256:9944b1f293816fc0b67c011ed651f6a750ed861f9617421340b3e2059f652d78

Observation 99ea1439-feae-4a62-ab6e-d6495588bfca · 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 Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect

Reference 74

Resolution
unresolved
no resolver link, observed 2026-07-31T05:29:29.901862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T05:29:29.901862Z digest=sha256:5ccb8bda901eed6336b8cc72966b85662cc438edf5a39b95aedc341505112a97