Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2410.24026.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T14:34:19.917670Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-19T10:22:14.408009Z
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 e4339c86-7f25-45f1-b10f-39cae0b29358 · inbound
A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter cites this paper.
A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:34:19.917670Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8d1bfe83-c553-492b-94f9-825c2d897268 · inbound
Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges cites this paper.
Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?
Reference 17
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T10:22:14.409589Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.