Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
How to detect gravitational waves through the cross-correlation of the galaxy distribution with the CMB polarization
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1201.5374.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T21:31:37.272273Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 eb91cf16-1d8d-4626-a9b9-9d72ed0e136d · inbound
Constraints on the remote quadrupole field from the polarized Sunyaev Zel'dovich effect cites this paper.
Constraints on the remote quadrupole field from the polarized Sunyaev Zel'dovich effect How to detect gravitational waves through the cross-correlation of the galaxy distribution with the CMB polarization
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T21:31:37.272273Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.