Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1004.3988.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T22:32:29.229125Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T14:43:18.255707Z
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 3f3e8975-0056-48b4-ad3e-1a13921258c0 · inbound
Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia cites this paper.
Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
Reference 92
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:30:00.354644Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a12baf12-08ff-42d6-9afc-03aee0feb973 · inbound
Cosmo-Learn: code for learning cosmology using different methods and mock data cites this paper.
Cosmo-Learn: code for learning cosmology using different methods and mock data Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
Reference 102
- Resolution
- verified exact
- local_arxiv, observed 2026-08-05T14:43:18.261719Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 70b8dd29-3a39-418c-aa37-d482c94a16fe · inbound
Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories cites this paper.
Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T22:32:29.229125Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.