Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1602.08503.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
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 2026-08-12T13:09:11.153329Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-14T19:07:49.225343Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation 8974c392-b700-43af-b830-04fb5ad3ba27 · inbound
Cosmic Structure Formation in the Non-linear Regime: Beyond Gaussian Statistics and Standard Cosmologies Improving lognormal models for cosmological fields
Reference 87
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 532d2a90-66a8-4735-a652-5a91ebd8edd3 · inbound
Diffusion-based mass map reconstruction from weak lensing data Improving lognormal models for cosmological fields
Reference 77
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 48a33031-6ad1-44fe-97c7-76c06d7c8de1 · inbound
Machine-learning applications for weak-lensing cosmology Improving lognormal models for cosmological fields
Reference 146
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.
Observation e557c036-d0c9-4827-87c2-a3fb0dcf16da · inbound
When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Improving lognormal models for cosmological fields
Reference 98
Source-reported events for the cited work
Unavailable: canonical work link unavailable.