Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Detection of Enhancement in Number Densities of Background Galaxies due to Magnification by Massive Galaxy Clusters
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1510.01745.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T05:02:57.825848Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T15:06:29.541030Z
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 b35eea65-98d6-4999-b6c9-03d6c58bc8db · inbound
Weak Lensing Reconstruction by Counting Galaxies: Improvement with DES Y3 Galaxies cites this paper.
Weak Lensing Reconstruction by Counting Galaxies: Improvement with DES Y3 Galaxies Detection of Enhancement in Number Densities of Background Galaxies due to Magnification by Massive Galaxy Clusters
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T05:02:57.825848Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f56673ee-a302-49db-b206-78dd3b9560b5 · inbound
Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies cites this paper.
Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies Detection of Enhancement in Number Densities of Background Galaxies due to Magnification by Massive Galaxy Clusters
Reference 21
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T15:06:29.556041Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.