Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2210.17318.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T05:02:57.846389Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T15:06:29.427788Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 e7d2ed6c-27d4-4615-885d-3eec2f85d1e2 · 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 Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T05:02:57.846389Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9f585b04-6afb-455d-ad6b-4b7ffc23d37c · 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 Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T15:06:29.431875Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.