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Paper Citation Record · LEDGER

Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2210.07853.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2210.07853 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:07:32.264034Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-11T16:11:07.971051Z

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 5b02fb7f-a611-4ac8-a742-fe50f290e8b9 · inbound

$4\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback cites this paper.

$4\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances

Reference 18

Resolution
verified exact
arxiv_id, observed 2026-05-11T16:11:07.977448Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-05-09T18:38:12.253954Z digest=sha256:f5898b28944739ec58fee537f79976d39b2feb495d9900b089a2dcfe3245e2de

Observation 5a009fe9-2b51-4535-ab2d-57f7515f8749 · inbound

Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation cites this paper.

Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-15T15:07:32.264034Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:07:32.264034Z digest=sha256:6ea3956fabf733f14934c3ac78751ceb87d319dcb1d0ddd8b6d1b4e8c5adc0a3