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Paper Citation Record · LEDGER

Cosmic variance of the galaxy cluster weak lensing signal

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1501.01632.

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

pith.paper-citation-record.v1
1501.01632 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:07:32.296059Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T22:19:00.094752Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 b3caaad7-1e2d-4136-9262-b589442fbcbc · inbound

Weak-lensing mass calibration of \emph{Planck} Sunyaev--Zel'dovich clusters with HSC-SSP Year~3 cites this paper.

Weak-lensing mass calibration of \emph{Planck} Sunyaev--Zel'dovich clusters with HSC-SSP Year~3 Cosmic variance of the galaxy cluster weak lensing signal

Reference 42

Resolution
verified exact
local_arxiv, observed 2026-07-03T22:19:00.096025Z

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=2026-06-26T23:40:05.299484Z digest=sha256:9e5492eef83a9ac446c97d7cd769fa1605407865abc125b559afe00443768553

Observation d3f321df-1e36-4e04-81b2-2f082e1313be · inbound

S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups cites this paper.

S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups Cosmic variance of the galaxy cluster weak lensing signal

Reference 16

Resolution
unresolved
no resolver link, observed 2026-07-12T07:35:44.141755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T07:35:44.141755Z digest=sha256:2c0582112db9c062fa1eb87ab31b78e3a13db70d72839e9930d455a2bf401039

Observation 8e697fa1-9b3e-4c88-9f57-951f25c754ee · 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 Cosmic variance of the galaxy cluster weak lensing signal

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-15T15:07:32.296059Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:07:32.296059Z digest=sha256:2f009e29aa4bdcfb3d8967008c1d32597b2869072ce4b942e38f59703555b1ca