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Paper Citation Record · LEDGER

Measuring the galaxy-mass and galaxy-dust correlations through magnification and reddening

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0902.4240.

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

pith.paper-citation-record.v1
0902.4240 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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T05:02:57.803303Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-12T00:36:14.397046Z

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 ea4b2021-08a0-43cc-b303-5e51aefdf955 · 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 Measuring the galaxy-mass and galaxy-dust correlations through magnification and reddening

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-12T05:02:57.803303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T05:02:57.803303Z digest=sha256:df5137017e602cd2a2708d108e3e8385cdbf883dcde608052ac78ca95e67c727

Observation afcbebd9-e27f-441e-9c25-3d173a930166 · inbound

Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe cites this paper.

Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe Measuring the galaxy-mass and galaxy-dust correlations through magnification and reddening

Reference 109

Resolution
verified exact
arxiv_id, observed 2026-07-04T19:31:58.834647Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-07T15:00:09.282977Z digest=sha256:00f43910f7491a24be73c811537cf9ee4ff389ea4114c988e4344bbf90e84bde