Paper Citation Record · LEDGER

The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:astro-ph/0312036.

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pith.paper-citation-record.v1
astro-ph/0312036 v2

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measured 7 of 7 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:02:33.248322Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T22:19:00.088214Z

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Outbound references

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Pith citing papers

Observation 6eb5c73e-252b-4524-8c45-1610ae097273 · inbound

Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing cites this paper.

Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

Reference 82

Resolution: verified exact; local_arxiv, observed 2026-05-19T09:35:13.337749Z

Source-reported events for the cited work

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Observation da0fde36-0615-4bb4-8873-6fde181b0a12 · inbound

Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration cites this paper.

Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-06T21:02:33.248322Z

Source-reported events for the cited work

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Observation df4cd2bf-5830-412b-a87d-3eb345348e6c · inbound

Cosmology and Source Redshift Constraints from Galaxy Clustering and Tomographic Weak Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model cites this paper.

Cosmology and Source Redshift Constraints from Galaxy Clustering and Tomographic Weak Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-06T20:59:57.711280Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d1fde32d-abdf-45ed-8da0-cd3290280ad9 · inbound

Constraining Neutrino Mass with the Void Weak Lensing Effect cites this paper.

Constraining Neutrino Mass with the Void Weak Lensing Effect The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

Reference 75

Resolution: verified exact; local_arxiv, observed 2026-05-21T12:35:07.967984Z

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Observation f12bb462-6b3f-44cc-8254-9870bd5f652c · 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 The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-07-03T22:19:00.089368Z

Source-reported events for the cited work

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Observation 5f0b7ec5-28c5-4f81-90b6-e65b0721aeaa · inbound

Revisiting the 'Lensing is Low' Problem with UNIONS cites this paper.

Revisiting the 'Lensing is Low' Problem with UNIONS The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

Reference 133

Resolution: verified exact; local_arxiv, observed 2026-06-26T07:19:07.057811Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c34afc46-fee5-49f8-8c2c-67cd59a53809 · inbound

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? cites this paper.

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

Reference 180

Resolution: verified exact; local_arxiv, observed 2026-07-01T04:15:21.372414Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.