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Paper Citation Record · LEDGER

On the efficiency and reliability of cluster mass estimates based on member galaxies

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0605151.

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

pith.paper-citation-record.v1
astro-ph/0605151 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T12:44:31.375055Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-12T00:41:15.543338Z

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 781b36e5-e9c3-493c-9ec8-542b558ad304 · inbound

Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos cites this paper.

Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos On the efficiency and reliability of cluster mass estimates based on member galaxies

Reference 98

Resolution
verified exact
arxiv_id, observed 2026-07-04T16:58:41.676148Z

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.

source=pdf_text observed=2026-05-07T14:53:02.246257Z digest=sha256:33ce3ca57615e5548e276a8f0f0fffe886e1e71c7b1b196e1848a1f862f40bf3

Observation 5055a88d-67f3-457d-ac80-64f773518cef · inbound

A pilot sample of Planck-selected strongly lensed sub-mm galaxies: NOEMA observations and physical characterisation cites this paper.

A pilot sample of Planck-selected strongly lensed sub-mm galaxies: NOEMA observations and physical characterisation On the efficiency and reliability of cluster mass estimates based on member galaxies

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-01T12:44:31.375055Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T12:44:31.375055Z digest=sha256:29fc5861aefbe9a7ed99ad373b5799e8550b8fc7cdf0ce69d3f4b7b1be1ffb3a