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Paper Citation Record · LEDGER

The luminosities, sizes and velocity dispersions of Brightest Cluster Galaxies: Implications for formation history

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0607117.

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

pith.paper-citation-record.v1
astro-ph/0607117 v2

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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T23:42:32.674332Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T07:59:08.400194Z

Reference resolution

0 of 0 outbound references displayed

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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 0db8ed33-2862-43fb-98ad-454ead10f7a0 · inbound

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters cites this paper.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The luminosities, sizes and velocity dispersions of Brightest Cluster Galaxies: Implications for formation history

Reference 25

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:59:08.401444Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:084a4df25cac3562789975dedda191312db75ce3eb24912a0ca9f85dcd93c6c5

Observation 04582c00-2158-4b75-b593-563d61cc36db · inbound

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy cites this paper.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The luminosities, sizes and velocity dispersions of Brightest Cluster Galaxies: Implications for formation history

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-01T23:42:32.674332Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:42:32.674332Z digest=sha256:1676a45b00e122a295d71b77b3c27fd879719ba69df289f7ef557051739c546f