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Paper Citation Record · LEDGER

Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0405340.

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

pith.paper-citation-record.v1
astro-ph/0405340 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T23:12:12.421722Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-21T20:14:20.132250Z

Reference resolution

0 of 0 outbound references displayed

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  • malformed identifier0
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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 7c80bfb9-34db-411c-8301-ac5e9a27e80e · inbound

Topological dark energy from black-hole formations and mergers through the gravity-thermodynamics approach cites this paper.

Topological dark energy from black-hole formations and mergers through the gravity-thermodynamics approach Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-10T23:12:12.421722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:12:12.421722Z digest=sha256:2723d69acb1149efa5015cfe2f84a5a0e3802e0cae20b772921c5e5645a1f72b

Observation ec42b0a1-54bf-48e9-81b4-b0f20daa60b2 · inbound

Observational Tests of Regular Black Holes with Scalar Hair and their Stability cites this paper.

Observational Tests of Regular Black Holes with Scalar Hair and their Stability Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters

Reference 16

Resolution
verified exact
local_arxiv, observed 2026-05-21T20:14:20.134076Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-21T20:13:41.585900Z digest=sha256:ce01db4ef4a8ff06bde563fb90d35a5041b4b96a627516af550a25604395805f

Observation 4963a834-5eed-47f7-84e6-4aaca2aa39f0 · inbound

Anomalous Decay Rate and Greybody Factors for Regular Black Holes with Scalar Hair cites this paper.

Anomalous Decay Rate and Greybody Factors for Regular Black Holes with Scalar Hair Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters

Reference 8

Resolution
verified exact
local_arxiv, observed 2026-05-15T21:50:20.948330Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-15T21:46:56.981507Z digest=sha256:6bf8a2e0a2a38732c504862cbffee0f143c9f5fcd4ba3c60f6038a76c5c72651

Observation 2f739507-7157-4254-b2fd-2d6ee4f43d70 · inbound

Time Like Geodesics of Regular Black Holes with Scalar Hair cites this paper.

Time Like Geodesics of Regular Black Holes with Scalar Hair Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters

Reference 20

Resolution
verified exact
arxiv_id, observed 2026-05-11T13:56:06.833848Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-09T23:49:10.346665Z digest=sha256:137630fd70905186c369a095da47b8bb296dcda7896cb6fc9bf6775221e43800