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Paper Citation Record · LEDGER

An inhomogeneous alternative to dark energy?

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0512006.

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

pith.paper-citation-record.v1
astro-ph/0512006 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T17:56:52.131424Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T23:00:12.457733Z

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 5ab752bf-6994-4df1-8955-e259dd0578bf · inbound

CMB dipoles and other low-order multipoles in the quasispherical Szekeres model cites this paper.

CMB dipoles and other low-order multipoles in the quasispherical Szekeres model An inhomogeneous alternative to dark energy?

Reference 13

Resolution
verified exact
local_arxiv, observed 2026-05-24T18:54:50.876194Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-24T18:53:10.493042Z digest=sha256:1beb46e20ed8efb2a6c6dabf037cfa5471cd82b43ed1a3b5c79ea4505d5ab7d2

Observation 851e7cba-256e-4fbe-8605-ed4427f2c37c · inbound

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions cites this paper.

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions An inhomogeneous alternative to dark energy?

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-08T17:56:52.131424Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T17:56:52.131424Z digest=sha256:2ca54dfb90ea44045b28681713276521212c241076375e0b1e8a36424c110927

Observation bed6db92-d214-46b2-a73e-7decaa74b9c6 · inbound

Impact of inhomogeneous curvature on growth rate measurements from magnitude fluctuations cites this paper.

Impact of inhomogeneous curvature on growth rate measurements from magnitude fluctuations An inhomogeneous alternative to dark energy?

Reference 171

Resolution
verified exact
local_arxiv, observed 2026-06-26T23:00:12.459470Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:964e396d53ff41ab529a0c19f5327c31e5ad52ed58249c990bcfdb69f24d5da7