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Paper Citation Record · LEDGER

Probing Dark Energy Using Its Density Instead of Its Equation of State

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0402208.

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

pith.paper-citation-record.v1
astro-ph/0402208 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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T00:32:11.495220Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T09:11:07.363051Z

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 8801b318-7144-45d7-8dce-79cf97a69b6e · inbound

Model-Independent Analysis of Type Ia Supernova Datasets and Implications for Dark Energy cites this paper.

Model-Independent Analysis of Type Ia Supernova Datasets and Implications for Dark Energy Probing Dark Energy Using Its Density Instead of Its Equation of State

Reference 20

Resolution
verified exact
arxiv_id, observed 2026-07-04T16:43:00.120530Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-10T16:10:57.497230Z digest=sha256:1b071d6a40d6044e130cf2b14c45705d9063cb4362fb6be5ec2a2769960b9cda

Observation f6606d56-2ca2-466f-b0e0-a7580a5397da · inbound

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Probing Dark Energy Using Its Density Instead of Its Equation of State

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-06T00:32:11.495220Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T00:32:11.495220Z digest=sha256:ec68d5dc189d66bbe83b2a81a4aeff955d6de030a31462e68d752e4b889efd61