Paper Citation Record · LEDGER

Median Statistics, H_0, and the Accelerating Universe

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0006103.

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

pith.paper-citation-record.v1
astro-ph/0006103 v2

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 2026-08-16T06:30:59.297886+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T11:44:44.501411Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-13T17:38:03.011403Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 6a481019-5947-4614-b1df-40e4460f19ab · inbound

Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\phi$CDM dark energy inflation cosmologies cites this paper.

Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\phi$CDM dark energy inflation cosmologies Median Statistics, H_0, and the Accelerating Universe

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-14T11:44:44.501411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e01064ff-548f-4c7b-8ea8-e26f918b4f24 · inbound

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Median Statistics, H_0, and the Accelerating Universe

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-10T22:01:00.043553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae5c7c27-2f6f-45e7-be58-15a469d3a983 · inbound

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models cites this paper.

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models Median Statistics, H_0, and the Accelerating Universe

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-04T13:43:12.363394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5130fdcf-360f-416d-be4d-e122e42f34ce · inbound

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? cites this paper.

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? Median Statistics, H_0, and the Accelerating Universe

Reference 91

Resolution: verified exact; arxiv_id, observed 2026-07-04T16:16:46.358423Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.