Paper Citation Record · LEDGER

Do we really see a cosmological constant in the supernovae data ?

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/9907206.

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

pith.paper-citation-record.v1
astro-ph/9907206 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:17:22.502959Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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External citation measurements

182
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 6f1cb94f-9cd1-415e-97a6-d0c90002591f · inbound

Inhomogeneous model with a space dependent Cosmological Constant cites this paper.

Inhomogeneous model with a space dependent Cosmological Constant Do we really see a cosmological constant in the supernovae data ?

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-10T20:38:29.841411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7698af89-c8c4-45c4-b0ff-1975581b511e · 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 Do we really see a cosmological constant in the supernovae data ?

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-08T17:56:52.127128Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39a9d9e8-a53e-4026-9470-eaa299ad8db5 · inbound

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude cites this paper.

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude Do we really see a cosmological constant in the supernovae data ?

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-16T12:17:22.502959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1188a850-aae7-420e-bedc-c7efa582e1d0 · 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 Do we really see a cosmological constant in the supernovae data ?

Reference 170

Resolution: verified exact; local_arxiv, observed 2026-06-26T23:00:12.296028Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 687f30b7-9a48-49cc-a8fd-313e223635ac · inbound

Dark Energy Bubble as Dynamical Dark Energy: Properties and CMB Constraints cites this paper.

Dark Energy Bubble as Dynamical Dark Energy: Properties and CMB Constraints Do we really see a cosmological constant in the supernovae data ?

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-01T15:41:47.575049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.