Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Do we really see a cosmological constant in the supernovae data ?
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/9907206.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T17:56:52.127128Z
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
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 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 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 2026-08-09T06:31:02.800959+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.