Pith. sign in

Paper Citation Record · LEDGER

Likely Values of the Cosmological Constant

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/9701099.

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

pith.paper-citation-record.v1
astro-ph/9701099 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:56:18.768581Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T00:32:14.086805Z

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 6df5a6ac-c02b-4616-8a9b-6d51770b1860 · inbound

Discretely Evanescent Dark Energy cites this paper.

Discretely Evanescent Dark Energy Likely Values of the Cosmological Constant

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-07T10:56:18.768581Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T10:56:18.768581Z digest=sha256:0ddd4286d3863818c6d82f64b7785a89e9dcb2f9c8d768e9be4158c063a1a5f6

Observation d2f3f2b2-3a96-4aa8-83b1-1051a03e2ac5 · 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? Likely Values of the Cosmological Constant

Reference 49

Resolution
verified exact
local_arxiv, observed 2026-08-06T00:32:14.091286Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-06T00:32:11.074887Z digest=sha256:8101da2afbf126bafaf9514065707564fcc6d02880e34ff724372f3fccd1fa06