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Paper Citation Record · LEDGER

WMAP 5-year constraints on time variation of $\alpha$ and $m_e$

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0910.1083.

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

pith.paper-citation-record.v1
0910.1083 v2

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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:18:05.560699Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T15:37:06.169670Z

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 e3036b5c-8a13-493a-a6b7-3c939525b160 · inbound

Towards degeneracy breaking of early universe models cites this paper.

Towards degeneracy breaking of early universe models WMAP 5-year constraints on time variation of $\alpha$ and $m_e$

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-14T14:18:05.560699Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:18:05.560699Z digest=sha256:cd059e9fab872d05eea66f422ba6390d28483bce16328d7c69099f562574e20f

Observation a7051da8-ee4e-47fa-982e-d2a50d6eff74 · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 WMAP 5-year constraints on time variation of $\alpha$ and $m_e$

Reference 153

Resolution
verified exact
local_arxiv, observed 2026-07-02T15:37:06.171004Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-06-27T23:47:15.644279Z digest=sha256:083ee4d5b39c58afa452a2d38e1b6463d34f84d23a8b0c92f84cb8e670a3daee