Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2410.10559.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T12:53:39.321325Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T08:05:16.230513Z
Reference resolution
0 of 0 outbound references displayed
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- 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 02466509-7aae-4b64-943e-5738ec3f82fe · inbound
BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.
BAO miscalibration cannot rescue late-time solutions to the Hubble tension Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T12:53:39.321325Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6dbcbbd9-d6cd-4d6d-b59b-3710ed2b6c44 · inbound
Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.
Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy
Reference 137
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T11:41:01.817857Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation c0bba374-4291-49cb-bc9a-8c7e5b3e54c0 · inbound
Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.
Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy
Reference 132
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T02:19:23.564909Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 004560b3-b626-48c2-b3c9-a18635b192a4 · inbound
Imprint of swampland-inspired coupled early dark energy cites this paper.
Imprint of swampland-inspired coupled early dark energy Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy
Reference 142
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T15:55:04.696857Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation b069ab79-8815-40f5-a7ce-ac62cd2467a0 · inbound
Hubble tension: the shape wall cites this paper.
Hubble tension: the shape wall Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy
Reference 150
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T08:08:48.173777Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.